{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,5,8]],"date-time":"2026-05-08T14:37:32Z","timestamp":1778251052641,"version":"3.51.4"},"reference-count":644,"publisher":"IOP Publishing","issue":"9","license":[{"start":{"date-parts":[[2023,4,4]],"date-time":"2023-04-04T00:00:00Z","timestamp":1680566400000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/publishingsupport.iopscience.iop.org\/iop-standard\/v1"},{"start":{"date-parts":[[2023,4,4]],"date-time":"2023-04-04T00:00:00Z","timestamp":1680566400000},"content-version":"tdm","delay-in-days":0,"URL":"https:\/\/iopscience.iop.org\/info\/page\/text-and-data-mining"}],"funder":[{"name":"China Manned Space Project","award":["CMS-CSST-2021-B01"],"award-info":[{"award-number":["CMS-CSST-2021-B01"]}]},{"DOI":"10.13039\/501100001809","name":"National Natural Science Foundation of China","doi-asserted-by":"crossref","award":["12105344"],"award-info":[{"award-number":["12105344"]}],"id":[{"id":"10.13039\/501100001809","id-type":"DOI","asserted-by":"crossref"}]},{"DOI":"10.13039\/501100003725","name":"National Research Foundation of Korea","doi-asserted-by":"crossref","id":[{"id":"10.13039\/501100003725","id-type":"DOI","asserted-by":"crossref"}]},{"name":"Korea government","award":["ISEF\/M\/400121"],"award-info":[{"award-number":["ISEF\/M\/400121"]}]},{"name":"POCH\/FSE"},{"name":"F.R.S.\u2013FNRS","award":["T.0116.21"],"award-info":[{"award-number":["T.0116.21"]}]},{"DOI":"10.13039\/501100002646","name":"Sogang University","doi-asserted-by":"crossref","id":[{"id":"10.13039\/501100002646","id-type":"DOI","asserted-by":"crossref"}]},{"name":"FCT","award":["2021.01214"],"award-info":[{"award-number":["2021.01214"]}]},{"DOI":"10.13039\/501100008530","name":"FEDER","doi-asserted-by":"crossref","award":["COMPETE 2020"],"award-info":[{"award-number":["COMPETE 2020"]}],"id":[{"id":"10.13039\/501100008530","id-type":"DOI","asserted-by":"crossref"}]}],"content-domain":{"domain":["iopscience.iop.org"],"crossmark-restriction":false},"short-container-title":["Class. Quantum Grav."],"published-print":{"date-parts":[[2023,5,4]]},"abstract":"<jats:title>Abstract<\/jats:title>\n               <jats:p>The cosmological principle (CP)\u2014the notion that the Universe is spatially isotropic and homogeneous on large scales\u2014underlies a century of progress in cosmology. It is conventionally formulated through the Friedmann-Lema\u00eetre-Robertson-Walker (FLRW) cosmologies as the spacetime metric, and culminates in the successful and highly predictive \u039b-Cold-Dark-Matter (\u039bCDM) model. Yet, tensions have emerged within the \u039bCDM model, most notably a statistically significant discrepancy in the value of the Hubble constant, <jats:italic>H<\/jats:italic>\n                  <jats:sub>0<\/jats:sub>. Since the notion of cosmic expansion determined by a single parameter is intimately tied to the CP, implications of the <jats:italic>H<\/jats:italic>\n                  <jats:sub>0<\/jats:sub> tension may extend beyond \u039bCDM to the CP itself. This review surveys current observational hints for deviations from the expectations of the CP, highlighting synergies and disagreements that warrant further study. Setting aside the debate about individual large structures, potential deviations from the CP include variations of cosmological parameters on the sky, discrepancies in the cosmic dipoles, and mysterious alignments in quasar polarizations and galaxy spins. While it is possible that a host of observational systematics are impacting results, it is equally plausible that precision cosmology may have outgrown the FLRW paradigm, an extremely pragmatic but non-fundamental symmetry assumption.<\/jats:p>","DOI":"10.1088\/1361-6382\/acbefc","type":"journal-article","created":{"date-parts":[[2023,2,24]],"date-time":"2023-02-24T17:45:15Z","timestamp":1677260715000},"page":"094001","update-policy":"https:\/\/doi.org\/10.1088\/crossmark-policy","source":"Crossref","is-referenced-by-count":188,"title":["Is the observable Universe consistent with the cosmological principle?"],"prefix":"10.1088","volume":"40","author":[{"given":"Pavan","family":"Kumar Aluri","sequence":"first","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0001-5267-1461","authenticated-orcid":true,"given":"Paolo","family":"Cea","sequence":"additional","affiliation":[]},{"given":"Pravabati","family":"Chingangbam","sequence":"additional","affiliation":[]},{"given":"Ming-Chung","family":"Chu","sequence":"additional","affiliation":[]},{"given":"Roger G","family":"Clowes","sequence":"additional","affiliation":[]},{"given":"Damien","family":"Hutsem\u00e9kers","sequence":"additional","affiliation":[]},{"given":"Joby P","family":"Kochappan","sequence":"additional","affiliation":[]},{"given":"Alexia M","family":"Lopez","sequence":"additional","affiliation":[]},{"given":"Lang","family":"Liu","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2839-1387","authenticated-orcid":true,"given":"Niels C M","family":"Martens","sequence":"additional","affiliation":[]},{"given":"C J A P","family":"Martins","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0451-0449","authenticated-orcid":true,"given":"Konstantinos","family":"Migkas","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0813-5156","authenticated-orcid":true,"given":"Eoin","family":"\u00d3 Colg\u00e1in","sequence":"additional","affiliation":[]},{"given":"Pratyush","family":"Pranav","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-6207-1491","authenticated-orcid":false,"given":"Lior","family":"Shamir","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-8479-7656","authenticated-orcid":true,"given":"Ashok K","family":"Singal","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-3728-230X","authenticated-orcid":false,"given":"M M","family":"Sheikh-Jabbari","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0002-4999-3838","authenticated-orcid":true,"given":"Jenny","family":"Wagner","sequence":"additional","affiliation":[]},{"given":"Shao-Jiang","family":"Wang","sequence":"additional","affiliation":[]},{"ORCID":"https:\/\/orcid.org\/0000-0003-1992-6682","authenticated-orcid":true,"given":"David L","family":"Wiltshire","sequence":"additional","affiliation":[]},{"given":"Shek","family":"Yeung","sequence":"additional","affiliation":[]},{"given":"Lu","family":"Yin","sequence":"additional","affiliation":[]},{"given":"Wen","family":"Zhao","sequence":"additional","affiliation":[]}],"member":"266","published-online":{"date-parts":[[2023,4,4]]},"reference":[{"key":"cqgacbefcbib1","author":"Hawking","year":"1973","type":"book"},{"key":"cqgacbefcbib2","first-page":"23","type":"journal-article","article-title":"Cosmological principles I. Symmetry principles","volume":"6","author":"Ellis","year":"1974","journal-title":"Comments Astrophys. Space Phys."},{"key":"cqgacbefcbib3","author":"Weinberg","year":"1972","type":"book"},{"key":"cqgacbefcbib4","article-title":"Alternatives to the cosmological principle: a survey","author":"Wiltshire","year":"2023","type":"other"},{"key":"cqgacbefcbib5","doi-asserted-by":"publisher","first-page":"9","DOI":"10.1038\/130009a0","type":"journal-article","article-title":"World structure and the expansion of the Universe","volume":"130","author":"Milne","year":"1932","journal-title":"Nature"},{"key":"cqgacbefcbib6","author":"Bondi","year":"1952","type":"book"},{"key":"cqgacbefcbib7","author":"Raychaudhuri","year":"1979","type":"book"},{"key":"cqgacbefcbib8","first-page":"pp 267","type":"book","article-title":"Thoughts on the Cosmological Principle","author":"Schwarz","year":"2010"},{"key":"cqgacbefcbib9","doi-asserted-by":"publisher","first-page":"5115","DOI":"10.1098\/rsta.2011.0289","type":"journal-article","article-title":"Is the Universe homogeneous?","volume":"369","author":"Maartens","year":"2011","journal-title":"Phil. Trans. R. Soc. A"},{"key":"cqgacbefcbib10","doi-asserted-by":"publisher","first-page":"682","DOI":"10.1016\/j.crhy.2012.04.005","type":"journal-article","article-title":"Establishing homogeneity of the universe in the shadow of dark energy","volume":"13","author":"Clarkson","year":"2012","journal-title":"C. R. Physique"},{"key":"cqgacbefcbib11","doi-asserted-by":"publisher","first-page":"1630007","DOI":"10.1142\/S021827181630007X","type":"journal-article","article-title":"Observational challenges for the standard FLRW model","volume":"25","author":"Buchert","year":"2016","journal-title":"Int. J. Mod. Phys. D"},{"key":"cqgacbefcbib12","doi-asserted-by":"publisher","DOI":"10.1098\/rsta.2021.0191","type":"journal-article","article-title":"100 years of mathematical cosmology: models, theories and problems, part A","volume":"380","author":"Cotsakis","year":"2022","journal-title":"Phil. Trans. R. Soc. A"},{"key":"cqgacbefcbib13","doi-asserted-by":"publisher","first-page":"2118","DOI":"10.1103\/PhysRevD.28.2118","type":"journal-article","article-title":"Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant","volume":"28","author":"Wald","year":"1983","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib14","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.85.123508","type":"journal-article","article-title":"Revisiting cosmic no-hair theorem for inflationary settings","volume":"85","author":"Maleknejad","year":"2012","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib15","doi-asserted-by":"publisher","first-page":"54","DOI":"10.1086\/429084","type":"journal-article","article-title":"Cosmic homogeneity demonstrated with luminous red galaxies","volume":"624","author":"Hogg","year":"2005","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib16","doi-asserted-by":"publisher","first-page":"601","DOI":"10.1111\/j.1365-2966.2005.09578.x","type":"journal-article","article-title":"Testing homogeneity on large scales in the Sloan digital sky survey data release one","volume":"364","author":"Yadav","year":"2005","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib17","doi-asserted-by":"publisher","first-page":"116","DOI":"10.1111\/j.1365-2966.2012.21402.x","type":"journal-article","article-title":"The WiggleZ dark energy survey: the transition to large-scale cosmic homogeneity","volume":"425","author":"Scrimgeour","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib18","doi-asserted-by":"publisher","first-page":"JCAP06(2017)019","DOI":"10.1088\/1475-7516\/2017\/06\/019","type":"journal-article","article-title":"Exploring cosmic homogeneity with the BOSS DR12 galaxy sample","author":"Ntelis","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib19","doi-asserted-by":"publisher","first-page":"4743","DOI":"10.1093\/mnras\/stz499","type":"journal-article","article-title":"Unravelling the cosmic web: an analysis of the Sloan Digital Sky Survey Data Release 14 with the local dimension","volume":"485","author":"Sarkar","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib20","doi-asserted-by":"publisher","first-page":"JCAP10(2022)088","DOI":"10.1088\/1475-7516\/2022\/10\/088","type":"journal-article","article-title":"The angular scale of homogeneity with SDSS-IV DR16 luminous red galaxies","author":"Andrade","year":"2022","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib21","doi-asserted-by":"publisher","first-page":"JCAP11(2016)060","DOI":"10.1088\/1475-7516\/2016\/11\/060","type":"journal-article","article-title":"A 14 h\u22123 Gpc3 study of cosmic homogeneity using BOSS DR12 quasar sample","author":"Laurent","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib22","doi-asserted-by":"publisher","first-page":"5270","DOI":"10.1093\/mnras\/sty2670","type":"journal-article","article-title":"Measuring the scale of cosmic homogeneity with SDSS-IV DR14 quasars","volume":"481","author":"Gon\u00e7alves","year":"2018","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib23","doi-asserted-by":"publisher","first-page":"JCAP03(2021)029","DOI":"10.1088\/1475-7516\/2021\/03\/029","type":"journal-article","article-title":"Measuring the cosmic homogeneity scale with SDSS-IV DR16 quasars","author":"Gon\u00e7alves","year":"2021","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib24","doi-asserted-by":"publisher","DOI":"10.1209\/0295-5075\/88\/59001","type":"journal-article","article-title":"Galaxy distribution and extreme-value statistics","volume":"88","author":"Antal","year":"2009","journal-title":"Europhys. Lett."},{"key":"cqgacbefcbib25","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/28\/16\/164003","type":"journal-article","article-title":"Inhomogeneities in the universe","volume":"28","author":"Sylos Labini","year":"2011","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib26","doi-asserted-by":"publisher","first-page":"1924","DOI":"10.1093\/mnras\/stx988","type":"journal-article","article-title":"The cosmological principle is not in the sky","volume":"469","author":"Park","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib27","doi-asserted-by":"publisher","first-page":"A114","DOI":"10.1051\/0004-6361\/202141081","type":"journal-article","article-title":"Zipf\u2019s law for cosmic structures: how large are the greatest structures in the universe?","volume":"651","author":"De Marzo","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib28","doi-asserted-by":"publisher","first-page":"A139","DOI":"10.1051\/0004-6361\/202141909","type":"journal-article","article-title":"CMASS galaxy sample and the ontological status of the cosmological principle","volume":"660","author":"Kim","year":"2022","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib29","doi-asserted-by":"publisher","first-page":"2009","DOI":"10.1111\/j.1365-2966.2010.16612.x","type":"journal-article","article-title":"Fractal dimension as a measure of the scale of homogeneity","volume":"405","author":"Yadav","year":"2010","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib30","doi-asserted-by":"publisher","first-page":"463","DOI":"10.1086\/428890","type":"journal-article","article-title":"A map of the Universe","volume":"624","author":"Gott","year":"2005","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib31","doi-asserted-by":"publisher","first-page":"2938","DOI":"10.1111\/j.1365-2966.2011.19453.x","type":"journal-article","article-title":"How unusual are the Shapley supercluster and the Sloan Great Wall?","volume":"417","author":"Sheth","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib32","doi-asserted-by":"publisher","first-page":"L7","DOI":"10.1088\/2041-8205\/759\/1\/L7","type":"journal-article","article-title":"The challenge of the largest structures in the Universe to cosmology","volume":"759","author":"Park","year":"2012","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib33","doi-asserted-by":"publisher","first-page":"2910","DOI":"10.1093\/mnras\/sts497","type":"journal-article","article-title":"A structure in the early Universe at z \u223c 1.3 that exceeds the homogeneity scale of the R-W concordance cosmology","volume":"429","author":"Clowes","year":"2013","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib34","doi-asserted-by":"publisher","first-page":"2236","DOI":"10.1093\/mnras\/stv1421","type":"journal-article","article-title":"A giant ring-like structure at 0.78<z<0.86 displayed by GRBs","volume":"452","author":"Bal\u00e1zs","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib35","doi-asserted-by":"publisher","first-page":"L12","DOI":"10.1051\/0004-6361\/201323020","type":"journal-article","article-title":"Possible structure in the GRB sky distribution at redshift two","volume":"561","author":"Horv\u00e1th","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib36","doi-asserted-by":"publisher","first-page":"A48","DOI":"10.1051\/0004-6361\/201424829","type":"journal-article","article-title":"New data support the existence of the Hercules-Corona Borealis Great Wall","volume":"584","author":"Horv\u00e1th","year":"2015","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib37","doi-asserted-by":"publisher","first-page":"2544","DOI":"10.1093\/mnras\/staa2460","type":"journal-article","article-title":"The clustering of gamma-ray bursts in the Hercules-Corona Borealis Great Wall: the largest structure in the Universe?","volume":"498","author":"Horvath","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib38","doi-asserted-by":"publisher","first-page":"1557","DOI":"10.1093\/mnras\/stac2204","type":"journal-article","article-title":"A Giant Arc on the Sky","volume":"516","author":"Lopez","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib39","doi-asserted-by":"publisher","first-page":"398","DOI":"10.1093\/mnras\/stt1028","type":"journal-article","article-title":"Seeing patterns in noise: gigaparsec-scale \u2018structures\u2019 that do not violate homogeneity","volume":"434","author":"Nadathur","year":"2013","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib40","doi-asserted-by":"publisher","first-page":"703","DOI":"10.1093\/mnras\/stv2350","type":"journal-article","article-title":"Investigation of redshift- and duration-dependent clustering of gamma-ray bursts","volume":"455","author":"Ukwatta","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib41","doi-asserted-by":"publisher","first-page":"4291","DOI":"10.1093\/mnras\/staa1448","type":"journal-article","article-title":"Re-examining the evidence of the Hercules-Corona Borealis Great Wall","volume":"495","author":"Christian","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib42","doi-asserted-by":"publisher","DOI":"10.1002\/asna.20220021","type":"journal-article","article-title":"Doubt on the statistical significance of the Giant GRB Ring","volume":"343","author":"Fujii","year":"2022","journal-title":"Astron. Nachr."},{"key":"cqgacbefcbib43","doi-asserted-by":"publisher","first-page":"29","DOI":"10.2298\/SAJ2204029F","type":"journal-article","article-title":"Large-scale homogeneity in the distribution of quasars in the Hercules-Corona Borealis Great Wall region","volume":"204","author":"Fujii","year":"2022","journal-title":"Serb. Astron. J."},{"key":"cqgacbefcbib44","doi-asserted-by":"publisher","first-page":"2267","DOI":"10.1093\/mnras\/stw1513","type":"journal-article","article-title":"Compatibility of the large quasar groups with the concordance cosmological model","volume":"461","author":"Marinello","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib45","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.103.103509","type":"journal-article","article-title":"Running Hubble tension and a H0 diagnostic","volume":"103","author":"Krishnan","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib46","article-title":"H 0 as a Universal FLRW diagnostic","author":"Krishnan","year":"2022","type":"preprint"},{"key":"cqgacbefcbib47","doi-asserted-by":"publisher","DOI":"10.3847\/2041-8213\/ac5c5b","type":"preprint","article-title":"A comprehensive measurement of the local value of the hubble constant with 1 km\u2009s\u22121\/Mpc uncertainty from the hubble space telescope and the SH0ES team","author":"Riess","year":"2021"},{"key":"cqgacbefcbib48","doi-asserted-by":"publisher","first-page":"A6","DOI":"10.1051\/0004-6361\/201833910","type":"journal-article","article-title":"Planck 2018 results. VI. Cosmological parameters","volume":"641","author":"(Planck Collaboration)","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib49","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/ac086d","type":"journal-article","article-title":"In the realm of the Hubble tension-a review of solutions","volume":"38","author":"Di Valentino","year":"2021","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib50","doi-asserted-by":"publisher","first-page":"49","DOI":"10.1016\/j.jheap.2022.04.002","type":"journal-article","article-title":"Cosmology intertwined: a review of the particle physics, astrophysics and cosmology associated with the cosmological tensions and anomalies","volume":"34","author":"Abdalla","year":"2022","journal-title":"J. High Energy Astrophys."},{"key":"cqgacbefcbib51","doi-asserted-by":"publisher","first-page":"119","DOI":"10.1088\/0004-637X\/730\/2\/119","type":"journal-article","article-title":"A 3% solution: determination of the hubble constant with the hubble space telescope and wide field camera 3","volume":"730","author":"Riess","year":"2011","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib52","doi-asserted-by":"publisher","first-page":"19","DOI":"10.1088\/0067-0049\/208\/2\/19","type":"journal-article","article-title":"Nine-year Wilkinson microwave anisotropy probe (WMAP) observations: cosmological parameter results","volume":"208","author":"Hinshaw","year":"2013","journal-title":"Astrophys. J. Suppl."},{"key":"cqgacbefcbib53","doi-asserted-by":"publisher","first-page":"5","DOI":"10.3847\/1538-4357\/ab5dbd","type":"journal-article","article-title":"Hubble space telescope observations of mira variables in the SN Ia Host NGC 1559: an alternative candle to measure the hubble constant","volume":"889","author":"Huang","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib54","doi-asserted-by":"publisher","first-page":"3402","DOI":"10.1093\/mnras\/staa1801","type":"journal-article","article-title":"A measurement of the Hubble constant from type II supernovae","volume":"496","author":"de Jaeger","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib55","doi-asserted-by":"publisher","first-page":"L1","DOI":"10.3847\/2041-8213\/ab75f0","type":"journal-article","article-title":"The megamaser cosmology project. XIII. Combined hubble constant constraints","volume":"891","author":"Pesce","year":"2020","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib56","doi-asserted-by":"publisher","first-page":"3","DOI":"10.3847\/1538-4357\/ab901c","type":"journal-article","article-title":"Cosmicflows-4: the calibration of optical and infrared Tully-Fisher relations","volume":"896","author":"Kourkchi","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib57","doi-asserted-by":"publisher","first-page":"71","DOI":"10.3847\/1538-3881\/ab9d88","type":"journal-article","article-title":"Using the baryonic tully-fisher relation to measure H o","volume":"160","author":"Schombert","year":"2020","journal-title":"Astron. J."},{"key":"cqgacbefcbib58","doi-asserted-by":"publisher","first-page":"A72","DOI":"10.1051\/0004-6361\/202039196","type":"journal-article","article-title":"A new measurement of the Hubble constant using Type Ia supernovae calibrated with surface brightness fluctuations","volume":"647","author":"Khetan","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib59","doi-asserted-by":"publisher","first-page":"65","DOI":"10.3847\/1538-4357\/abe86a","type":"journal-article","article-title":"The hubble constant from infrared surface brightness fluctuation distances","volume":"911","author":"Blakeslee","year":"2021","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib60","doi-asserted-by":"publisher","first-page":"16","DOI":"10.3847\/1538-4357\/ac0e95","type":"journal-article","article-title":"Measurements of the hubble constant: tensions in perspective","volume":"919","author":"Freedman","year":"2021","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib61","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.102.023518","type":"journal-article","article-title":"New physics in light of the H0 tension: an alternative view","volume":"102","author":"Vagnozzi","year":"2020","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib62","doi-asserted-by":"publisher","first-page":"2845","DOI":"10.1093\/mnras\/staa2348","type":"journal-article","article-title":"The KBC void and Hubble tension contradict \u039bCDM on a Gpc scale\u2014Milgromian dynamics as a possible solution","volume":"499","author":"Haslbauer","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib63","doi-asserted-by":"publisher","DOI":"10.3847\/1538-4357\/ac756e","type":"preprint","article-title":"Sensitivity of the hubble constant determination to cepheid calibration","author":"Mortsell","year":"2021"},{"key":"cqgacbefcbib64","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.123511","type":"journal-article","article-title":"Hubble tension or a transition of the Cepheid SnIa calibrator parameters?","volume":"104","author":"Perivolaropoulos","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib65","doi-asserted-by":"publisher","DOI":"10.1209\/0295-5075\/ac52dc","type":"journal-article","article-title":"Did the Universe experience a pressure non-crushing type cosmological singularity in the recent past?","volume":"137","author":"Odintsov","year":"2022","journal-title":"Europhys. Lett."},{"key":"cqgacbefcbib66","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/ac1a81","type":"journal-article","article-title":"Does Hubble tension signal a breakdown in FLRW cosmology?","volume":"38","author":"Krishnan","year":"2021","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib67","doi-asserted-by":"publisher","DOI":"10.1016\/j.jheap.2022.07.004","type":"preprint","article-title":"Implications for the Hubble tension from the ages of the oldest astrophysical objects","author":"Vagnozzi","year":"2021"},{"key":"cqgacbefcbib68","doi-asserted-by":"publisher","first-page":"14","DOI":"10.1086\/382267","type":"journal-article","article-title":"Asymmetries in the cosmic microwave background anisotropy field","volume":"605","author":"Eriksen","year":"2004","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib69","doi-asserted-by":"publisher","first-page":"313","DOI":"10.1111\/j.1365-2966.2004.07500.x","type":"journal-article","article-title":"Non-Gaussian signatures in the temperature fluctuation observed by the Wilkinson Microwave anisotropy probe","volume":"349","author":"Park","year":"2004","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib70","doi-asserted-by":"publisher","first-page":"641","DOI":"10.1111\/j.1365-2966.2004.08229.x","type":"journal-article","article-title":"Testing the cosmological principle of isotropy: local power-spectrum estimates of the WMAP data","volume":"354","author":"Hansen","year":"2004","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib71","doi-asserted-by":"publisher","first-page":"L81","DOI":"10.1086\/518091","type":"journal-article","article-title":"Hemispherical power asymmetry in the third-Year Wilkinson microwave anisotropy probe sky maps","volume":"660","author":"Eriksen","year":"2007","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib72","doi-asserted-by":"publisher","first-page":"1448","DOI":"10.1088\/0004-637X\/704\/2\/1448","type":"journal-article","article-title":"Power asymmetry in cosmic microwave background fluctuations from full sky to sub-degree scales: is the universe isotropic?","volume":"704","author":"Hansen","year":"2009","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib73","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.69.063516","type":"journal-article","article-title":"Significance of the largest scale CMB fluctuations in WMAP","volume":"69","author":"de Oliveira-Costa","year":"2004","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib74","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.93.221301","type":"journal-article","article-title":"Is the low- \u2113 microwave background cosmic?","volume":"93","author":"Schwarz","year":"2004","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib75","doi-asserted-by":"publisher","first-page":"1857","DOI":"10.1142\/S0218271804005948","type":"journal-article","article-title":"The virgo alignment puzzle in propagation of radiation on cosmological scales","volume":"13","author":"Ralston","year":"2004","journal-title":"Int. J. Mod. Phys. D"},{"key":"cqgacbefcbib76","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.72.101302","type":"journal-article","article-title":"Is the Universe odd?","volume":"72","author":"Land","year":"2005","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib77","doi-asserted-by":"publisher","first-page":"JCAP07(2012)049","DOI":"10.1088\/1475-7516\/2012\/07\/049","type":"journal-article","article-title":"Searching for hidden mirror symmetries in CMB fluctuations from WMAP 7 year maps","author":"Finelli","year":"2012","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib78","doi-asserted-by":"publisher","first-page":"39","DOI":"10.1088\/0004-637X\/748\/1\/39","type":"journal-article","article-title":"Parity in the cosmic microwave background: space oddity","volume":"748","author":"Ben-David","year":"2012","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib79","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.82.063002","type":"journal-article","article-title":"Anomalous parity asymmetry of WMAP 7-year power spectrum data at low multipoles: Is it cosmological or systematics?","volume":"82","author":"Kim","year":"2010","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib80","doi-asserted-by":"publisher","first-page":"3378","DOI":"10.1111\/j.1365-2966.2011.19981.x","type":"journal-article","article-title":"Parity asymmetry in the CMBR temperature power spectrum","volume":"419","author":"Aluri","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib81","doi-asserted-by":"publisher","first-page":"898","DOI":"10.1103\/PhysRevLett.39.898","type":"journal-article","article-title":"Detection of anisotropy in the cosmic blackbody radiation","volume":"39","author":"Smoot","year":"1977","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib82","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/25\/12\/125006","type":"journal-article","article-title":"Do we live in a \u2018small Universe\u2019?","volume":"25","author":"Aurich","year":"2008","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib83","doi-asserted-by":"publisher","first-page":"609","DOI":"10.1111\/j.1365-2966.2009.14682.x","type":"journal-article","article-title":"The study of topology of the Universe using multipole vectors","volume":"396","author":"Bielewicz","year":"2009","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib84","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/29\/23\/235028","type":"journal-article","article-title":"Cosmic topology of polyhedral double-action manifolds","volume":"29","author":"Aurich","year":"2012","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib85","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/31\/16\/165009","type":"journal-article","article-title":"The Hantzsche-Wendt manifold in cosmic topology","volume":"31","author":"Aurich","year":"2014","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib86","article-title":"Topology and the suppression of CMB large-angle correlations","author":"Bernui","year":"2018","type":"preprint"},{"key":"cqgacbefcbib87","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/ac27f0","type":"journal-article","article-title":"The variance of the CMB temperature gradient: a new signature of a multiply connected Universe","volume":"38","author":"Aurich","year":"2021","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib88","article-title":"The Search for the Topology of the Universe Has Just Begun","author":"Akrami","year":"2022","type":"preprint"},{"key":"cqgacbefcbib89","doi-asserted-by":"publisher","first-page":"108","DOI":"10.1007\/BF01645908","type":"journal-article","article-title":"A class of homogeneous cosmological models","volume":"12","author":"Ellis","year":"1969","journal-title":"Commun. Math. Phys."},{"key":"cqgacbefcbib90","doi-asserted-by":"publisher","first-page":"5840","DOI":"10.1093\/mnras\/stab1193","type":"journal-article","article-title":"Explaining cosmological anisotropy: evidence for causal horizons from CMB data","volume":"504","author":"Fosalba","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib91","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.105.083508","type":"journal-article","article-title":"Directional variations of cosmological parameters from the Planck CMB data","volume":"105","author":"Yeung","year":"2022","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib92","doi-asserted-by":"publisher","first-page":"L3","DOI":"10.1088\/2041-8205\/773\/1\/L3","type":"journal-article","article-title":"Directional dependence of \u039bCDM cosmological parameters","volume":"773","author":"Axelsson","year":"2013","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib93","doi-asserted-by":"publisher","first-page":"JCAP06(2016)042","DOI":"10.1088\/1475-7516\/2016\/06\/042","type":"journal-article","article-title":"Direction dependence of cosmological parameters due to cosmic hemispherical asymmetry","author":"Mukherjee","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib94","doi-asserted-by":"publisher","first-page":"JCAP01(2018)042","DOI":"10.1088\/1475-7516\/2018\/01\/042","type":"journal-article","article-title":"Making maps of cosmological parameters","author":"Mukherjee","year":"2018","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib95","doi-asserted-by":"publisher","first-page":"359","DOI":"10.1093\/mnras\/175.2.359","type":"journal-article","article-title":"Light elements and the isotropy of the Universe","volume":"175","author":"Barrow","year":"1976","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib96","doi-asserted-by":"publisher","first-page":"L1","DOI":"10.1086\/444454","type":"journal-article","article-title":"Evidence of vorticity and shear at large angular scales in the WMAP data: a violation of cosmological isotropy?","volume":"629","author":"Jaffe","year":"2005","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib97","doi-asserted-by":"publisher","first-page":"701","DOI":"10.1086\/503893","type":"journal-article","article-title":"On the viability of bianchi type VII h models with dark energy","volume":"644","author":"Jaffe","year":"2006","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib98","doi-asserted-by":"publisher","first-page":"A26","DOI":"10.1051\/0004-6361\/201321546","type":"journal-article","article-title":"Planck 2013 results. XXVI. Background geometry and topology of the Universe","volume":"571","author":"Collaboration","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib99","doi-asserted-by":"publisher","first-page":"A18","DOI":"10.1051\/0004-6361\/201525829","type":"journal-article","article-title":"Planck 2015 results. XVIII. Background geometry and topology of the Universe","volume":"594","author":"Collaboration","year":"2016","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib100","doi-asserted-by":"publisher","first-page":"307","DOI":"10.1093\/mnras\/162.4.307","type":"journal-article","article-title":"The rotation and distortion of the Universe","volume":"162","author":"Collins","year":"1973","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib101","doi-asserted-by":"publisher","first-page":"917","DOI":"10.1093\/mnras\/213.4.917","type":"journal-article","article-title":"Universal rotation\u2014how large can it be?","volume":"213","author":"Barrow","year":"1985","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib102","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.97.131302","type":"journal-article","article-title":"Ellipsoidal universe can solve the cosmic microwave background quadrupole problem","volume":"97","author":"Campanelli","year":"2006","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib103","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.77.023534","type":"journal-article","article-title":"Anisotropic cosmological constant and the CMB quadrupole anomaly","volume":"77","author":"Rodrigues","year":"2008","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib104","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1086\/587451","type":"journal-article","article-title":"Accelerating cosmologies with an anisotropic equation of state","volume":"679","author":"Koivisto","year":"2008","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib105","doi-asserted-by":"publisher","first-page":"1473","DOI":"10.1111\/j.1365-2966.2007.11616.x","type":"journal-article","article-title":"Markov chain Monte Carlo analysis of Bianchi VII h models","volume":"377","author":"Bridges","year":"2007","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib106","doi-asserted-by":"publisher","first-page":"3680","DOI":"10.1093\/mnras\/stt1855","type":"journal-article","article-title":"Bayesian analysis of anisotropic cosmologies: bianchi VII h and WMAP","volume":"436","author":"McEwen","year":"2013","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib107","doi-asserted-by":"publisher","first-page":"1387","DOI":"10.1111\/j.1365-2966.2007.12221.x","type":"journal-article","article-title":"Bianchi model CMB polarization and its implications for CMB anomalies","volume":"380","author":"Pontzen","year":"2007","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib108","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.79.103518","type":"journal-article","article-title":"Rogues\u2019 gallery: the full freedom of the bianchi CMB anomalies","volume":"79","author":"Pontzen","year":"2009","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib109","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.117.131302","type":"journal-article","article-title":"How isotropic is the universe?","volume":"117","author":"Saadeh","year":"2016","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib110","doi-asserted-by":"publisher","first-page":"A151","DOI":"10.1051\/0004-6361\/202140296","type":"journal-article","article-title":"Cosmological implications of the anisotropy of ten galaxy cluster scaling relations","volume":"649","author":"Migkas","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib111","doi-asserted-by":"publisher","first-page":"L23","DOI":"10.1088\/2041-8205\/742\/2\/L23","type":"journal-article","article-title":"Large peculiar motion of the solar system from the dipole anisotropy in sky brightness due to distant radio sources","volume":"742","author":"Singal","year":"2011","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib112","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.100.063501","type":"journal-article","article-title":"Large disparity in cosmic reference frames determined from the sky distributions of radio sources and the microwave background radiation","volume":"100","author":"Singal","year":"2019","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib113","doi-asserted-by":"publisher","first-page":"L51","DOI":"10.3847\/2041-8213\/abdd40","type":"journal-article","article-title":"A test of the cosmological principle with quasars","volume":"908","author":"Secrest","year":"2021","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib114","doi-asserted-by":"publisher","first-page":"31","DOI":"10.1088\/0004-637X\/749\/1\/31","type":"journal-article","article-title":"Is the cosmic microwave background asymmetry due to the kinematic dipole?","volume":"749","author":"Naselsky","year":"2012","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib115","doi-asserted-by":"publisher","first-page":"A1","DOI":"10.1051\/0004-6361\/201527101","type":"journal-article","article-title":"Planck 2015 results. I. Overview of products and scientific results","volume":"594","author":"Collaboration","year":"2016","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib116","doi-asserted-by":"publisher","first-page":"A23","DOI":"10.1051\/0004-6361\/201321534","type":"journal-article","article-title":"Planck 2013 results. XXIII. Isotropy and statistics of the CMB","volume":"571","author":"Collaboration","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib117","doi-asserted-by":"publisher","first-page":"L42","DOI":"10.1088\/2041-8205\/784\/2\/L42","type":"journal-article","article-title":"Power asymmetry in WMAP and planck temperature sky maps as measured by a local variance estimator","volume":"784","author":"Akrami","year":"2014","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib118","doi-asserted-by":"publisher","first-page":"19","DOI":"10.1086\/166066","type":"journal-article","article-title":"Photometry and spectroscopy of elliptical galaxies. V. Galaxy streaming toward the new supergalactic center","volume":"326","author":"Lynden-Bell","year":"1988","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib119","doi-asserted-by":"publisher","first-page":"JCAP12(2010)012","DOI":"10.1088\/1475-7516\/2010\/12\/012","type":"journal-article","article-title":"Searching for a cosmological preferred axis: Union2 data analysis and comparison with other probes","author":"Antoniou","year":"2010","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib120","doi-asserted-by":"publisher","first-page":"77","DOI":"10.1088\/0004-637X\/719\/1\/77","type":"journal-article","article-title":"The error budget of the dark flow measurement","volume":"719","author":"Atrio-Barandela","year":"2010","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib121","doi-asserted-by":"publisher","first-page":"1445","DOI":"10.1111\/j.1365-2966.2010.17773.x","type":"journal-article","article-title":"New constraints on parity symmetry from a re-analysis of the WMAP-7 low-resolution power spectra","volume":"411","author":"Gruppuso","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib122","doi-asserted-by":"publisher","first-page":"377","DOI":"10.1093\/mnras\/206.2.377","type":"journal-article","article-title":"On the expected anisotropy of radio source counts","volume":"206","author":"Ellis","year":"1984","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib123","doi-asserted-by":"publisher","first-page":"A1","DOI":"10.1051\/0004-6361\/201833880","type":"journal-article","article-title":"Planck 2018 results. I. Overview and the cosmological legacy of Planck","volume":"641","author":"Collaboration","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib124","doi-asserted-by":"publisher","first-page":"JCAP03(2016)062","DOI":"10.1088\/1475-7516\/2016\/03\/062","type":"journal-article","article-title":"Revisiting the NVSS number count dipole","author":"Tiwari","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib125","doi-asserted-by":"publisher","first-page":"A117","DOI":"10.1051\/0004-6361\/201321215","type":"journal-article","article-title":"Cosmic radio dipole from NVSS and WENSS","volume":"555","author":"Rubart","year":"2013","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib126","doi-asserted-by":"publisher","first-page":"JCAP04(2018)031","DOI":"10.1088\/1475-7516\/2018\/04\/031","type":"journal-article","article-title":"Probing the Cosmological Principle in the counts of radio galaxies at different frequencies","author":"Bengaly","year":"2018","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib127","doi-asserted-by":"publisher","first-page":"A9","DOI":"10.1051\/0004-6361\/202039840","type":"journal-article","article-title":"Cosmic radio dipole: Estimators and frequency dependence","volume":"653","author":"Siewert","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib128","doi-asserted-by":"publisher","first-page":"5969","DOI":"10.1093\/mnras\/stac1986","type":"journal-article","article-title":"Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology","volume":"515","author":"Singal","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib129","doi-asserted-by":"publisher","first-page":"1819","DOI":"10.1093\/mnras\/stac144","type":"journal-article","article-title":"Solar system peculiar motion from the Hubble diagram of quasars and testing the cosmological principle","volume":"511","author":"Singal","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib130","article-title":"A challenge to the standard cosmological model","author":"Secrest","year":"2022","type":"preprint"},{"key":"cqgacbefcbib131","doi-asserted-by":"publisher","first-page":"150","DOI":"10.1038\/416150a","type":"journal-article","article-title":"A velocity dipole in the distribution of radio galaxies","volume":"416","author":"Blake","year":"2002","journal-title":"Nature"},{"key":"cqgacbefcbib132","doi-asserted-by":"publisher","DOI":"10.1051\/0004-6361\/202142640","type":"preprint","article-title":"Inference of the cosmic rest-frame from supernovae Ia","author":"Horstmann","year":"2021"},{"key":"cqgacbefcbib133","doi-asserted-by":"publisher","DOI":"10.3847\/2041-8213\/ac6f08","type":"preprint","article-title":"The universe is brighter in the direction of our motion: galaxy counts and fluxes are consistent with the CMB Dipole","author":"Darling","year":"2022"},{"key":"cqgacbefcbib134","doi-asserted-by":"publisher","first-page":"JCAP10(2012)036","DOI":"10.1088\/1475-7516\/2012\/10\/036","type":"journal-article","article-title":"The scale of cosmic isotropy","author":"Marinoni","year":"2012","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib135","doi-asserted-by":"publisher","first-page":"A78","DOI":"10.1051\/0004-6361\/201628536","type":"journal-article","article-title":"The GMRT 150 MHz all-sky radio survey. First alternative data release TGSS ADR1","volume":"598","author":"Intema","year":"2017","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib136","doi-asserted-by":"publisher","first-page":"A148","DOI":"10.1051\/0004-6361\/201834317","type":"journal-article","article-title":"Clustering properties of TGSS radio sources","volume":"623","author":"Dolfi","year":"2019","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib137","doi-asserted-by":"publisher","first-page":"3895","DOI":"10.1093\/mnras\/stac726","type":"journal-article","article-title":"On the kinematic cosmic dipole tension","volume":"512","author":"Dalang","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib138","doi-asserted-by":"publisher","first-page":"3098","DOI":"10.1093\/mnras\/stab3652","type":"journal-article","article-title":"The effects of lensing by local structures on the dipole of radio source counts","volume":"510","author":"Murray","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib139","article-title":"Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole","author":"Guandalin","year":"2022","type":"preprint"},{"key":"cqgacbefcbib140","doi-asserted-by":"publisher","first-page":"A104","DOI":"10.1051\/0004-6361\/201629313","type":"journal-article","article-title":"The LOFAR two-metre sky survey. I. Survey description and preliminary data release","volume":"598","author":"Shimwell","year":"2017","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib141","doi-asserted-by":"publisher","first-page":"e007","DOI":"10.1017\/pasa.2019.51","type":"journal-article","article-title":"Cosmology with phase 1 of the square kilometre array red book 2018: technical specifications and performance forecasts","volume":"37","author":"(Square kilometre array cosmology science working group)","year":"2020","journal-title":"Publ. Astron. Soc. Aust."},{"key":"cqgacbefcbib142","article-title":"Probing cosmology beyond \u039bCDM using the SKA","author":"Ghosh","year":"2023","type":"preprint"},{"key":"cqgacbefcbib143","doi-asserted-by":"publisher","first-page":"A16","DOI":"10.1051\/0004-6361\/201526681","type":"journal-article","article-title":"Planck 2015 results. XVI. Isotropy and statistics of the CMB","volume":"594","author":"Collaboration","year":"2016","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib144","doi-asserted-by":"publisher","first-page":"A7","DOI":"10.1051\/0004-6361\/201935201","type":"journal-article","article-title":"Planck 2018 results. VII. Isotropy and statistics of the CMB","volume":"641","author":"Collaboration","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib145","doi-asserted-by":"publisher","first-page":"A90","DOI":"10.1051\/0004-6361\/201321880","type":"journal-article","article-title":"Measuring cosmic bulk flows with type Ia supernovae from the nearby supernova factory","volume":"560","author":"Feindt","year":"2013","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib146","doi-asserted-by":"publisher","first-page":"0036","DOI":"10.1038\/s41550-016-0036","type":"journal-article","article-title":"The dipole repeller","volume":"1","author":"Hoffman","year":"2017","journal-title":"Nat. Astron."},{"key":"cqgacbefcbib147","doi-asserted-by":"publisher","first-page":"765","DOI":"10.1134\/1.1424358","type":"journal-article","article-title":"The bulk motion of flat galaxies on scales of 100 Mpc in the quadrupole and octupole approximations","volume":"27","author":"Parnovsky","year":"2001","journal-title":"Astron. Lett."},{"key":"cqgacbefcbib148","doi-asserted-by":"publisher","first-page":"1121","DOI":"10.1111\/j.1365-2966.2012.21750.x","type":"journal-article","article-title":"(Mis)interpreting supernovae observations in a lumpy universe","volume":"426","author":"Clarkson","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib149","doi-asserted-by":"publisher","first-page":"JCAP05(2021)008","DOI":"10.1088\/1475-7516\/2021\/05\/008","type":"journal-article","article-title":"Multipole decomposition of the general luminosity distance \u2018Hubble law\u2019\u2014a new framework for observational cosmology","author":"Heinesen","year":"2021","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib150","doi-asserted-by":"publisher","first-page":"4841","DOI":"10.1093\/mnras\/stac3812","type":"journal-article","article-title":"The quadrupole in the local Hubble parameter: first constraints using Type Ia supernova data and forecasts for future surveys","volume":"519","author":"Dhawan","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib151","doi-asserted-by":"publisher","first-page":"47","DOI":"10.1086\/320638","type":"journal-article","article-title":"Final results from the hubble space telescope key project to measure the Hubble constant","volume":"553","author":"Freedman","year":"2001","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib152","doi-asserted-by":"publisher","first-page":"533","DOI":"10.1016\/j.newast.2007.03.005","type":"journal-article","article-title":"Anisotropy in the Hubble constant as observed in the HST extragalactic distance scale key project results","volume":"12","author":"McClure","year":"2007","journal-title":"New Astron."},{"key":"cqgacbefcbib153","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.88.083529","type":"journal-article","article-title":"Hubble flow variance and the cosmic rest frame","volume":"88","author":"Wiltshire","year":"2013","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib154","doi-asserted-by":"publisher","first-page":"743","DOI":"10.1111\/j.1365-2966.2008.14089.x","type":"journal-article","article-title":"Consistently large cosmic flows on scales of 100 h\u22121 Mpc: a challenge for the standard \u039bCDM cosmology","volume":"392","author":"Watkins","year":"2009","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib155","doi-asserted-by":"publisher","first-page":"L49","DOI":"10.1086\/592947","type":"journal-article","article-title":"A measurement of large-scale peculiar velocities of clusters of galaxies: results and cosmological implications","volume":"686","author":"Kashlinsky","year":"2008","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib156","doi-asserted-by":"publisher","first-page":"483","DOI":"10.1088\/0004-637X\/709\/1\/483","type":"journal-article","article-title":"Cosmic flow from two micron all-sky redshift survey: the origin of cosmic microwave background dipole and implications for \u039bCDM cosmology","volume":"709","author":"Lavaux","year":"2010","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib157","first-page":"pp 336","type":"book","article-title":"Measuring the cosmic bulk flow with 6dFGSv","volume":"vol 308","author":"Magoulas","year":"2016"},{"key":"cqgacbefcbib158","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/stac1681","type":"preprint","article-title":"The sloan digital sky survey peculiar velocity catalogue","author":"Howlett","year":"2022"},{"key":"cqgacbefcbib159","doi-asserted-by":"publisher","first-page":"A15","DOI":"10.1051\/0004-6361\/201936602","type":"journal-article","article-title":"Probing cosmic isotropy with a new X-ray galaxy cluster sample through the L X -T scaling relation","volume":"636","author":"Migkas","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib160","doi-asserted-by":"publisher","first-page":"101","DOI":"10.3847\/1538-4357\/aab9bb","type":"journal-article","article-title":"The complete light-curve sample of spectroscopically confirmed SNe Ia from Pan-STARRS1 and cosmological constraints from the combined pantheon sample","volume":"859","author":"Scolnic","year":"2018","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib161","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.105.063514","type":"journal-article","article-title":"Hints of FLRW breakdown from supernovae","volume":"105","author":"Krishnan","year":"2022","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib162","doi-asserted-by":"publisher","first-page":"1409","DOI":"10.1111\/j.1365-2966.2009.15755.x","type":"journal-article","article-title":"Does the Universe accelerate equally in all directions?","volume":"401","author":"Cooke","year":"2010","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib163","doi-asserted-by":"publisher","first-page":"2653","DOI":"10.1140\/epjc\/s10052-013-2653-x","type":"journal-article","article-title":"\u039bCDM model with a scalar perturbation vs. preferred direction of the universe","volume":"73","author":"Li","year":"2013","journal-title":"Eur. Phys. J. C"},{"key":"cqgacbefcbib164","doi-asserted-by":"publisher","first-page":"47","DOI":"10.1088\/0004-637X\/810\/1\/47","type":"journal-article","article-title":"Probing the isotropy of cosmic acceleration traced by type Ia supernovae","volume":"810","author":"Javanmardi","year":"2015","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib165","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/stac2414","type":"preprint","article-title":"The XMM cluster survey analysis of the SDSS DR8 redMaPPer catalogue: implications for scatter, selection bias and isotropy in cluster scaling relations","author":"Giles","year":"2022"},{"key":"cqgacbefcbib166","doi-asserted-by":"publisher","first-page":"104","DOI":"10.1088\/0004-637X\/785\/2\/104","type":"journal-article","article-title":"redMaPPer. I. Algorithm and SDSS DR8 catalog","volume":"785","author":"Rykoff","year":"2014","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib167","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.105.103510","type":"journal-article","article-title":"Larger H0 values in the CMB dipole direction","volume":"105","author":"Luongo","year":"2022","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib168","doi-asserted-by":"publisher","first-page":"1994","DOI":"10.1111\/j.1365-2966.2012.22032.x","type":"journal-article","article-title":"Dipoles in the sky","volume":"427","author":"Gibelyou","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib169","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.87.043511","type":"journal-article","article-title":"CMB maximum temperature asymmetry axis: alignment with other cosmic asymmetries","volume":"87","author":"Mariano","year":"2013","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib170","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.86.083517","type":"journal-article","article-title":"Is there correlation between fine structure and dark energy cosmic dipoles?","volume":"86","author":"Mariano","year":"2012","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib171","author":"Ellis","year":"2012","type":"book"},{"key":"cqgacbefcbib172","doi-asserted-by":"publisher","first-page":"897","DOI":"10.1126\/science.246.4932.897","type":"journal-article","article-title":"Mapping the Universe","volume":"246","author":"Geller","year":"1989","journal-title":"Science"},{"key":"cqgacbefcbib173","author":"Gabrielli","year":"2005","type":"book"},{"key":"cqgacbefcbib174","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1007\/BF01877593","type":"journal-article","article-title":"Isotropic solutions of the Einstein-Boltzmann equations","volume":"23","author":"Treciokas","year":"1971","journal-title":"Commun. Math. Phys."},{"key":"cqgacbefcbib175","doi-asserted-by":"publisher","first-page":"218","DOI":"10.1093\/mnras\/249.2.218","type":"journal-article","article-title":"A 100\u2013200 Mpc group of quasars","volume":"249","author":"Clowes","year":"1991","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib176","doi-asserted-by":"publisher","first-page":"JCAP10(2020)052","DOI":"10.1088\/1475-7516\/2020\/10\/052","type":"journal-article","article-title":"Cosmological homogeneity scale estimates are dressed","author":"Heinesen","year":"2020","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib177","doi-asserted-by":"publisher","first-page":"241","DOI":"10.1093\/mnras\/stu1118","type":"journal-article","article-title":"Direct Minkowski Functional analysis of large redshift surveys: a new high-speed code tested on the luminous red galaxy Sloan digital Sky Survey-DR7 catalogue","volume":"443","author":"Wiegand","year":"2014","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib178","doi-asserted-by":"publisher","first-page":"71","DOI":"10.1038\/nature13674","type":"journal-article","article-title":"The Laniakea supercluster of galaxies","volume":"513","author":"Tully","year":"2014","journal-title":"Nature"},{"key":"cqgacbefcbib179","doi-asserted-by":"publisher","first-page":"133","DOI":"10.3847\/1538-4357\/ab9952","type":"journal-article","article-title":"Cosmicflows-3: the South Pole Wall","volume":"897","author":"Pomar\u00e8de","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib180","doi-asserted-by":"publisher","first-page":"130","DOI":"10.1088\/0004-637X\/770\/2\/130","type":"journal-article","article-title":"The JHU-SDSS metal absorption line catalog: redshift evolution and properties of Mg II absorbers","volume":"770","author":"Zhu","year":"2013","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib181","doi-asserted-by":"publisher","first-page":"73","DOI":"10.1111\/j.2517-6161.1990.tb01773.x","type":"journal-article","article-title":"Spatial clustering for inhomogeneous populations","volume":"52","author":"Cuzick","year":"1990","journal-title":"J. R. Stat. Soc. B"},{"key":"cqgacbefcbib182","doi-asserted-by":"publisher","first-page":"556","DOI":"10.1111\/j.1365-2966.2011.19719.x","type":"journal-article","article-title":"Two close large quasar groups of size \u2009 350 Mpc at z\u223c1.2","volume":"419","author":"Clowes","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib183","doi-asserted-by":"publisher","first-page":"61","DOI":"10.1093\/mnras\/175.1.61","type":"journal-article","article-title":"The clustering of radio sources\u2014I. The theory of power-spectrum analysis","volume":"175","author":"Webster","year":"1976","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib184","doi-asserted-by":"publisher","first-page":"8","DOI":"10.3847\/1538-4365\/aba623","type":"journal-article","article-title":"The Sloan digital sky survey quasar catalog: sixteenth data release","volume":"250","author":"Lyke","year":"2020","journal-title":"Astrophys. J. Suppl. Ser."},{"key":"cqgacbefcbib185","doi-asserted-by":"publisher","first-page":"3169","DOI":"10.1093\/mnras\/stx2550","type":"journal-article","article-title":"Some statistical remarks on the giant GRB ring","volume":"473","author":"Bal\u00e1zs","year":"2018","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib186","doi-asserted-by":"publisher","DOI":"10.1016\/j.dark.2020.100565","type":"journal-article","article-title":"Duel of cosmological screening lengths","volume":"29","author":"Canay","year":"2020","journal-title":"Phys. Dark Universe"},{"key":"cqgacbefcbib187","doi-asserted-by":"publisher","DOI":"10.1016\/j.newar.2022.101659","type":"preprint","article-title":"Challenges for \u039bCDM: an update","author":"Perivolaropoulos","year":"2021"},{"key":"cqgacbefcbib188","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/33\/18\/184001","type":"journal-article","article-title":"CMB anomalies after Planck","volume":"33","author":"Schwarz","year":"2016","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib189","doi-asserted-by":"publisher","first-page":"733","DOI":"10.1007\/s10909-013-0996-1","type":"journal-article","article-title":"Mission design of LiteBIRD","volume":"176","author":"Matsumura","year":"2014","journal-title":"J. Low Temp. Phys."},{"key":"cqgacbefcbib190","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.083504","type":"journal-article","article-title":"Most constraining cosmological neutrino mass bounds","volume":"104","author":"Di Valentino","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib191","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2022\/09\/006","type":"preprint","article-title":"Neutrino masses and mass hierarchy: evidence for the normal hierarchy","author":"Jimenez","year":"2022"},{"key":"cqgacbefcbib192","doi-asserted-by":"publisher","first-page":"A104","DOI":"10.1051\/0004-6361\/202039070","type":"journal-article","article-title":"KiDS-1000 cosmology: cosmic shear constraints and comparison between two point statistics","volume":"645","author":"Asgari","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib193","doi-asserted-by":"publisher","first-page":"A140","DOI":"10.1051\/0004-6361\/202039063","type":"journal-article","article-title":"KiDS-1000 cosmology: multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints","volume":"646","author":"Heymans","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib194","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.105.023514","type":"journal-article","article-title":"Dark energy survey year 3 results: cosmology from cosmic shear and robustness to data calibration","volume":"105","author":"Amon","year":"2022","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib195","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.105.023520","type":"journal-article","article-title":"Dark energy survey year 3 results: cosmological constraints from galaxy clustering and weak lensing","volume":"105","author":"Abbott","year":"2022","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib196","first-page":"pp 72","type":"conference-proceedings","article-title":"Question isotropy","volume":"vol 1274","author":"Ralston","year":"2010"},{"key":"cqgacbefcbib197","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.127.101301","type":"journal-article","article-title":"First constraints on the intrinsic CMB dipole and our velocity with doppler and aberration","volume":"127","author":"Ferreira","year":"2021","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib198","doi-asserted-by":"publisher","first-page":"JCAP10(2021)072","DOI":"10.1088\/1475-7516\/2021\/10\/072","type":"journal-article","article-title":"Bayesian estimation of our local motion from the Planck-2018 CMB temperature map","author":"Saha","year":"2021","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib199","doi-asserted-by":"publisher","DOI":"10.1155\/2010\/378203","type":"journal-article","article-title":"Testing gaussianity, homogeneity and isotropy with the cosmic microwave background","volume":"2010","author":"Abramo","year":"2010","journal-title":"Adv. Astron."},{"key":"cqgacbefcbib200","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.110.011301","type":"journal-article","article-title":"Cosmic microwave background power asymmetry from non-Gaussian modulation","volume":"110","author":"Schmidt","year":"2013","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib200","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.110.059902","type":"journal-article","volume":"110","author":"Schmidt","year":"2013","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib201","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.88.083527","type":"journal-article","article-title":"Hemispherical asymmetry and local non-gaussianity: a consistency condition","volume":"88","author":"Namjoo","year":"2013","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib202","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.93.023524","type":"journal-article","article-title":"Large-scale anomalies in the cosmic microwave background as signatures of non-Gaussianity","volume":"93","author":"Adhikari","year":"2016","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib203","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/aa5ce2","type":"journal-article","article-title":"Model-independent analyses of non-Gaussianity in Planck CMB maps using Minkowski functionals","volume":"34","author":"Buchert","year":"2017","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib204","doi-asserted-by":"publisher","first-page":"1718","DOI":"10.1111\/j.1365-2966.2008.12960.x","type":"journal-article","article-title":"Testing isotropy of cosmic microwave background radiation","volume":"385","author":"Samal","year":"2008","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib205","doi-asserted-by":"publisher","first-page":"750","DOI":"10.1086\/497263","type":"journal-article","article-title":"Multipole vector anomalies in the first-year WMAP data: a cut-sky analysis","volume":"635","author":"Bielewicz","year":"2005","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib206","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.74.023005","type":"journal-article","article-title":"CMB multipole measurements in the presence of foregrounds","volume":"74","author":"de Oliveira-Costa","year":"2006","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib207","doi-asserted-by":"publisher","first-page":"1032","DOI":"10.1111\/j.1365-2966.2011.18410.x","type":"journal-article","article-title":"Effect of foregrounds on the cosmic microwave background radiation multipole alignment","volume":"414","author":"Aluri","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib208","doi-asserted-by":"publisher","first-page":"3458","DOI":"10.1093\/mnras\/stv501","type":"journal-article","article-title":"Large-scale alignments from WMAP and Planck","volume":"449","author":"Copi","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib209","doi-asserted-by":"publisher","first-page":"JCAP06(2015)047","DOI":"10.1088\/1475-7516\/2015\/06\/047","type":"journal-article","article-title":"On the proper kinetic quadrupole CMB removal and the quadrupole anomalies","author":"Notari","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib210","doi-asserted-by":"publisher","DOI":"10.1088\/1742-6596\/484\/1\/012029","type":"journal-article","article-title":"Dipole leakage and low CMB multipoles","volume":"484","author":"Das","year":"2014","journal-title":"J. Phys.: Conf. Ser."},{"key":"cqgacbefcbib211","doi-asserted-by":"publisher","DOI":"10.1142\/S0218271813300115","type":"journal-article","article-title":"Recent developments in astrophysical and cosmological exploitation of microwave surveys","volume":"22","author":"Burigana","year":"2013","journal-title":"Int. J. Mod. Phys. D"},{"key":"cqgacbefcbib212","doi-asserted-by":"publisher","first-page":"A9","DOI":"10.1051\/0004-6361\/201525690","type":"journal-article","article-title":"Microwave thermal emission from the zodiacal dust cloud predicted with contemporary meteoroid models","volume":"584","author":"Dikarev","year":"2015","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib213","doi-asserted-by":"publisher","first-page":"511","DOI":"10.1111\/j.1365-2966.2009.14728.x","type":"journal-article","article-title":"Signals of statistical anisotropy in WMAP foreground-cleaned maps","volume":"396","author":"Samal","year":"2009","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib214","doi-asserted-by":"publisher","DOI":"10.1142\/S021773231550131X","type":"journal-article","article-title":"Testing isotropy of cosmos with WMAP and PLANCK data","volume":"30","author":"Rath","year":"2015","journal-title":"Mod. Phys. Lett. A"},{"key":"cqgacbefcbib215","doi-asserted-by":"publisher","first-page":"209","DOI":"10.1111\/j.1365-2966.2008.13149.x","type":"journal-article","article-title":"A low cosmic microwave background variance in the Wilkinson Microwave Anisotropy Probe data","volume":"387","author":"Monteser\u00edn","year":"2008","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib216","doi-asserted-by":"publisher","first-page":"2383","DOI":"10.1111\/j.1365-2966.2010.18067.x","type":"journal-article","article-title":"Anomalous variance in the WMAP data and Galactic foreground residuals","volume":"412","author":"Cruz","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib217","doi-asserted-by":"publisher","first-page":"JCAP07(2013)047","DOI":"10.1088\/1475-7516\/2013\/07\/047","type":"journal-article","article-title":"Low variance at large scales of WMAP 9 year data","author":"Gruppuso","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib218","doi-asserted-by":"publisher","first-page":"JCAP09(2008)023","DOI":"10.1088\/1475-7516\/2008\/09\/023","type":"journal-article","article-title":"Hemispherical power asymmetry: parameter estimation from cosmic microwave background WMAP5 data","author":"Lew","year":"2008","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib219","doi-asserted-by":"publisher","first-page":"399","DOI":"10.1111\/j.1365-2966.2010.16905.x","type":"journal-article","article-title":"Power asymmetries in the cosmic microwave background temperature and polarization patterns","volume":"407","author":"Paci","year":"2010","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib220","doi-asserted-by":"publisher","first-page":"JCAP12(2013)014","DOI":"10.1088\/1475-7516\/2013\/12\/014","type":"journal-article","article-title":"Testing the dipole modulation model in CMBR","author":"Rath","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib221","doi-asserted-by":"publisher","first-page":"JCAP09(2013)033","DOI":"10.1088\/1475-7516\/2013\/09\/033","type":"journal-article","article-title":"The small scale power asymmetry in the cosmic microwave background","author":"Flender","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib222","doi-asserted-by":"publisher","first-page":"JCAP01(2015)008","DOI":"10.1088\/1475-7516\/2015\/01\/008","type":"journal-article","article-title":"On the significance of power asymmetries in Planck CMB data at all scales","author":"Quartin","year":"2015","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib223","doi-asserted-by":"publisher","first-page":"4232","DOI":"10.1093\/mnras\/stu2408","type":"journal-article","article-title":"Local variance asymmetries in Planck temperature anisotropy maps","volume":"446","author":"Adhikari","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib224","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.92.063008","type":"journal-article","article-title":"Microwave background correlations from dipole anisotropy modulation","volume":"92","author":"Aiola","year":"2015","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib225","doi-asserted-by":"publisher","first-page":"JCAP08(2019)007","DOI":"10.1088\/1475-7516\/2019\/08\/007","type":"journal-article","article-title":"Joint Bayesian analysis of large angular scale CMB temperature anomalies","author":"Shaikh","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib226","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.72.103002","type":"journal-article","article-title":"Spontaneous isotropy breaking: a mechanism for CMB multipole alignments","volume":"72","author":"Gordon","year":"2005","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib227","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.80.063004","type":"journal-article","article-title":"Estimators for CMB statistical anisotropy","volume":"80","author":"Hanson","year":"2009","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib228","doi-asserted-by":"publisher","first-page":"17","DOI":"10.1088\/0067-0049\/192\/2\/17","type":"journal-article","article-title":"Seven-year wilkinson microwave anisotropy probe (WMAP) observations: are there cosmic microwave background anomalies?","volume":"192","author":"Bennett","year":"2011","journal-title":"Astrophys. J. Suppl."},{"key":"cqgacbefcbib229","doi-asserted-by":"publisher","first-page":"985","DOI":"10.1088\/0004-637X\/699\/2\/985","type":"journal-article","article-title":"Increasing evidence for hemispherical power asymmetry in the five-year WMAP data","volume":"699","author":"Hoftuft","year":"2009","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib230","doi-asserted-by":"publisher","first-page":"L5","DOI":"10.1086\/379757","type":"journal-article","article-title":"Measuring the statistical isotropy of the cosmic microwave background anisotropy","volume":"597","author":"Hajian","year":"2003","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib231","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.74.123521","type":"journal-article","article-title":"Testing global isotropy of three-year Wilkinson microwave anisotropy probe (WMAP) data: temperature analysis","volume":"74","author":"Hajian","year":"2006","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib232","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.92.083015","type":"journal-article","article-title":"Novel approach to reconstructing signals of isotropy violation from a masked CMB sky","volume":"92","author":"Aluri","year":"2015","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib233","first-page":"622","type":"journal-article","article-title":"New restrictions on spatial topology of the universe from microwave background temperature fluctuations","volume":"57","author":"Starobinskij","year":"1993","journal-title":"Sov. J. Exp. Theor. Phys. Lett."},{"key":"cqgacbefcbib234","doi-asserted-by":"publisher","first-page":"20","DOI":"10.1103\/PhysRevLett.71.20","type":"journal-article","article-title":"Microwave background anisotropy in a toroidal universe","volume":"71","author":"Stevens","year":"1993","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib235","doi-asserted-by":"publisher","DOI":"10.1155\/2012\/960509","type":"journal-article","article-title":"Symmetry and antisymmetry of the CMB anisotropy pattern","volume":"2012","author":"Kim","year":"2012","journal-title":"Adv. Astron."},{"key":"cqgacbefcbib236","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.89.023010","type":"journal-article","article-title":"Directional dependence of CMB parity asymmetry","volume":"89","author":"Zhao","year":"2014","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib237","doi-asserted-by":"publisher","first-page":"445","DOI":"10.1016\/j.physletb.2016.04.030","type":"journal-article","article-title":"Preferred axis of CMB parity asymmetry in the masked maps","volume":"757","author":"Cheng","year":"2016","journal-title":"Phys. Lett. B"},{"key":"cqgacbefcbib238","doi-asserted-by":"publisher","first-page":"2410","DOI":"10.1093\/mnras\/stx2112","type":"journal-article","article-title":"Alignments of parity even\/odd-only multipoles in CMB","volume":"472","author":"Aluri","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib239","doi-asserted-by":"publisher","first-page":"A16","DOI":"10.1051\/0004-6361\/201321591","type":"journal-article","article-title":"Planck 2013 results. XVI. Cosmological parameters","volume":"571","author":"Collaboration","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib240","doi-asserted-by":"publisher","first-page":"20","DOI":"10.1088\/0067-0049\/208\/2\/20","type":"journal-article","article-title":"Nine-year Wilkinson microwave anisotropy probe (WMAP) observations: final maps and results","volume":"208","author":"Bennett","year":"2013","journal-title":"Astrophys. J. Suppl."},{"key":"cqgacbefcbib241","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1086\/377253","type":"journal-article","article-title":"First-year wilkinson microwave anisotropy probe (WMAP) observations: preliminary maps and basic results","volume":"148","author":"Bennett","year":"2003","journal-title":"Astrophys. J. Suppl. Ser."},{"key":"cqgacbefcbib242","doi-asserted-by":"publisher","first-page":"2978","DOI":"10.1093\/mnras\/stv1143","type":"journal-article","article-title":"Lack of large-angle TT correlations persists in WMAP and Planck","volume":"451","author":"Copi","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib243","doi-asserted-by":"publisher","first-page":"2766","DOI":"10.1093\/mnras\/staa1000","type":"journal-article","article-title":"The size of our causal Universe","volume":"494","author":"Gazta naga","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib244","doi-asserted-by":"publisher","first-page":"436","DOI":"10.1093\/mnras\/stab056","type":"journal-article","article-title":"The cosmological constant as a zero action boundary","volume":"502","author":"Gazta naga","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib245","article-title":"The black hole universe (BHU)","author":"Gazta naga","year":"2021","type":"other"},{"key":"cqgacbefcbib246","doi-asserted-by":"publisher","first-page":"257","DOI":"10.3390\/universe8050257","type":"journal-article","article-title":"How the big bang ends up inside a black hole","volume":"8","author":"Gazta naga","year":"2022","journal-title":"Universe"},{"key":"cqgacbefcbib247","doi-asserted-by":"publisher","first-page":"A11","DOI":"10.1051\/0004-6361\/201526926","type":"journal-article","article-title":"Planck 2015 results. XI. CMB power spectra, likelihoods and robustness of parameters","volume":"594","author":"Collaboration","year":"2016","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib248","doi-asserted-by":"publisher","first-page":"3370","DOI":"10.1111\/j.1365-2966.2012.20852.x","type":"journal-article","article-title":"Spatial variation in the fine-structure constant\u2014new results from VLT\/UVES","volume":"422","author":"King","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib249","doi-asserted-by":"publisher","first-page":"603","DOI":"10.1038\/380603a0","type":"journal-article","article-title":"How filaments of galaxies are woven into the cosmic web","volume":"380","author":"Bond","year":"1996","journal-title":"Nature"},{"key":"cqgacbefcbib250","doi-asserted-by":"publisher","first-page":"341","DOI":"10.1086\/164347","type":"journal-article","article-title":"The sponge-like topology of large-scale structure in the universe","volume":"306","author":"Gott III","year":"1986","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib251","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1086\/164571","type":"journal-article","article-title":"The topology of the large-scale structure of the universe","volume":"309","author":"Hamilton","year":"1986","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib252","doi-asserted-by":"publisher","first-page":"843","DOI":"10.1007\/BF01048319","type":"journal-article","article-title":"Euler characteristic and related measures for random geometric sets","volume":"64","author":"Mecke","year":"1991","journal-title":"J. Stat. Phys."},{"key":"cqgacbefcbib253","doi-asserted-by":"publisher","first-page":"473","DOI":"10.1086\/306259","type":"journal-article","article-title":"Cosmic microwave background anisotropy correlation function and topology from simulated maps for MAP","volume":"506","author":"Park","year":"1998","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib254","doi-asserted-by":"publisher","first-page":"125","DOI":"10.5303\/JKAS.2013.46.3.125","type":"journal-article","article-title":"Betti numbers of gaussian fields","volume":"46","author":"Park","year":"2013","journal-title":"J. Korean Astron. Soci."},{"key":"cqgacbefcbib255","first-page":"697","type":"journal-article","article-title":"Robust morphological measures for large-scale structure in the Universe","volume":"288","author":"Mecke","year":"1994","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib256","doi-asserted-by":"publisher","first-page":"L1+","DOI":"10.1086\/310680","type":"journal-article","article-title":"Beyond genus statistics: a unifying approach to the morphology of cosmic structure","volume":"482","author":"Schmalzing","year":"1997","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib257","doi-asserted-by":"publisher","first-page":"355","DOI":"10.1046\/j.1365-8711.1998.01467.x","type":"journal-article","article-title":"Minkowski functionals used in the morphological analysis of cosmic microwave background anisotropy maps","volume":"297","author":"Schmalzing","year":"1998","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib258","doi-asserted-by":"publisher","first-page":"2104","DOI":"10.1093\/mnras\/sts483","type":"journal-article","article-title":"Non-Gaussianity and Minkowski functionals: forecasts for Planck","volume":"429","author":"Ducout","year":"2013","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib259","doi-asserted-by":"publisher","first-page":"108","DOI":"10.3847\/1538-4357\/ac562a","type":"journal-article","article-title":"Minkowski functionals of SDSS-III BOSS: hints of possible anisotropy in the density field?","volume":"928","author":"Appleby","year":"2022","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib260","doi-asserted-by":"publisher","first-page":"255","DOI":"10.1090\/S0273-0979-09-01249-X","type":"journal-article","article-title":"Topology and data","volume":"46","author":"Carlsson","year":"2009","journal-title":"Bull. Am. Math. Soc."},{"key":"cqgacbefcbib261","article-title":"On the bootstrap for persistence diagrams and landscapes","author":"Chazal","year":"2013","type":"preprint"},{"key":"cqgacbefcbib262","doi-asserted-by":"publisher","DOI":"10.1214\/14-AOS1252","type":"preprint","article-title":"Statistical inference for persistent homology: confidence sets for persistence diagrams","author":"Fasy","year":"2013"},{"key":"cqgacbefcbib263","article-title":"Stability determiniation in turning using persistent homology and time series analysis","author":"Khasawneh","year":"2014","type":"conference-proceedings"},{"key":"cqgacbefcbib264","first-page":"77","type":"journal-article","article-title":"Statistical topological data analysis using persistence landscapes","volume":"16","author":"Bubenik","year":"2015","journal-title":"J. Mach. Learn. Res."},{"key":"cqgacbefcbib265","doi-asserted-by":"publisher","first-page":"49","DOI":"10.1142\/S1793525312500057","type":"journal-article","article-title":"Euler integration of gaussian random fields and persistent homology","volume":"04","author":"Bobrowski","year":"2012","journal-title":"J. Topol. Anal."},{"key":"cqgacbefcbib266","article-title":"Statistical analysis of persistence intensity functions","author":"Chen","year":"2015","type":"preprint"},{"key":"cqgacbefcbib267","doi-asserted-by":"publisher","DOI":"10.2139\/ssrn.3275996","type":"journal-article","article-title":"Persistent-homology-based machine learning and its applications\u2014a survey","author":"Pun","year":"2018","journal-title":"SSRN Electron. J."},{"key":"cqgacbefcbib268","article-title":"Computational topology for biomedical image and data analysis: theory and Applications","author":"Moraleda","year":"2019","type":"book"},{"key":"cqgacbefcbib269","doi-asserted-by":"publisher","DOI":"10.1038\/s41598-019-50202-3","type":"journal-article","article-title":"Persistent homology of unweighted complex networks via discrete Morse theory","volume":"9","author":"Kannan","year":"2019","journal-title":"Sci. Rep."},{"key":"cqgacbefcbib270","doi-asserted-by":"publisher","first-page":"130","DOI":"10.1109\/MSP.2021.3075187","type":"journal-article","article-title":"Computational topology for biomedical images and data: theory and applications (Book Review)","volume":"38","author":"Pranav","year":"2021","journal-title":"IEEE Signal Process. Mag."},{"key":"cqgacbefcbib271","doi-asserted-by":"publisher","first-page":"L1","DOI":"10.1086\/523669","type":"journal-article","article-title":"The three-dimensional skeleton of the SDSS","volume":"672","author":"Sousbie","year":"2008","journal-title":"Astrophys. J. l"},{"key":"cqgacbefcbib272","doi-asserted-by":"publisher","first-page":"350","DOI":"10.1111\/j.1365-2966.2011.18394.x","type":"journal-article","article-title":"The persistent cosmic web and its filamentary structure\u2014I. Theory and implementation","volume":"414","author":"Sousbie","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib273","doi-asserted-by":"publisher","first-page":"1745","DOI":"10.1109\/TVCG.2015.2452919","type":"journal-article","article-title":"Felix: a topology based framework for visual exploration of cosmic filaments","volume":"22","author":"Shivashankar","year":"2016","journal-title":"IEEE Trans. Vis. Comput. Graph."},{"key":"cqgacbefcbib274","doi-asserted-by":"publisher","first-page":"34","DOI":"10.1016\/j.ascom.2019.02.003","type":"journal-article","article-title":"Finding cosmic voids and filament loops using topological data analysis","volume":"27","author":"Xu","year":"2019","journal-title":"Astron. Comput."},{"key":"cqgacbefcbib275","article-title":"A study on the baryon acoustic oscillation with topological data analysis","author":"Kono","year":"2020","type":"preprint"},{"key":"cqgacbefcbib276","doi-asserted-by":"publisher","DOI":"10.1017\/S0022377818000752","type":"journal-article","article-title":"Topological data analysis and diagnostics of compressible MHD turbulence","volume":"84","author":"Makarenko","year":"2018","journal-title":"J. Plasma Phys."},{"key":"cqgacbefcbib277","type":"book","article-title":"Alpha, betti and the megaparsec universe: on the topology of the cosmic web","volume":"vol 14","author":"van de Weygaert","year":"2011","edition":"ed"},{"key":"cqgacbefcbib278","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/sty1643","type":"preprint","article-title":"On the connectivity of the cosmic web: theory and implications for cosmology and galaxy formation","author":"Codis","year":"2018"},{"key":"cqgacbefcbib279","doi-asserted-by":"publisher","first-page":"2968","DOI":"10.1093\/mnras\/stab2326","type":"journal-article","article-title":"Persistent homology of the cosmic web\u2014I. Hierarchical topology in \u039bCDM cosmologies","volume":"507","author":"Wilding","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib280","article-title":"Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology","author":"Cisewski-Kehe","year":"2022","type":"preprint"},{"key":"cqgacbefcbib281","doi-asserted-by":"publisher","first-page":"JCAP03(2018)025","DOI":"10.1088\/1475-7516\/2018\/03\/025","type":"journal-article","article-title":"Persistent homology and non-Gaussianity","author":"Cole","year":"2018","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib282","doi-asserted-by":"publisher","first-page":"JCAP09(2019)052","DOI":"10.1088\/1475-7516\/2019\/09\/052","type":"journal-article","article-title":"Stochastic homology of gaussian vs. non-gaussian random fields: graphs towards betti numbers and persistence diagrams","author":"Feldbrugge","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib283","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2021\/04\/061","type":"preprint","article-title":"The persistence of large scale structures I: primordial non-Gaussianity","author":"Biagetti","year":"2020"},{"key":"cqgacbefcbib284","author":"Munkres","year":"1984","type":"book"},{"key":"cqgacbefcbib285","doi-asserted-by":"publisher","first-page":"511","DOI":"10.1007\/s00454-002-2885-2","type":"journal-article","article-title":"Topological persistence and simplification","volume":"28","author":"Edelsbrunner","year":"2002","journal-title":"Discrete Comput. Geom."},{"key":"cqgacbefcbib286","author":"Edelsbrunner","year":"2010","type":"book"},{"key":"cqgacbefcbib287","doi-asserted-by":"publisher","first-page":"4281","DOI":"10.1093\/mnras\/stw2862","type":"journal-article","article-title":"The topology of the cosmic web in terms of persistent Betti numbers","volume":"465","author":"Pranav","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib288","doi-asserted-by":"publisher","first-page":"140","DOI":"10.1007\/BF02420029","type":"journal-article","article-title":"Sopra gli spazi di un numero qualunque di dimensioni","volume":"2","author":"Betti","year":"1871","journal-title":"Ann. Mat."},{"key":"cqgacbefcbib289","doi-asserted-by":"publisher","first-page":"759","DOI":"10.1086\/427976","type":"journal-article","article-title":"HEALPix: a framework for high-resolution discretization and fast analysis of data distributed on the sphere","volume":"622","author":"G\u00f3rski","year":"2005","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib290","doi-asserted-by":"publisher","first-page":"A163","DOI":"10.1051\/0004-6361\/201834916","type":"journal-article","article-title":"Unexpected topology of the temperature fluctuations in the cosmic microwave background","volume":"627","author":"Pranav","year":"2019","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib291","doi-asserted-by":"publisher","DOI":"10.1051\/0004-6361\/202140291","type":"preprint","article-title":"Loops abound in the cosmic microwave background: a 4\u03c3 anomaly on super-horizon scales","author":"Pranav","year":"2021"},{"key":"cqgacbefcbib292","doi-asserted-by":"publisher","first-page":"A115","DOI":"10.1051\/0004-6361\/202140291","type":"journal-article","article-title":"Anomalies in the topology of the temperature fluctuations in the cosmic microwave background: an analysis of the NPIPE and FFP10 data releases","volume":"659","author":"Pranav","year":"2022","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib293","doi-asserted-by":"publisher","first-page":"64","DOI":"10.1086\/422570","type":"journal-article","article-title":"Testing for non-gaussianity in the wilkinson microwave anisotropy probe data: minkowski functionals and the length of the skeleton","volume":"612","author":"Eriksen","year":"2004","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib294","doi-asserted-by":"publisher","first-page":"11878","DOI":"10.1073\/pnas.1706885114","type":"journal-article","article-title":"Modeling and replicating statistical topology and evidence for CMB nonhomogeneity","volume":"114","author":"Adler","year":"2017","journal-title":"Proc. Natl Acad. Sci."},{"key":"cqgacbefcbib295","doi-asserted-by":"publisher","first-page":"JCAP06(2017)023","DOI":"10.1088\/1475-7516\/2017\/06\/023","type":"journal-article","article-title":"Tensor minkowski functionals: first application to the CMB","author":"Ganesan","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib296","doi-asserted-by":"publisher","first-page":"JCAP12(2017)023","DOI":"10.1088\/1475-7516\/2017\/12\/023","type":"journal-article","article-title":"Tensor Minkowski Functionals for random fields on the sphere","author":"Chingangbam","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib297","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.123516","type":"journal-article","article-title":"Geometrical meaning of statistical isotropy of smooth random fields in two dimensions","volume":"104","author":"Chingangbam","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib298","doi-asserted-by":"publisher","first-page":"57","DOI":"10.1111\/j.1365-2818.2009.03331.x","type":"journal-article","article-title":"Tensorial Minkowski functionals and anisotropy measures for planar patterns","volume":"238","author":"Schr\u00f6der-Turk","year":"2010","journal-title":"J. Microsc."},{"key":"cqgacbefcbib299","doi-asserted-by":"publisher","first-page":"JCAP01(2019)009","DOI":"10.1088\/1475-7516\/2019\/01\/009","type":"journal-article","article-title":"Search for anomalous alignments of structures in Planck data using Minkowski Tensors","author":"Joby","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib300","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.103.123523","type":"journal-article","article-title":"Application of the contour Minkowski tensor and D statistic to the Planck E-mode data","volume":"103","author":"Kochappan","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib301","doi-asserted-by":"publisher","first-page":"22","DOI":"10.1086\/421007","type":"journal-article","article-title":"Detection of non-gaussianity in the wilkinson microwave anisotropy probe first-year data using spherical wavelets","volume":"609","author":"Vielva","year":"2004","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib302","doi-asserted-by":"publisher","first-page":"29","DOI":"10.1111\/j.1365-2966.2004.08419.x","type":"journal-article","article-title":"Detection of a non-Gaussian spot in WMAP","volume":"356","author":"Cruz","year":"2005","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib303","doi-asserted-by":"publisher","first-page":"57","DOI":"10.1111\/j.1365-2966.2006.10312.x","type":"journal-article","article-title":"The non-Gaussian cold spot in Wilkinson microwave anisotropy probe: significance, morphology and foreground contribution","volume":"369","author":"Cruz","year":"2006","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib304","doi-asserted-by":"publisher","first-page":"51","DOI":"10.1086\/423021","type":"journal-article","article-title":"Wavelets and Wilkinson microwave anisotropy probe non-Gaussianity","volume":"613","author":"Mukherjee","year":"2004","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib305","doi-asserted-by":"publisher","first-page":"1583","DOI":"10.1111\/j.1365-2966.2005.09007.x","type":"journal-article","article-title":"A high-significance detection of non-Gaussianity in the Wilkinson microwave anisotropy probe 1-yr data using directional spherical wavelets","volume":"359","author":"McEwen","year":"2005","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib306","doi-asserted-by":"publisher","first-page":"826","DOI":"10.1111\/j.1365-2966.2005.09277.x","type":"journal-article","article-title":"Higher Criticism statistic: detecting and identifying non-Gaussianity in the WMAP first-year data","volume":"362","author":"Cay\u00f3n","year":"2005","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib307","doi-asserted-by":"publisher","first-page":"69","DOI":"10.1016\/j.astropartphys.2009.11.005","type":"journal-article","article-title":"Disks in the sky: a reassessment of the WMAP \u201ccold spot\u201d","volume":"33","author":"Zhang","year":"2010","journal-title":"Astropart. Phys."},{"key":"cqgacbefcbib308","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.90.103510","type":"journal-article","article-title":"Can a supervoid explain the cold spot?","volume":"90","author":"Nadathur","year":"2014","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib309","doi-asserted-by":"publisher","first-page":"452","DOI":"10.1088\/0004-637X\/722\/1\/452","type":"journal-article","article-title":"Bayesian analysis of an anisotropic Universe model: systematics and polarization","volume":"722","author":"Groeneboom","year":"2010","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib310","doi-asserted-by":"publisher","first-page":"1807","DOI":"10.1088\/0004-637X\/690\/2\/1807","type":"journal-article","article-title":"Bayesian analysis of sparse anisotropic universe models and application to the five-year WMAP data","volume":"690","author":"Groeneboom","year":"2009","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib311","author":"Varshalovich","year":"1988","type":"book"},{"key":"cqgacbefcbib312","doi-asserted-by":"publisher","first-page":"A97","DOI":"10.1051\/0004-6361\/201424164","type":"journal-article","article-title":"Statistical isotropy violation in WMAP CMB maps resulting from non-circular beams","volume":"591","author":"Das","year":"2016","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib313","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.81.103003","type":"journal-article","article-title":"Asymmetric beams and CMB statistical anisotropy","volume":"81","author":"Hanson","year":"2010","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib314","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.98.023521","type":"journal-article","article-title":"Covariance of CMB anomalies","volume":"98","author":"Muir","year":"2018","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib315","doi-asserted-by":"publisher","first-page":"196","DOI":"10.1038\/s41550-019-0906-9","type":"journal-article","article-title":"Planck evidence for a closed Universe and a possible crisis for cosmology","volume":"4","author":"Di Valentino","year":"2020","journal-title":"Nat. Astron."},{"key":"cqgacbefcbib316","doi-asserted-by":"publisher","first-page":"15","DOI":"10.1093\/mnras\/stac903","type":"journal-article","article-title":"Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars","volume":"513","author":"Kov\u00e1cs","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib317","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/stac2011","type":"preprint","article-title":"Dark energy survey year 3 results: imprints of cosmic voids and superclusters in the Planck CMB lensing map","author":"Kov\u00e1cs","year":"2022"},{"key":"cqgacbefcbib318","doi-asserted-by":"publisher","first-page":"891","DOI":"10.1038\/s41550-019-0902-0","type":"journal-article","article-title":"Tensions between the early and late Universe","volume":"3","author":"Verde","year":"2019","journal-title":"Nat. Astron."},{"key":"cqgacbefcbib319","doi-asserted-by":"publisher","first-page":"159","DOI":"10.3847\/1538-4357\/ac12cf","type":"journal-article","article-title":"Early universe physics insensitive and uncalibrated cosmic standards: constraints on \u03a9m and implications for the Hubble tension","volume":"920","author":"Lin","year":"2021","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib320","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.106.063530","type":"preprint","article-title":"Determining the hubble constant without the sound horizon: a 3.6% constraint on H0 from galaxy surveys, CMB lensing and supernovae","author":"Philcox","year":"2022"},{"key":"cqgacbefcbib321","doi-asserted-by":"publisher","first-page":"50","DOI":"10.3847\/0004-6256\/152\/2\/50","type":"journal-article","article-title":"Cosmicflows-3","volume":"152","author":"Tully","year":"2016","journal-title":"Astron. J."},{"key":"cqgacbefcbib322","doi-asserted-by":"publisher","first-page":"59","DOI":"10.3847\/1538-4357\/ac249d","type":"journal-article","article-title":"Cosmic flow measurement and mock sampling algorithm of cosmicflows-4 tully-fisher catalog","volume":"922","author":"Qin","year":"2021","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib323","doi-asserted-by":"publisher","first-page":"A50","DOI":"10.1051\/0004-6361\/201731222","type":"journal-article","article-title":"Anisotropy of the galaxy cluster X-ray luminosity-temperature relation","volume":"611","author":"Migkas","year":"2018","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib324","doi-asserted-by":"publisher","first-page":"JCAP01(2017)038","DOI":"10.1088\/1475-7516\/2017\/01\/038","type":"journal-article","article-title":"The need for accurate redshifts in supernova cosmology","author":"Calcino","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib325","first-page":"p 344","type":"conference-proceedings","article-title":"Hubble\u2019s deviations from pure hubble flow: a review","volume":"vol 4","author":"Gunn","year":"1988"},{"key":"cqgacbefcbib326","doi-asserted-by":"publisher","first-page":"184","DOI":"10.1086\/527428","type":"journal-article","article-title":"Our peculiar motion away from the local void","volume":"676","author":"Tully","year":"2008","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib327","doi-asserted-by":"publisher","first-page":"2948","DOI":"10.1093\/mnras\/stz2652","type":"journal-article","article-title":"Can redshift errors bias measurements of the Hubble constant?","volume":"490","author":"Davis","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib328","doi-asserted-by":"publisher","first-page":"98","DOI":"10.1088\/0004-637X\/737\/2\/98","type":"journal-article","article-title":"Measuring the galaxy cluster bulk flow from WMAP data","volume":"737","author":"Osborne","year":"2011","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib329","doi-asserted-by":"publisher","first-page":"L67","DOI":"10.1086\/312735","type":"journal-article","article-title":"Measuring cosmological bulk flows via the kinematic Sunyaev-Zeldovich effect in the upcoming cosmic microwave background maps","volume":"536","author":"Kashlinsky","year":"2000","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib330","doi-asserted-by":"publisher","first-page":"1479","DOI":"10.1088\/0004-637X\/691\/2\/1479","type":"journal-article","article-title":"A measurement of large-scale peculiar velocities of clusters of galaxies: technical details","volume":"691","author":"Kashlinsky","year":"2009","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib331","doi-asserted-by":"publisher","first-page":"L81","DOI":"10.1088\/2041-8205\/712\/1\/L81","type":"journal-article","article-title":"A new measurement of the bulk flow of X-ray luminous clusters of galaxies","volume":"712","author":"Kashlinsky","year":"2010","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib332","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1088\/0004-637X\/732\/1\/1","type":"journal-article","article-title":"Measuring the dark flow with public X-ray cluster data","volume":"732","author":"Kashlinsky","year":"2011","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib333","article-title":"Measuring bulk motion of X-ray clusters via the kinematic Sunyaev-Zeldovich effect: summarizing the \u201cdark flow\u201d evidence and its implications","author":"Kashlinsky","year":"2012","type":"preprint"},{"key":"cqgacbefcbib334","doi-asserted-by":"publisher","first-page":"545","DOI":"10.1093\/mnras\/279.2.545","type":"journal-article","article-title":"Using the kinematic Sunyaev-Zeldovich effect to determine the peculiar velocities of clusters of galaxies","volume":"279","author":"Haehnelt","year":"1996","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib335","doi-asserted-by":"publisher","first-page":"L42","DOI":"10.1088\/0004-637X\/707\/1\/L42","type":"journal-article","article-title":"The statistical significance of the \u201cDark Flow\u201d","volume":"707","author":"Keisler","year":"2009","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib336","doi-asserted-by":"publisher","first-page":"143","DOI":"10.1088\/0004-637X\/810\/2\/143","type":"journal-article","article-title":"Probing the dark flow signal in WMAP 9-year and planck cosmic microwave background maps","volume":"810","author":"Atrio-Barandela","year":"2015","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib337","doi-asserted-by":"publisher","first-page":"A97","DOI":"10.1051\/0004-6361\/201321299","type":"journal-article","article-title":"Planck intermediate results. XIII. Constraints on peculiar velocities","volume":"561","author":"Collaboration","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib338","doi-asserted-by":"publisher","first-page":"A116","DOI":"10.1051\/0004-6361\/201321579","type":"journal-article","article-title":"On the statistical significance of the bulk flow measured by the Planck satellite","volume":"557","author":"Atrio-Barandela","year":"2013","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib339","doi-asserted-by":"publisher","first-page":"264","DOI":"10.1111\/j.1365-2966.2011.18402.x","type":"journal-article","article-title":"Probing the anisotropic local Universe and beyond with SNe Ia data","volume":"414","author":"Colin","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib340","doi-asserted-by":"publisher","first-page":"JCAP04(2011)015","DOI":"10.1088\/1475-7516\/2011\/04\/015","type":"journal-article","article-title":"Measuring the cosmological bulk flow using the peculiar velocities of supernovae","author":"Dai","year":"2011","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib341","doi-asserted-by":"publisher","first-page":"447","DOI":"10.1111\/j.1365-2966.2011.20050.x","type":"journal-article","article-title":"Cosmic flows in the nearby universe from Type Ia supernovae","volume":"420","author":"Turnbull","year":"2012","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib342","doi-asserted-by":"publisher","first-page":"76","DOI":"10.1088\/0004-637X\/801\/2\/76","type":"journal-article","article-title":"Probing Bulk Flow with Nearby SNe Ia Data","volume":"801","author":"Appleby","year":"2015","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib343","doi-asserted-by":"publisher","DOI":"10.3847\/1538-4357\/ac8e04","type":"preprint","article-title":"The Pantheon+ Analysis: cosmological constraints","author":"Brout","year":"2022"},{"key":"cqgacbefcbib344","doi-asserted-by":"publisher","first-page":"418","DOI":"10.1086\/173997","type":"journal-article","article-title":"The motion of the local group with respect to the 15,000 Kilometer per second abell cluster inertial frame","volume":"425","author":"Lauer","year":"1994","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib345","doi-asserted-by":"publisher","first-page":"61","DOI":"10.1111\/j.1365-2966.2004.07893.x","type":"journal-article","article-title":"Streaming motions of galaxy clusters within 12 000 km s\u22121-V. The peculiar velocity field","volume":"352","author":"Hudson","year":"2004","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib346","first-page":"426","type":"journal-article","article-title":"A new method of determining distances to galaxies","volume":"7","author":"Tully","year":"1975","journal-title":"Bull. Am. Astron. Soc."},{"key":"cqgacbefcbib347","doi-asserted-by":"publisher","first-page":"59","DOI":"10.1086\/164948","type":"journal-article","article-title":"Fundamental properties of elliptical galaxies","volume":"313","author":"Djorgovski","year":"1987","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib348","doi-asserted-by":"publisher","first-page":"42","DOI":"10.1086\/164947","type":"journal-article","article-title":"Spectroscopy and photometry of elliptical galaxies. I. New distance estimator","volume":"313","author":"Dressler","year":"1987","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib349","doi-asserted-by":"publisher","first-page":"69","DOI":"10.1088\/0004-6256\/146\/3\/69","type":"journal-article","article-title":"Cosmography of the local Universe","volume":"146","author":"Courtois","year":"2013","journal-title":"Astron. J."},{"key":"cqgacbefcbib350","doi-asserted-by":"publisher","first-page":"93","DOI":"10.1088\/0004-637X\/736\/2\/93","type":"journal-article","article-title":"The cosmological bulk flow: consistency with \u039bCDM and z\u2009\u2248\u20090 constraints on \u03c3 8 and \u03b3","volume":"736","author":"Nusser","year":"2011","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib351","doi-asserted-by":"publisher","first-page":"2017","DOI":"10.1093\/mnras\/sts178","type":"journal-article","article-title":"Cosmic bulk flows on 50 h\u22121 Mpc scales: a Bayesian hyper-parameter method and multishell likelihood analysis","volume":"428","author":"Ma","year":"2013","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib352","doi-asserted-by":"publisher","first-page":"402","DOI":"10.1093\/mnras\/stu1774","type":"journal-article","article-title":"2MTF\u2014IV. A bulk flow measurement of the local Universe","volume":"445","author":"Hong","year":"2014","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib353","doi-asserted-by":"publisher","first-page":"386","DOI":"10.1093\/mnras\/stv2146","type":"journal-article","article-title":"The 6dF galaxy survey: bulk flows on 50-70 h \u22121 Mpc scales","volume":"455","author":"Scrimgeour","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib354","doi-asserted-by":"publisher","first-page":"5150","DOI":"10.1093\/mnras\/sty928","type":"journal-article","article-title":"Bulk flow in the combined 2MTF and 6dFGSv surveys","volume":"477","author":"Qin","year":"2018","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib355","doi-asserted-by":"publisher","first-page":"1920","DOI":"10.1093\/mnras\/sty2826","type":"journal-article","article-title":"Bulk flow and shear in the local Universe: 2MTF and COSMICFLOWS-3","volume":"482","author":"Qin","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib356","doi-asserted-by":"publisher","first-page":"2703","DOI":"10.1093\/mnras\/staa2485","type":"journal-article","article-title":"Cosmic flows in the nearby Universe: new peculiar velocities from SNe and cosmological constraints","volume":"498","author":"Boruah","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib357","doi-asserted-by":"publisher","first-page":"2349","DOI":"10.1093\/mnras\/stab1446","type":"journal-article","article-title":"Peculiar-velocity cosmology with Types Ia and II supernovae","volume":"505","author":"Stahl","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib358","doi-asserted-by":"publisher","first-page":"3285","DOI":"10.1093\/mnras\/stw128","type":"journal-article","article-title":"Defining the frame of minimum non-linear Hubble expansion variation","volume":"457","author":"McKay","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib359","doi-asserted-by":"publisher","first-page":"2328","DOI":"10.1111\/j.1365-2966.2010.17052.x","type":"journal-article","article-title":"Cosmic flows on 100 h\u22121 Mpc scales: standardized minimum variance bulk flow, shear and octupole moments","volume":"407","author":"Feldman","year":"2010","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib360","doi-asserted-by":"publisher","first-page":"86","DOI":"10.1088\/0004-6256\/146\/4\/86","type":"journal-article","article-title":"Cosmicflows-2: the data","volume":"146","author":"Tully","year":"2013","journal-title":"Astron. J."},{"key":"cqgacbefcbib361","doi-asserted-by":"publisher","first-page":"1697","DOI":"10.1088\/0264-9381\/4\/6\/025","type":"journal-article","article-title":"The \u2018fitting problem\u2019 in cosmology","volume":"4","author":"Ellis","year":"1987","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib362","doi-asserted-by":"publisher","first-page":"377","DOI":"10.1088\/1367-2630\/9\/10\/377","type":"journal-article","article-title":"Cosmic clocks, cosmic variance and cosmic averages","volume":"9","author":"Wiltshire","year":"2007","journal-title":"New J. Phys."},{"key":"cqgacbefcbib363","doi-asserted-by":"publisher","first-page":"JCAP06(2016)035","DOI":"10.1088\/1475-7516\/2016\/06\/035","type":"journal-article","article-title":"Differential cosmic expansion and the Hubble flow anisotropy","author":"Bolejko","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib364","doi-asserted-by":"publisher","first-page":"JCAP10(2016)016","DOI":"10.1088\/1475-7516\/2016\/10\/016","type":"journal-article","article-title":"Frames of most uniform Hubble flow","author":"Kraljic","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib365","doi-asserted-by":"publisher","first-page":"JCAP03(2019)001","DOI":"10.1088\/1475-7516\/2019\/03\/001","type":"journal-article","article-title":"Is the local Hubble flow consistent with concordance cosmology?","author":"Bengaly","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib366","doi-asserted-by":"publisher","first-page":"323","DOI":"10.1093\/mnras\/222.2.323","type":"journal-article","article-title":"Evolution and clustering of rich clusters","volume":"222","author":"Kaiser","year":"1986","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib367","doi-asserted-by":"publisher","first-page":"247","DOI":"10.1007\/s11214-013-9994-5","type":"journal-article","article-title":"Scaling relations for galaxy clusters: properties and evolution","volume":"177","author":"Giodini","year":"2013","journal-title":"Space Sci. Rev."},{"key":"cqgacbefcbib368","doi-asserted-by":"publisher","first-page":"38","DOI":"10.1086\/177846","type":"journal-article","article-title":"The dipole observed in the COBE DMR 4 year data","volume":"470","author":"Lineweaver","year":"1996","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib369","doi-asserted-by":"publisher","first-page":"225","DOI":"10.1088\/0067-0049\/180\/2\/225","type":"journal-article","article-title":"Five-year Wilkinson microwave anisotropy probe observations: data processing, sky maps and basic results","volume":"180","author":"Hinshaw","year":"2009","journal-title":"Astrophys. J. Suppl."},{"key":"cqgacbefcbib370","first-page":"pp 215","type":"conference-proceedings","article-title":"Relativistic cosmology: its nature, aims and problems","author":"Ellis","year":"1984"},{"key":"cqgacbefcbib371","author":"Schneider","year":"1992","type":"book"},{"key":"cqgacbefcbib372","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1016\/j.astropartphys.2014.06.004","type":"journal-article","article-title":"Dipole anisotropy in sky brightness and source count distribution in radio NVSS data","volume":"61","author":"Tiwari","year":"2015","journal-title":"Astropart. Phys."},{"key":"cqgacbefcbib373","doi-asserted-by":"publisher","first-page":"JCAP01(2018)013","DOI":"10.1088\/1475-7516\/2018\/01\/013","type":"journal-article","article-title":"The kinematic dipole in galaxy redshift surveys","author":"Maartens","year":"2018","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib374","doi-asserted-by":"publisher","first-page":"A111","DOI":"10.1051\/0004-6361\/201423583","type":"journal-article","article-title":"Impact of local structure on the cosmic radio dipole","volume":"565","author":"Rubart","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib375","doi-asserted-by":"publisher","first-page":"85","DOI":"10.1088\/0004-637X\/812\/1\/85","type":"journal-article","article-title":"The clustering of radio galaxies: biasing and evolution versus stellar mass","volume":"812","author":"Nusser","year":"2015","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib376","doi-asserted-by":"publisher","first-page":"887","DOI":"10.1088\/0004-637X\/692\/1\/887","type":"journal-article","article-title":"Detecting the cosmic dipole anisotropy in large-scale radio surveys","volume":"692","author":"Crawford","year":"2009","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib377","doi-asserted-by":"publisher","first-page":"1350","DOI":"10.1093\/mnras\/stz832","type":"journal-article","article-title":"Testing the standard model of cosmology with the SKA: the cosmic radio dipole","volume":"486","author":"Bengaly","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib378","doi-asserted-by":"publisher","first-page":"259","DOI":"10.1051\/aas:1997358","type":"journal-article","article-title":"The Westerbork Northern Sky Survey (WENSS), I. A 570 square degree Mini-Survey around the North Ecliptic Pole","volume":"124","author":"Rengelink","year":"1997","journal-title":"Astron. Astrophys. Suppl. Ser."},{"key":"cqgacbefcbib379","doi-asserted-by":"publisher","first-page":"1693","DOI":"10.1086\/300337","type":"journal-article","article-title":"The NRAO VLA sky survey","volume":"115","author":"Condon","year":"1998","journal-title":"Astron. J."},{"key":"cqgacbefcbib380","doi-asserted-by":"publisher","first-page":"1117","DOI":"10.1046\/j.1365-8711.2003.06605.x","type":"journal-article","article-title":"SUMSS: a wide-field radio imaging survey of the southern sky\u2014II. The source catalogue","volume":"342","author":"Mauch","year":"2003","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib381","doi-asserted-by":"publisher","first-page":"382","DOI":"10.1111\/j.1365-2966.2007.12379.x","type":"journal-article","article-title":"The second epoch molonglo galactic plane survey: compact source catalogue","volume":"382","author":"Murphy","year":"2007","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib382","doi-asserted-by":"publisher","first-page":"1045","DOI":"10.1093\/mnras\/stx1631","type":"journal-article","article-title":"High-redshift radio galaxies and divergence from the CMB dipole","volume":"471","author":"Colin","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib383","doi-asserted-by":"publisher","first-page":"175","DOI":"10.3847\/1538-4357\/ab54c8","type":"journal-article","article-title":"The galaxy power spectrum from TGSS ADR1 and the effect of flux calibration systematics","volume":"887","author":"Tiwari","year":"2019","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib384","article-title":"A rescaled subset of the alternative data release 1 of the TIFR GMRT sky survey","author":"Hurley-Walker","year":"2017","type":"preprint"},{"key":"cqgacbefcbib385","doi-asserted-by":"publisher","first-page":"215","DOI":"10.1071\/AS11021","type":"journal-article","article-title":"EMU: evolutionary map of the Universe","volume":"28","author":"Norris","year":"2011","journal-title":"Publ. Astron. Soc. Aust."},{"key":"cqgacbefcbib386","doi-asserted-by":"publisher","first-page":"1868","DOI":"10.1088\/0004-6256\/140\/6\/1868","type":"journal-article","article-title":"The wide-field infrared survey explorer (WISE): mission description and initial on-orbit performance","volume":"140","author":"Wright","year":"2010","journal-title":"Astron. J."},{"key":"cqgacbefcbib387","doi-asserted-by":"publisher","first-page":"12","DOI":"10.1088\/0067-0049\/221\/1\/12","type":"journal-article","article-title":"Identification of 1.4 million active galactic nuclei in the mid-infrared using WISE Data","volume":"221","author":"Secrest","year":"2015","journal-title":"Astrophys. J. Suppl. Ser."},{"key":"cqgacbefcbib388","doi-asserted-by":"publisher","first-page":"69","DOI":"10.3847\/1538-4365\/ab7f2a","type":"journal-article","article-title":"The CatWISE preliminary catalog: motions from WISE and NEOWISE data","volume":"247","author":"Eisenhardt","year":"2020","journal-title":"Astrophys. J. Suppl. Ser."},{"key":"cqgacbefcbib389","doi-asserted-by":"publisher","first-page":"120","DOI":"10.1088\/0004-637X\/794\/2\/120","type":"journal-article","article-title":"The sloan digital sky survey coadd: 275 deg2 of deep sloan digital sky survey imaging on stripe 82","volume":"794","author":"Annis","year":"2014","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib390","doi-asserted-by":"publisher","DOI":"10.3847\/1538-4357\/acacf8","type":"preprint","article-title":"The clustering properties of AGNs\/quasars in CatWISE2020 catalog","author":"Tiwari","year":"2022"},{"key":"cqgacbefcbib391","doi-asserted-by":"publisher","first-page":"107","DOI":"10.3390\/universe7040107","type":"journal-article","article-title":"Our peculiar motion inferred from number counts of mid infra red AGNs and the discordance seen with the cosmological principle","volume":"7","author":"Singal","year":"2021","journal-title":"Universe"},{"key":"cqgacbefcbib392","doi-asserted-by":"publisher","first-page":"30","DOI":"10.1088\/0004-637X\/753\/1\/30","type":"journal-article","article-title":"Mid-infrared selection of active galactic nuclei with the wide-field infrared survey explorer. I. Characterizing WISE-selected active galactic nuclei in COSMOS","volume":"753","author":"Stern","year":"2012","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib393","doi-asserted-by":"publisher","first-page":"L104","DOI":"10.1093\/mnrasl\/slz107","type":"journal-article","article-title":"Peculiar motion of the solar system derived from a dipole anisotropy in the redshift distribution of distant quasars","volume":"488","author":"Singal","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib394","doi-asserted-by":"publisher","first-page":"653","DOI":"10.1093\/mnras\/228.3.653","type":"journal-article","article-title":"The magnitude-redshift relation in a perturbed Friedmann universe","volume":"228","author":"Sasaki","year":"1987","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib395","doi-asserted-by":"publisher","first-page":"317","DOI":"10.1093\/mnras\/stv547","type":"journal-article","article-title":"Cosmological parameters from the comparison of peculiar velocities with predictions from the 2M++ density field","volume":"450","author":"Carrick","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib396","doi-asserted-by":"publisher","first-page":"JCAP05(2017)015","DOI":"10.1088\/1475-7516\/2017\/05\/015","type":"journal-article","article-title":"Testing \u039bCDM at the lowest redshifts with SN Ia and galaxy velocities","author":"Huterer","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib397","article-title":"The impact of peculiar velocities on supernova cosmology","author":"Mohayaee","year":"2020","type":"preprint"},{"key":"cqgacbefcbib398","doi-asserted-by":"publisher","first-page":"14","DOI":"10.3847\/1538-4357\/abb140","type":"journal-article","article-title":"Effects of supernova redshift uncertainties on the determination of cosmological parameters","volume":"902","author":"Steinhardt","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib399","article-title":"Concerns about the reliability of publicly available SNe Ia data","author":"Rameez","year":"2019","type":"preprint"},{"key":"cqgacbefcbib400","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/ac0f39","type":"journal-article","article-title":"Is there really a Hubble tension?","volume":"38","author":"Rameez","year":"2021","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib401","doi-asserted-by":"publisher","DOI":"10.3847\/1538-4357\/ac4698","type":"preprint","article-title":"The Pantheon+ Analysis: evaluating peculiar velocity corrections in cosmological analyses with nearby type Ia supernovae","author":"Peterson","year":"2021"},{"key":"cqgacbefcbib402","doi-asserted-by":"publisher","DOI":"10.3847\/1538-4357\/ac8b7a","type":"preprint","article-title":"The Pantheon+ Analysis: the full dataset and light-curve release","author":"Scolnic","year":"2021"},{"key":"cqgacbefcbib403","doi-asserted-by":"publisher","first-page":"34","DOI":"10.1063\/1.3021960","type":"journal-article","article-title":"Cosmology: a search for two numbers","volume":"23","author":"Sandage","year":"1970","journal-title":"Phys. Today"},{"key":"cqgacbefcbib404","doi-asserted-by":"publisher","first-page":"1009","DOI":"10.1086\/300499","type":"journal-article","article-title":"Observational evidence from supernovae for an accelerating universe and a cosmological constant","volume":"116","author":"Riess","year":"1998","journal-title":"Astron. J."},{"key":"cqgacbefcbib405","doi-asserted-by":"publisher","first-page":"565","DOI":"10.1086\/307221","type":"journal-article","article-title":"Measurements of \u03a9 and \u039b from 42 High-Redshift Supernovae","volume":"517","author":"Perlmutter","year":"1999","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib406","doi-asserted-by":"publisher","first-page":"1420","DOI":"10.1093\/mnras\/stz3094","type":"journal-article","article-title":"H0LiCOW\u2014XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3\u03c3 tension between early- and late-Universe probes","volume":"498","author":"Wong","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib407","doi-asserted-by":"publisher","first-page":"A101","DOI":"10.1051\/0004-6361\/201937351","type":"journal-article","article-title":"TDCOSMO. I. An exploration of systematic uncertainties in the inference of H0 from time-delay cosmography","volume":"639","author":"Millon","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib408","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.106.L041301","type":"preprint","article-title":"Revealing intrinsic Flat \u039bCDM biases with standardizable candles","author":"Colg\u00e1in","year":"2022"},{"key":"cqgacbefcbib409","article-title":"Putting Flat \u039bCDM In The (Redshift) Bin","author":"Colg\u00e1in","year":"2022","type":"preprint"},{"key":"cqgacbefcbib410","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.102.103525","type":"journal-article","article-title":"Is there an early Universe solution to Hubble tension?","volume":"102","author":"Krishnan","year":"2020","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib411","doi-asserted-by":"publisher","first-page":"150","DOI":"10.3847\/1538-4357\/abeb73","type":"journal-article","article-title":"On the Hubble constant tension in the SNe Ia pantheon sample","volume":"912","author":"Dainotti","year":"2021","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib412","doi-asserted-by":"publisher","first-page":"24","DOI":"10.3390\/galaxies10010024","type":"journal-article","article-title":"On the evolution of the Hubble constant with the SNe Ia pantheon sample and baryon acoustic oscillations: a feasibility study for GRB-Cosmology in 2030","volume":"10","author":"Dainotti","year":"2022","journal-title":"Galaxies"},{"key":"cqgacbefcbib413","doi-asserted-by":"publisher","first-page":"6072","DOI":"10.1093\/mnras\/staa828","type":"journal-article","article-title":"STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354","volume":"494","author":"Shajib","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib414","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.106.103527","type":"preprint","article-title":"Sample variance for supernovae distance measurements and the hubble tension","author":"Zhai","year":"2022"},{"key":"cqgacbefcbib415","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.84.063503","type":"journal-article","article-title":"Peculiar motions, accelerated expansion and the cosmological axis","volume":"84","author":"Tsagas","year":"2011","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib416","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.92.043515","type":"journal-article","article-title":"Deceleration parameter in tilted Friedmann Universes","volume":"92","author":"Tsagas","year":"2015","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib417","doi-asserted-by":"publisher","first-page":"L13","DOI":"10.1051\/0004-6361\/201936373","type":"journal-article","article-title":"Evidence for anisotropy of cosmic acceleration","volume":"631","author":"Colin","year":"2019","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib418","doi-asserted-by":"publisher","first-page":"33","DOI":"10.1088\/0004-637X\/815\/1\/33","type":"journal-article","article-title":"A Hubble diagram for quasars","volume":"815","author":"Risaliti","year":"2015","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib419","doi-asserted-by":"publisher","first-page":"272","DOI":"10.1038\/s41550-018-0657-z","type":"journal-article","article-title":"Cosmological constraints from the Hubble diagram of quasars at high redshifts","volume":"3","author":"Risaliti","year":"2019","journal-title":"Nat. Astron."},{"key":"cqgacbefcbib420","doi-asserted-by":"publisher","first-page":"A150","DOI":"10.1051\/0004-6361\/202038899","type":"journal-article","article-title":"Quasars as standard candles. III. Validation of a new sample for cosmological studies","volume":"642","author":"Lusso","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib421","doi-asserted-by":"publisher","first-page":"A112","DOI":"10.1051\/0004-6361\/201628909","type":"journal-article","article-title":"Cosmology with gamma-ray bursts. I. The Hubble diagram through the calibrated E p,I -E iso correlation","volume":"598","author":"Demianski","year":"2017","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib422","doi-asserted-by":"publisher","first-page":"6140","DOI":"10.1093\/mnras\/stab486","type":"journal-article","article-title":"Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters","volume":"502","author":"Khadka","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib423","doi-asserted-by":"publisher","first-page":"A59","DOI":"10.1051\/0004-6361\/201423969","type":"journal-article","article-title":"Baryon acoustic oscillations in the Ly\u03b1 forest of BOSS DR11 quasars","volume":"574","author":"Delubac","year":"2015","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib424","doi-asserted-by":"publisher","first-page":"153","DOI":"10.3847\/1538-4357\/abb085","type":"journal-article","article-title":"The completed SDSS-IV extended baryon oscillation spectroscopic survey: baryon acoustic oscillations with Ly\u03b1 forests","volume":"901","author":"du Mas des Bourboux","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib425","doi-asserted-by":"publisher","first-page":"JCAP04(2022)060","DOI":"10.1088\/1475-7516\/2022\/04\/060","type":"journal-article","article-title":"Variability in quasar light curves: using quasars as standard candles","author":"Solomon","year":"2022","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib426","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6633\/aa860e","type":"journal-article","article-title":"The status of varying constants: a review of the physics, searches and implications","volume":"80","author":"Martins","year":"2017","journal-title":"Rep. Prog. Phys."},{"key":"cqgacbefcbib427","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.107.191101","type":"journal-article","article-title":"Indications of a spatial variation of the fine structure constant","volume":"107","author":"Webb","year":"2011","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib428","doi-asserted-by":"publisher","first-page":"446","DOI":"10.1093\/mnras\/stu2420","type":"journal-article","article-title":"Impact of instrumental systematic errors on fine-structure constant measurements with quasar spectra","volume":"447","author":"Whitmore","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib429","doi-asserted-by":"publisher","first-page":"1568","DOI":"10.1093\/mnras\/stx381","type":"journal-article","article-title":"Modelling long-range wavelength distortions in quasar absorption echelle spectra","volume":"468","author":"Dumont","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib430","doi-asserted-by":"publisher","first-page":"4930","DOI":"10.1093\/mnras\/stx1949","type":"journal-article","article-title":"Subaru Telescope limits on cosmological variations in the fine-structure constant","volume":"471","author":"Murphy","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib431","doi-asserted-by":"publisher","first-page":"eaay9672","DOI":"10.1126\/sciadv.aay9672","type":"journal-article","article-title":"Four direct measurements of the fine-structure constant 13 billion years ago","volume":"6","author":"Wilczynska","year":"2020","journal-title":"Sci. Adv."},{"key":"cqgacbefcbib432","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1093\/mnras\/staa3217","type":"journal-article","article-title":"A new era of fine structure constant measurements at high redshift","volume":"500","author":"Milakovi\u0107","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib433","doi-asserted-by":"publisher","first-page":"1411","DOI":"10.1093\/mnras\/staa807","type":"journal-article","article-title":"A bound on the 12 C\/ 13 C ratio in near-pristine gas with ESPRESSO","volume":"494","author":"Welsh","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib434","doi-asserted-by":"publisher","first-page":"A123","DOI":"10.1051\/0004-6361\/202142257","type":"journal-article","article-title":"Fundamental physics with ESPRESSO: precise limit on variations in the fine-structure constant towards the bright quasar HE 0515\u20134414","volume":"658","author":"Murphy","year":"2022","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib435","doi-asserted-by":"publisher","DOI":"10.1016\/j.physletb.2022.137002","type":"journal-article","article-title":"Varying fine-structure constant cosmography","volume":"827","author":"Martins","year":"2022","journal-title":"Phys. Lett. B"},{"key":"cqgacbefcbib436","doi-asserted-by":"publisher","first-page":"178","DOI":"10.1093\/mnras\/stv2099","type":"journal-article","article-title":"On methods of estimating cosmological bulk flows","volume":"455","author":"Nusser","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib437","doi-asserted-by":"publisher","first-page":"1772","DOI":"10.1093\/mnras\/sty619","type":"journal-article","article-title":"The dipole anisotropy of AllWISE galaxies","volume":"477","author":"Rameez","year":"2018","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib438","article-title":"Measurement of parity-odd modes in the large-scale 4-point correlation function of SDSS BOSS DR12 CMASS and LOWZ galaxies","author":"Hou","year":"2022","type":"preprint"},{"key":"cqgacbefcbib439","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.106.063501","type":"preprint","article-title":"Probing Parity-Violation with the Four-Point Correlation Function of BOSS Galaxies","author":"Philcox","year":"2022"},{"key":"cqgacbefcbib440","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.125.221301","type":"journal-article","article-title":"New extraction of the cosmic birefringence from the Planck 2018 polarization data","volume":"125","author":"Minami","year":"2020","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib441","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.128.091302","type":"journal-article","article-title":"Cosmic Birefringence from the Planck Data Release 4","volume":"128","author":"Diego-Palazuelos","year":"2022","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib442","doi-asserted-by":"publisher","first-page":"465","DOI":"10.1086\/161911","type":"journal-article","article-title":"A comparison of the properties of highly polarized QSOs versus low-polarization QSOs","volume":"279","author":"Moore","year":"1984","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib443","doi-asserted-by":"publisher","first-page":"485","DOI":"10.1086\/161912","type":"journal-article","article-title":"The optical polarization properties of \u201cnormal\u201d quasars","volume":"279","author":"Stockman","year":"1984","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib444","doi-asserted-by":"publisher","first-page":"869","DOI":"10.1086\/191523","type":"journal-article","article-title":"An optical polarization survey of the palomar-green bright quasar sample","volume":"74","author":"Berriman","year":"1990","journal-title":"Astrophys. J. Suppl."},{"key":"cqgacbefcbib445","doi-asserted-by":"publisher","first-page":"30","DOI":"10.1086\/113704","type":"journal-article","article-title":"Alignment of radio and optical polarization with VLBI structure","volume":"90","author":"Rusk","year":"1985","journal-title":"Astron. J."},{"key":"cqgacbefcbib446","first-page":"410","type":"journal-article","article-title":"Evidence for very large-scale coherent orientations of quasar polarization vectors","volume":"332","author":"Hutsemekers","year":"1998","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib447","doi-asserted-by":"publisher","first-page":"381","DOI":"10.1051\/0004-6361:20000443","type":"journal-article","article-title":"Confirmation of the existence of coherent orientations of quasar polarization vectors on cosmological scales","volume":"367","author":"Hutsem\u00e9kers","year":"2001","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib448","doi-asserted-by":"publisher","first-page":"915","DOI":"10.1051\/0004-6361:20053337","type":"journal-article","article-title":"Mapping extreme-scale alignments of quasar polarization vectors","volume":"441","author":"Hutsem\u00e9kers","year":"2005","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib449","doi-asserted-by":"publisher","first-page":"394","DOI":"10.1111\/j.1365-2966.2004.07169.x","type":"journal-article","article-title":"Large-scale alignment of optical polarizations from distant QSOs using coordinate-invariant statistics","volume":"347","author":"Jain","year":"2004","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib450","doi-asserted-by":"publisher","first-page":"1239","DOI":"10.1093\/mnras\/stu966","type":"journal-article","article-title":"A new analysis of quasar polarization alignments","volume":"442","author":"Pelgrims","year":"2014","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib451","article-title":"A large scale pattern from optical quasar polarization vectors","author":"Shurtleff","year":"2013","type":"preprint"},{"key":"cqgacbefcbib452","doi-asserted-by":"publisher","first-page":"757","DOI":"10.1051\/0004-6361:20042163","type":"journal-article","article-title":"New optical polarization measurements of quasi-stellar objects. The data","volume":"433","author":"Sluse","year":"2005","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib453","first-page":"p 498","type":"conference-proceedings","article-title":"Large scale correlations of quasar polarization vectors: hints of extreme scale structures?","volume":"vol 343","author":"Cabanac","year":"2005"},{"key":"cqgacbefcbib454","first-page":"pp 144","type":"conference-proceedings","article-title":"Large-scale coherent orientations of quasar polarisation vectors: interpretation in terms of axion-like particles","volume":"vol 1274","author":"Payez","year":"2010"},{"key":"cqgacbefcbib455","doi-asserted-by":"publisher","first-page":"A145","DOI":"10.1051\/0004-6361\/201731294","type":"journal-article","article-title":"Cosmological-scale coherent orientations of quasar optical polarization vectors in the Planck era. Investigating the Galactic dust contamination scenario","volume":"622","author":"Pelgrims","year":"2019","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib456","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1086\/153481","type":"journal-article","article-title":"Propagation of electromagnetic polarization effects in anisotropic cosmologies","volume":"197","author":"Brans","year":"1975","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib457","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.66.085007","type":"journal-article","article-title":"Electromagnetic polarization effects due to axion-photon mixing","volume":"66","author":"Jain","year":"2002","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib458","doi-asserted-by":"publisher","first-page":"JCAP06(2005)002","DOI":"10.1088\/1475-7516\/2005\/06\/002","type":"journal-article","article-title":"Probing light pseudoscalars with light propagation, resonance and spontaneous polarization","author":"Das","year":"2005","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib459","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.75.043011","type":"journal-article","article-title":"Evolution of polarization orientations in a flat universe with vector perturbations: CMB and quasistellar objects","volume":"75","author":"Morales","year":"2007","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib460","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.84.085029","type":"journal-article","article-title":"Can axionlike particles explain the alignments of the polarizations of light from quasars?","volume":"84","author":"Payez","year":"2011","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib461","doi-asserted-by":"publisher","DOI":"10.1142\/S0217732312502215","type":"journal-article","article-title":"Electrodynamic Effect of Anisotropic Expansions in the Universe","volume":"27","author":"Ciarcelluti","year":"2012","journal-title":"Mod. Phys. Lett. A"},{"key":"cqgacbefcbib462","doi-asserted-by":"publisher","first-page":"497","DOI":"10.1023\/A:1018867011142","type":"journal-article","article-title":"Effect of the Global Rotation of the Universe on the Formation of Galaxies","volume":"30","author":"Li","year":"1998","journal-title":"Gen. Relativ. Gravit."},{"key":"cqgacbefcbib463","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.105.161301","type":"journal-article","article-title":"Can primordial magnetic fields seeded by electroweak strings cause an alignment of quasar axes on cosmological scales?","volume":"105","author":"Poltis","year":"2010","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib464","doi-asserted-by":"publisher","first-page":"1643","DOI":"10.1142\/S0218271811019475","type":"journal-article","article-title":"Global and local effects of rotation:. observational aspects","volume":"20","author":"God\u0142owski","year":"2011","journal-title":"Int. J. Mod. Phys. D"},{"key":"cqgacbefcbib465","doi-asserted-by":"publisher","first-page":"3369","DOI":"10.1093\/mnras\/stv1570","type":"journal-article","article-title":"Spin alignments within the cosmic web: a theory of constrained tidal torques near filaments","volume":"452","author":"Codis","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib466","doi-asserted-by":"publisher","DOI":"10.1142\/S0218271818500943","type":"journal-article","article-title":"Evidence of cosmic strings by the observation of the alignment of quasar polarization axes on Mpc scale","volume":"27","author":"Slagter","year":"2018","journal-title":"Int. J. Mod. Phys. D"},{"key":"cqgacbefcbib467","doi-asserted-by":"publisher","first-page":"14","DOI":"10.3390\/universe6010014","type":"journal-article","article-title":"In the Quest for Cosmic Rotation","volume":"6","author":"Korotky","year":"2020","journal-title":"Universe"},{"key":"cqgacbefcbib468","doi-asserted-by":"publisher","first-page":"604","DOI":"10.1093\/mnras\/stac887","type":"journal-article","article-title":"A mechanism to explain galaxy alignment over a range of scales","volume":"513","author":"Tiwari","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib469","doi-asserted-by":"publisher","first-page":"162","DOI":"10.1111\/j.1365-2966.2007.12028.x","type":"journal-article","article-title":"A survey of polarization in the JVAS\/CLASS flat-spectrum radio source surveys\u2014II. A search for aligned radio polarizations","volume":"380","author":"Joshi","year":"2007","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib470","doi-asserted-by":"publisher","DOI":"10.1142\/S0218271813500892","type":"journal-article","article-title":"Polarization Alignment in Jvas\/class Flat Spectrum Radio Surveys","volume":"22","author":"Tiwari","year":"2013","journal-title":"Int. J. Mod. Phys. D"},{"key":"cqgacbefcbib471","doi-asserted-by":"publisher","first-page":"4161","DOI":"10.1093\/mnras\/stv917","type":"journal-article","article-title":"Polarization alignments of quasars from the JVAS\/CLASS 8.4-GHz surveys","volume":"450","author":"Pelgrims","year":"2015","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib472","doi-asserted-by":"publisher","first-page":"L42","DOI":"10.1088\/2041-8205\/775\/2\/L42","type":"journal-article","article-title":"Galaxy spin alignment in filaments and sheets: observational evidence","volume":"775","author":"Tempel","year":"2013","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib473","doi-asserted-by":"publisher","first-page":"160","DOI":"10.1088\/0004-637X\/779\/2\/160","type":"journal-article","article-title":"Alignments of Galaxies within Cosmic Filaments from SDSS DR7","volume":"779","author":"Zhang","year":"2013","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib474","doi-asserted-by":"publisher","first-page":"0157","DOI":"10.1038\/s41550-017-0157","type":"journal-article","article-title":"Ten billion years of brightest cluster galaxy alignments","volume":"1","author":"West","year":"2017","journal-title":"Nat. Astron."},{"key":"cqgacbefcbib475","doi-asserted-by":"publisher","first-page":"A18","DOI":"10.1051\/0004-6361\/201424631","type":"journal-article","article-title":"Alignment of quasar polarizations with large-scale structures","volume":"572","author":"Hutsem\u00e9kers","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib476","doi-asserted-by":"publisher","first-page":"A53","DOI":"10.1051\/0004-6361\/201526979","type":"journal-article","article-title":"Evidence for the alignment of quasar radio polarizations with large quasar group axes","volume":"590","author":"Pelgrims","year":"2016","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib477","article-title":"Correlations between multiple tracers of the cosmic web","author":"Friday","year":"2020","type":"preprint"},{"key":"cqgacbefcbib478","doi-asserted-by":"publisher","first-page":"L36","DOI":"10.1093\/mnrasl\/slw038","type":"journal-article","article-title":"Alignments of radio galaxies in deep radio imaging of ELAIS N1","volume":"459","author":"Taylor","year":"2016","journal-title":"Mon. Not. R. Astron. Soc,"},{"key":"cqgacbefcbib479","doi-asserted-by":"publisher","first-page":"636","DOI":"10.1093\/mnras\/stx1977","type":"journal-article","article-title":"Radio Galaxy Zoo: cosmological alignment of radio sources","volume":"472","author":"Contigiani","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib480","doi-asserted-by":"publisher","first-page":"1226","DOI":"10.1093\/mnras\/staa2975","type":"journal-article","article-title":"Alignment of radio galaxy axes using FIRST catalogue","volume":"499","author":"Panwar","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib481","doi-asserted-by":"publisher","first-page":"A70","DOI":"10.1051\/0004-6361\/202037680","type":"journal-article","article-title":"Alignment in the orientation of LOFAR radio sources","volume":"642","author":"Osinga","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib482","doi-asserted-by":"publisher","first-page":"A102","DOI":"10.1051\/0004-6361\/202037444","type":"journal-article","article-title":"Global alignments of parsec-scale AGN radio jets and their polarization planes","volume":"635","author":"Blinov","year":"2020","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib483","doi-asserted-by":"publisher","first-page":"A123","DOI":"10.1051\/0004-6361\/202140764","type":"journal-article","article-title":"Local alignments of parsec-scale AGN radiojets","volume":"653","author":"Mandarakas","year":"2021","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib484","doi-asserted-by":"publisher","first-page":"1361","DOI":"10.1093\/mnras\/stab1872","type":"journal-article","article-title":"Large-scale clustering amongst Fermi blazars; evidence for axis alignments?","volume":"507","author":"March a","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib485","doi-asserted-by":"publisher","first-page":"683","DOI":"10.1093\/mnras\/199.3.683","type":"journal-article","article-title":"The clustering of quasars from an objective-prism survey","volume":"199","author":"Webster","year":"1982","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib486","doi-asserted-by":"publisher","first-page":"129","DOI":"10.1086\/165045","type":"journal-article","article-title":"The Space Distribution of Faint Quasars from the CFHT Survey","volume":"314","author":"Crampton","year":"1987","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib487","doi-asserted-by":"publisher","first-page":"4159","DOI":"10.1093\/mnras\/stac269","type":"journal-article","article-title":"Correlated orientations of the axes of large quasar groups on Gpc scales","volume":"511","author":"Friday","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib488","doi-asserted-by":"publisher","first-page":"70","DOI":"10.1214\/aos\/1176346577","type":"journal-article","article-title":"The dip test of unimodality","volume":"13","author":"Hartigan","year":"1985","journal-title":"Ann. Stat."},{"key":"cqgacbefcbib489","article-title":"Large-scale alignments of quasar polarization vectors. Observational evidence and possible implications for cosmology","author":"Hutsem\u00e9kers","year":"2021","type":"other"},{"key":"cqgacbefcbib490","doi-asserted-by":"publisher","first-page":"217","DOI":"10.5303\/JKAS.2011.44.6.217","type":"journal-article","article-title":"The New Horizon Run Cosmological N-Body Simulations","volume":"44","author":"Kim","year":"2011","journal-title":"J. Korean Astron. Soc."},{"key":"cqgacbefcbib491","first-page":"269","type":"journal-article","article-title":"The anisotropy of the spatial orientations of galaxies in the Local Supercluster","volume":"145","author":"MacGillivray","year":"1985","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib492","doi-asserted-by":"publisher","first-page":"112","DOI":"10.1086\/170101","type":"journal-article","article-title":"A catalog of spin orientation of southern galaxies","volume":"374","author":"Iye","year":"1991","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib493","doi-asserted-by":"publisher","first-page":"224","DOI":"10.1016\/j.physletb.2011.04.008","type":"journal-article","article-title":"Detection of a dipole in the handedness of spiral galaxies with redshifts z\u223c0.04","volume":"699","author":"Longo","year":"2011","journal-title":"Phys. Lett. B"},{"key":"cqgacbefcbib494","doi-asserted-by":"publisher","first-page":"104","DOI":"10.3847\/1538-4357\/ab3fa3","type":"journal-article","article-title":"Mysterious coherence in several-megaparsec scales between galaxy rotation and neighbor motion","volume":"884","author":"Lee","year":"2019","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib495","doi-asserted-by":"publisher","first-page":"32","DOI":"10.3847\/0004-637X\/823\/1\/32","type":"journal-article","article-title":"Asymmetry between galaxies with clockwise handedness and counterclockwise handedness","volume":"823","author":"Shamir","year":"2016","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib496","doi-asserted-by":"publisher","first-page":"1686","DOI":"10.1111\/j.1365-2966.2008.13490.x","type":"journal-article","article-title":"Galaxy Zoo: the large-scale spin statistics of spiral galaxies in the Sloan Digital Sky Survey","volume":"388","author":"Land","year":"2008","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib497","doi-asserted-by":"publisher","DOI":"10.1016\/j.ascom.2022.100545","type":"journal-article","article-title":"Systematic biases when using deep neural networks for annotating large catalogs of astronomical images","volume":"38","author":"Dhar","year":"2022","journal-title":"Astron. Comput."},{"key":"cqgacbefcbib498","doi-asserted-by":"publisher","first-page":"87","DOI":"10.1088\/0004-637X\/790\/2\/87","type":"journal-article","article-title":"SpArcFiRe: Scalable Automated Detection of Spiral Galaxy Arm Segments","volume":"790","author":"Davis","year":"2014","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib499","doi-asserted-by":"publisher","first-page":"3928","DOI":"10.1093\/mnras\/stw3290","type":"journal-article","article-title":"On the nature and correction of the spurious S-wise spiral galaxy winding bias in Galaxy Zoo 1","volume":"466","author":"Hayes","year":"2017","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib500","doi-asserted-by":"publisher","first-page":"141","DOI":"10.1088\/0004-637X\/736\/2\/141","type":"journal-article","article-title":"Ganalyzer: a tool for automatic galaxy image analysis","volume":"736","author":"Shamir","year":"2011","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib501","doi-asserted-by":"publisher","first-page":"25","DOI":"10.1016\/j.physletb.2012.07.054","type":"journal-article","article-title":"Handedness asymmetry of spiral galaxies with z < 0.3 shows cosmic parity violation and a dipole axis","volume":"715","author":"Shamir","year":"2012","journal-title":"Phys. Lett. B"},{"key":"cqgacbefcbib502","doi-asserted-by":"publisher","first-page":"136","DOI":"10.1007\/s10509-020-03850-1","type":"journal-article","article-title":"Patterns of galaxy spin directions in SDSS and Pan-STARRS show parity violation and multipoles","volume":"365","author":"Shamir","year":"2020","journal-title":"Astrophys. Space Sci."},{"key":"cqgacbefcbib503","doi-asserted-by":"publisher","first-page":"e053","DOI":"10.1017\/pasa.2020.46","type":"journal-article","article-title":"Galaxy spin direction distribution in HST and SDSS show similar large-scale asymmetry","volume":"37","author":"Shamir","year":"2020","journal-title":"Publ. Astron. Soc. Aust."},{"key":"cqgacbefcbib504","doi-asserted-by":"publisher","DOI":"10.1002\/asna.20220010","type":"preprint","article-title":"Large-scale asymmetry in galaxy spin directions\u2014analysis of galaxies with spectra in DES, SDSS and DESI Legacy Survey","author":"Shamir","year":"2022"},{"key":"cqgacbefcbib505","doi-asserted-by":"publisher","first-page":"e037","DOI":"10.1017\/pasa.2021.27","type":"journal-article","article-title":"Large-scale asymmetry in galaxy spin directions: evidence from the Southern hemisphere","volume":"38","author":"Shamir","year":"2021","journal-title":"Publ. Astron. Soc. Aust."},{"key":"cqgacbefcbib506","doi-asserted-by":"publisher","first-page":"24","DOI":"10.1007\/s12036-022-09809-8","type":"journal-article","article-title":"New evidence and analysis of cosmological-scale asymmetry in galaxy spin directions","volume":"43","author":"Shamir","year":"2022","journal-title":"J. Astrophys. Astron."},{"key":"cqgacbefcbib507","doi-asserted-by":"publisher","first-page":"123","DOI":"10.3847\/1538-4357\/abb3bb","type":"journal-article","article-title":"Spin parity of spiral galaxies. III. Dipole analysis of the distribution of SDSS spirals with 3D random walk simulations","volume":"907","author":"Iye","year":"2021","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib508","doi-asserted-by":"publisher","first-page":"1114","DOI":"10.1093\/pasj\/psac058","type":"journal-article","article-title":"Using 3D and 2D analysis for analyzing large-scale asymmetry in galaxy spin directions","volume":"74","author":"Shamir","year":"2022","journal-title":"Publ. Astron. Soc. Japan"},{"key":"cqgacbefcbib509","doi-asserted-by":"publisher","DOI":"10.1155\/2022\/8462363","type":"journal-article","article-title":"Analysis of \u223c106 spiral galaxies from four telescopes shows large-scale patterns of asymmetry in galaxy spin directions","volume":"2022","author":"Shamir","year":"2022","journal-title":"Adv. Astron."},{"key":"cqgacbefcbib510","doi-asserted-by":"publisher","first-page":"e011","DOI":"10.1017\/pasa.2017.4","type":"journal-article","article-title":"Photometric asymmetry between clockwise and counterclockwise spiral galaxies in SDSS","volume":"34","author":"Shamir","year":"2017","journal-title":"Publ. Astron. Soc. Aust."},{"key":"cqgacbefcbib511","type":"journal-article","article-title":"Analysis of dipole alignment in large-scale distribution of galaxy spin directions","volume":"2022","author":"Shamir","year":"2022","journal-title":"Astrophys. Sour. Code Libr."},{"key":"cqgacbefcbib512","doi-asserted-by":"publisher","first-page":"707","DOI":"10.1086\/300738","type":"journal-article","article-title":"BVRI light curves for 22 Type IA supernovae","volume":"117","author":"Riess","year":"1999","journal-title":"Astron. J."},{"key":"cqgacbefcbib513","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1103\/RevModPhys.61.1","type":"journal-article","article-title":"The cosmological constant problem","volume":"61","author":"Weinberg","year":"1989","journal-title":"Rev. Mod. Phys."},{"key":"cqgacbefcbib514","doi-asserted-by":"publisher","DOI":"10.1016\/j.dark.2022.101163","type":"preprint","article-title":"Simultaneously solving the H 0 \u03c3 8 tensions with late dark energy","author":"Heisenberg","year":"2022"},{"key":"cqgacbefcbib515","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.106.043503","type":"preprint","article-title":"Can late-time extensions solve the H 0 \u03c3 8 tensions?","author":"Heisenberg","year":"2022"},{"key":"cqgacbefcbib516","doi-asserted-by":"publisher","first-page":"JCAP04(2022)004","DOI":"10.1088\/1475-7516\/2022\/04\/004","type":"journal-article","article-title":"Is local H 0 at odds with dark energy EFT?","author":"Lee","year":"2022","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib517","article-title":"The accelerated expansion of the universe challenged by an effect of the inhomogeneities. a review","author":"C\u00e9l\u00e9rier","year":"2007","type":"preprint"},{"key":"cqgacbefcbib518","doi-asserted-by":"publisher","first-page":"2363","DOI":"10.1088\/0264-9381\/15\/8\/016","type":"journal-article","article-title":"The distortion of the area distance-redshift relation in inhomogeneous isotropic universes","volume":"15","author":"Mustapha","year":"1998","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib519","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.78.123531","type":"journal-article","article-title":"Dark energy or apparent acceleration due to a relativistic cosmological model more complex than the Friedmann-Lemaitre-Robertson-Walker model?","volume":"78","author":"Ishak","year":"2008","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib520","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.103.083513","type":"journal-article","article-title":"Question of measuring spatial curvature in an inhomogeneous universe","volume":"103","author":"Tian","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib521","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.101.011301","type":"journal-article","article-title":"A General Test of the Copernican Principle","volume":"101","author":"Clarkson","year":"2008","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib522","doi-asserted-by":"publisher","first-page":"JCAP08(2007)011","DOI":"10.1088\/1475-7516\/2007\/08\/011","type":"journal-article","article-title":"Dynamical dark energy or simply cosmic curvature?","author":"Clarkson","year":"2007","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib523","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/25\/19\/195001","type":"journal-article","article-title":"On the curvature of the present-day universe","volume":"25","author":"Buchert","year":"2008","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib524","first-page":"51","type":"journal-article","article-title":"L\u2019Univers en expansion","volume":"A53","author":"Lema\u00eetre","year":"1933","journal-title":"Ann. Soc. Sci. Brux."},{"key":"cqgacbefcbib524","doi-asserted-by":"publisher","first-page":"637","DOI":"10.1023\/A:1018855621348","type":"journal-article","volume":"29","author":"Lema\u00eetre","year":"1997","journal-title":"Gen. Relativ. Gravit."},{"key":"cqgacbefcbib525","doi-asserted-by":"publisher","first-page":"169","DOI":"10.1073\/pnas.20.3.169","type":"journal-article","article-title":"Effect of inhomogeneity on cosmological models","volume":"20","author":"Tolman","year":"1934","journal-title":"Proc. Natl Acad. Sci."},{"key":"cqgacbefcbib526","doi-asserted-by":"publisher","first-page":"410","DOI":"10.1093\/mnras\/107.5-6.410","type":"journal-article","article-title":"Spherically symmetrical models in general relativity","volume":"107","author":"Bondi","year":"1947","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib527","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.79.083011","type":"journal-article","article-title":"Testing backreaction effects with observations","volume":"79","author":"Larena","year":"2009","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib528","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.80.123512","type":"journal-article","article-title":"Average observational quantities in the timescape cosmology","volume":"80","author":"Wiltshire","year":"2009","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib529","doi-asserted-by":"publisher","first-page":"JCAP12(2013)051","DOI":"10.1088\/1475-7516\/2013\/12\/051","type":"journal-article","article-title":"Average expansion rate and light propagation in a cosmological Tardis spacetime","author":"Lavinto","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib530","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.81.083537","type":"journal-article","article-title":"Model independent tests of the standard cosmological model","volume":"81","author":"Shafieloo","year":"2010","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib531","doi-asserted-by":"publisher","first-page":"37","DOI":"10.1086\/340549","type":"journal-article","article-title":"Constraining cosmological parameters based on relative galaxy ages","volume":"573","author":"Jimenez","year":"2002","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib532","doi-asserted-by":"publisher","first-page":"JCAP05(2016)014","DOI":"10.1088\/1475-7516\/2016\/05\/014","type":"journal-article","article-title":"A 6% measurement of the Hubble parameter at z \u223c 0.45: direct evidence of the epoch of cosmic re-acceleration","author":"Moresco","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib533","doi-asserted-by":"publisher","first-page":"82","DOI":"10.3847\/1538-4357\/ab9eb0","type":"journal-article","article-title":"Setting the stage for cosmic chronometers. II. Impact of stellar population synthesis models systematics and full covariance matrix","volume":"898","author":"Moresco","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib534","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/stac1978","type":"preprint","article-title":"On the use of galaxies as clocks and the universal expansion","author":"Ahlstrom Kjerrgren","year":"2021"},{"key":"cqgacbefcbib535","doi-asserted-by":"publisher","first-page":"358","DOI":"10.1038\/281358a0","type":"journal-article","article-title":"An evolution free test for non-zero cosmological constant","volume":"281","author":"Alcock","year":"1979","journal-title":"Nature"},{"key":"cqgacbefcbib536","doi-asserted-by":"publisher","first-page":"JCAP03(2019)003","DOI":"10.1088\/1475-7516\/2019\/03\/003","type":"journal-article","article-title":"Baryon acoustic oscillation methods for generic curvature: application to the SDSS-III Baryon oscillation spectroscopic survey","author":"Heinesen","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib537","doi-asserted-by":"publisher","first-page":"JCAP01(2020)038","DOI":"10.1088\/1475-7516\/2020\/01\/038","type":"journal-article","article-title":"Quantifying the accuracy of the Alcock-Paczy\u0144ski scaling of baryon acoustic oscillation measurements","author":"Heinesen","year":"2020","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib538","doi-asserted-by":"publisher","first-page":"2231","DOI":"10.1111\/j.1365-2966.2010.16627.x","type":"journal-article","article-title":"Rendering dark energy void","volume":"405","author":"February","year":"2010","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib539","article-title":"A model independent measure of the large scale curvature of the Universe","author":"Mortsell","year":"2011","type":"preprint"},{"key":"cqgacbefcbib540","doi-asserted-by":"publisher","first-page":"JCAP03(2017)028","DOI":"10.1088\/1475-7516\/2017\/03\/028","type":"journal-article","article-title":"Constraining cosmic curvature by using age of galaxies and gravitational lenses","author":"Rana","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib541","doi-asserted-by":"publisher","first-page":"45","DOI":"10.3847\/1538-4357\/aa8725","type":"journal-article","article-title":"Model-independent constraints on cosmic curvature and opacity","volume":"847","author":"Wang","year":"2017","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib542","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.97.083510","type":"journal-article","article-title":"Null tests of the standard model using the linear model formalism","volume":"97","author":"Marra","year":"2018","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib543","doi-asserted-by":"publisher","first-page":"29","DOI":"10.3847\/1538-4357\/aae696","type":"journal-article","article-title":"Model-independent curvature determination from gravitational-wave standard sirens and cosmic chronometers","volume":"868","author":"Wei","year":"2018","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib544","doi-asserted-by":"publisher","first-page":"JCAP12(2019)034","DOI":"10.1088\/1475-7516\/2019\/12\/034","type":"journal-article","article-title":"The cosmological consistency relation in a Universe with structure","author":"Rustagi","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib545","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/ab954b","type":"journal-article","article-title":"Solving the curvature and Hubble parameter inconsistencies through structure formation-induced curvature","volume":"37","author":"Heinesen","year":"2020","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib546","doi-asserted-by":"publisher","first-page":"5714","DOI":"10.1093\/mnras\/staa4044","type":"journal-article","article-title":"Machine learning the cosmic curvature in a model-independent way","volume":"501","author":"Wang","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib547","doi-asserted-by":"publisher","DOI":"10.3847\/1538-4357\/ac641e","type":"preprint","article-title":"Multiple measurements of gravitational waves acting as standard probes: model-independent constraints on the cosmic curvature with DECIGO","author":"Zhang","year":"2022"},{"key":"cqgacbefcbib548","doi-asserted-by":"publisher","first-page":"A67","DOI":"10.1051\/0004-6361\/202142503","type":"journal-article","article-title":"Euclid: Forecast constraints on consistency tests of the \u039bCDM model","volume":"660","author":"Nesseris","year":"2022","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib549","doi-asserted-by":"publisher","first-page":"3092","DOI":"10.1093\/mnras\/stab1085","type":"journal-article","article-title":"Measurement on the cosmic curvature using the Gaussian process method","volume":"504","author":"Yang","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib550","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.90.023012","type":"journal-article","article-title":"Curvature versus distances: Testing the FLRW cosmology","volume":"90","author":"Sapone","year":"2014","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib551","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/30\/17\/175006","type":"journal-article","article-title":"Timescape cosmology with radiation fluid","volume":"30","author":"Duley","year":"2013","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib552","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.115.101301","type":"journal-article","article-title":"New test of the Friedmann-Lema\u00eetre-Robertson-Walker metric using the distance sum rule","volume":"115","author":"R\u00e4s\u00e4nen","year":"2015","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib553","author":"Peebles","year":"1993","type":"book"},{"key":"cqgacbefcbib554","doi-asserted-by":"publisher","first-page":"70","DOI":"10.3847\/1538-4357\/aa697e","type":"journal-article","article-title":"Test of the FLRW metric and curvature with strong lens time delays","volume":"839","author":"Liao","year":"2017","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib555","doi-asserted-by":"publisher","first-page":"JCAP03(2018)041","DOI":"10.1088\/1475-7516\/2018\/03\/041","type":"journal-article","article-title":"Cosmic curvature tested directly from observations","author":"Denissenya","year":"2018","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib556","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.100.023530","type":"journal-article","article-title":"Strongly gravitationally lensed type Ia supernovae: direct test of the Friedman-Lema\u00eetre-Robertson-Walker metric","volume":"100","author":"Qi","year":"2019","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib557","doi-asserted-by":"publisher","first-page":"1104","DOI":"10.1093\/mnras\/sty3175","type":"journal-article","article-title":"The distance sum rule from strong lensing systems and quasars\u2014test of cosmic curvature and beyond","volume":"483","author":"Qi","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib558","doi-asserted-by":"publisher","first-page":"37","DOI":"10.3847\/1538-4357\/ab037e","type":"journal-article","article-title":"Constraining cosmological parameters in the FLRW metric with lensed GW+EM signals","volume":"873","author":"Li","year":"2019","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib559","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.99.083514","type":"journal-article","article-title":"Constraints on cosmic curvature with lensing time delays and gravitational waves","volume":"99","author":"Liao","year":"2019","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib560","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.123.231101","type":"journal-article","article-title":"Model-independent determination of H0 \u03a9K0 from strong lensing and Type Ia supernovae","volume":"123","author":"Collett","year":"2019","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib561","doi-asserted-by":"publisher","DOI":"10.1038\/s41598-019-47616-4","type":"journal-article","article-title":"Direct test of the FLRW metric from strongly lensed gravitational wave observations","volume":"9","author":"Cao","year":"2019","journal-title":"Sci. Rep."},{"key":"cqgacbefcbib562","doi-asserted-by":"publisher","first-page":"100","DOI":"10.3847\/1538-4357\/ab9b22","type":"journal-article","article-title":"Cosmological model-independent constraints on spatial curvature from strong gravitational lensing and SN Ia observations","volume":"898","author":"Wang","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib563","doi-asserted-by":"publisher","first-page":"186","DOI":"10.3847\/1538-4357\/ab5f61","type":"journal-article","article-title":"Model-independent estimations for the cosmic curvature from the latest strong gravitational lensing systems","volume":"889","author":"Zhou","year":"2020","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib564","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.103.063511","type":"journal-article","article-title":"Constraining cosmological and galaxy parameters using strong gravitational lensing systems","volume":"103","author":"Kumar","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib565","doi-asserted-by":"publisher","first-page":"708","DOI":"10.1093\/mnras\/staa1539","type":"journal-article","article-title":"Testing the cosmic curvature at high redshifts: the combination of LSST strong lensing systems and quasars as new standard candles","volume":"496","author":"Liu","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib566","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.103532","type":"journal-article","article-title":"Complementary consistency test of the Copernican principle via Noether\u2019s theorem and machine learning forecasts","volume":"104","author":"Arjona","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib567","doi-asserted-by":"publisher","first-page":"85","DOI":"10.3847\/0004-637X\/828\/2\/85","type":"journal-article","article-title":"New model-independent method to test the curvature of the Universe","volume":"828","author":"Yu","year":"2016","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib568","doi-asserted-by":"publisher","first-page":"1913","DOI":"10.1093\/mnras\/stz2717","type":"journal-article","article-title":"Generalized model-independent characterization of strong gravitational lenses V: reconstructing the lensing distance ratio by supernovae for a general Friedmann universe","volume":"490","author":"Wagner","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib569","doi-asserted-by":"publisher","first-page":"1725","DOI":"10.1093\/mnras\/staa344","type":"journal-article","article-title":"Overconstrained gravitational lens models and the Hubble constant","volume":"493","author":"Kochanek","year":"2020","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib570","doi-asserted-by":"publisher","first-page":"5021","DOI":"10.1093\/mnras\/staa4033","type":"journal-article","article-title":"Overconstrained models of time delay lenses redux: how the angular tail wags the radial dog","volume":"501","author":"Kochanek","year":"2021","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib571","doi-asserted-by":"publisher","first-page":"A86","DOI":"10.1051\/0004-6361\/201834218","type":"journal-article","article-title":"Generalised model-independent characterisation of strong gravitational lenses. IV. Formalism-intrinsic degeneracies","volume":"620","author":"Wagner","year":"2018","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib572","doi-asserted-by":"publisher","first-page":"4492","DOI":"10.1093\/mnras\/stz1587","type":"journal-article","article-title":"Generalised model-independent characterisation of strong gravitational lenses\u2014VI. The origin of the formalism intrinsic degeneracies and their influence on H0","volume":"487","author":"Wagner","year":"2019","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib573","doi-asserted-by":"publisher","first-page":"61","DOI":"10.1007\/s10714-020-02715-w","type":"journal-article","article-title":"Cosmic structures from a mathematical perspective 1: dark matter halo mass density profiles","volume":"52","author":"Wagner","year":"2020","journal-title":"Gen. Relativ. Gravit."},{"key":"cqgacbefcbib574","article-title":"Euclid assessment study report for the ESA cosmic visions","author":"Laureijs","year":"2009","type":"preprint"},{"key":"cqgacbefcbib575","article-title":"Euclid definition study report","author":"Laureijs","year":"2011","type":"preprint"},{"key":"cqgacbefcbib576","doi-asserted-by":"publisher","first-page":"146","DOI":"10.3847\/1538-4357\/aaa76f","type":"journal-article","article-title":"Curvature from strong gravitational lensing: a spatially closed universe or systematics?","volume":"854","author":"Li","year":"2018","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib577","doi-asserted-by":"publisher","first-page":"JCAP01(2017)015","DOI":"10.1088\/1475-7516\/2017\/01\/015","type":"journal-article","article-title":"Model-independent test of the FLRW metric, the flatness of the Universe and non-local estimation of H0 r d","author":"L\u2019Huillier","year":"2017","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib578","doi-asserted-by":"publisher","first-page":"1770","DOI":"10.1093\/mnras\/stw066","type":"journal-article","article-title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12","volume":"457","author":"Cuesta","year":"2016","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib579","doi-asserted-by":"publisher","first-page":"560","DOI":"10.1086\/466512","type":"journal-article","article-title":"Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies","volume":"633","author":"Eisenstein","year":"2005","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib580","doi-asserted-by":"publisher","first-page":"761","DOI":"10.1080\/14786443309462220","type":"journal-article","article-title":"On the definition of distance in general relativity","volume":"15","author":"Etherington","year":"1933","journal-title":"Phil. Mag."},{"key":"cqgacbefcbib581","doi-asserted-by":"publisher","first-page":"JCAP06(2009)012","DOI":"10.1088\/1475-7516\/2009\/06\/012","type":"journal-article","article-title":"Consistency among distance measurements: transparency, BAO scale and accelerated expansion","author":"Avgoustidis","year":"2009","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib582","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.88.161302","type":"journal-article","article-title":"Dimming Supernovae without Cosmic Acceleration","volume":"88","author":"Cs\u00e1ki","year":"2002","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib583","doi-asserted-by":"publisher","first-page":"33","DOI":"10.1016\/S0370-2693(02)01765-3","type":"journal-article","article-title":"Effects of the intergalactic plasma on supernova dimming via photon-axion oscillations","volume":"535","author":"Cs\u00e1ki","year":"2002","journal-title":"Phys. Lett. B"},{"key":"cqgacbefcbib584","doi-asserted-by":"publisher","first-page":"661","DOI":"10.1086\/383520","type":"journal-article","article-title":"Cosmic acceleration versus Axion-Photon mixing","volume":"607","author":"Bassett","year":"2004","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib585","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.69.101305","type":"journal-article","article-title":"Cosmic distance-duality as a probe of exotic physics and acceleration","volume":"69","author":"Bassett","year":"2004","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib586","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.77.043009","type":"journal-article","article-title":"Supernova brightening from chameleon-photon mixing","volume":"77","author":"Burrage","year":"2008","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib587","doi-asserted-by":"publisher","DOI":"10.1016\/j.dark.2022.100966","type":"journal-article","article-title":"A null test of the Cosmological Principle with BAO measurements","volume":"35","author":"Bengaly","year":"2022","journal-title":"Phys. Dark Universe"},{"key":"cqgacbefcbib588","doi-asserted-by":"publisher","first-page":"4004","DOI":"10.1093\/mnras\/stac1030","type":"journal-article","article-title":"The resilience of the Etherington-Hubble relation","volume":"513","author":"Renzi","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib589","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.101.104046","type":"journal-article","article-title":"Cosmological signatures of torsion and how to distinguish torsion from the dark sector","volume":"101","author":"Bolejko","year":"2020","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib590","article-title":"Teleparallel gravity: from theory to cosmology","author":"Bahamonde","year":"2021","type":"preprint"},{"key":"cqgacbefcbib591","doi-asserted-by":"publisher","first-page":"JCAP03(2013)023","DOI":"10.1088\/1475-7516\/2013\/03\/023","type":"journal-article","article-title":"Galaxy correlations and the BAO in a void universe: structure formation as a test of the Copernican Principle","author":"February","year":"2013","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib592","doi-asserted-by":"publisher","first-page":"JCAP10(2012)009","DOI":"10.1088\/1475-7516\/2012\/10\/009","type":"journal-article","article-title":"Tension in the void: cosmic rulers strain inhomogeneous cosmologies","author":"Zumalac\u00e1rregui","year":"2012","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib593","doi-asserted-by":"publisher","first-page":"145","DOI":"10.3847\/1538-4357\/ab0ebf","type":"journal-article","article-title":"The local perspective on the Hubble tension: local structure does not impact measurement of the Hubble constant","volume":"875","author":"Kenworthy","year":"2019","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib594","doi-asserted-by":"publisher","DOI":"10.1088\/1361-6382\/ac8635","type":"preprint","article-title":"A void in the Hubble tension? The end of the line for the Hubble bubble","author":"Camarena","year":"2022"},{"key":"cqgacbefcbib595","doi-asserted-by":"publisher","first-page":"1291","DOI":"10.1093\/mnras\/stab3077","type":"journal-article","article-title":"The Copernican principle in light of the latest cosmological data","volume":"509","author":"Camarena","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib596","doi-asserted-by":"publisher","first-page":"1821","DOI":"10.1103\/PhysRevD.52.1821","type":"journal-article","article-title":"Geocentrism reexamined","volume":"52","author":"Goodman","year":"1995","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib597","doi-asserted-by":"publisher","first-page":"413","DOI":"10.1093\/mnras\/190.3.413","type":"journal-article","article-title":"The velocity of clusters of galaxies relative to the microwave background\u2014the possibility of its measurement","volume":"190","author":"Sunyaev","year":"1980","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib598","doi-asserted-by":"publisher","first-page":"JCAP09(2008)016","DOI":"10.1088\/1475-7516\/2008\/09\/016","type":"journal-article","article-title":"Looking the void in the eyes\u2014the kinematic Sunyaev Zeldovich effect in Lema\u00eetre Tolman Bondi models","author":"Garc\u00eda-Bellido","year":"2008","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib599","doi-asserted-by":"publisher","first-page":"JCAP10(2010)011","DOI":"10.1088\/1475-7516\/2010\/10\/011","type":"journal-article","article-title":"CMB observations in LTB universes. Part II: the kSZ effect in an LTB universe","author":"Yoo","year":"2010","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib600","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.107.041301","type":"journal-article","article-title":"Confirmation of the copernican principle at Gpc radial scale and above from the kinetic Sunyaev-Zel\u2019dovich effect power spectrum","volume":"107","author":"Zhang","year":"2011","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib601","doi-asserted-by":"publisher","DOI":"10.1088\/0264-9381\/28\/16\/164005","type":"journal-article","article-title":"Linear kinetic Sunyaev-Zel\u2019dovich effect and void models for acceleration","volume":"28","author":"Zibin","year":"2011","journal-title":"Class. Quantum Grav."},{"key":"cqgacbefcbib602","doi-asserted-by":"publisher","first-page":"JCAP02(2011)013","DOI":"10.1088\/1475-7516\/2011\/02\/013","type":"journal-article","article-title":"The cosmic microwave background in an inhomogeneous universe","author":"Clarkson","year":"2011","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib603","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.100.191302","type":"journal-article","article-title":"A Test of the Copernican Principle","volume":"100","author":"Caldwell","year":"2008","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib604","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.83.103515","type":"journal-article","article-title":"Precision cosmology defeats void models for acceleration","volume":"83","author":"Moss","year":"2011","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib605","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.84.123508","type":"journal-article","article-title":"Can decaying modes save void models for acceleration?","volume":"84","author":"Zibin","year":"2011","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib606","doi-asserted-by":"publisher","first-page":"319","DOI":"10.1086\/147385","type":"journal-article","article-title":"The change of redshift and apparent luminosity of galaxies due to the deceleration of selected expanding Universes","volume":"136","author":"Sandage","year":"1962","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib607","first-page":"334","type":"journal-article","article-title":"Appendix to the change of redshift and apparent luminosity of galaxies due to the deceleration of selected expanding Universes","volume":"136","author":"McVittie","year":"1962","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib608","doi-asserted-by":"publisher","first-page":"L111","DOI":"10.1086\/311375","type":"journal-article","article-title":"Direct measurement of cosmological parameters from the cosmic deceleration of extragalactic objects","volume":"499","author":"Loeb","year":"1998","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib609","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.76.063508","type":"journal-article","article-title":"Testing the \u039b cold dark matter model (and more) with the time evolution of the redshift","volume":"76","author":"Lake","year":"2007","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib610","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.77.021301","type":"journal-article","article-title":"Time drift of cosmological redshifts and its variance","volume":"77","author":"Uzan","year":"2008","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib611","doi-asserted-by":"publisher","first-page":"81","DOI":"10.1016\/j.physletb.2007.11.094","type":"journal-article","article-title":"Peculiar acceleration","volume":"660","author":"Amendola","year":"2008","journal-title":"Phys. Lett. B"},{"key":"cqgacbefcbib612","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.100.191303","type":"journal-article","article-title":"Time Drift of Cosmological Redshifts as a Test of the Copernican Principle","volume":"100","author":"Uzan","year":"2008","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib613","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.83.043527","type":"journal-article","article-title":"Redshift drift in Lema\u00eetre-Tolman-Bondi void universes","volume":"83","author":"Yoo","year":"2011","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib614","doi-asserted-by":"publisher","first-page":"JCAP01(2016)009","DOI":"10.1088\/1475-7516\/2016\/01\/009","type":"journal-article","article-title":"Redshift drift in an inhomogeneous universe: averaging and the backreaction conjecture","author":"Koksbang","year":"2016","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib615","doi-asserted-by":"publisher","first-page":"JCAP10(2019)036","DOI":"10.1088\/1475-7516\/2019\/10\/036","type":"journal-article","article-title":"Another look at redshift drift and the backreaction conjecture","author":"Koksbang","year":"2019","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib616","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.123527","type":"journal-article","article-title":"Redshift drift cosmography for model-independent cosmological inference","volume":"104","author":"Heinesen","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib617","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.102.151302","type":"journal-article","article-title":"Possibility of Detecting Anisotropic Expansion of the Universe by Very Accurate Astrometry Measurements","volume":"102","author":"Quercellini","year":"2009","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib618","doi-asserted-by":"publisher","first-page":"JCAP09(2011)035","DOI":"10.1088\/1475-7516\/2011\/09\/035","type":"journal-article","article-title":"Testing homogeneity with the fossil record of galaxies","author":"Heavens","year":"2011","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib619","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.82.023516","type":"journal-article","article-title":"Cosmic age test in inhomogeneous cosmological models mimicking \u039bCDM on the light cone","volume":"82","author":"Lan","year":"2010","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib620","doi-asserted-by":"publisher","first-page":"JCAP12(2008)002","DOI":"10.1088\/1475-7516\/2008\/12\/002","type":"journal-article","article-title":"Can the Copernican principle be tested using the cosmic neutrino background?","author":"Jia","year":"2008","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib621","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevLett.125.211101","type":"journal-article","article-title":"What is the price of abandoning dark matter? Cosmological constraints on alternative gravity theories","volume":"125","author":"Pardo","year":"2020","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib622","doi-asserted-by":"publisher","first-page":"73","DOI":"10.1140\/epjh\/e2017-80061-7","type":"journal-article","article-title":"One hundred years of the cosmological constant: from \u201csuperfluous stunt\u201d to dark energy","volume":"43","author":"O\u2019Raifeartaigh","year":"2018","journal-title":"Eur. Phys. J. H"},{"key":"cqgacbefcbib623","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.103.L081305","type":"journal-article","article-title":"Hubble sinks in the low-redshift swampland","volume":"103","author":"Banerjee","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib624","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.103.083533","type":"journal-article","article-title":"Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory","volume":"103","author":"Alam","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib625","first-page":"pp 1","type":"book","article-title":"Cosmological Models (Carg\u00e8se lectures 1998)","author":"Ellis","year":"1999"},{"key":"cqgacbefcbib626","first-page":"pp 142","type":"other","article-title":"Kosmologische Betrachtungen zur allgemeinen Relativit\u00e4tstheorie","author":"Einstein","year":"1917"},{"key":"cqgacbefcbib627","doi-asserted-by":"publisher","first-page":"213","DOI":"10.1073\/pnas.18.3.213","type":"journal-article","article-title":"On the Relation between the expansion and the mean density of the Universe","volume":"18","author":"Einstein","year":"1932","journal-title":"Proc. Natl Acad. Sci"},{"key":"cqgacbefcbib628","doi-asserted-by":"publisher","first-page":"A27","DOI":"10.1051\/0004-6361\/201321556","type":"journal-article","article-title":"Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove","volume":"571","author":"Collaboration","year":"2014","journal-title":"Astron. Astrophys."},{"key":"cqgacbefcbib629","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.063503","type":"journal-article","article-title":"Disentangling Doppler modulation, aberration and the temperature dipole in the CMB","volume":"104","author":"Ferreira","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib630","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2022\/10\/019","type":"preprint","article-title":"Galaxy number-count dipole and superhorizon fluctuations","author":"Dom\u00e8nech","year":"2022"},{"key":"cqgacbefcbib631","doi-asserted-by":"publisher","first-page":"L11","DOI":"10.1093\/mnrasl\/slac045","type":"journal-article","article-title":"Probing the rest-frame of the Universe with the near-IR cosmic infrared background","volume":"515","author":"Kashlinsky","year":"2022","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib632","doi-asserted-by":"publisher","first-page":"419","DOI":"10.1086\/148307","type":"journal-article","article-title":"A measurement of excess antenna temperature at 4080 Mc\/s","volume":"142","author":"Penzias","year":"1965","journal-title":"Astrophys. J."},{"key":"cqgacbefcbib633","doi-asserted-by":"publisher","first-page":"557","DOI":"10.1103\/PhysRevLett.18.557","type":"journal-article","article-title":"Isotropy and homogeneity of the Universe from measurements of the cosmic microwave background","volume":"18","author":"Partridge","year":"1967","journal-title":"Phys. Rev. Lett."},{"key":"cqgacbefcbib634","doi-asserted-by":"publisher","first-page":"L1","DOI":"10.1086\/186504","type":"journal-article","article-title":"Structure in the COBE differential microwave radiometer first-year maps","volume":"396","author":"Smoot","year":"1992","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib635","doi-asserted-by":"publisher","first-page":"L1","DOI":"10.1086\/310075","type":"journal-article","article-title":"Four-Year COBE DMR cosmic microwave background observations: maps and basic results","volume":"464","author":"Bennett","year":"1996","journal-title":"Astrophys. J. Lett."},{"key":"cqgacbefcbib636","doi-asserted-by":"publisher","first-page":"JCAP12(2020)045","DOI":"10.1088\/1475-7516\/2020\/12\/045","type":"journal-article","article-title":"The atacama cosmology telescope: a measurement of the cosmic microwave background power spectra at 98 and 150 GHz","author":"Choi","year":"2020","journal-title":"J. Cosmol. Astropart. Phys."},{"key":"cqgacbefcbib637","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.104.022003","type":"journal-article","article-title":"Measurements of the E-mode polarization and temperature-E-mode correlation of the CMB from SPT-3G 2018 data","volume":"104","author":"Dutcher","year":"2021","journal-title":"Phys. Rev. D"},{"key":"cqgacbefcbib638","doi-asserted-by":"publisher","first-page":"1335","DOI":"10.1111\/j.1365-2966.2008.13486.x","type":"journal-article","article-title":"A semi-empirical simulation of the extragalactic radio continuum sky for next generation radio telescopes","volume":"388","author":"Wilman","year":"2008","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib639","first-page":"p 32","type":"conference-proceedings","article-title":"Testing foundations of modern cosmology with SKA all-sky surveys","author":"Schwarz","year":"2015"},{"key":"cqgacbefcbib640","doi-asserted-by":"publisher","first-page":"357","DOI":"10.1016\/S1387-6473(03)00045-9","type":"journal-article","article-title":"The microJansky and nanoJansky population","volume":"47","author":"Windhorst","year":"2003","journal-title":"New Astron. Rev."},{"key":"cqgacbefcbib641","doi-asserted-by":"publisher","first-page":"1547","DOI":"10.1111\/j.1365-2966.2010.17789.x","type":"journal-article","article-title":"The microjansky and nanojansky radio sky: source population and multiwavelength properties","volume":"411","author":"Padovani","year":"2011","journal-title":"Mon. Not. R. Astron. Soc."},{"key":"cqgacbefcbib642","doi-asserted-by":"publisher","first-page":"87","DOI":"10.1088\/0004-6256\/150\/3\/87","type":"journal-article","article-title":"The host galaxies of Micro-Jansky radio sources","volume":"150","author":"Luchsinger","year":"2015","journal-title":"Astron. J."}],"container-title":["Classical and Quantum Gravity"],"original-title":[],"link":[{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc","content-type":"text\/html","content-version":"am","intended-application":"text-mining"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc\/pdf","content-type":"application\/pdf","content-version":"am","intended-application":"text-mining"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc","content-type":"text\/html","content-version":"vor","intended-application":"text-mining"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc\/pdf","content-type":"application\/pdf","content-version":"vor","intended-application":"text-mining"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc\/pdf","content-type":"application\/pdf","content-version":"am","intended-application":"syndication"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc\/pdf","content-type":"application\/pdf","content-version":"vor","intended-application":"syndication"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc\/pdf","content-type":"application\/pdf","content-version":"am","intended-application":"similarity-checking"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc\/pdf","content-type":"application\/pdf","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2025,9,6]],"date-time":"2025-09-06T13:52:14Z","timestamp":1757166734000},"score":1,"resource":{"primary":{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1361-6382\/acbefc"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2023,4,4]]},"references-count":644,"journal-issue":{"issue":"9","published-online":{"date-parts":[[2023,4,4]]},"published-print":{"date-parts":[[2023,5,4]]}},"URL":"https:\/\/doi.org\/10.1088\/1361-6382\/acbefc","relation":{},"ISSN":["0264-9381","1361-6382"],"issn-type":[{"value":"0264-9381","type":"print"},{"value":"1361-6382","type":"electronic"}],"subject":[],"published":{"date-parts":[[2023,4,4]]},"assertion":[{"value":"Is the observable Universe consistent with the cosmological principle?","name":"article_title","label":"Article Title"},{"value":"Classical and Quantum Gravity","name":"journal_title","label":"Journal Title"},{"value":"paper","name":"article_type","label":"Article Type"},{"value":"\u00a9 2023 IOP Publishing Ltd. All rights, including for text and data mining, AI training, and similar technologies, are reserved.","name":"copyright_information","label":"Copyright Information"},{"value":"2022-10-25","name":"date_received","label":"Date Received","group":{"name":"publication_dates","label":"Publication dates"}},{"value":"2023-02-24","name":"date_accepted","label":"Date Accepted","group":{"name":"publication_dates","label":"Publication dates"}},{"value":"2023-04-04","name":"date_epub","label":"Online publication date","group":{"name":"publication_dates","label":"Publication dates"}}]}}