{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,3,26]],"date-time":"2026-03-26T16:37:00Z","timestamp":1774543020146,"version":"3.50.1"},"reference-count":98,"publisher":"IOP Publishing","issue":"12","license":[{"start":{"date-parts":[[2021,12,21]],"date-time":"2021-12-21T00:00:00Z","timestamp":1640044800000},"content-version":"vor","delay-in-days":20,"URL":"https:\/\/iopscience.iop.org\/page\/copyright"},{"start":{"date-parts":[[2021,12,21]],"date-time":"2021-12-21T00:00:00Z","timestamp":1640044800000},"content-version":"tdm","delay-in-days":20,"URL":"https:\/\/iopscience.iop.org\/info\/page\/text-and-data-mining"}],"content-domain":{"domain":["iopscience.iop.org"],"crossmark-restriction":false},"short-container-title":["J. Cosmol. Astropart. Phys."],"published-print":{"date-parts":[[2021,12,1]]},"abstract":"<jats:title>Abstract<\/jats:title>\n               <jats:p>We investigate and quantify the impact of mixed (cold and\n  warm) dark matter models on large-scale structure observables.  In\n  this scenario, dark matter comes in two phases, a cold one (CDM) and\n  a warm one (WDM): the presence of the latter causes a suppression in\n  the matter power spectrum which is allowed by current constraints\n  and may be detected in present-day and upcoming surveys.  We run a\n  large set of N-body simulations in order to build an efficient and\n  accurate emulator to predict the aforementioned suppression with\n  percent precision over a wide range of values for the WDM mass,\n  M<jats:sub>wdm<\/jats:sub>, and its fraction with respect to the totality of dark\n  matter, f<jats:sub>wdm<\/jats:sub>.  The suppression in the matter power spectrum is\n  found to be independent of changes in the cosmological parameters at\n  the 2% level for k\u2272 10  h\/Mpc and z\u2264 3.5.  In the\n  same ranges, by applying a <jats:italic>baryonification<\/jats:italic> procedure on both\n  \u039bCDM  and CWDM simulations to account for the effect of feedback, we\n  find a similar level of agreement between the two scenarios.  We\n  examine the impact that such suppression has on weak lensing and\n  angular galaxy clustering power spectra.  Finally, we discuss the\n  impact of mixed dark matter on the shape of the halo mass function\n  and which analytical prescription yields the best agreement with\n  simulations. We provide the reader with an application to galaxy\n  cluster number\u00a0counts.<\/jats:p>","DOI":"10.1088\/1475-7516\/2021\/12\/044","type":"journal-article","created":{"date-parts":[[2021,12,21]],"date-time":"2021-12-21T15:24:32Z","timestamp":1640100272000},"page":"044","update-policy":"https:\/\/doi.org\/10.1088\/crossmark-policy","source":"Crossref","is-referenced-by-count":32,"title":["Mixed dark matter: matter power spectrum and halo mass function"],"prefix":"10.1088","volume":"2021","author":[{"given":"G.","family":"Parimbelli","sequence":"first","affiliation":[]},{"given":"G.","family":"Scelfo","sequence":"additional","affiliation":[]},{"given":"S.K.","family":"Giri","sequence":"additional","affiliation":[]},{"given":"A.","family":"Schneider","sequence":"additional","affiliation":[]},{"given":"M.","family":"Archidiacono","sequence":"additional","affiliation":[]},{"given":"S.","family":"Camera","sequence":"additional","affiliation":[]},{"given":"M.","family":"Viel","sequence":"additional","affiliation":[]}],"member":"266","published-online":{"date-parts":[[2021,12,21]]},"reference":[{"key":"b6a3e501f6a8c5828dc01bd372f8e39b4","doi-asserted-by":"publisher","first-page":"82","DOI":"10.1086\/307643","article-title":"Where are the missing Galactic satellites?","volume":"522","author":"Klypin","year":"1999","journal-title":"Astrophys. J."},{"key":"b8d632ebdf51e2c43e4e0601cc8151d79","doi-asserted-by":"publisher","first-page":"L19","DOI":"10.1086\/312287","article-title":"Dark matter substructure within galactic halos","volume":"524","author":"Moore","year":"1999","journal-title":"Astrophys. J. Lett."},{"key":"bfb90ae68a5f9686f41264188434f732f","doi-asserted-by":"publisher","first-page":"1147","DOI":"10.1046\/j.1365-8711.1999.03039.x","article-title":"Cold collapse and the core catastrophe","volume":"310","author":"Moore","year":"1999","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b0c8dab94c230410bf70b065bb81a1a02","doi-asserted-by":"publisher","first-page":"142","DOI":"10.1088\/0004-637X\/745\/2\/142","article-title":"On the assembly of the Milky Way dwarf satellites and their common mass scale","volume":"745","author":"Rashkov","year":"2012","journal-title":"Astrophys. J."},{"key":"b64312c8e8b29d7a3fcc0af16970d01eb","doi-asserted-by":"publisher","first-page":"1260","DOI":"10.1086\/587545","article-title":"Dark matter subhalos and the dwarf satellites of the Milky Way","volume":"679","author":"Madau","year":"2008","journal-title":"Astrophys. J."},{"key":"bee7ebf7739909ff5747cf0eed651e56e","doi-asserted-by":"publisher","first-page":"1995","DOI":"10.1111\/j.1365-2966.2009.16031.x","article-title":"On the origin and properties of Ultrafaint Milky Way Satellites in a LCDM Universe","volume":"402","author":"Maccio'","year":"2010","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b0bde9e7a16aa85f5c470a5a313fd719d","doi-asserted-by":"publisher","first-page":"4825","DOI":"10.1093\/mnras\/sty146","article-title":"Another baryon miracle? Testing solutions to the `missing dwarfs' problem","volume":"475","author":"Trujillo-Gomez","year":"2018","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b8935c1d58f101fda1b2f0ebcdc1c24d2","doi-asserted-by":"publisher","first-page":"3650","DOI":"10.1093\/mnras\/stv1504","article-title":"The unexpected diversity of dwarf galaxy rotation curves","volume":"452","author":"Oman","year":"2015","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bea8fe8904ab82064dc8f2b3e31710fd2","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1016\/j.physrep.2017.11.004","article-title":"Dark Matter Self-interactions and Small Scale Structure","volume":"730","author":"Tulin","year":"2018","journal-title":"Phys. Rept."},{"key":"b2ce5386933f04718e296a5ffc48aacb8","doi-asserted-by":"publisher","first-page":"1169","DOI":"10.1111\/j.1365-2966.2009.15004.x","article-title":"A constant dark matter halo surface density in galaxies","volume":"397","author":"Donato","year":"2009","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b9cca2bfd8cca64cdf11c5aca5f5ba485","article-title":"The Nature of dark matter","author":"Moore","year":"1994"},{"key":"b23998dac927cd7c48f80440a2683559b","doi-asserted-by":"publisher","first-page":"665","DOI":"10.1111\/j.1365-2966.2005.09601.x","article-title":"Cusps in cold dark matter haloes","volume":"364","author":"Diemand","year":"2005","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bc536f5ebb25940822d72093c3c134079","doi-asserted-by":"publisher","first-page":"1105","DOI":"10.1111\/j.1365-2966.2012.21284.x","article-title":"Cores in warm dark matter haloes: a Catch 22 problem","volume":"424","author":"Maccio","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b056cc0c71d0129d48104c28b7910a68a","doi-asserted-by":"publisher","first-page":"L40","DOI":"10.1111\/j.1745-3933.2011.01074.x","article-title":"Too big to fail? The puzzling darkness of massive Milky Way subhaloes","volume":"415","author":"Boylan-Kolchin","year":"2011","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"ba1652f03d435b26e2d4e60decf87e8b0","doi-asserted-by":"publisher","first-page":"2318","DOI":"10.1111\/j.1365-2966.2011.20200.x","article-title":"The Haloes of Bright Satellite Galaxies in a Warm Dark Matter Universe","volume":"420","author":"Lovell","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b1c4b40e2cee3d9d90af4224e13247436"},{"key":"bed2b9f59dfa5a815d01cc5b8e92f0247","doi-asserted-by":"publisher","first-page":"12249","DOI":"10.1073\/pnas.1308716112","article-title":"Cold dark matter: controversies on small scales","volume":"112","author":"Weinberg","year":"2015","journal-title":"Proc. Nat. Acad. Sci."},{"key":"b77a1be2bc4d149a6236c8fc59f47b754","doi-asserted-by":"publisher","first-page":"1975","DOI":"10.1111\/j.1365-2966.2010.17576.x","article-title":"Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies","volume":"410","author":"Wadepuhl","year":"2011","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b93b42e347b80857e89ef1d33b3f12175","doi-asserted-by":"publisher","first-page":"3304","DOI":"10.1111\/j.1365-2966.2011.19971.x","article-title":"The Baryons in the Milky Way Satellites","volume":"419","author":"Parry","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b3b0872cece71d6cf739d33624e59796d","doi-asserted-by":"publisher","first-page":"1231","DOI":"10.1111\/j.1365-2966.2012.20696.x","article-title":"Cuspy No More: How Outflows Affect the Central Dark Matter and Baryon Distribution in Lambda CDM Galaxies","volume":"422","author":"Governato","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bd1cbf5be02bad229366ac6a93c325dbb","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1016\/j.physrep.2018.07.003","article-title":"Gravitational probes of dark matter physics","volume":"761","author":"Buckley","year":"2018","journal-title":"Phys. Rept."},{"key":"b2ec0e7cc0902830473053b6a7a0162c1","doi-asserted-by":"publisher","first-page":"51","DOI":"10.1038\/s41586-018-0542-z","article-title":"A new era in the search for dark matter","volume":"562","author":"Bertone","year":"2018","journal-title":"Nature"},{"key":"b1b8fff85b79ccfdd6fba160b969ae637","doi-asserted-by":"publisher","first-page":"3403","DOI":"10.1093\/mnras\/staa2579","article-title":"ETHOS \u2013 an effective parametrization and classification for structure formation: the non-linear regime at z \u2273 5","volume":"498","author":"Bohr","year":"2020","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b76563028dde3f73bfce7a8fe30d40952","article-title":"Axion Dark Matter: What is it and Why Now?","author":"Chadha-Day","year":"2021"},{"key":"b674225e2ca0adb569d0c3442ce375ac9","doi-asserted-by":"publisher","first-page":"93","DOI":"10.1086\/321541","article-title":"Halo formation in warm dark matter models","volume":"556","author":"Bode","year":"2001","journal-title":"Astrophys. J."},{"key":"b563e398e36d0234a4b094a0c4f34510f","doi-asserted-by":"publisher","first-page":"453","DOI":"10.1016\/0550-3213(84)90461-9","article-title":"Supersymmetric Relics from the Big Bang","volume":"238","author":"Ellis","year":"1984","journal-title":"Nucl. Phys. B"},{"key":"bf2f24de260eec692c15943f14d743b47","doi-asserted-by":"publisher","first-page":"289","DOI":"10.1016\/0370-2693(93)91434-O","article-title":"Cosmological constraints on the light stable gravitino","volume":"303","author":"Moroi","year":"1993","journal-title":"Phys. Lett. B"},{"key":"b580840ff3a27d838160045bca523205f","doi-asserted-by":"publisher","first-page":"055","DOI":"10.1088\/1126-6708\/2008\/12\/055","article-title":"Is gravitino still a warm dark matter candidate?","volume":"12","author":"Gorbunov","year":"2008","journal-title":"JHEP"},{"key":"b3d6a921b7ea05a33803680555cac3c62","doi-asserted-by":"publisher","first-page":"17","DOI":"10.1103\/PhysRevLett.72.17","article-title":"Sterile-neutrinos as dark matter","volume":"72","author":"Dodelson","year":"1994","journal-title":"Phys. Rev. Lett."},{"key":"bfd6e643971df07445698d00c8ffaa163","doi-asserted-by":"publisher","first-page":"414","DOI":"10.1016\/j.physletb.2006.06.063","article-title":"The nuMSM, inflation, and dark matter","volume":"639","author":"Shaposhnikov","year":"2006","journal-title":"Phys. Lett. B"},{"key":"bbce5e8e24f8186b50163a3e98b0bbdde","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.96.023522","article-title":"New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman-\u03b1 forest data","volume":"96","author":"Ir\u0161i\u010d","year":"2017","journal-title":"Phys. Rev. D"},{"key":"b8dba3a8590a38687da14082706b50799","doi-asserted-by":"publisher","first-page":"6077","DOI":"10.1093\/mnras\/stz3480","article-title":"Warm dark matter chills out: constraints on the halo mass function and the free-streaming length of dark matter with eight quadruple-image strong gravitational lenses","volume":"491","author":"Gilman","year":"2020","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b52273571a77e116e9ee12baa7f673fea","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2021\/08\/062","article-title":"Constraints on the properties of warm dark matter using the satellite galaxies of the Milky Way","volume":"08","author":"Newton","year":"2021","journal-title":"JCAP"},{"key":"b57e5839d40e83f4402a0c58d696ad53d","doi-asserted-by":"publisher","first-page":"4","DOI":"10.1093\/mnras\/stab1960","article-title":"Joint constraints on thermal relic dark matter from strong gravitational lensing, the Lyman-\u03b1 forest, and Milky Way satellites","volume":"506","author":"Enzi","year":"2021","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b51713ba75e5baa2db35e525d9d7e66f5","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2013\/03\/014","article-title":"Hints on the Nature of Dark Matter from the Properties of Milky Way Satellites","volume":"03","author":"Anderhalden","year":"2013","journal-title":"JCAP"},{"key":"bfe743ec72c6121e085340176555a9d04","doi-asserted-by":"publisher","first-page":"882","DOI":"10.1093\/mnras\/sts078","article-title":"The inner structure of haloes in Cold+Warm dark matter models","volume":"428","author":"Maccio","year":"2013","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b88aec81a436046f2c83f958378116ea9","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2009\/05\/012","article-title":"Lyman-alpha constraints on warm and on warm-plus-cold dark matter models","volume":"05","author":"Boyarsky","year":"2009","journal-title":"JCAP"},{"key":"b0da0b2a83a7b6925678a14f17b7aaec7","doi-asserted-by":"publisher","first-page":"306","DOI":"10.1088\/0067-0049\/180\/2\/306","article-title":"Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data","volume":"180","author":"Dunkley","year":"2009","journal-title":"Astrophys. J. Suppl."},{"key":"b0608107cd97562429dcff06cc31a6291","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2017\/06\/008","article-title":"Cold dark matter plus not-so-clumpy dark relics","volume":"06","author":"Diamanti","year":"2017","journal-title":"JCAP"},{"key":"b5e1f8cf50f91e4132e41c7b5430665d2","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.94.023522","article-title":"Constraints on mixed dark matter from anomalous strong lens systems","volume":"94","author":"Kamada","year":"2016","journal-title":"Phys. Rev. D"},{"key":"bacae96fcca5be0b92d86de6f800fb2cc","doi-asserted-by":"publisher","first-page":"50","DOI":"10.1111\/j.1365-2966.2011.19910.x","article-title":"The Non-Linear Matter Power Spectrum in Warm Dark Matter Cosmologies","volume":"421","author":"Viel","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b0fb700e96eca798728f7e71784373676"},{"key":"bc5df37e40bf1641ba1624bc6dc18ef87","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2019\/03\/020","article-title":"Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation","volume":"03","author":"Schneider","year":"2019","journal-title":"JCAP"},{"key":"b3e38ee5056fd93d78f802418cb4153e5","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2015\/12\/049","article-title":"A new method to quantify the effects of baryons on the matter power spectrum","volume":"12","author":"Schneider","year":"2015","journal-title":"JCAP"},{"key":"b5017e911b16c7294fbe524d1b7827960","doi-asserted-by":"publisher","first-page":"1573","DOI":"10.1093\/mnras\/stt829","article-title":"Halo Mass Function and the Free Streaming Scale","volume":"433","author":"Schneider","year":"2013","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bb0256c6c63c8fb78c301a5b9ff55fc10","doi-asserted-by":"publisher","first-page":"3117","DOI":"10.1093\/mnras\/stv1169","article-title":"Structure formation with suppressed small-scale perturbations","volume":"451","author":"Schneider","year":"2015","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bdbb736fd7e36d3ef2cf68702750686ee","doi-asserted-by":"publisher","first-page":"629","DOI":"10.1038\/nature03597","article-title":"Simulating the joint evolution of quasars, galaxies and their large-scale distribution","volume":"435","author":"Springel","year":"2005","journal-title":"Nature"},{"key":"bbb2ed74a3e57d1f2039562603115f090","article-title":"The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview","author":"Lesgourgues","year":"2011"},{"key":"bfe778f16445043dd34f9507e79ada7d2","doi-asserted-by":"publisher","first-page":"109","DOI":"10.1088\/0004-637X\/762\/2\/109","article-title":"The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores","volume":"762","author":"Behroozi","year":"2013","journal-title":"Astrophys. J."},{"key":"bde7c29f76755f817c8539b925cd9189e","doi-asserted-by":"publisher","first-page":"300","DOI":"10.1093\/mnras\/stt2431","article-title":"The properties of warm dark matter haloes","volume":"439","author":"Lovell","year":"2014","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bf3dad91e27ea9f695a6cb32cf333c493","doi-asserted-by":"publisher","first-page":"684","DOI":"10.1111\/j.1365-2966.2012.21252.x","article-title":"Nonlinear Evolution of Cosmological Structures in Warm Dark Matter Models","volume":"424","author":"Schneider","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b3483ff058deda3dad41fa7925fab2dac"},{"key":"b2ed0b6ee4b0feb636d87d8c85e99e001"},{"key":"b635ffbfa17d79b89ad0a986849de7144","doi-asserted-by":"publisher","first-page":"5869","DOI":"10.1093\/mnras\/stab2018","article-title":"The BACCO simulation project: exploiting the full power of large-scale structure for cosmology","volume":"507","author":"Angulo","year":"2021","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bbf1191ab00aa47860e180353b800f795","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2019\/02\/050","article-title":"An Emulator for the Lyman-alpha Forest","volume":"02","author":"Bird","year":"2019","journal-title":"JCAP"},{"key":"b1374f75446f4ae1c7f992ba6c86fe5e8","doi-asserted-by":"publisher","first-page":"4728","DOI":"10.1093\/mnras\/staa487","article-title":"Constraining the intergalactic medium at z\u2248 9.1 using LOFAR Epoch of Reionization observations","volume":"493","author":"Ghara","year":"2020","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"be63bfc28d8391468cc0b9e16b93cc6b7"},{"key":"b478a63e21480ab05e7bbb0e1f789d8ca"},{"key":"b282ff8bc3f283eb2b1f26647d127f04f","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.71.063534","article-title":"Constraining warm dark matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest","volume":"71","author":"Viel","year":"2005","journal-title":"Phys. Rev. D"},{"key":"bd401c6db81b5c246fbfb47d14b87430a","doi-asserted-by":"publisher","first-page":"A140","DOI":"10.1051\/0004-6361\/202039063","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":"bd528ad93fef48d2b7d8c9a4693093f5c","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.102.023509","article-title":"Dark Energy Survey Year 1 Results: Cosmological constraints from cluster abundances and weak lensing","volume":"102","author":"Abbott","year":"2020","journal-title":"Phys. Rev. D"},{"key":"bf1f6e6565bbce4d2521e616dd426a0b5","article-title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","author":"Abbott","year":"2021"},{"key":"b3fcae46c77a1eb568adc5a7112b7db96","doi-asserted-by":"publisher","first-page":"151","DOI":"10.1093\/mnras\/sty099","article-title":"Statistical inconsistencies in the KiDS-450 data set","volume":"476","author":"Efstathiou","year":"2018","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bd37cd777979acbc68fd11bae5d9b5176","doi-asserted-by":"publisher","first-page":"4412","DOI":"10.1093\/mnras\/stx1820","article-title":"KiDS-450: The tomographic weak lensing power spectrum and constraints on cosmological parameters","volume":"471","author":"K\u00f6hlinger","year":"2017","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b5ed6492466eccae0602e42227bc6b89f","doi-asserted-by":"publisher","first-page":"1454","DOI":"10.1093\/mnras\/stw2805","article-title":"KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing","volume":"465","author":"Hildebrandt","year":"2017","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b5aadbe25699ab70912538e726a66bf8f","doi-asserted-by":"publisher","first-page":"3024","DOI":"10.1093\/mnras\/stx258","article-title":"Lensing is Low: Cosmology, Galaxy Formation, or New Physics?","volume":"467","author":"Leauthaud","year":"2017","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b911ad02bb011fae37a41d962d55821d5","doi-asserted-by":"publisher","first-page":"A191","DOI":"10.1051\/0004-6361\/202038071","article-title":"Euclid preparation: VII. Forecast validation for Euclid cosmological probes","volume":"642","author":"Blanchard","year":"2020","journal-title":"Astron. Astrophys."},{"key":"bd0eb4a58550144ffe86438713c6179f9","doi-asserted-by":"publisher","first-page":"3649","DOI":"10.1111\/j.1365-2966.2011.18981.x","article-title":"The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology","volume":"415","author":"van Daalen","year":"2011","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b311678bcaaf13942decc3b2a65e4e859","doi-asserted-by":"publisher","first-page":"2997","DOI":"10.1093\/mnras\/stu482","article-title":"The impact of baryonic processes on the two-point correlation functions of galaxies, subhaloes and matter","volume":"440","author":"van Daalen","year":"2014","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b0832474a807b7bfd03dfcd0d9ffc69ed","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2019\/01\/010","article-title":"On the degeneracy between baryon feedback and massive neutrinos as probed by matter clustering and weak lensing","volume":"01","author":"Parimbelli","year":"2019","journal-title":"JCAP"},{"key":"bc07a9469cce0a4735dcc7524f2957ef3","doi-asserted-by":"publisher","first-page":"2020","DOI":"10.1111\/j.1365-2966.2011.19385.x","article-title":"Quantifying the effect of baryon physics on weak lensing tomography","volume":"417","author":"Semboloni","year":"2011","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b479c642bce374370e85ce83e3d2d7318","doi-asserted-by":"publisher","first-page":"1652","DOI":"10.1093\/mnras\/stz1714","article-title":"Modelling baryonic physics in future weak lensing surveys","volume":"488","author":"Huang","year":"2019","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b26827418e1b2557bc0eae4f2f7a91a48","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2020\/04\/019","article-title":"Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix","volume":"04","author":"Schneider","year":"2020","journal-title":"JCAP"},{"key":"b25faba95d25266114df833b690ee9509","doi-asserted-by":"publisher","first-page":"A100","DOI":"10.1051\/0004-6361\/202039835","article-title":"Euclid: Impact of non-linear and baryonic feedback prescriptions on cosmological parameter estimation from weak lensing cosmic shear","volume":"649","author":"Martinelli","year":"2021","journal-title":"Astron. Astrophys."},{"key":"b7bd619fad1cc49a68571855df653ff35","doi-asserted-by":"publisher","first-page":"1212","DOI":"10.1093\/mnras\/stv646","article-title":"Baryons, Neutrinos, Feedback and Weak Gravitational Lensing","volume":"450","author":"Harnois-D\u00e9raps","year":"2015","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b5e78bed8f2a74827c67f97c156be9dee","doi-asserted-by":"publisher","first-page":"227","DOI":"10.1093\/mnras\/stx1469","article-title":"The separate and combined effects of baryon physics and neutrino free-streaming on large-scale structure","volume":"471","author":"Mummery","year":"2017","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"baf5bb204ee53f7601509e99bc6e803c7","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2016\/04\/047","article-title":"Matter power spectrum and the challenge of percent accuracy","volume":"04","author":"Schneider","year":"2016","journal-title":"JCAP"},{"key":"b2c56a21c62be1434e0c4f98099197bf1","doi-asserted-by":"publisher","first-page":"2126","DOI":"10.1093\/mnras\/stx2082","article-title":"Precision calculations of the cosmic shear power spectrum projection","volume":"472","author":"Kilbinger","year":"2017","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b87943e605ff2052429a4aeb1d8ffb017","doi-asserted-by":"publisher","first-page":"A70","DOI":"10.1051\/0004-6361\/202038313","article-title":"Euclid: The importance of galaxy clustering and weak lensing cross-correlations within the photometric Euclid survey","volume":"643","author":"Tutusaus","year":"2020","journal-title":"Astron. Astrophys."},{"key":"b9d49e1cef80e897179d52eeec57d6798","doi-asserted-by":"publisher","first-page":"A26","DOI":"10.1051\/0004-6361\/201015621","article-title":"Constraints on intrinsic alignment contamination of weak lensing surveys using the MegaZ-LRG sample","volume":"527","author":"Joachimi","year":"2011","journal-title":"Astron. Astrophys."},{"key":"b663e16880ec7fe937c9f3bb2f9a521a5","doi-asserted-by":"publisher","first-page":"444","DOI":"10.1088\/1367-2630\/9\/12\/444","article-title":"Dark energy constraints from cosmic shear power spectra: impact of intrinsic alignments on photometric redshift requirements","volume":"9","author":"Bridle","year":"2007","journal-title":"New J. Phys."},{"key":"b16bac1ce2db54843437eb29d7ae8267a","doi-asserted-by":"publisher","DOI":"10.1093\/mnras\/stab082","article-title":"HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback","author":"Mead","year":"2020"},{"key":"b7dd113bfe84f264140c81c6f7fe8dc43","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2018\/06\/015","article-title":"Complete super-sample lensing covariance in the response approach","volume":"06","author":"Barreira","year":"2018","journal-title":"JCAP"},{"key":"b7ab9ff32c3f1e5a6aba654fe418bb0f6","doi-asserted-by":"publisher","first-page":"2100","DOI":"10.1093\/mnras\/stx1261","article-title":"cosmolike \u2013 cosmological likelihood analyses for photometric galaxy surveys","volume":"470","author":"Krause","year":"2017","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bee232e8ebe9b9262685f801170f7a958","doi-asserted-by":"publisher","first-page":"440","DOI":"10.1086\/170520","article-title":"Excursion set mass functions for hierarchical Gaussian fluctuations","volume":"379","author":"Bond","year":"1991","journal-title":"Astrophys. J."},{"key":"bc17880cc11e2fceccfef809bc14f7e9d","doi-asserted-by":"crossref","first-page":"627","DOI":"10.1093\/mnras\/262.3.627","article-title":"Merger rates in hierarchical models of galaxy formation","volume":"262","author":"Lacey","year":"1993","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b62a3dafb10572f4bb56fa0b6e518a593","doi-asserted-by":"publisher","first-page":"L102","DOI":"10.1111\/j.1745-3933.2012.01266.x","article-title":"One step beyond: The excursion set approach with correlated steps","volume":"423","author":"Musso","year":"2012","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b1013e3d8701ec1a94d17c1d598dced8b","doi-asserted-by":"publisher","first-page":"425","DOI":"10.1086\/152650","article-title":"Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation","volume":"187","author":"Press","year":"1974","journal-title":"Astrophys. J."},{"key":"b2424af46bfd2dd92327d03ed61325f1b","doi-asserted-by":"publisher","first-page":"119","DOI":"10.1046\/j.1365-8711.1999.02692.x","article-title":"Large scale bias and the peak background split","volume":"308","author":"Sheth","year":"1999","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b70184791982f8f0cafaa3b0ae727dd6f","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1046\/j.1365-8711.2001.04006.x","article-title":"Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes","volume":"323","author":"Sheth","year":"2001","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"bc2ab11c8c15141a330c1352ec75d206e","doi-asserted-by":"publisher","first-page":"1774","DOI":"10.1093\/mnras\/sts159","article-title":"Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter","volume":"428","author":"Benson","year":"2013","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b50c0d76d48097a46311bcc0adcb742b0","doi-asserted-by":"publisher","DOI":"10.1088\/1475-7516\/2018\/04\/010","article-title":"A new smooth-k space filter approach to calculate halo abundances","volume":"04","author":"Leo","year":"2018","journal-title":"JCAP"},{"key":"b0fb6de128d018b46ddb2a6b2647680a4","doi-asserted-by":"publisher","first-page":"3773","DOI":"10.1093\/mnras\/stab1116","article-title":"Dark acoustic oscillations: imprints on the matter power spectrum and the halo mass function","volume":"504","author":"Schaeffer","year":"2021","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b28df8f6c85d3cee0c7c12794a0a2cf90","doi-asserted-by":"publisher","first-page":"483","DOI":"10.1086\/306436","article-title":"Cluster abundance constraints on quintessence models","volume":"508","author":"Wang","year":"1998","journal-title":"Astrophys. J."},{"key":"bfe54cfe59fdfa71bff9a1a6e854eefee","doi-asserted-by":"publisher","first-page":"409","DOI":"10.1146\/annurev-astro-081710-102514","article-title":"Cosmological Parameters from Observations of Galaxy Clusters","volume":"49","author":"Allen","year":"2011","journal-title":"Ann. Rev. Astron. Astrophys."},{"key":"b3b4b47c0161f2b77920f7d213c5bcbd5","doi-asserted-by":"publisher","first-page":"1764","DOI":"10.1093\/mnras\/stw630","article-title":"Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey","volume":"459","author":"Sartoris","year":"2016","journal-title":"Mon. Not. Roy. Astron. Soc."},{"key":"b9f87c4aa470b4745adf84a67be259c2f","doi-asserted-by":"publisher","DOI":"10.1103\/PhysRevD.70.043504","article-title":"Self - calibration of cluster dark energy studies: Counts in cells","volume":"70","author":"Lima","year":"2004","journal-title":"Phys. Rev. D"},{"key":"b87d711416bbee8f461bb30f665c912c0","doi-asserted-by":"publisher","first-page":"A20","DOI":"10.1051\/0004-6361\/202038465","article-title":"Impact of systematics on cosmological parameters from future galaxy cluster surveys","volume":"643","author":"Salvati","year":"2020","journal-title":"Astron. Astrophys."}],"container-title":["Journal of Cosmology and Astroparticle Physics"],"original-title":[],"link":[{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1475-7516\/2021\/12\/044","content-type":"text\/html","content-version":"vor","intended-application":"text-mining"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1475-7516\/2021\/12\/044\/pdf","content-type":"application\/pdf","content-version":"vor","intended-application":"text-mining"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1475-7516\/2021\/12\/044\/pdf","content-type":"application\/pdf","content-version":"vor","intended-application":"syndication"},{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1475-7516\/2021\/12\/044\/pdf","content-type":"application\/pdf","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2022,2,17]],"date-time":"2022-02-17T14:11:49Z","timestamp":1645107109000},"score":1,"resource":{"primary":{"URL":"https:\/\/iopscience.iop.org\/article\/10.1088\/1475-7516\/2021\/12\/044"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2021,12,1]]},"references-count":98,"journal-issue":{"issue":"12","published-online":{"date-parts":[[2021,12,21]]},"published-print":{"date-parts":[[2021,12,1]]}},"URL":"https:\/\/doi.org\/10.1088\/1475-7516\/2021\/12\/044","relation":{},"ISSN":["1475-7516"],"issn-type":[{"value":"1475-7516","type":"electronic"}],"subject":[],"published":{"date-parts":[[2021,12,1]]},"assertion":[{"value":"Mixed dark matter: matter power spectrum and halo mass function","name":"article_title","label":"Article Title"},{"value":"Journal of Cosmology and Astroparticle Physics","name":"journal_title","label":"Journal Title"},{"value":"paper","name":"article_type","label":"Article Type"},{"value":"\u00a9 2021 IOP Publishing Ltd and Sissa Medialab","name":"copyright_information","label":"Copyright Information"},{"value":"2021-06-15","name":"date_received","label":"Date Received","group":{"name":"publication_dates","label":"Publication dates"}},{"value":"2021-11-23","name":"date_accepted","label":"Date Accepted","group":{"name":"publication_dates","label":"Publication dates"}},{"value":"2021-12-21","name":"date_epub","label":"Online publication date","group":{"name":"publication_dates","label":"Publication dates"}}]}}