{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,3,18]],"date-time":"2026-03-18T04:45:45Z","timestamp":1773809145970,"version":"3.50.1"},"reference-count":227,"publisher":"Frontiers Media SA","license":[{"start":{"date-parts":[[2024,3,15]],"date-time":"2024-03-15T00:00:00Z","timestamp":1710460800000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"content-domain":{"domain":["frontiersin.org"],"crossmark-restriction":true},"short-container-title":["Front. Astron. Space Sci."],"abstract":"<jats:p>While the mission\u2019s primary goal was focused on exoplanet detection and characterization, <jats:italic>Kepler<\/jats:italic> made and continues to make extraordinary advances in stellar physics. Stellar rotation and magnetic activity are no exceptions. <jats:italic>Kepler<\/jats:italic> allowed for these properties to be determined for tens of thousands of stars from the main sequence up to the red giant branch. From photometry, this can be achieved by investigating the brightness fluctuations due to active regions, which cause surface inhomogeneities, or through asteroseismology as oscillation modes are sensitive to rotation and magnetic fields. This review summarizes the rotation and magnetic activity properties of the single main-sequence solar-like stars within the <jats:italic>Kepler<\/jats:italic> field. We contextualize the <jats:italic>Kepler<\/jats:italic> sample by comparing it to known transitions in the stellar rotation and magnetic-activity evolution, such as the convergence to the rotation sequence (from the saturated to the unsaturated regime of magnetic activity) and the Vaughan-Preston gap. While reviewing the publicly available data, we also uncover one interesting finding related to the intermediate-rotation gap seen in <jats:italic>Kepler<\/jats:italic> and other surveys. We find evidence for this rotation gap in previous ground-based data for the X-ray luminosity. Understanding the complex evolution and interplay between rotation and magnetic activity in solar-like stars is crucial, as it sheds light on fundamental processes governing stellar evolution, including the evolution of our own Sun.<\/jats:p>","DOI":"10.3389\/fspas.2024.1356379","type":"journal-article","created":{"date-parts":[[2024,3,15]],"date-time":"2024-03-15T04:58:35Z","timestamp":1710478715000},"update-policy":"https:\/\/doi.org\/10.3389\/crossmark-policy","source":"Crossref","is-referenced-by-count":12,"title":["Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution"],"prefix":"10.3389","volume":"11","author":[{"given":"\u00c2ngela R. G.","family":"Santos","sequence":"first","affiliation":[]},{"given":"Diego","family":"Godoy-Rivera","sequence":"additional","affiliation":[]},{"given":"Adam J.","family":"Finley","sequence":"additional","affiliation":[]},{"given":"Savita","family":"Mathur","sequence":"additional","affiliation":[]},{"given":"Rafael A.","family":"Garc\u00eda","sequence":"additional","affiliation":[]},{"given":"Sylvain N.","family":"Breton","sequence":"additional","affiliation":[]},{"given":"Anne-Marie","family":"Broomhall","sequence":"additional","affiliation":[]}],"member":"1965","published-online":{"date-parts":[[2024,3,15]]},"reference":[{"key":"B1","doi-asserted-by":"publisher","first-page":"35","DOI":"10.3847\/1538-4365\/ac4414","article-title":"The seventeenth data Release of the sloan digital sky surveys: complete Release of MaNGA, MaStar, and APOGEE-2 data","volume":"259","author":"Abdurro\u2019uf Accetta","year":"2022","journal-title":"ApJS"},{"key":"B2","doi-asserted-by":"publisher","first-page":"11","DOI":"10.1111\/j.1365-2966.2012.20802.x","article-title":"The rotation of field stars from CoRoT data","volume":"424","author":"Affer","year":"2012","journal-title":"MNRAS"},{"key":"B3","doi-asserted-by":"publisher","first-page":"108","DOI":"10.3847\/1538-4357\/ab6173","article-title":"The impact of metallicity on the evolution of the rotation and magnetic activity of sun-like stars","volume":"889","author":"Amard","year":"2020","journal-title":"ApJ"},{"key":"B4","doi-asserted-by":"publisher","first-page":"3481","DOI":"10.1093\/mnras\/staa3038","article-title":"Evidence for metallicity-dependent spin evolution in the Kepler field","volume":"499","author":"Amard","year":"2020","journal-title":"MNRAS"},{"key":"B5","doi-asserted-by":"publisher","first-page":"A27","DOI":"10.1051\/0004-6361\/202243462","article-title":"Gaia data Release 3. Analysis of the Gaia BP\/RP spectra using the general stellar parameterizer from photometry","volume":"674","author":"Andrae","year":"2023","journal-title":"A&A"},{"key":"B6","doi-asserted-by":"publisher","first-page":"1787","DOI":"10.1093\/mnras\/stv423","article-title":"Calibrating gyrochronology using Kepler asteroseismic targets","volume":"450","author":"Angus","year":"2015","journal-title":"MNRAS"},{"key":"B7","doi-asserted-by":"publisher","first-page":"90","DOI":"10.3847\/1538-3881\/ab91b2","article-title":"Exploring the evolution of stellar rotation using galactic kinematics","volume":"160","author":"Angus","year":"2020","journal-title":"AJ"},{"key":"B8","doi-asserted-by":"publisher","first-page":"A20","DOI":"10.1051\/0004-6361\/201323317","article-title":"Oscillation mode linewidths and heights of 23 main-sequence stars observed by Kepler","volume":"566","author":"Appourchaux","year":"2014","journal-title":"A&A"},{"key":"B9","doi-asserted-by":"publisher","first-page":"A134","DOI":"10.1051\/0004-6361\/201118496","article-title":"Oscillation mode linewidths of main-sequence and subgiant stars observed by Kepler","volume":"537","author":"Appourchaux","year":"2012","journal-title":"A&A"},{"key":"B10","first-page":"33","article-title":"Scientific objectives for a minisat: CoRoT","volume-title":"Proceedings of \u201cthe CoRoT mission pre-launch status - stellar seismology and planet finding\u201d (ESA SP-1306)","author":"Baglin","year":"2006"},{"key":"B11","doi-asserted-by":"publisher","first-page":"781","DOI":"10.1103\/RevModPhys.67.781","article-title":"Solar models with helium and heavy-element diffusion","volume":"67","author":"Bahcall","year":"1995","journal-title":"RMP"},{"key":"B12","doi-asserted-by":"publisher","first-page":"269","DOI":"10.1086\/175072","article-title":"Chromospheric variations in main-sequence stars","volume":"438","author":"Baliunas","year":"1995","journal-title":"ApJ"},{"key":"B13","doi-asserted-by":"publisher","first-page":"1281","DOI":"10.1111\/j.1365-2966.2006.10375.x","article-title":"Rotation speed and stellar axis inclination from p modes: how CoRoT would see other suns","volume":"369","author":"Ballot","year":"2006","journal-title":"MNRAS"},{"key":"B14","doi-asserted-by":"publisher","first-page":"2714","DOI":"10.1093\/mnras\/stu2651","article-title":"Flare stars across the H-R diagram","volume":"447","author":"Balona","year":"2015","journal-title":"MNRAS"},{"key":"B15","doi-asserted-by":"publisher","first-page":"2112","DOI":"10.1093\/mnras\/stz2808","article-title":"Evidence for spots on hot stars suggests major revision of stellar physics","volume":"490","author":"Balona","year":"2019","journal-title":"MNRAS"},{"key":"B16","doi-asserted-by":"publisher","first-page":"L145","DOI":"10.1086\/374681","article-title":"A connection between the morphology of the X-ray emission and rotation for solar-type stars in open clusters","volume":"586","author":"Barnes","year":"","journal-title":"ApJL"},{"key":"B17","doi-asserted-by":"publisher","first-page":"464","DOI":"10.1086\/367639","article-title":"On the rotational evolution of solar- and late-type stars, its magnetic origins, and the possibility of stellar gyrochronology","volume":"586","author":"Barnes","year":"","journal-title":"ApJ"},{"key":"B18","doi-asserted-by":"publisher","first-page":"1167","DOI":"10.1086\/519295","article-title":"Ages for illustrative field stars using gyrochronology: viability, limitations, and errors","volume":"669","author":"Barnes","year":"2007","journal-title":"ApJ"},{"key":"B19","doi-asserted-by":"publisher","first-page":"16","DOI":"10.3847\/0004-637X\/823\/1\/16","article-title":"Rotation periods for cool stars in the 4 Gyr old open cluster M67, the solar-stellar connection, and the applicability of gyrochronology to at least solar age","volume":"823","author":"Barnes","year":"2016","journal-title":"ApJ"},{"key":"B20","doi-asserted-by":"publisher","first-page":"L155","DOI":"10.1088\/2041-8205\/713\/2\/L155","article-title":"Photometric variability in kepler target stars: the sun among stars\u2014a first look","volume":"713","author":"Basri","year":"2010","journal-title":"ApJL"},{"key":"B21","doi-asserted-by":"publisher","first-page":"43","DOI":"10.1088\/0004-637X\/758\/1\/43","article-title":"Thinning of the sun\u2019s magnetic layer: the peculiar solar minimum could have been predicted","volume":"758","author":"Basu","year":"2012","journal-title":"ApJ"},{"key":"B22","doi-asserted-by":"publisher","first-page":"183","DOI":"10.3847\/1538-3881\/ac5683","article-title":"Five decades of chromospheric activity in 59 sun-like stars and new maunder minimum candidate hd 166620","volume":"163","author":"Baum","year":"2022","journal-title":"AJ"},{"key":"B23","doi-asserted-by":"publisher","first-page":"A125","DOI":"10.1051\/0004-6361\/201834594","article-title":"Latitudinal differential rotation in the solar analogues 16 Cygni A and B","volume":"623","author":"Bazot","year":"2019","journal-title":"A&A"},{"key":"B24","doi-asserted-by":"publisher","first-page":"1231","DOI":"10.1126\/science.aao6571","article-title":"Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars","volume":"361","author":"Benomar","year":"2018","journal-title":"Science"},{"key":"B25","doi-asserted-by":"publisher","first-page":"2654","DOI":"10.1093\/mnras\/stv1493","article-title":"Nearly uniform internal rotation of solar-like main-sequence stars revealed by space-based asteroseismology and spectroscopic measurements","volume":"452","author":"Benomar","year":"2015","journal-title":"MNRAS"},{"key":"B26","doi-asserted-by":"publisher","first-page":"486","DOI":"10.1086\/510482","article-title":"Chromospheric activity in G and K main-sequence stars, and what it tells us about stellar dynamos","volume":"657","author":"B\u00f6hm-Vitense","year":"2007","journal-title":"ApJ"},{"key":"B27","doi-asserted-by":"publisher","first-page":"L26","DOI":"10.3847\/2041-8213\/ac9c05","article-title":"On the origin of the dichotomy of stellar activity cycles","volume":"939","author":"Bonanno","year":"2022","journal-title":"ApJ"},{"key":"B28","doi-asserted-by":"publisher","first-page":"A108","DOI":"10.1051\/0004-6361\/201629518","article-title":"Chromospheric activity catalogue of 4454 cool stars. Questioning the active branch of stellar activity cycles","volume":"616","author":"Boro Saikia","year":"2018","journal-title":"A&A"},{"key":"B29","doi-asserted-by":"publisher","first-page":"977","DOI":"10.1126\/science.1185402","article-title":"Kepler planet-detection mission: introduction and first results","volume":"327","author":"Borucki","year":"2010","journal-title":"Science"},{"key":"B30","doi-asserted-by":"publisher","first-page":"L3","DOI":"10.3847\/2041-8213\/acc589","article-title":"The empirical limits of gyrochronology","volume":"947","author":"Bouma","year":"2023","journal-title":"ApJ"},{"key":"B31","doi-asserted-by":"publisher","first-page":"L51","DOI":"10.1086\/311297","article-title":"Time evolution of the magnetic activity cycle period","volume":"498","author":"Brandenburg","year":"1998","journal-title":"ApJL"},{"key":"B32","doi-asserted-by":"publisher","first-page":"A104","DOI":"10.1051\/0004-6361\/202346601","article-title":"In search of gravity mode signatures in main sequence solar-type stars observed by Kepler","volume":"679","author":"Breton","year":"2023","journal-title":"A&A"},{"key":"B33","doi-asserted-by":"publisher","first-page":"A125","DOI":"10.1051\/0004-6361\/202039947","article-title":"ROOSTER: a machine-learning analysis tool for Kepler stellar rotation periods","volume":"647","author":"Breton","year":"2021","journal-title":"A&A"},{"key":"B34","doi-asserted-by":"publisher","first-page":"1405","DOI":"10.1111\/j.1365-2966.2011.20123.x","article-title":"Quasi-biennial variations in helioseismic frequencies: can the source of the variation be localized?","volume":"420","author":"Broomhall","year":"2012","journal-title":"MNRAS"},{"key":"B35","doi-asserted-by":"publisher","first-page":"191","DOI":"10.1007\/s11214-014-0101-3","article-title":"The sun\u2019s interior structure and dynamics, and the solar cycle","volume":"186","author":"Broomhall","year":"2014","journal-title":"Space Sci. Rev."},{"key":"B36","doi-asserted-by":"publisher","first-page":"4300","DOI":"10.1093\/mnras\/stac1291","article-title":"Linking chromospheric activity and magnetic field properties for late-type dwarf stars","volume":"514","author":"Brown","year":"2022","journal-title":"MNRAS"},{"key":"B37","doi-asserted-by":"publisher","first-page":"101","DOI":"10.1088\/0004-637X\/789\/2\/101","article-title":"The metastable dynamo model of stellar rotational evolution","volume":"789","author":"Brown","year":"2014","journal-title":"ApJ"},{"key":"B38","doi-asserted-by":"publisher","first-page":"66","DOI":"10.3847\/1538-4357\/ac0635","article-title":"Brightness fluctuation spectra of sun-like stars. I. The mid-frequency continuum","volume":"916","author":"Brown","year":"2021","journal-title":"ApJ"},{"key":"B39","doi-asserted-by":"publisher","first-page":"4","DOI":"10.1007\/s41116-017-0007-8","article-title":"Magnetism, dynamo action and the solar-stellar connection","volume":"14","author":"Brun","year":"2017","journal-title":"Living Rev. Sol. Phys."},{"key":"B40","doi-asserted-by":"publisher","first-page":"21","DOI":"10.3847\/1538-4357\/ac469b","article-title":"Powering stellar magnetism: energy transfers in cyclic dynamos of sun-like stars","volume":"926","author":"Brun","year":"2022","journal-title":"ApJ"},{"key":"B41","doi-asserted-by":"publisher","first-page":"2165","DOI":"10.1093\/mnras\/stac2706","article-title":"Star-spots and magnetism: testing the activity paradigm in the Pleiades and M67","volume":"517","author":"Cao","year":"2022","journal-title":"MNRAS"},{"key":"B42","doi-asserted-by":"publisher","first-page":"A111","DOI":"10.1051\/0004-6361\/201629884","article-title":"Surface rotation of Kepler red giant stars","volume":"605","author":"Ceillier","year":"2017","journal-title":"A&A"},{"key":"B43","doi-asserted-by":"publisher","first-page":"L5","DOI":"10.1088\/2041-8205\/732\/1\/L5","article-title":"Evidence for the impact of stellar activity on the detectability of solar-like oscillations observed by kepler","volume":"732","author":"Chaplin","year":"2011","journal-title":"ApJL"},{"key":"B44","doi-asserted-by":"publisher","first-page":"32","DOI":"10.1046\/j.1365-8711.2000.03176.x","article-title":"Variations in the excitation and damping of low- solar p modes over the solar activity cycle","volume":"313","author":"Chaplin","year":"2000","journal-title":"MNRAS"},{"key":"B45","doi-asserted-by":"publisher","first-page":"1102","DOI":"10.1111\/j.1365-2966.2004.07998.x","article-title":"The solar cycle as seen by low-\u2113 p-mode frequencies: comparison with global and decomposed activity proxies","volume":"352","author":"Chaplin","year":"2004","journal-title":"MNRAS"},{"key":"B46","doi-asserted-by":"publisher","first-page":"47","DOI":"10.3847\/1538-4357\/ad159a","article-title":"TESS stellar rotation up to 80 days in the southern continuous viewing zone","volume":"962","author":"Claytor","year":"2023","journal-title":"ApJ"},{"key":"B47","doi-asserted-by":"publisher","first-page":"43","DOI":"10.3847\/1538-4357\/ab5c24","article-title":"Chemical evolution in the milky way: rotation-based ages for APOGEE-kepler cool dwarf stars","volume":"888","author":"Claytor","year":"2020","journal-title":"ApJ"},{"key":"B48","doi-asserted-by":"publisher","first-page":"190","DOI":"10.1088\/0004-637X\/757\/2\/190","article-title":"Asteroseismology of the open clusters NGC 6791, NGC 6811, and NGC 6819 from 19 Months of kepler photometry","volume":"757","author":"Corsaro","year":"2012","journal-title":"ApJ"},{"key":"B49","doi-asserted-by":"publisher","first-page":"49","DOI":"10.3847\/1538-4357\/ab2393","article-title":"A temporary epoch of stalled spin-down for low-mass stars: insights from NGC 6811 with Gaia and kepler","volume":"879","author":"Curtis","year":"2019","journal-title":"ApJ"},{"key":"B50","volume-title":"PyA: Python astronomy-related packages","author":"Czesla","year":"2019"},{"key":"B51","doi-asserted-by":"publisher","first-page":"23","DOI":"10.3847\/0004-637X\/829\/1\/23","article-title":"The kepler catalog of stellar flares","volume":"829","author":"Davenport","year":"2016","journal-title":"ApJ"},{"key":"B52","doi-asserted-by":"publisher","first-page":"16","DOI":"10.3847\/1538-4357\/835\/1\/16","article-title":"Rotating stars from kepler observed with Gaia DR1","volume":"835","author":"Davenport","year":"2017","journal-title":"ApJ"},{"key":"B53","doi-asserted-by":"publisher","first-page":"151","DOI":"10.3847\/1538-4357\/aae842","article-title":"Rotating stars from kepler observed with Gaia DR2","volume":"868","author":"Davenport","year":"2018","journal-title":"ApJ"},{"key":"B54","doi-asserted-by":"publisher","first-page":"114","DOI":"10.3847\/1538-4357\/ac6dd3","article-title":"Further evidence of modified spin-down in sun-like stars: pileups in the temperature-period distribution","volume":"933","author":"David","year":"2022","journal-title":"ApJ"},{"key":"B55","doi-asserted-by":"publisher","first-page":"2959","DOI":"10.1093\/mnras\/stu2331","article-title":"Asteroseismic inference on rotation, gyrochronology and planetary system dynamics of 16 Cygni","volume":"446","author":"Davies","year":"2015","journal-title":"MNRAS"},{"key":"B56","doi-asserted-by":"publisher","first-page":"A20","DOI":"10.1051\/0004-6361\/202244178","article-title":"Gaia Data Release 3. Rotational modulation and patterns of colour variation in solar-like variables","volume":"674","author":"Distefano","year":"2023","journal-title":"A&A"},{"key":"B57","first-page":"1135","article-title":"Zeeman-Doppler imaging of active stars. V. Sensitivity of maximum entropy magnetic maps to field orientation","volume":"326","author":"Donati","year":"1997","journal-title":"A&A"},{"key":"B58","doi-asserted-by":"publisher","first-page":"100","DOI":"10.3847\/1538-4357\/ab2468","article-title":"K2 rotation periods for low-mass hyads and a quantitative comparison of the distribution of slow rotators in the hyades and Praesepe","volume":"879","author":"Douglas","year":"2019","journal-title":"ApJ"},{"key":"B59","doi-asserted-by":"publisher","first-page":"118","DOI":"10.3847\/1538-4357\/ac90be","article-title":"A 4 Gyr M-dwarf gyrochrone from CFHT\/MegaPrime monitoring of the open cluster M67","volume":"938","author":"Dungee","year":"2022","journal-title":"ApJ"},{"key":"B60","unstructured":"Long-term variability of the sun in the context of solar-analog stars\n            EgelandR.\n          United StatesMontana state university2017"},{"key":"B61","doi-asserted-by":"publisher","first-page":"322","DOI":"10.1038\/345322a0","article-title":"Variation of low-order acoustic solar oscillations over the solar cycle","volume":"345","author":"Elsworth","year":"1990","journal-title":"Nature"},{"key":"B62","doi-asserted-by":"publisher","first-page":"23","DOI":"10.1088\/0004-6256\/142\/1\/23","article-title":"Stellar activity in the broadband ultraviolet","volume":"142","author":"Findeisen","year":"2011","journal-title":"AJ"},{"key":"B63","doi-asserted-by":"publisher","first-page":"A42","DOI":"10.1051\/0004-6361\/202245642","article-title":"Accounting for differential rotation in calculations of the sun\u2019s angular momentum-loss rate","volume":"674","author":"Finley","year":"2023","journal-title":"A&A"},{"key":"B64","doi-asserted-by":"publisher","first-page":"67","DOI":"10.3847\/1538-4357\/ab3729","article-title":"Solar angular momentum loss over the past several millennia","volume":"883","author":"Finley","year":"","journal-title":"ApJ"},{"key":"B65","doi-asserted-by":"publisher","first-page":"L30","DOI":"10.3847\/2041-8213\/ab4ff4","article-title":"Direct detection of solar angular momentum loss with the wind spacecraft","volume":"885","author":"Finley","year":"","journal-title":"ApJL"},{"key":"B66","doi-asserted-by":"publisher","first-page":"78","DOI":"10.3847\/1538-4357\/aaaab5","article-title":"The effect of combined magnetic geometries on thermally driven winds. ii. dipolar, quadrupolar, and octupolar topologies","volume":"854","author":"Finley","year":"2018","journal-title":"ApJ"},{"key":"B67","doi-asserted-by":"publisher","first-page":"125","DOI":"10.3847\/1538-4357\/aad7b6","article-title":"The effect of magnetic variability on stellar angular momentum loss. I. The solar wind torque during sunspot cycles 23 and 24","volume":"864","author":"Finley","year":"2018","journal-title":"ApJ"},{"key":"B68","doi-asserted-by":"publisher","first-page":"A110","DOI":"10.1051\/0004-6361\/201833587","article-title":"Spectroscopic membership for the populous 300 Myr-old open cluster NGC 3532","volume":"622","author":"Fritzewski","year":"2019","journal-title":"A&A"},{"key":"B69","doi-asserted-by":"publisher","first-page":"A103","DOI":"10.1051\/0004-6361\/202140896","article-title":"A detailed understanding of the rotation-activity relationship using the 300 Myr old open cluster NGC 3532","volume":"656","author":"Fritzewski","year":"","journal-title":"A&A"},{"key":"B70","doi-asserted-by":"publisher","first-page":"A60","DOI":"10.1051\/0004-6361\/202140894","article-title":"Rotation periods for cool stars in the open cluster NGC 3532. The transition from fast to slow rotation","volume":"652","author":"Fritzewski","year":"","journal-title":"A&A"},{"key":"B71","doi-asserted-by":"publisher","DOI":"10.1051\/0004-6361\/202243782","article-title":"Gaia Data Release 3: stellar multiplicity, a teaser for the hidden treasure","volume":"674","author":"Arenou","year":"2023","journal-title":"A&A"},{"key":"B72","doi-asserted-by":"publisher","first-page":"A1","DOI":"10.1051\/0004-6361\/202243940","article-title":"Gaia Data Release 3. Summary of the content and survey properties","volume":"674","author":"Vallenari","year":"2023","journal-title":"A&A"},{"key":"B73","doi-asserted-by":"publisher","first-page":"1006","DOI":"10.1086\/301488","article-title":"Spectroscopy and photometry of nearby young solar analogs","volume":"120","author":"Gaidos","year":"2000","journal-title":"AJ"},{"key":"B74","doi-asserted-by":"publisher","first-page":"A36","DOI":"10.1051\/0004-6361\/201321302","article-title":"Improved angular momentum evolution model for solar-like stars","volume":"556","author":"Gallet","year":"2013","journal-title":"A&A"},{"key":"B75","doi-asserted-by":"publisher","first-page":"A34","DOI":"10.1051\/0004-6361\/201423888","article-title":"Rotation and magnetism ofKeplerpulsating solar-like stars: towards asteroseismically calibrated age-rotation relations\u22c6","volume":"572","author":"Garc\u00eda","year":"","journal-title":"A&A"},{"key":"B76","doi-asserted-by":"publisher","first-page":"L12","DOI":"10.1051\/0004-6361\/202346933","article-title":"Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars. Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models","volume":"679","author":"Garc\u00eda","year":"2023","journal-title":"A&A"},{"key":"B77","doi-asserted-by":"publisher","first-page":"L6","DOI":"10.1111\/j.1745-3933.2011.01042.x","article-title":"Preparation of Kepler light curves for asteroseismic analyses","volume":"414","author":"Garc\u00eda","year":"2011","journal-title":"MNRAS"},{"key":"B78","doi-asserted-by":"publisher","first-page":"A10","DOI":"10.1051\/0004-6361\/201323326","article-title":"Impact on asteroseismic analyses of regular gaps in Kepler data","volume":"568","author":"Garc\u00eda","year":"","journal-title":"A&A"},{"key":"B79","doi-asserted-by":"publisher","first-page":"1032","DOI":"10.1126\/science.1191064","article-title":"CoRoT reveals a magnetic activity cycle in a sun-like star","volume":"329","author":"Garc\u00eda","year":"2010","journal-title":"Science"},{"key":"B80","doi-asserted-by":"publisher","first-page":"A110","DOI":"10.1051\/0004-6361\/201628367","article-title":"The missing magnetic morphology term in stellar rotation evolution","volume":"595","author":"Garraffo","year":"2016","journal-title":"A&A"},{"key":"B81","doi-asserted-by":"publisher","first-page":"90","DOI":"10.3847\/1538-4357\/aace5d","article-title":"The revolution revolution: magnetic morphology driven spin-down","volume":"862","author":"Garraffo","year":"2018","journal-title":"ApJ"},{"key":"B82","doi-asserted-by":"publisher","first-page":"A116","DOI":"10.1051\/0004-6361\/202245083","article-title":"Surface magnetism of rapidly rotating red giants: single versus close binary stars","volume":"668","author":"Gehan","year":"2022","journal-title":"A&A"},{"key":"B83","volume-title":"Magnetic activity of red giants: a near-UV and H$\u2216alpha$ view, and the enhancing role of tidal interactions","author":"Gehan","year":"2024"},{"key":"B84","doi-asserted-by":"publisher","first-page":"13267","DOI":"10.1073\/pnas.1303291110","article-title":"Seismic constraints on rotation of Sun-like star and mass of exoplanet","volume":"110","author":"Gizon","year":"2013","journal-title":"Proc. Natl. Acad. Sci."},{"key":"B85","doi-asserted-by":"publisher","first-page":"1009","DOI":"10.1086\/374715","article-title":"Determining the inclination of the rotation Axis of a sun-like star","volume":"589","author":"Gizon","year":"2003","journal-title":"ApJ"},{"key":"B86","doi-asserted-by":"publisher","first-page":"46","DOI":"10.3847\/1538-4365\/ac2058","article-title":"Stellar rotation in the Gaia era: revised open clusters\u2019 sequences","volume":"257","author":"Godoy-Rivera","year":"","journal-title":"ApJS"},{"key":"B87","doi-asserted-by":"publisher","first-page":"19","DOI":"10.3847\/1538-4357\/abf8ba","article-title":"Testing the limits of precise subgiant characterization with APOGEE and Gaia: opening a window to unprecedented astrophysical studies","volume":"915","author":"Godoy-Rivera","year":"","journal-title":"ApJ"},{"key":"B88","doi-asserted-by":"publisher","first-page":"A77","DOI":"10.1051\/0004-6361\/202039765","article-title":"Stellar chromospheric activity of 1674 FGK stars from the AMBRE-HARPS sample. I. A catalogue of homogeneous chromospheric activity","volume":"646","author":"Gomes da Silva","year":"2021","journal-title":"A&A"},{"key":"B89","doi-asserted-by":"publisher","first-page":"70","DOI":"10.3847\/1538-4357\/abf63e","article-title":"Stellar rotation in the K2 sample: evidence for modified spin-down","volume":"913","author":"Gordon","year":"2021","journal-title":"ApJ"},{"key":"B90","doi-asserted-by":"publisher","first-page":"5","DOI":"10.3847\/1538-4357\/ac3668","article-title":"Observationally constraining the starspot properties of magnetically active M67 sub-subgiant S1063","volume":"925","author":"Gosnell","year":"2022","journal-title":"ApJ"},{"key":"B91","doi-asserted-by":"publisher","first-page":"200","DOI":"10.3847\/1538-4357\/836\/2\/200","article-title":"Placing the spotted T tauri star LkCa 4 on an HR diagram","volume":"836","author":"Gully-Santiago","year":"2017","journal-title":"ApJ"},{"key":"B92","doi-asserted-by":"publisher","first-page":"60","DOI":"10.3847\/1538-3881\/ab5d3a","article-title":"Stellar flares from the first TESS data Release: exploring a new sample of M dwarfs","volume":"159","author":"G\u00fcnther","year":"2020","journal-title":"AJ"},{"key":"B93","doi-asserted-by":"publisher","first-page":"153","DOI":"10.1086\/142452","article-title":"The magnetic polarity of sun-spots","volume":"49","author":"Hale","year":"1919","journal-title":"ApJ"},{"key":"B94","doi-asserted-by":"publisher","first-page":"707","DOI":"10.1038\/s41550-021-01335-x","article-title":"Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs","volume":"5","author":"Hall","year":"2021","journal-title":"Nat. Astron."},{"key":"B95","doi-asserted-by":"publisher","first-page":"4","DOI":"10.1007\/lrsp-2015-4","article-title":"The solar cycle","volume":"12","author":"Hathaway","year":"2015","journal-title":"Living Rev. Sol. Phys."},{"key":"B96","doi-asserted-by":"publisher","first-page":"216","DOI":"10.1093\/mnras\/stad153","article-title":"Rotational modulation in A and F stars: magnetic stellar spots or convective core rotation?","volume":"520","author":"Henriksen","year":"2023","journal-title":"MNRAS"},{"key":"B97","doi-asserted-by":"publisher","first-page":"439","DOI":"10.1086\/117796","article-title":"A survey of Ca II H and K chromospheric emission in southern solar-type stars","volume":"111","author":"Henry","year":"1996","journal-title":"AJ"},{"key":"B98","doi-asserted-by":"publisher","first-page":"398","DOI":"10.1086\/676406","article-title":"The K2 mission: characterization and early results","volume":"126","author":"Howell","year":"2014","journal-title":"PASP"},{"key":"B99","doi-asserted-by":"publisher","first-page":"A133","DOI":"10.1051\/0004-6361\/201834400","article-title":"Flares in open clusters with K2 . I. M 45 (Pleiades), M 44 (Praesepe), and M 67","volume":"622","author":"Ilin","year":"2019","journal-title":"A&A"},{"key":"B100","doi-asserted-by":"publisher","first-page":"A42","DOI":"10.1051\/0004-6361\/202039198","article-title":"Flares in open clusters with K2. II. Pleiades, hyades, Praesepe, Ruprecht 147, and M 67","volume":"645","author":"Ilin","year":"2021","journal-title":"A&A"},{"key":"B101","doi-asserted-by":"publisher","first-page":"1567","DOI":"10.1088\/0004-637X\/695\/2\/1567","article-title":"Solar activity phases and intermediate-degree mode frequencies","volume":"695","author":"Jain","year":"2009","journal-title":"ApJ"},{"key":"B102","doi-asserted-by":"publisher","first-page":"58","DOI":"10.1088\/0004-6256\/146\/3\/58","article-title":"WOCS 40007: a detached eclipsing binary near the turnoff of the open cluster NGC 6819","volume":"146","author":"Jeffries","year":"2013","journal-title":"AJ"},{"key":"B103","doi-asserted-by":"publisher","first-page":"L87","DOI":"10.1088\/2041-8205\/713\/2\/L87","article-title":"Overview of the kepler science processing pipeline","volume":"713","author":"Jenkins","year":"2010","journal-title":"ApJL"},{"key":"B104","doi-asserted-by":"publisher","first-page":"247","DOI":"10.1023\/A:1021226503589","article-title":"Variation of the low-degree solar acoustic mode parameters over the solar cycle","volume":"209","author":"Jim\u00e9nez","year":"2002","journal-title":"Sol. Phys."},{"key":"B105","first-page":"1119","article-title":"Solar activity cycle frequency shifts of low-degree p-modes","volume":"329","author":"Jim\u00e9nez-Reyes","year":"1998","journal-title":"A&A"},{"key":"B106","doi-asserted-by":"publisher","first-page":"433","DOI":"10.1146\/annurev-astro-082214-122238","article-title":"How to characterize habitable worlds and signs of life","volume":"55","author":"Kaltenegger","year":"2017","journal-title":"ARA&A"},{"key":"B107","doi-asserted-by":"publisher","first-page":"11058","DOI":"10.1038\/ncomms11058","article-title":"Observational evidence for enhanced magnetic activity of superflare stars","volume":"7","author":"Karoff","year":"2016","journal-title":"Nat. Commun."},{"key":"B108","doi-asserted-by":"publisher","first-page":"46","DOI":"10.3847\/1538-4357\/aaa026","article-title":"The influence of metallicity on stellar differential rotation and magnetic activity","volume":"852","author":"Karoff","year":"2018","journal-title":"ApJ"},{"key":"B109","doi-asserted-by":"publisher","first-page":"255101","DOI":"10.1103\/physrevlett.127.255101","article-title":"Parker solar probe enters the magnetically dominated solar corona","volume":"127","author":"Kasper","year":"2021","journal-title":"Phys. Rev. Lett."},{"key":"B110","doi-asserted-by":"publisher","first-page":"A5","DOI":"10.1051\/0004-6361\/202244220","article-title":"Gaia Data Release 3. Properties and validation of the radial velocities","volume":"674","author":"Katz","year":"2023","journal-title":"A&A"},{"key":"B111","doi-asserted-by":"publisher","first-page":"236","DOI":"10.1086\/166740","article-title":"Angular momentum loss in low-mass stars","volume":"333","author":"Kawaler","year":"1988","journal-title":"ApJ"},{"key":"B112","doi-asserted-by":"publisher","first-page":"A77","DOI":"10.1051\/0004-6361\/201628469","article-title":"Stellar magnetic activity and variability of oscillation parameters: an investigation of 24 solar-like stars observed by Kepler","volume":"598","author":"Kiefer","year":"2017","journal-title":"A&A"},{"key":"B113","doi-asserted-by":"publisher","first-page":"68","DOI":"10.3847\/0004-6256\/151\/3\/68","article-title":"Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire kepler data set","volume":"151","author":"Kirk","year":"2016","journal-title":"AJ"},{"key":"B114","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1007\/s00159-020-00130-3","article-title":"Magnetic fields of M dwarfs","volume":"29","author":"Kochukhov","year":"2021","journal-title":"A&ARv"},{"key":"B115","doi-asserted-by":"publisher","first-page":"551","DOI":"10.1086\/149359","article-title":"Studies of stellar rotation. V. The dependence of rotation on age among solar-type stars","volume":"150","author":"Kraft","year":"1967","journal-title":"ApJ"},{"key":"B116","doi-asserted-by":"publisher","first-page":"157","DOI":"10.3847\/1538-4357\/ab1aa2","article-title":"Evidence of new magnetic transitions in late-type dwarfs from Gaia DR2","volume":"877","author":"Lanzafame","year":"2019","journal-title":"ApJ"},{"key":"B117","doi-asserted-by":"publisher","first-page":"A16","DOI":"10.1051\/0004-6361\/201833334","article-title":"Gaia data Release 2 - rotational modulation in late-type dwarfs","volume":"616","author":"Lanzafame","year":"2018","journal-title":"A&A"},{"key":"B118","doi-asserted-by":"publisher","first-page":"110","DOI":"10.3847\/1538-4357\/abe621","article-title":"A knee point in the rotation-activity scaling of late-type stars with a connection to dynamo transitions","volume":"910","author":"Lehtinen","year":"2021","journal-title":"ApJ"},{"key":"B119","doi-asserted-by":"publisher","first-page":"366","DOI":"10.1086\/146727","article-title":"Observations of solar magnetic fields in plage regions","volume":"130","author":"Leighton","year":"1959","journal-title":"ApJ"},{"key":"B120","doi-asserted-by":"crossref","DOI":"10.3847\/1538-4357\/ad1e59","volume-title":"Do faculae affect autocorrelation rotation periods in sun-like stars?","author":"Li","year":"2024"},{"key":"B121","doi-asserted-by":"publisher","first-page":"A73","DOI":"10.1051\/0004-6361\/201629294","article-title":"The solar twin planet search. The age-chromospheric activity relation","volume":"619","author":"Lorenzo-Oliveira","year":"2018","journal-title":"A&A"},{"key":"B122","doi-asserted-by":"publisher","first-page":"L68","DOI":"10.1093\/mnrasl\/slz034","article-title":"Constraining the evolution of stellar rotation using solar twins","volume":"485","author":"Lorenzo-Oliveira","year":"2019","journal-title":"MNRAS"},{"key":"B123","volume-title":"In this day and age: an empirical gyrochronology relation for partially and fully convective single field stars","author":"Lu","year":"2023"},{"key":"B124","doi-asserted-by":"publisher","first-page":"251","DOI":"10.3847\/1538-3881\/ac9bee","article-title":"Bridging the gap-the disappearance of the intermediate period gap for fully convective stars, uncovered by new ZTF rotation periods","volume":"164","author":"Lu","year":"2022","journal-title":"AJ"},{"key":"B125","doi-asserted-by":"publisher","first-page":"172","DOI":"10.3847\/1538-4357\/835\/2\/172","article-title":"Standing on the shoulders of dwarfs: the kepler asteroseismic LEGACY sample. I. Oscillation mode parameters","volume":"835","author":"Lund","year":"2017","journal-title":"ApJ"},{"key":"B126","doi-asserted-by":"publisher","first-page":"1264","DOI":"10.1086\/591785","article-title":"Improved age estimation for solar-type dwarfs using activity-rotation diagnostics","volume":"687","author":"Mamajek","year":"2008","journal-title":"ApJ"},{"key":"B127","doi-asserted-by":"publisher","first-page":"5623","DOI":"10.1093\/mnras\/stab3650","article-title":"Inferring the rotation period distribution of stars from their projected rotation velocities and radii: application to late-F\/early-G Kepler stars","volume":"510","author":"Masuda","year":"2022","journal-title":"MNRAS"},{"key":"B128","doi-asserted-by":"publisher","first-page":"131","DOI":"10.3847\/1538-4357\/acd118","article-title":"Magnetic activity evolution of solar-like stars. I. S ph-age relation derived from kepler observations","volume":"952","author":"Mathur","year":"2023","journal-title":"ApJ"},{"key":"B129","doi-asserted-by":"publisher","first-page":"A124","DOI":"10.1051\/0004-6361\/201322707","article-title":"Magnetic activity of F stars observed by Kepler","volume":"562","author":"Mathur","year":"","journal-title":"A&A"},{"key":"B130","doi-asserted-by":"publisher","first-page":"46","DOI":"10.3389\/fspas.2019.00046","article-title":"Revisiting the impact of stellar magnetic activity on the detectability of solar-like oscillations by kepler","volume":"6","author":"Mathur","year":"2019","journal-title":"FrASS"},{"key":"B131","doi-asserted-by":"publisher","first-page":"A15","DOI":"10.1051\/swsc\/2014011","article-title":"Photometric magnetic-activity metrics tested with the Sun: application to Kepler M dwarfs","volume":"4","author":"Mathur","year":"","journal-title":"JSWSC"},{"key":"B132","doi-asserted-by":"publisher","first-page":"A14","DOI":"10.1051\/0004-6361\/201628429","article-title":"Ap stars with resolved magnetically split lines: magnetic field determinations from Stokes I and V spectra","volume":"601","author":"Mathys","year":"2017","journal-title":"A&A"},{"key":"B133","doi-asserted-by":"publisher","first-page":"L23","DOI":"10.1088\/2041-8205\/799\/2\/L23","article-title":"The mass-dependence of angular momentum evolution in sun-like stars","volume":"799","author":"Matt","year":"2015","journal-title":"ApJ"},{"key":"B134","doi-asserted-by":"publisher","first-page":"1203","DOI":"10.1093\/mnras\/stt536","article-title":"Measuring the rotation period distribution of field M dwarfs with Kepler","volume":"432","author":"McQuillan","year":"2013","journal-title":"MNRAS"},{"key":"B135","doi-asserted-by":"publisher","first-page":"24","DOI":"10.1088\/0067-0049\/211\/2\/24","article-title":"Rotation periods of 34,030 kepler main-sequence stars: the full autocorrelation sample","volume":"211","author":"McQuillan","year":"2014","journal-title":"ApJS"},{"key":"B136","doi-asserted-by":"publisher","first-page":"589","DOI":"10.1038\/nature14118","article-title":"A spin-down clock for cool stars from observations of a 2.5-billion-year-old cluster","volume":"517","author":"Meibom","year":"2015","journal-title":"Nature"},{"key":"B137","doi-asserted-by":"publisher","first-page":"L2","DOI":"10.3847\/2041-8205\/826\/1\/L2","article-title":"Stellar evidence that the solar dynamo may Be in transition","volume":"826","author":"Metcalfe","year":"2016","journal-title":"ApJL"},{"key":"B138","doi-asserted-by":"publisher","first-page":"L17","DOI":"10.3847\/2041-8213\/ac794d","article-title":"The origin of weakened magnetic braking in old solar analogs","volume":"933","author":"Metcalfe","year":"2022","journal-title":"ApJL"},{"key":"B139","doi-asserted-by":"publisher","first-page":"L6","DOI":"10.3847\/2041-8213\/acce38","article-title":"Constraints on magnetic braking from the G8 dwarf stars 61 UMa and \u03c4 cet","volume":"948","author":"Metcalfe","year":"2023","journal-title":"ApJL"},{"key":"B140","doi-asserted-by":"publisher","first-page":"126","DOI":"10.1007\/s11207-017-1157-5","article-title":"Magnetic evolution and the disappearance of sun-like activity cycles","volume":"292","author":"Metcalfe","year":"2017","journal-title":"Sol. Phys."},{"key":"B141","doi-asserted-by":"publisher","first-page":"122","DOI":"10.3847\/1538-4357\/ac1f19","article-title":"Magnetic and rotational evolution of \u03c1 CrB from asteroseismology with TESS","volume":"921","author":"Metcalfe","year":"2021","journal-title":"ApJ"},{"key":"B142","doi-asserted-by":"publisher","first-page":"A77","DOI":"10.1051\/0004-6361\/202038710","article-title":"Activity time series of old stars from late F to early K. V. Effect on exoplanet detectability with high-precision astrometry","volume":"644","author":"Meunier","year":"2020","journal-title":"A&A"},{"key":"B143","doi-asserted-by":"publisher","first-page":"116","DOI":"10.3847\/1538-4357\/aa9e00","article-title":"Long-term photometric variability in kepler full-frame images: magnetic cycles of sun-like stars","volume":"851","author":"Montet","year":"2017","journal-title":"ApJ"},{"key":"B144","doi-asserted-by":"publisher","first-page":"85","DOI":"10.3847\/1538-4357\/834\/1\/85","article-title":"The H\u03b1 emission of nearby M dwarfs and its relation to stellar rotation","volume":"834","author":"Newton","year":"2017","journal-title":"ApJ"},{"key":"B145","doi-asserted-by":"publisher","first-page":"L10","DOI":"10.1051\/0004-6361\/201321912","article-title":"Rotation periods of 12 000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations","volume":"557","author":"Nielsen","year":"2013","journal-title":"A&A"},{"key":"B146","doi-asserted-by":"publisher","first-page":"A6","DOI":"10.1051\/0004-6361\/201730896","article-title":"Limits on radial differential rotation in Sun-like stars from parametric fits to oscillation power spectra","volume":"603","author":"Nielsen","year":"2017","journal-title":"A&A"},{"key":"B147","doi-asserted-by":"publisher","first-page":"A144","DOI":"10.1051\/0004-6361\/202141946","article-title":"Impact of anti-solar differential rotation in mean-field solar-type dynamos-exploring possible magnetic cycles in slowly rotating stars","volume":"658","author":"Noraz","year":"2022","journal-title":"A&A"},{"key":"B148","doi-asserted-by":"publisher","first-page":"58","DOI":"10.3847\/1538-4357\/ab14e6","article-title":"Do kepler superflare stars really include slowly rotating sun-like stars?results using APO 3.5 m telescope spectroscopic observations and gaia-DR2 data","volume":"876","author":"Notsu","year":"2019","journal-title":"ApJ"},{"key":"B149","doi-asserted-by":"publisher","first-page":"763","DOI":"10.1086\/161945","article-title":"Rotation, convection, and magnetic activity in lower main-sequence stars","volume":"279","author":"Noyes","year":"1984","journal-title":"ApJ"},{"key":"B150","doi-asserted-by":"publisher","first-page":"703","DOI":"10.1051\/0004-6361\/200811304","article-title":"Multiple and changing cycles of active stars. II. Results","volume":"501","author":"Ol\u00e1h","year":"2009","journal-title":"A&A"},{"key":"B151","doi-asserted-by":"publisher","first-page":"A19","DOI":"10.1051\/0004-6361\/201321309","article-title":"Effect of stellar spots on high-precision transit light-curve","volume":"556","author":"Oshagh","year":"2013","journal-title":"ASTRONOMY ASTROPHYSICS"},{"key":"B152","doi-asserted-by":"publisher","first-page":"67","DOI":"10.1146\/annurev-earth-053018-060246","article-title":"Atmospheric escape and the evolution of close-in exoplanets","volume":"47","author":"Owen","year":"2019","journal-title":"AREPS"},{"key":"B153","doi-asserted-by":"publisher","first-page":"L8","DOI":"10.1051\/0004-6361\/201220364","article-title":"Chromospheric activity as age indicator: an L-shaped chromospheric-activity versus age diagram\u22c6","volume":"551","author":"Pace","year":"2013","journal-title":"A&A"},{"key":"B154","doi-asserted-by":"publisher","first-page":"279","DOI":"10.1086\/159152","article-title":"Relations among stellar X-ray emission observed from Einstein, stellar rotation and bolometric luminosity","volume":"248","author":"Pallavicini","year":"1981","journal-title":"ApJ"},{"key":"B155","doi-asserted-by":"publisher","first-page":"993","DOI":"10.1051\/0004-6361:20054003","article-title":"Deep X-ray survey of the young open cluster NGC 2516 with XMM-Newton","volume":"450","author":"Pillitteri","year":"2006","journal-title":"A&A"},{"key":"B156","doi-asserted-by":"publisher","first-page":"424","DOI":"10.1086\/167210","article-title":"Evolutionary models of the rotating sun","volume":"338","author":"Pinsonneault","year":"1989","journal-title":"ApJ"},{"key":"B157","doi-asserted-by":"publisher","first-page":"147","DOI":"10.1051\/0004-6361:20021560","article-title":"The stellar activity-rotation relationship revisited: dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs","volume":"397","author":"Pizzolato","year":"2003","journal-title":"A&A"},{"key":"B158","doi-asserted-by":"publisher","first-page":"2675","DOI":"10.1093\/mnras\/stad1085","article-title":"Photometric variations from stellar activity as an age indicator for solar-twins","volume":"522","author":"Ponte","year":"2023","journal-title":"MNRAS"},{"key":"B159","doi-asserted-by":"publisher","first-page":"279","DOI":"10.1051\/0004-6361:20011308","article-title":"No planet for HD 166435","volume":"379","author":"Queloz","year":"2001","journal-title":"A&A"},{"key":"B160","doi-asserted-by":"publisher","first-page":"465","DOI":"10.1086\/430102","article-title":"The effective temperature scale of FGK stars. II. Teff:Color:[Fe\/H] calibrations","volume":"626","author":"Ram\u00edrez","year":"2005","journal-title":"ApJ"},{"key":"B161","doi-asserted-by":"publisher","first-page":"249","DOI":"10.1007\/s10686-014-9383-4","article-title":"The PLATO 2.0 mission","volume":"38","author":"Rauer","year":"2014","journal-title":"Exp. Astron."},{"key":"B162","doi-asserted-by":"publisher","first-page":"A41","DOI":"10.1051\/0004-6361\/202243251","article-title":"Magnetism, rotation, and nonthermal emission in cool stars - average magnetic field measurements in 292 M dwarfs","volume":"662","author":"Reiners","year":"2022","journal-title":"A&A"},{"key":"B163","doi-asserted-by":"publisher","first-page":"A21","DOI":"10.1051\/0004-6361\/201833754","article-title":"Transition from spot to faculae domination. An alternate explanation for the dearth of intermediate Kepler rotation periods","volume":"621","author":"Reinhold","year":"2019","journal-title":"A&A"},{"key":"B164","doi-asserted-by":"publisher","first-page":"A43","DOI":"10.1051\/0004-6361\/201936887","article-title":"Stellar rotation periods from K2 Campaigns 0-18. Evidence for rotation period bimodality and simultaneous variability decrease","volume":"635","author":"Reinhold","year":"2020","journal-title":"A&A"},{"key":"B165","doi-asserted-by":"publisher","first-page":"A4","DOI":"10.1051\/0004-6361\/201321970","article-title":"Rotation and differential rotation of active Kepler stars","volume":"560","author":"Reinhold","year":"2013","journal-title":"A&A"},{"key":"B166","doi-asserted-by":"publisher","first-page":"A24","DOI":"10.1051\/0004-6361\/202346789","article-title":"New rotation period measurements of 67 163 Kepler stars","volume":"678","author":"Reinhold","year":"2023","journal-title":"A&A"},{"key":"B167","doi-asserted-by":"publisher","first-page":"116","DOI":"10.1088\/0004-637X\/798\/2\/116","article-title":"The effect of magnetic topology on thermally driven wind: toward a general formulation of the braking law","volume":"798","author":"R\u00e9ville","year":"2015","journal-title":"ApJ"},{"key":"B168","first-page":"914320","article-title":"Transiting exoplanet survey satellite (TESS) 9143","author":"Ricker","year":"2014"},{"key":"B169","doi-asserted-by":"publisher","first-page":"6","DOI":"10.1007\/s41116-018-0013-5","article-title":"The Sun\u2019s supergranulation","volume":"15","author":"Rincon","year":"2018","journal-title":"Living Rev. Sol. Phys."},{"key":"B170","doi-asserted-by":"publisher","first-page":"L11","DOI":"10.1051\/0004-6361\/201834347","article-title":"Direct evidence of a full dipole flip during the magnetic cycle of a sun-like star","volume":"620","author":"Saikia","year":"2018","journal-title":"A&A"},{"key":"B171","doi-asserted-by":"publisher","first-page":"A31","DOI":"10.1051\/0004-6361\/201628583","article-title":"Photospheric and chromospheric magnetic activity of seismic solar analogs: observational inputs on the solar-stellar connection fromKeplerand Hermes \u22c6","volume":"596","author":"Salabert","year":"2016","journal-title":"A&A"},{"key":"B172","doi-asserted-by":"publisher","first-page":"A87","DOI":"10.1051\/0004-6361\/201731560","article-title":"Photospheric activity of the Sun with VIRGO and GOLF. Comparison with standard activity proxies","volume":"608","author":"Salabert","year":"2017","journal-title":"A&A"},{"key":"B173","doi-asserted-by":"publisher","first-page":"A137","DOI":"10.1051\/0004-6361\/201425236","article-title":"Seismic sensitivity to sub-surface solar activity from 18 yr of GOLF\/SoHO observations","volume":"578","author":"Salabert","year":"2015","journal-title":"A&A"},{"key":"B174","doi-asserted-by":"publisher","first-page":"17","DOI":"10.3847\/1538-4365\/ac033f","article-title":"Surface rotation and photometric activity for kepler targets. II. G and F Main-sequence stars and cool subgiant stars","volume":"255","author":"Santos","year":"2021","journal-title":"ApJS"},{"key":"B175","doi-asserted-by":"publisher","first-page":"17","DOI":"10.3847\/1538-4365\/aac9b6","article-title":"Signatures of magnetic activity in the seismic data of solar-type stars observed by kepler","volume":"237","author":"Santos","year":"2018","journal-title":"ApJS"},{"key":"B176","doi-asserted-by":"publisher","first-page":"21","DOI":"10.3847\/1538-4365\/ab3b56","article-title":"Surface rotation and photometric activity for kepler targets. I. M and K Main-sequence stars","volume":"244","author":"Santos","year":"2019","journal-title":"ApJS"},{"key":"B177","doi-asserted-by":"publisher","first-page":"A56","DOI":"10.1051\/0004-6361\/202245430","article-title":"Temporal variation of the photometric magnetic activity for the Sun and Kepler solar-like stars","volume":"672","author":"Santos","year":"2023","journal-title":"A&A"},{"key":"B178","first-page":"138","article-title":"Stellar cruise control: weakened magnetic braking leads to sustained rapid rotation of old stars","volume-title":"ApJ","author":"Saunders","year":"2023"},{"key":"B179","doi-asserted-by":"publisher","first-page":"392","DOI":"10.1086\/176149","article-title":"The X-ray view of the low-mass stars in the solar neighborhood","volume":"450","author":"Schmitt","year":"1995","journal-title":"ApJ"},{"key":"B180","doi-asserted-by":"publisher","first-page":"A24","DOI":"10.1051\/0004-6361\/201525937","article-title":"Asteroseismic inversions for radial differential rotation of Sun-like stars: sensitivity to uncertainties","volume":"586","author":"Schunker","year":"","journal-title":"A&A"},{"key":"B181","doi-asserted-by":"publisher","first-page":"A79","DOI":"10.1051\/0004-6361\/201527485","article-title":"Asteroseismic inversions for radial differential rotation of Sun-like stars: ensemble fits","volume":"586","author":"Schunker","year":"","journal-title":"A&A"},{"key":"B182","doi-asserted-by":"publisher","first-page":"120","DOI":"10.3847\/1538-4357\/ab46b2","article-title":"Do non-dipolar magnetic fields contribute to spin-down torques?","volume":"886","author":"See","year":"","journal-title":"ApJ"},{"key":"B183","doi-asserted-by":"publisher","first-page":"118","DOI":"10.3847\/1538-4357\/ab1096","article-title":"Estimating magnetic filling factors from zeeman-Doppler magnetograms","volume":"876","author":"See","year":"","journal-title":"ApJ"},{"key":"B184","doi-asserted-by":"publisher","first-page":"5781","DOI":"10.1093\/mnras\/stad2020","article-title":"Further evidence of the link between activity and metallicity using the flaring properties of stars in the Kepler field","volume":"524","author":"See","year":"2023","journal-title":"MNRAS"},{"key":"B185","doi-asserted-by":"publisher","first-page":"127","DOI":"10.3847\/1538-4357\/abed47","article-title":"Photometric variability as a proxy for magnetic activity and its dependence on metallicity","volume":"912","author":"See","year":"2021","journal-title":"ApJ"},{"key":"B186","first-page":"456","article-title":"Zeeman-Doppler imaging of active stars. I - basic principles","volume":"225","author":"Semel","year":"1989","journal-title":"A&A"},{"key":"B187","first-page":"A46","article-title":"Are solar brightness variations faculae- or spot-dominated?","volume-title":"A&A","author":"Shapiro","year":"2016"},{"key":"B188","doi-asserted-by":"publisher","first-page":"71","DOI":"10.3847\/1538-4357\/acfa72","article-title":"Formulating mass-loss rates for sun-like stars: a hybrid model approach","volume":"957","author":"Shoda","year":"2023","journal-title":"ApJ"},{"key":"B189","doi-asserted-by":"publisher","first-page":"123","DOI":"10.3847\/1538-4357\/ab94bf","article-title":"Alfv\u00e9n-wave-driven magnetic rotator winds from low-mass stars. i. rotation dependences of magnetic braking and mass-loss rate","volume":"896","author":"Shoda","year":"2020","journal-title":"ApJ"},{"key":"B190","doi-asserted-by":"publisher","first-page":"5947","DOI":"10.1093\/mnras\/stad1803","article-title":"The breakdown of current gyrochronology as evidenced by old coeval stars","volume":"523","author":"Silva-Beyer","year":"2023","journal-title":"MNRAS"},{"key":"B191","doi-asserted-by":"publisher","first-page":"174","DOI":"10.3847\/1538-4357\/aaf97c","article-title":"Rapid rotation in the kepler field: not a single star phenomenon","volume":"871","author":"Simonian","year":"2019","journal-title":"ApJ"},{"key":"B192","doi-asserted-by":"publisher","first-page":"565","DOI":"10.1086\/151310","article-title":"Time scales for CA II emission decay, rotational braking, and lithium depletion","volume":"171","author":"Skumanich","year":"1972","journal-title":"ApJ"},{"key":"B193","doi-asserted-by":"publisher","first-page":"722","DOI":"10.1086\/170238","article-title":"The chromospheric emission\u2013age relation for stars of the lower main sequence and its implications for the star formation rate","volume":"375","author":"Soderblom","year":"1991","journal-title":"ApJ"},{"key":"B194","doi-asserted-by":"publisher","first-page":"315","DOI":"10.1086\/191767","article-title":"Rotation and chromospheric emission among F, G, and K dwarfs of the Pleiades","volume":"85","author":"Soderblom","year":"1993","journal-title":"ApJS"},{"key":"B195","doi-asserted-by":"publisher","first-page":"153","DOI":"10.1007\/s00159-003-0018-4","article-title":"Sunspots: an overview","volume":"11","author":"Solanki","year":"2003","journal-title":"A&ARv"},{"key":"B196","doi-asserted-by":"publisher","first-page":"L33","DOI":"10.1086\/186989","article-title":"An interpretation of cycle periods of stellar chromospheric activity","volume":"414","author":"Soon","year":"1993","journal-title":"ApJ"},{"key":"B197","doi-asserted-by":"publisher","first-page":"A76","DOI":"10.1051\/0004-6361\/201936384","article-title":"Competing effect of wind braking and interior coupling in the rotational evolution of solar-like stars","volume":"636","author":"Spada","year":"2020","journal-title":"A&A"},{"key":"B198","doi-asserted-by":"publisher","first-page":"337","DOI":"10.1086\/165371","article-title":"The distribution of rotational velocities for low-mass stars in the Pleiades","volume":"318","author":"Stauffer","year":"1987","journal-title":"ApJ"},{"key":"B199","doi-asserted-by":"publisher","first-page":"L199","DOI":"10.1086\/311379","article-title":"Keck spectra of Pleiades Brown dwarf candidates and a precise determination of the lithium depletion edge in the Pleiades","volume":"499","author":"Stauffer","year":"1998","journal-title":"ApJ"},{"key":"B200","doi-asserted-by":"crossref","first-page":"1833","DOI":"10.1007\/978-3-319-55333-7_25","article-title":"Models of star-planet magnetic interaction","volume-title":"Handbook of exoplanets","author":"Strugarek","year":"2018"},{"key":"B201","doi-asserted-by":"publisher","first-page":"4772","DOI":"10.1093\/mnras\/stx771","article-title":"Characterization of the radial velocity signal induced by rotation in late-type dwarfs","volume":"468","author":"Su\u00e1rez Mascare\u00f1o","year":"2017","journal-title":"MNRAS"},{"key":"B202","doi-asserted-by":"publisher","first-page":"3857","DOI":"10.1093\/mnras\/stz672","article-title":"Asteroseismic constraints on active latitudes of solar-type stars: HD 173701 has active bands at higher latitudes than the Sun","volume":"485","author":"Thomas","year":"2019","journal-title":"MNRAS"},{"key":"B203","doi-asserted-by":"publisher","first-page":"418","DOI":"10.1093\/mnras\/stad103","article-title":"Transition of latitudinal differential rotation as a possible cause of weakened magnetic braking of solar-type stars","volume":"520","author":"Tokuno","year":"2023","journal-title":"MNRAS"},{"key":"B204","doi-asserted-by":"publisher","first-page":"162","DOI":"10.3847\/1538-4357\/ab911b","article-title":"Eclipsing binaries in the open cluster Ruprecht 147. III. The triple system EPIC 219552514 at the main-sequence turnoff","volume":"896","author":"Torres","year":"2020","journal-title":"ApJ"},{"key":"B205","doi-asserted-by":"publisher","first-page":"012055","DOI":"10.1088\/1742-6596\/271\/1\/012055","article-title":"Angular-degree dependence of p-mode frequencies during solar cycle 23","volume":"271","author":"Tripathy","year":"2011","journal-title":"J. Phys. Conf. Ser."},{"key":"B206","doi-asserted-by":"publisher","first-page":"141","DOI":"10.1086\/430500","article-title":"Spectroscopic properties of cool stars (SPOCS). I. 1040 F, G, and K dwarfs from keck, lick, and AAT planet search programs","volume":"159","author":"Valenti","year":"2005","journal-title":"ApJS"},{"key":"B207","doi-asserted-by":"publisher","first-page":"1","DOI":"10.1007\/lrsp-2015-1","article-title":"Evolution of active regions","volume":"12","author":"van Driel-Gesztelyi","year":"2015","journal-title":"Living Rev. Sol. Phys."},{"key":"B208","doi-asserted-by":"publisher","first-page":"181","DOI":"10.1038\/nature16168","article-title":"Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars","volume":"529","author":"van Saders","year":"2016","journal-title":"Nature"},{"key":"B209","doi-asserted-by":"publisher","first-page":"16","DOI":"10.1088\/0004-637X\/746\/1\/16","article-title":"The sensitivity of convection zone depth to stellar abundances: an absolute stellar abundance scale from asteroseismology","volume":"746","author":"van Saders","year":"2012","journal-title":"ApJ"},{"key":"B210","doi-asserted-by":"publisher","first-page":"67","DOI":"10.1088\/0004-637X\/776\/2\/67","article-title":"Fast star, slow star; old star, young star: subgiant rotation as a population and stellar physics diagnostic","volume":"776","author":"van Saders","year":"2013","journal-title":"ApJ"},{"key":"B211","doi-asserted-by":"publisher","first-page":"128","DOI":"10.3847\/1538-4357\/aafafe","article-title":"Forward modeling of the kepler stellar rotation period distribution: interpreting periods from mixed and biased stellar populations","volume":"872","author":"van Saders","year":"2019","journal-title":"ApJ"},{"key":"B212","doi-asserted-by":"publisher","first-page":"392","DOI":"10.1086\/130684","article-title":"Comparison of activity cycles in old and young main-sequence stars","volume":"92","author":"Vaughan","year":"1980","journal-title":"PASP"},{"key":"B213","doi-asserted-by":"publisher","first-page":"385","DOI":"10.1086\/130683","article-title":"A survey of chromospheric CA II H and K emission in field stars of the solar neighborhood","volume":"92","author":"Vaughan","year":"1980","journal-title":"PASP"},{"key":"B214","doi-asserted-by":"publisher","first-page":"2361","DOI":"10.1093\/mnras\/stu728","article-title":"Stellar magnetism: empirical trends with age and rotation","volume":"441","author":"Vidotto","year":"2014","journal-title":"MNRAS"},{"key":"B215","doi-asserted-by":"publisher","first-page":"671","DOI":"10.1086\/158842","article-title":"On the coronae of rapidly rotating stars. I. The relation between rotation and coronal activity in RS CVn systems","volume":"245","author":"Walter","year":"1981","journal-title":"ApJ"},{"key":"B216","doi-asserted-by":"publisher","first-page":"217","DOI":"10.1086\/149138","article-title":"The angular momentum of the solar wind","volume":"148","author":"Weber","year":"1967","journal-title":"ApJ"},{"key":"B217","doi-asserted-by":"publisher","first-page":"832","DOI":"10.1086\/147689","article-title":"A probable correlation between chromospheric activity and age in main-sequence stars","volume":"138","author":"Wilson","year":"1963","journal-title":"ApJ"},{"key":"B218","doi-asserted-by":"publisher","first-page":"221","DOI":"10.1086\/149652","article-title":"Flux measurements at the centers of stellar H- and K-lines","volume":"153","author":"Wilson","year":"1968","journal-title":"ApJ"},{"key":"B219","doi-asserted-by":"publisher","first-page":"379","DOI":"10.1086\/156618","article-title":"Chromospheric variations in main-sequence stars","volume":"226","author":"Wilson","year":"1978","journal-title":"ApJ"},{"key":"B220","doi-asserted-by":"publisher","first-page":"37","DOI":"10.3847\/1538-4357\/abfda5","article-title":"New observational constraints on the winds of M dwarf stars*","volume":"915","author":"Wood","year":"2021","journal-title":"ApJ"},{"key":"B221","doi-asserted-by":"publisher","first-page":"449","DOI":"10.1038\/318449a0","article-title":"Change of solar oscillation eigenfrequencies with the solar cycle","volume":"318","author":"Woodard","year":"1985","journal-title":"Nature"},{"key":"B222","doi-asserted-by":"publisher","first-page":"526","DOI":"10.1038\/nature18638","article-title":"Solar-type dynamo behaviour in fully convective stars without a tachocline","volume":"535","author":"Wright","year":"2016","journal-title":"Nature"},{"key":"B223","doi-asserted-by":"publisher","first-page":"48","DOI":"10.1088\/0004-637X\/743\/1\/48","article-title":"The stellar-activity-rotation relationship and the evolution of stellar dynamos","volume":"743","author":"Wright","year":"2011","journal-title":"ApJ"},{"key":"B224","doi-asserted-by":"publisher","first-page":"2351","DOI":"10.1093\/mnras\/sty1670","article-title":"The stellar rotation\u2013activity relationship in fully convective M dwarfs","volume":"479","author":"Wright","year":"2018","journal-title":"MNRAS"},{"key":"B225","doi-asserted-by":"publisher","first-page":"29","DOI":"10.3847\/1538-4365\/ab0d28","article-title":"The flare catalog and the flare activity in the kepler mission","volume":"241","author":"Yang","year":"2019","journal-title":"ApJS"},{"key":"B226","doi-asserted-by":"publisher","first-page":"227","DOI":"10.3390\/universe9050227","article-title":"Magnetic activity of different types of variable stars observed by TESS mission","volume":"9","author":"Zhong","year":"2023","journal-title":"Universe"},{"key":"B227","doi-asserted-by":"publisher","first-page":"328","DOI":"10.1007\/BF00221318","article-title":"Active regions. I: the occurrence of solar flares and the development of active regions","volume":"14","author":"Zirin","year":"1970","journal-title":"Sol. Phys."}],"container-title":["Frontiers in Astronomy and Space Sciences"],"original-title":[],"link":[{"URL":"https:\/\/www.frontiersin.org\/articles\/10.3389\/fspas.2024.1356379\/full","content-type":"unspecified","content-version":"vor","intended-application":"similarity-checking"}],"deposited":{"date-parts":[[2024,3,15]],"date-time":"2024-03-15T04:58:44Z","timestamp":1710478724000},"score":1,"resource":{"primary":{"URL":"https:\/\/www.frontiersin.org\/articles\/10.3389\/fspas.2024.1356379\/full"}},"subtitle":[],"short-title":[],"issued":{"date-parts":[[2024,3,15]]},"references-count":227,"alternative-id":["10.3389\/fspas.2024.1356379"],"URL":"https:\/\/doi.org\/10.3389\/fspas.2024.1356379","relation":{},"ISSN":["2296-987X"],"issn-type":[{"value":"2296-987X","type":"electronic"}],"subject":[],"published":{"date-parts":[[2024,3,15]]},"article-number":"1356379"}}