APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields
In the third APOKASC catalog, we present data for the complete sample of 15,808 evolved stars with APOGEE spectroscopic parameters and Kepler asteroseismology. We used 10 independent asteroseismic analysis techniques and anchor our system on fundamental radii derived from Gaia L and spectroscopic T...
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author | Marc H. Pinsonneault Joel C. Zinn Jamie Tayar Aldo Serenelli Rafael A. García Savita Mathur Mathieu Vrard Yvonne P. Elsworth Benoit Mosser Dennis Stello Keaton J. Bell Lisa Bugnet Enrico Corsaro Patrick Gaulme Saskia Hekker Marc Hon Daniel Huber Thomas Kallinger Kaili Cao Jennifer A. Johnson Bastien Liagre Rachel A. Patton Ângela R. G. Santos Sarbani Basu Paul G. Beck Timothy C. Beers William J. Chaplin Katia Cunha Peter M. Frinchaboy Léo Girardi Diego Godoy-Rivera Jon A. Holtzman Henrik Jönsson Szabolcs Mészáros Claudia Reyes Hans-Walter Rix Matthew Shetrone Verne V. Smith Taylor Spoo Keivan G. Stassun Ji Wang |
author_facet | Marc H. Pinsonneault Joel C. Zinn Jamie Tayar Aldo Serenelli Rafael A. García Savita Mathur Mathieu Vrard Yvonne P. Elsworth Benoit Mosser Dennis Stello Keaton J. Bell Lisa Bugnet Enrico Corsaro Patrick Gaulme Saskia Hekker Marc Hon Daniel Huber Thomas Kallinger Kaili Cao Jennifer A. Johnson Bastien Liagre Rachel A. Patton Ângela R. G. Santos Sarbani Basu Paul G. Beck Timothy C. Beers William J. Chaplin Katia Cunha Peter M. Frinchaboy Léo Girardi Diego Godoy-Rivera Jon A. Holtzman Henrik Jönsson Szabolcs Mészáros Claudia Reyes Hans-Walter Rix Matthew Shetrone Verne V. Smith Taylor Spoo Keivan G. Stassun Ji Wang |
author_sort | Marc H. Pinsonneault |
collection | DOAJ |
description | In the third APOKASC catalog, we present data for the complete sample of 15,808 evolved stars with APOGEE spectroscopic parameters and Kepler asteroseismology. We used 10 independent asteroseismic analysis techniques and anchor our system on fundamental radii derived from Gaia L and spectroscopic T _eff . We provide evolutionary state, asteroseismic surface gravity, mass, radius, age, and the data used to derive them for 12,418 stars. This includes 10,036 exceptionally precise measurements, with median fractional uncertainties in ${\nu }_{{\rm{\max }}}$ , Δ ν , mass, radius, and age of 0.6%, 0.6%, 3.8%, 1.8%, and 11.1%, respectively. We provide more limited data for 1624 additional stars that either have lower-quality data or are outside of our primary calibration domain. Using lower red giant branch (RGB) stars, we find a median age for the chemical thick disk of 9.14 ± 0.05(ran) ± 0.9(sys) Gyr with an age dispersion of 1.1 Gyr, consistent with our error model. We calibrate our red clump (RC) mass loss to derive an age consistent with the lower RGB and provide asymptotic GB and RGB ages for luminous stars. We also find a sharp upper-age boundary in the chemical thin disk. We find that scaling relations are precise and accurate on the lower RGB and RC, but they become more model dependent for more luminous giants and break down at the tip of the RGB. We recommend the use of multiple methods, calibration to a fundamental scale, and the use of stellar models to interpret frequency spacings. |
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spelling | doaj-art-8fff16a54d284d4cbf3765eb43d4e2052025-02-05T13:40:17ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492025-01-0127626910.3847/1538-4365/ad9fefAPOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler FieldsMarc H. Pinsonneault0https://orcid.org/0000-0002-7549-7766Joel C. Zinn1https://orcid.org/0000-0002-7550-7151Jamie Tayar2https://orcid.org/0000-0002-4818-7885Aldo Serenelli3https://orcid.org/0000-0001-6359-2769Rafael A. García4https://orcid.org/0000-0002-8854-3776Savita Mathur5https://orcid.org/0000-0002-0129-0316Mathieu Vrard6Yvonne P. Elsworth7Benoit Mosser8https://orcid.org/0000-0002-7547-1208Dennis Stello9https://orcid.org/0000-0002-4879-3519Keaton J. Bell10https://orcid.org/0000-0002-0656-032XLisa Bugnet11https://orcid.org/0000-0003-0142-4000Enrico Corsaro12https://orcid.org/0000-0001-8835-2075Patrick Gaulme13https://orcid.org/0000-0001-8330-5464Saskia Hekker14https://orcid.org/0000-0002-1463-726XMarc Hon15https://orcid.org/0000-0003-2400-6960Daniel Huber16https://orcid.org/0000-0001-8832-4488Thomas Kallinger17https://orcid.org/0000-0003-3627-2561Kaili Cao18https://orcid.org/0000-0002-1699-6944Jennifer A. Johnson19Bastien Liagre20https://orcid.org/0009-0008-7869-7430Rachel A. Patton21Ângela R. G. Santos22https://orcid.org/0000-0001-7195-6542Sarbani Basu23https://orcid.org/0000-0002-6163-3472Paul G. Beck24https://orcid.org/0000-0003-4745-2242Timothy C. Beers25https://orcid.org/0000-0003-4573-6233William J. Chaplin26https://orcid.org/0000-0002-5714-8618Katia Cunha27https://orcid.org/0000-0001-6476-0576Peter M. Frinchaboy28https://orcid.org/0000-0002-0740-8346Léo Girardi29https://orcid.org/0000-0002-6301-3269Diego Godoy-Rivera30https://orcid.org/0000-0003-4556-1277Jon A. Holtzman31https://orcid.org/0000-0002-9771-9622Henrik Jönsson32https://orcid.org/0000-0002-4912-8609Szabolcs Mészáros33https://orcid.org/0000-0001-8237-5209Claudia Reyes34https://orcid.org/0000-0001-9632-2706Hans-Walter Rix35https://orcid.org/0000-0003-4996-9069Matthew Shetrone36https://orcid.org/0000-0003-0509-2656Verne V. Smith37https://orcid.org/0000-0002-0134-2024Taylor Spoo38https://orcid.org/0000-0003-4019-5167Keivan G. Stassun39https://orcid.org/0000-0002-3481-9052Ji Wang40https://orcid.org/0000-0002-4361-8885Department of Astronomy, The Ohio State University , Columbus, OH 43210, USADepartment of Physics and Astronomy, California State University , Long Beach, Long Beach, CA 90840, USADepartment of Astronomy, University of Florida , Gainesville, FL 32611, USAInstitute of Space Sciences (ICE, CSIC) , Carrer de Can Magrans S/N, Campus UAB, E-08193 Bellaterra, Spain; Institut d’Estudis Espacials de Catalunya , Carrer Esteve Terradas, 1, Edifici RDIT, Campus PMT-UPC, E-08860, Castelldefels, SpainUniversité Paris-Saclay , Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, FranceInstituto de Astrofsica de Canarias (IAC) , C/Va Lactea, s/n, E-38200 La Laguna, Tenerife, Spain; Universidad de La Laguna (ULL) , Departamento de Astrofísica, E-38206 La Laguna, Tenerife, Spain; Space Science Institute , 4750 Walnut Street, Suite 205, Boulder, CO 80301, USADepartment of Astronomy, The Ohio State University , Columbus, OH 43210, USA; Observatoire de la Côte d’Azur , CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, 06304 Nice Cedex 4, FranceUniversity of Birmingham , School of Physics and Astronomy, Edgbaston, Birmingham B15 2TT, UK; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University , Ny Munkegade 120, DK-8000 Aarhus C, DenmarkLESIA, Observatoire de Paris, Université PSL , CNRS, Sorbonne Université, Université de Paris, 92195 Meudon, FranceSchool of Physics, University of New South Wales , NSW 2052, Australia; Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney , NSW 2006, Australia; ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D) , AustraliaDepartment of Physics, Queens College, City University of New York , Flushing, NY 11367, USAInstitute of Science and Technology Austria (ISTA) , Am campus 1, Klosterneuburg, AustriaINAF—Osservatorio Astrofisico di Catania , via S. Sofia 78, 95123 Catania, ItalyThüringer Landessternwarte , Sternwarte 5, 07778 Tautenburg, Germany; Department of Astronomy, MSC 4500, New Mexico State University , P.O. Box 30001, Las Cruces, NM 88003, USAStellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University , Ny Munkegade 120, DK-8000 Aarhus C, Denmark; Heidelberg University (ZAH/LSW) , Königstuhl 12, 69118 Heidelberg, Germany; Heidelberg Institute for Theoretical Studies , Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, GermanyKavli Institute for Astrophysics and Space Research , Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA; Institute for Astronomy, University of Hawai‘i , 2680 Woodlawn Drive, Honolulu, HI 96822, USASydney Institute for Astronomy (SIfA), School of Physics, University of Sydney , NSW 2006, Australia; Institute for Astronomy, University of Hawai‘i , 2680 Woodlawn Drive, Honolulu, HI 96822, USAInstitute for Astronomy, University of Vienna , Türkenschanzstrasse 17, A-1180 Vienna, AustriaCenter for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA; Department of Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USADepartment of Astronomy, The Ohio State University , Columbus, OH 43210, USA; Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USAUniversité Paris-Saclay , Université Paris Cité, CEA, CNRS, AIM, 91191, Gif-sur-Yvette, France; Instituto de Astrofsica de Canarias (IAC) , C/Va Lactea, s/n, E-38200 La Laguna, Tenerife, Spain; ENS Paris-Saclay, Université Paris-Saclay , 91190, Gif-sur-Yvette, FranceDepartment of Astronomy, The Ohio State University , Columbus, OH 43210, USA; Center for Cosmology and AstroParticle Physics (CCAPP), The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USAInstituto de Astrofísica e Ciências do Espaço , Universidade do Porto, CAUP, Rua das Estrelas, PT4150-762 Porto, Portugal; Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto , Rua do Campo Alegre 687, PT4169-007 Porto, PortugalDepartment of Astronomy, Yale University , P.O. Box 208101, New Haven CT, 06520-8101, USAInstituto de Astrofsica de Canarias (IAC) , C/Va Lactea, s/n, E-38200 La Laguna, Tenerife, Spain; Universidad de La Laguna (ULL) , Departamento de Astrofísica, E-38206 La Laguna, Tenerife, SpainDepartment of Physics and Astronomy, and JINA Center for the Evolution of the Elements University of Notre Dame , Notre Dame, IN 46556, USAUniversity of Birmingham , School of Physics and Astronomy, Edgbaston, Birmingham B15 2TT, UK; Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University , Ny Munkegade 120, DK-8000 Aarhus C, DenmarkUniversity of Arizona , Steward Observatory, Tucson, AZ 85719, USA; Observatório Nacional , São Cristóvão, Rio de Janeiro, BrazilDepartment of Physics and Astronomy, Texas Christian University , TCU Box 298840, Fort Worth, TX 76129, USA; Maunakea Spectroscopic Explorer , Canada-France-Hawaii-Telescope, Kamuela, HI 96743, USAOsservatorio Astronomico di Padova , INAF, Vicolo dell Osservatorio 5, I35122 Padova, ItalyInstituto de Astrofsica de Canarias (IAC) , C/Va Lactea, s/n, E-38200 La Laguna, Tenerife, Spain; Universidad de La Laguna (ULL) , Departamento de Astrofísica, E-38206 La Laguna, Tenerife, SpainDepartment of Astronomy, MSC 4500, New Mexico State University , P.O. Box 30001, Las Cruces, NM 88003, USAMaterials Science and Applied Mathematics, Malmö University , SE-205 06 Malmö, SwedenELTE Eötvös Loránd University , Gothard Astrophysical Observatory, Szombathely, Hungary; MTA-ELTE Lendület “Momentum” Milky Way Research Group , HungarySchool of Physics, University of New South Wales , NSW 2052, AustraliaMax Planck Institute for Astronomy , Königstuhl 17, 69117 Heidelberg, GermanyUniversity of California Observatories, University of California Santa Cruz , 1156 High Street, Santa Cruz, CA 95064, USANSF’s NOIRLab , Tucson, AZ 85719, USADepartment of Physics and Astronomy, Texas Christian University , TCU Box 298840, Fort Worth, TX 76129, USADepartment of Physics and Astronomy, Vanderbilt University , Nashville, TN 37235, USADepartment of Astronomy, The Ohio State University , Columbus, OH 43210, USAIn the third APOKASC catalog, we present data for the complete sample of 15,808 evolved stars with APOGEE spectroscopic parameters and Kepler asteroseismology. We used 10 independent asteroseismic analysis techniques and anchor our system on fundamental radii derived from Gaia L and spectroscopic T _eff . We provide evolutionary state, asteroseismic surface gravity, mass, radius, age, and the data used to derive them for 12,418 stars. This includes 10,036 exceptionally precise measurements, with median fractional uncertainties in ${\nu }_{{\rm{\max }}}$ , Δ ν , mass, radius, and age of 0.6%, 0.6%, 3.8%, 1.8%, and 11.1%, respectively. We provide more limited data for 1624 additional stars that either have lower-quality data or are outside of our primary calibration domain. Using lower red giant branch (RGB) stars, we find a median age for the chemical thick disk of 9.14 ± 0.05(ran) ± 0.9(sys) Gyr with an age dispersion of 1.1 Gyr, consistent with our error model. We calibrate our red clump (RC) mass loss to derive an age consistent with the lower RGB and provide asymptotic GB and RGB ages for luminous stars. We also find a sharp upper-age boundary in the chemical thin disk. We find that scaling relations are precise and accurate on the lower RGB and RC, but they become more model dependent for more luminous giants and break down at the tip of the RGB. We recommend the use of multiple methods, calibration to a fundamental scale, and the use of stellar models to interpret frequency spacings.https://doi.org/10.3847/1538-4365/ad9fefAsteroseismologyStellar evolutionStellar agesStellar populationsStellar pulsationsStellar masses |
spellingShingle | Marc H. Pinsonneault Joel C. Zinn Jamie Tayar Aldo Serenelli Rafael A. García Savita Mathur Mathieu Vrard Yvonne P. Elsworth Benoit Mosser Dennis Stello Keaton J. Bell Lisa Bugnet Enrico Corsaro Patrick Gaulme Saskia Hekker Marc Hon Daniel Huber Thomas Kallinger Kaili Cao Jennifer A. Johnson Bastien Liagre Rachel A. Patton Ângela R. G. Santos Sarbani Basu Paul G. Beck Timothy C. Beers William J. Chaplin Katia Cunha Peter M. Frinchaboy Léo Girardi Diego Godoy-Rivera Jon A. Holtzman Henrik Jönsson Szabolcs Mészáros Claudia Reyes Hans-Walter Rix Matthew Shetrone Verne V. Smith Taylor Spoo Keivan G. Stassun Ji Wang APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields The Astrophysical Journal Supplement Series Asteroseismology Stellar evolution Stellar ages Stellar populations Stellar pulsations Stellar masses |
title | APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields |
title_full | APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields |
title_fullStr | APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields |
title_full_unstemmed | APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields |
title_short | APOKASC-3: The Third Joint Spectroscopic and Asteroseismic Catalog for Evolved Stars in the Kepler Fields |
title_sort | apokasc 3 the third joint spectroscopic and asteroseismic catalog for evolved stars in the kepler fields |
topic | Asteroseismology Stellar evolution Stellar ages Stellar populations Stellar pulsations Stellar masses |
url | https://doi.org/10.3847/1538-4365/ad9fef |
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