VizieR Online Data Catalog: Kepler asteroseismic LEGACY sample. II. (Silva Aguirre+, 2017)

V. Silva Aguirre (1) , M. N. Lund , H. M. Antia (2) , W. H. Ball (3) , S. Basu (4) , J. Christensen-Dalsgaard (5) , Y. Lebreton (6, 7) , D. R. Reese (8) , K. Verma (9) , L. Casagrande (10) , A. B. Justesen , J. R. Mosumgaard , W. J. Chaplin (11) , T. R. Bedding (12) , G. R. Davies (13) , R. Handberg (14) , G. Houdek (15) , D. Huber (12) , H. Kjeldsen (14) , D. W. Latham , T. R. White , H. R. Coelho (16) , A. Miglio (8) , B. Rendle

1 KITP - Kavli Institute for Theoretical Physics [Santa Barbara]
2 TIFR - Tata Institute for Fundamental Research
3 PMOD/WRC - Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center
4 GREGH - Groupement de Recherche et d'Etudes en Gestion à HEC
5 OHP - Observatoire de Haute-Provence
6 IPR - Institut de Physique de Rennes
7 LESIA (UMR_8109) - Laboratoire d'études spatiales et d'instrumentation en astrophysique
8 Institut d'Astrophysique et de Géophysique [Liège]
9 LRR-TUM - Institut für Informatik
10 RSAA - Research School of Astronomy and Astrophysics [Canberra]
11 School of Physics and Astronomy
12 SIfA - Sydney Institute for Astronomy
13 University of Birmingham [Birmingham]
14 Department of Physics and Astronomy [Aarhus]
15 Institute for Astronomy [Vienna]
16 University of Exeter

The 66 stars comprising the LEGACY sample were chosen from more than 500 main-sequence and subgiant targets in which Kepler detected oscillations (Chaplin+ 2014, J/ApJS/210/1). We selected all targets that had more than one year of short-cadence observations, and where inspection of the power spectrum did not reveal any clear signature of bumped l=1 modes. (3 data files).

Mots clés: Stars: masses; Stars: ages; Stars: diameters; Stars: distances; Abundances

Domaines: Physique [physics]; Astrophysique stellaire et solaire [astro-ph.SR]

V. Silva Aguirre, M. N. Lund, H. M. Antia, W. H. Ball, S. Basu, et al.. VizieR Online Data Catalog: Kepler asteroseismic LEGACY sample. II. (Silva Aguirre+, 2017). 2017. ⟨hal-02386902⟩