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5 catalogs found
  
J/ApJ/884/107
  The BAM pipeline applied to K2 LCs of red giants (Zinn+, 2019)
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    J/ApJ/884/107/table3(c)Campaign 1 non-GAP BAM asteroseismic parameters for giants and giant candidates (104 rows)
  
J/MNRAS/469/4578
  Deep learning classification in asteroseismology (Hon+, 2017)
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    J/MNRAS/469/4578/test(c)*Population class predictions for 1008 Kepler red giants (test set) (Note) (1008 rows)
    J/MNRAS/469/4578/unclass(c)*Population class predictions for 7655 Kepler red giants (the unclassified set) (Note) (7655 rows)
  
J/MNRAS/488/572
  Bayesian hierarchical inferred inclinations (Kuszlewicz+, 2019)
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    J/MNRAS/488/572/tablef1(c)Derived inclination angles for the stars in the real sample (89 rows)
  
J/MNRAS/495/2738
  Luminosities of 34 slowly pulsating B stars (Pedersen+, 2020)
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    J/MNRAS/495/2738/table3(c)Distances determined by Bailer-Jones et al. (2018AJ....156...58B, Cat. I/347) and Anders et al. (2019A&A...628A..94A, Cat. I/349) using the Gaia parallaxes (34 rows)
    J/MNRAS/495/2738/tablea1Photometric passband filter information for available photometric data (27 rows)
    J/MNRAS/495/2738/tablee1Apparant magnitudes available for the SPB stars in each filter (34 rows)
    J/MNRAS/495/2738/tablef1Stellar parameters available from spectroscopy, the Kepler Input Catalog (KIC), and Gaia parameters provided by Anders et al. (2019A&A...628A..94A, Cat. I/349) (34 rows)
    J/MNRAS/495/2738/tableg1Luminosities derived using the statistical models 1, 2, and 3 (L1, L2, L3) based on the LTE+NLTE and LTE bolometric correction grids (34 rows)
    J/MNRAS/495/2738/tableg2Luminosities derived using 4 different methods (34 rows)
    J/MNRAS/495/2738/tableg3Luminosities derived based on the statistical model 1, 2, and 3 (L1, L2, L3) representations of the bolometric corrections, using the stellar parameters from Gaia and KIC (34 rows)
  
J/MNRAS/500/54
  Asteroseismic modelling of solar-type stars (Nsamba+, 2021)
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    J/MNRAS/500/54/table1(c)Global asteroseismic and spectroscopic parameters of our stellar sample (32 rows)
    J/MNRAS/500/54/grida(c)Stellar properties for our sample derived from grid A (34 rows)
    J/MNRAS/500/54/gridbStellar properties for our sample derived from grid B (34 rows)
    J/MNRAS/500/54/gridcStellar properties for our sample derived from grid C (34 rows)

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       (c)  indicates tables which contain celestial coordinates 
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