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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/ApJS/241/12
  The Asteroseismic Target List (ATL) for TESS (Schofield+, 2019)
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    J/ApJS/241/12/table1(c)The solar-like Asteroseismic Target List (ATL) (24997 rows)
  
J/ApJS/251/23
  K2 GAP DR2: campaigns 4, 6 & 7 (Zinn+, 2020)
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    J/ApJS/251/23/table2(c)*Raw asteroseismic νmax and Δν values for K2 Galactic Archaeology Program (GAP) DR2 for each pipeline, with evolutionary states (Note) (19032 rows)
    J/ApJS/251/23/table4*Derived asteroseismic νmax and Δν values for K2 GAP DR2 (Note) (4618 rows)
    J/ApJS/251/23/table6*Radius and mass coefficients (Note) (4514 rows)
  
J/MNRAS/489/4641
  APOKASC Evolutionary state of red-giant stars (Elsworth+, 2019)
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    J/MNRAS/489/4641/tablea1(c)Table of evolutionary states giving the consensus state and the individual ones for a sample of stars (6661 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)

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       (c)  indicates tables which contain celestial coordinates 
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