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Article overview
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Revised Stellar Properties of Kepler Targets for the Q1-17 (DR25) Transit Detection Run | Savita Mathur
; Daniel Huber
; Natalie M. Batalha
; David R. Ciardi
; Fabienne A. Bastien
; Allyson Bieryla
; Lars A. Buchhave
; William D. Cochran
; Michael Endl
; Gilbert A. Esquerdo
; Elise Furlan
; Andrew W. Howard
; Steve B. Howell
; Howard Isaacson
; David W. Latham
; Phillip J. MacQueen
; David R. Silva
; | Date: |
14 Sep 2016 | Abstract: | The determination of exoplanet properties and occurrence rates using Kepler
data critically depends on our knowledge of the fundamental properties (such as
temperature, radius and mass) of the observed stars. We present revised stellar
properties for 197,096 Kepler targets observed between Quarters 1-17 (Q1-17),
which were used for the final transiting planet search run by the Kepler
Mission (Data Release 25, DR25). Similar to the Q1--16 catalog by Huber et al.
the classifications are based on conditioning published atmospheric parameters
on a grid of Dartmouth isochrones, with significant improvements in the adopted
methodology and over 29,000 new sources for temperatures, surface gravities or
metallicities. In addition to fundamental stellar properties the new catalog
also includes distances and extinctions, and we provide posterior samples for
each stellar parameter of each star. Typical uncertainties are ~27% in radius,
~17% in mass, and ~51% in density, which is somewhat smaller than previous
catalogs due to the larger number of improved logg constraints and the
inclusion of isochrone weighting when deriving stellar posterior distributions.
On average, the catalog includes a significantly larger number of evolved
solar-type stars, with an increase of 43.5% in the number of subgiants. We
discuss the overall changes of radii and masses of Kepler targets as a function
of spectral type, with particular focus on exoplanet host stars. | Source: | arXiv, 1609.4128 | Services: | Forum | Review | PDF | Favorites |
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