Mining the Kepler Field: Atmospheric Parameters, Bolometric Corrections, and Luminosities

Fuente: arXiv
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Hauptverfasser: Godoy-Rivera, Diego, Grossmann, Desmond H., Richey-Yowell, Tyler, Santos, Angela R. G., Mathur, Savita, Garcia, Rafael A.
Format: Preprint
Veröffentlicht: 2026
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author Godoy-Rivera, Diego
Grossmann, Desmond H.
Richey-Yowell, Tyler
Santos, Angela R. G.
Mathur, Savita
Garcia, Rafael A.
author_facet Godoy-Rivera, Diego
Grossmann, Desmond H.
Richey-Yowell, Tyler
Santos, Angela R. G.
Mathur, Savita
Garcia, Rafael A.
contents The ~ 200,000 stars observed by the Kepler mission have provided unprecedented constraints across astrophysics. With the advent of modern spectroscopic and photometric surveys, new limits in stellar characterizations are within reach. In this work, we report a compilation of atmospheric parameters (Teff, logg, and [M/H]) for the Kepler stars by crossmatching with several spectroscopic and spectro-photometric surveys. We use these to calculate bolometric corrections, which combined with color-magnitude diagram (CMD) information from Gaia yield self-consistent luminosities on a survey-by-survey basis. These properties will aid in future explorations of Kepler data towards new astrophysical insights. We make our catalog publicly available online in Zenodo (doi:10.5281/zenodo.18620911).
format Preprint
id arxiv_https___arxiv_org_abs_2603_18152
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Mining the Kepler Field: Atmospheric Parameters, Bolometric Corrections, and Luminosities
Godoy-Rivera, Diego
Grossmann, Desmond H.
Richey-Yowell, Tyler
Santos, Angela R. G.
Mathur, Savita
Garcia, Rafael A.
Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
The ~ 200,000 stars observed by the Kepler mission have provided unprecedented constraints across astrophysics. With the advent of modern spectroscopic and photometric surveys, new limits in stellar characterizations are within reach. In this work, we report a compilation of atmospheric parameters (Teff, logg, and [M/H]) for the Kepler stars by crossmatching with several spectroscopic and spectro-photometric surveys. We use these to calculate bolometric corrections, which combined with color-magnitude diagram (CMD) information from Gaia yield self-consistent luminosities on a survey-by-survey basis. These properties will aid in future explorations of Kepler data towards new astrophysical insights. We make our catalog publicly available online in Zenodo (doi:10.5281/zenodo.18620911).
title Mining the Kepler Field: Atmospheric Parameters, Bolometric Corrections, and Luminosities
topic Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2603.18152