J/A+A/696/A243      Kepler Field with Gaia DR3             (Godoy-Rivera+, 2025)

Kepler meets Gaia DR3: Homogeneous extinction-corrected color-magnitude diagram and binary classification. Godoy-Rivera D., Mathur S., Garcia R.A., Pinsonneault M.H., Santos A.R.G., Beck P.G., Grossmann D.H., Schimak L., Bedell M., Merc J., Escorza A. <Astron. Astrophys. 696, A243 (2025)> =2025A&A...696A.243G 2025A&A...696A.243G (SIMBAD/NED BibCode)
ADC_Keywords: Stars, double and multiple ; Stars, variable ; Binaries, eclipsing ; Binaries, spectroscopic ; Stars, dwarfs ; Stellar distribution ; Stars, distances Keywords: methods: data analysis - catalogs - binaries: general - stars: evolution - Hertzsprung-Russell and C-M diagrams - stars: variables: general Abstract: The original Kepler mission has delivered unprecedented high-quality photometry. These data have impacted numerous research fields (e.g., asteroseismology and exoplanets), and continue to be an astrophysical goldmine. Because of this, thorough investigations of the ∼200000 stars observed by Kepler remain of paramount importance. In this paper, we present a state-of-the-art characterization of the Kepler targets based on Gaia DR3 data. We placed the stars on the color-magnitude diagram (CMD), accounted for the effects of inter- stellar extinction, and classified targets into several CMD categories (dwarfs, subgiants, red giants, photometric binaries, and others). Additionally, we report various categories of candidate binary systems spanning a range of detection methods, such as renormalised unit weight error, radial velocity variables, Gaia non-single stars, Kepler and Gaia eclipsing binaries from the literature, among others. First and foremost, our work can assist in the selection of stellar and exoplanet host samples regarding CMD and binary populations. We further complemented our catalog by quantifying the impact that astrometric differences between Gaia data releases have on CMD location, assessing the contamination in asteroseismic targets with properties at odds with Gaia, and identifying stars flagged as photometrically variable by Gaia. We make our catalog publicly available as a resource to the community when researching the stars observed by Kepler. Description: In this work, we perform a color-magnitude (CMD) diagram and binary characterization of the ∼200,000 stars observed by the Kepler mission using the Gaia DR3 data and complementary data bases. The derived CMD classifications and binary categories are reported, together with CMD locations and other properties derived throughout the paper. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 714 196762 Kepler-Gaia DR3 catalog tablef1.dat 40 1265 Coordinates of the color-magnitude diagram regions -------------------------------------------------------------------------------- See also: V/133 : Kepler Input Catalog (Kepler Mission Team, 2009) I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022) IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 I8 --- KIC KIC ID (KIC) 10- 28 I19 --- GaiaDR3 Gaia DR3 Source ID (GaiaDR3) 30- 38 I9 --- TIC ? TIC ID (TIC) 40- 56 A17 --- 2MASS 2MASS ID (2MASS) 58- 79 E22.20 mas plxc ? Parallax corrected for zero-point effect (parallax_corrected) 81-100 F20.18 mas e_plxc ? Parallax error corrected for inflation factor (eparallaxcorrected) 102-124 F23.15 pc Dist ? Distance (distance) 126-156 F31.19 pc e_Dist ? Distance error (e_distance) 158-163 F6.1 K Teffg-S ? gspspec temperature (Teff_gspspec) 165-170 F6.1 K bTeffg-S ? 16th percentile of gspspec temperature (Teffgspspec16th) 172-178 F7.1 K BTeffg-S ? 84th percentile of gspspec temperature (Teffgspspec84th) 180-198 F19.17 [cm/s2] loggg-S ? Calibrated gspspec surface gravity (logggspspeccalibrated) 200-204 F5.2 [cm/s2] bloggg-S ? 16th percentile of gspspec surface gravity (logggspspec16th) 206-209 F4.2 [cm/s2] Bloggg-S ? 84th percentile of gspspec surface gravity (logggspspec84th) 211-233 E23.20 [-] [M/H]-S ? Calibrated gspspec metallicity ([M/H]gspspeccalibrated) 235-239 F5.2 [-] b[M/H]-S ? 16th percentile of gspspec metallicity ([M/H]gspspec16th) 241-245 F5.2 [-] B[M/H]-S ? 84th percentile of gspspec metallicity ([M/H]gspspec84th) 247-249 A3 --- Qualg-S [f fm fmb] gspspec quality sample(s) if any (Quality_gspspec) 251-357 A107 --- FlQualcuts Identifies failed quality criteria if any (Flagqualitycuts) 359-368 F10.7 mag Gmag G band magnitude (raw) (G) 370-383 F14.11 mag BP-RP ? BP-RP color (raw) (BPmRP) 385-406 E22.19 mag G0MAG ? Absolute de-reddened G band magnitude (MG0) 408-430 E23.15 mag BP-RP0 ? De-reddened (BP-RP) color (BPmRP_0) 432-452 F21.19 mag e_G0MAG ? Absolute de-reddened G band magnitude error (eMG_0) 454-474 F21.19 mag e_BP-RP0 ? De-reddened (BP-RP) color error (eBPmRP0) 476-482 F7.5 mag ExtA0 ? Monochromatic extinction (extinction_A0) 484-504 F21.19 mag e_ExtA0 ? Monochromatic extinction error (eextinctionA0) 506-527 A22 --- FlagCMD Identifies CMD category (Flag_CMD) 529-533 F5.3 --- ProbCMD ? Probability of CMD category (Probability_CMD) 535-539 F5.3 --- ProbCMDmh ? Probability of CMD category including metallicity standard deviation (ProbabilityCMDmh) 541 I1 --- FlMetPoTail [0/1] Identifies targets in the metal-poor distribution tail (FlagMetalPoorTail) 543 I1 --- FlMetRiTail [0/1] Identifies targets in the metal-rich distribution tail (FlagMetalRichTail) 545-567 E23.19 mag DMGmag0 ? Magnitude difference to lower CMD envelope (DeltaMGmag0) 569-579 F11.8 --- RUWE ? Renormalised Unit Weight Error (RUWE) 581 I1 --- FlRUWE [0/1] Identifies targets with RUWE≥1.4 (Flag_RUWE) 583 I1 --- FlRVvar [0/1] Identifies targets classified as RV Variable (Flag_RVvariable) 585 I1 --- FlNSS [0/1] Identifies targets in NSS tables (Flag_NSS) 587-611 A25 --- NSSBinType Binary type from NSS (NSSBinaryType) 613-618 A6 --- NSStables Union of acronyms of NSS tables (NSS_tables) 620 I1 --- FlEBKepler [0/1] Identifies Kepler eclipsing binaries (FlagEBKepler) 622 I1 --- FlEBGaia [0/1] Identifies Gaia eclipsing binaries (FlagEBGaia) 624 I1 --- FlGaiaVarBin [0/1] Identifies Gaia variable binaries (FlagGaiaVariable_Binaries) 626 I1 --- FlSB9 [0/1] Identifies targets in the SB9 catalog (Flag_SB9) 628 I1 --- FlNEAsysnum [0/1] Identifies multiple systems from NEA (FlagNEAsy_snum) 630 I1 --- NEAsysnum [1/4]? sy_snum value from NEA database (NEAsysnum) 632 I1 --- FlHGCAHchi2 [0/1] Identifies targets with Hipparcos-Gaia chi2>11.8 (FlagHGCAHighchi2) 634 I1 --- FlWDS [0/1] Identifies targets in the WDS catalog (Flag_WDS) 636-645 A10 --- WDS Name in the WDS catalog (WDS) 647 I1 --- FlBinUnion [0/1] Union of the ten non- CMD binary flags (FlagBinaryUnion) 649-671 E23.20 mag DeltaDM ? Distance modulus difference (DR3-DR2) (Delta_DM) 673 I1 --- FlDeltaDM [0/1]?=- Identifies changes in Flag_CMD due to Delta_DM (FlagDeltaDM) 675-687 A13 --- FlPhotVar Photvariableflag from Gaia DR3 (Flagphotometricvariability) 689-714 A26 --- PhotVClass ? Bestclassname from Gaia DR3 (photometricvariabilityclass) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablef1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 22 A22 --- Region CMD region (Region) 24- 31 F8.5 mag BP-RP0 De-reddened (BP-RP) color (BPmRP_0) 33- 40 F8.5 mag G0MAG Absolute de-reddened G band magnitude (MG0) -------------------------------------------------------------------------------- Acknowledgements: Diego Godoy-Rivera, diego.godoy.rivera(at)iac.es
(End) Patricia Vannier [CDS] 28-Mar-2025
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line