The catalogs for the paper ''The bimodal distribution of donor stars in X-ray binaries''

The compressed file contains four catalogs, which are associated with the paper "The bimodal distribution of donor stars in X-ray binaries" 1. "Table1_all3964_Identical to the table within the paper.fits" This file is identical to Table 3 in the paper. It is the complete X-ray binary catalog of 3964 objects, which includes basic information such as the star name, coordinates and their errors (from the Simbad database), the X-ray binary type, and the bibcodes for the coordinate and type references. Parameters Unit Description Name Star name from Simbad RA deg Right Ascension from Simbad DEC deg Declination from Simbad COO_ERR_MAJA sec major axis of the error ellipse from Simbad COO_ERR_MINA sec the minor axis of the error ellipse from Simbad type type of XRBs (HXB or LXB) COO_BIBCODE_ref reference BIBCODE for the coordinates type_BIBCODE_ref reference BIBCODE for the type of XRBs 2. "Table2_pars288_Identical to the table within the paper.fits" This file is identical to Table 4 in the paper. The first four columns contain the results of the cross-matching with Gaia DR3. The subsequent five columns list the absolute parameters that we determined based on atmospheric parameters and the MIST stellar evolution model. The final parameter is the orbital period from F. Fortin et al. (2023), A. Avakyan et al. (2023), and M. Neumann et al. (2023). Parameters Unit Description Name Star name from Simbad Teff K Effective temperature from GSP-Phot Aeneas best library using BP/RP spectra b_Teff K Lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra B_Teff K Upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra logg dex (cm/s2) Surface gravity from GSP-Phot Aeneas best library using BP/RP spectra b_logg dex (cm/s2) Lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra B_logg dex (cm/s2) Upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra [Fe/H] dex Iron abundance from GSP-Phot Aeneas best library using BP/RP spectra b_[Fe/H] dex Lower confidence level (16%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra B_[Fe/H] dex Upper confidence level (84%) of iron abundance from GSP-Phot Aeneas best library using BP/RP spectra Mass solar mass Mass derived based on atmoshperic parameters (Teff, logg, [Fe/H]) by MIST model Mass_lower solar mass Lower confidence level (16%) of Mass Mass_upper solar mass Upper confidence level (84%) of Mass Radius solar radius Radius derived based on atmoshperic parameters (Teff, logg, [Fe/H]) by MIST model Radius_lower solar radius Lower confidence level (16%) of Radius Radius_upper solar radius Upper confidence level (84%) of radius L solar luminosity Luminosity derived based on atmoshperic parameters (Teff, logg, [Fe/H]) by MIST model L_lower solar luminosity Lower confidence level (16%) of Luminosity L_upper solar luminosity Upper confidence level (84%) of Luminosity Age Gyr Age derived based on atmoshperic parameters (Teff, logg, [Fe/H]) by MIST model Age_lower Gyr Lower confidence level (16%) of Age Age_upper Gyr Upper confidence level (84%) of Age EEP Equivalent evolutionary point EEP_lower Lower confidence level (16%) of EEP EEP_upper Upper confidence level (16%) of EEP Period day binary orbital period (Below are the extended versions of the two tables above, with additional parameters added.) 3. "Table1_all3964_with extra parameters.fits" This file is an enhanced version of Table 3 from the paper. It includes additional parameters from Simbad, F. Fortin et al. (2023), A. Avakyan et al. (2023), M. Neumann et al. (2023), and the International Variable Star Index (VSX). 4. "Table2_pars288_with extra parameters.fits" This file is an enhanced version of Table 4 from the paper. It includes additional parameters from Simbad, F. Fortin et al. (2023), A. Avakyan et al. (2023), M. Neumann et al. (2023), the International Variable Star Index (VSX), as well as the absolute parameters we determined from the PARSEC model.