DOI: 10.5281/zenodo.17150017
title: The catalogs for the paper ''The bimodal distribution of donor stars in X-ray binaries''

description: 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.