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Table A.1.

Description of the columns for the input catalogs of the eRASS1 simulation.

DESCRIPTION

NAME Input Catalogs: Clusters, AGN, Stars
SRC_ID Source ID, STAR: >= 107 < 4×108, CLUSTER: >= 4×108 and < 109, AGN: >= 109
RA Right Ascension [deg]
DEC Declination [deg]
FLUX Input Flux in the 0.5 - 2.0 keV band
tile Number of the eROSITA tile
healpix Number of the HEALPix field
ID_contam ID of the contaminating source
RA_eSASS Right Ascension of the corresponding eSASS detection [deg]
DEC_eSASS Declination of the corresponding eSASS detection [deg]
Separation Separation between the source and the corresponding eSASS detection [arcsec]
DET_LIKE_0 Detection likelihood of the corresponding eSASS detection
EXT_LIKE extension likelihood of the corresponding eSASS detection
EXT Extent of the corresponding eSASS detection
ML_CTS_0 Maximum likelihood number of counts from eSASS
ML_RATE_0 Maximum likelihood count rate from eSASS
ML_FLUX_0 Maximum likelihood flux estimate from eSASS
RADEC_ERR Positional error from eSASS
srcRAD Source radius
detected Flag to identify simulated source that are detected by eSASS
Input Catalogs: in common between Clusters and AGN
dL Luminosity distance [cm] in the cosmology adopted by Comparat et al. (2020)
nH Column density [cm−2]
redshift_R Redshift in real space
redshift_S Redshift in redshift space
FX_soft_attenuated Observed flux in the 0.5–2.0 keV band, corrected by galactic absorption
LX_soft Rest-frame X-ray luminosity in the 0.5–2.0 keV band
Bg3Model Average Value of the eSASS background maps in the nearest 20 pixels [cts/pixel]
TexpModel Average Value of the eSASS exposure maps in the nearest 20 pixels [sec]

Input Catalogs: only Clusters

g_lat Galactic latitude [deg]
g_lon Galactic longitude [deg]
HALO_pid Halo flag in the dark matter light cone (-1 for distinct halos, >0 for subhalos)
HALO_Mvir Halo mass within the virial radius [M]
HALO_Rvir Halo virial radius [kpc]
HALO_rs Halo scale radius [kpc]
HALO_M200c Halo mass within the R200c [M]
HALO_500c Halo mass within the R500c [M]
HALO_Xoff Halo offset parameter [kpc]
HALO_b_to_a_500c Halo ellipticity
kT Temperature of the cluster [keV]
R500c_kpc Halo R500c [kpc]
R500c_arcmin Halo R500c [arcmin]
EM0 Central Emissivity
LX_soft_obs Observer-frame X-ray luminosity in the 0.5–2.0 keV band
COUNTS_02_23_CLU_CLU Counts by clusters in [0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, 1.5, 2.0]×R500c_arcmin
COUNTS_02_23_CLU_AGN Counts by AGN in [0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, 1.5, 2.0]×R500c_arcmin
COUNTS_02_23_CLU_STA Counts by stars in [0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, 1.5, 2.0]×R500c_arcmin
COUNTS_02_23_CLU_BKG Counts by the background in [0.1, 0.2, 0.3, 0.4, 0.5, 0.6, 0.7, 0.8, 0.9, 1.0, 1.5, 2.0]×R500c_arcmin
ErsenModel Average Value of the eSASS sensitivity maps for extended sources in the nearest 20 pixels [erg/s/cm2]

Input Catalogs: only AGN

LX_hard Rest-frame X-ray luminosity in the 2.0-10.0 keV band
galaxy_SMHMR_mass Host galaxy stellar mass
COUNTS_02_23_AGN_AGN Counts by AGN in [10, 20, 30, 40, 50, 60] arcsec
COUNTS_02_23_AGN_CLU Counts by clusters in [10, 20, 30, 40, 50, 60] arcsec
COUNTS_02_23_AGN_STA Counts by stars in [10, 20, 30, 40, 50, 60] arcsec
COUNTS_02_23_AGN_BKG Counts by the background in [10, 20, 30, 40, 50, 60] arcsec

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