Open Access

Table 3

Description of the Columns in the Primary Cluster Catalog FITS File.

Column Units Description
The primary galaxy clusters and groups catalog

DETUID Unique X-ray detection no. This column should be used for matching sources with the main eRASS1 X-ray catalog by Merloni et al. (2024)
Name Cluster Name in the IAU format
RA degrees (J2000) RA of the X-ray detection
Dec degrees (J2000) Dec of the X-ray detection
RA_XFIT degrees (J2000) RA of the cluster after the image is fit with MBProj2D
Dec_XFIT degrees (J2000) Dec in degrees (J2000) of cluster after the image is fit with MBProj2D
𝓛ext Extent likelihood of the X-ray detection by ermldet
𝓛det Detection likelihood of the X-ray detection by ermldet
Exp. Average exposure in seconds
zbest Best available cluster redshift. Spectroscopic, or photometric, or literature values (see Kluge et al. 2024, for details)
Pcont Probability of the detection being contamination assigned by the mixture model
CR [300 kpc, R500] Counts s−1 Count rate in 0.2–2.3 keV within 300 kpc and R500
CTS [300 kpc, R500] Counts Total X-ray counts in 0.2–2.3 keV within 300 kpc and R500
FX [300 kpc, R500] ergs s−1 cm−2 X-ray flux in 0.2–2.3 keV within 300 kpc and R500
LX [300 kpc, R500] ergs s−1 Integrated X-ray luminosity in 0.2–2.3 keV within 300 kpc and R500
CR0520 [300 kpc, R500] Counts s−1 Count Rate in 0.5–2.0 keV within 300 kpc and R500
CTS0520 [300 kpc, R500] Counts Total X-ray counts in 0.5–2.0 keV within 300 kpc and R500
F0520 [300 kpc, R500] ergs s−1 cm−2 X-ray Flux in 0.5–2.0 keV within 300 kpc and R500
L0520 [300 kpc, R500] ergs s−1 Integrated X-ray LUMINOSITY in 0.5–2.0 keV within 300 kpc and R500
Lbol [R500] ergs s−1 Bolometric luminosity within R500
kT keV ICM temperature
Mgas ,R500${M_{{\rm{gas }},{R_{500}}}}$ Msun Calibrated cluster gas mass within R500
YX,R500${Y_{X,{R_{500}}}}$ Msun× keV The mass proxy in R500
M500 Msun Cluster total mass
M500_PDF_array Msun PDF of cluster total mass
fgas,500 Cluster gas mass fraction
R500 kpc Overdensity radius
Match name Name of the cluster if matched to a known confirmed source within 2′ radius

The cosmology sample

zλ Photometric redshift of the cluster based on the LS DR10 data
CR Counts s−1 Count rate measured at zΛ
LX ergs s−1 Integrated X-ray luminosity within R500 at zΛ
kT keV ICM temperature at zΛ
Mgas Msun Cluster gas mass within R500 at zλ
YX Msun× keV The mass proxy in R500 at zλ

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