Cross-correlations between X-ray clusters and the general galaxy population

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Volume 700 (August 2025)

A&A, 700 (2025) A271

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Table 1.

Description of the galaxy and cluster sample combinations considered.

Name	Cluster samples				Galaxy samples				Section

	z min	z max	${log}_{10} (\frac{L_{X}}{[erg / s]})$ $\log_{10}\left(\frac{L_X}{[\mathrm{erg/s}]}\right)$	N	z min	z max	${log}_{10} (\frac{M^{}}{[M_{⊙}]})$ $\log_{10}\left(\frac{M^}{[M_\odot]}\right)$	N
C0 x G1025	0.1	0.2	42.7	1650	0.1	0.2	10.25	2 255 070	3.1
& RS								1 438 690
& BC								538 145
C1 x G1075	0.1	0.3	43.1	2993	0.1	0.3	10.75	2 480 941	3.1
& RS								1 871 758
& BC								383 972
C2 x BGS	0.1	0.4	43.4	3732	–	–	–	13 881 761	3.2

Notes. N gives the total number of sources in each sample. The quantities in the ${log}_{10} (\frac{L_{X}}{[erg / s]})$ $\log_{10}\left(\frac{L_X}{[\mathrm{erg/s}]}\right)$ and ${log}_{10} (\frac{M^{*}}{[M_{⊙}]})$ $\log_{10}\left(\frac{M^*}{[M_\odot]}\right)$ columns correspond to the minimum selection thresholds applied.

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