Galaxy clustering in the CFHTLS-Wide: the changing relationship between galaxies and haloes since z ~ 1.2

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Volume 542 (June 2012)

A&A, 542 (2012) A5

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Table C.7

Best-fitting parameters (from Eqs. (29) and (30)) of b_g and log ⟨ M_halo ⟩ as function of redshift. Results are given for all and red samples.

All galaxies
		Galaxy bias b_g		Mean halo mass log ⟨ M_halo ⟩
	Redshift	a_bias	b_bias	a_h	b_h

	0.2 < z < 0.4	1.071 ± 0.006	0.211 ± 0.011	13.106 ± 0.002	0.111 ± 0.002
	0.4 < z < 0.6	1.166 ± 0.002	0.288 ± 0.003	13.002 ± 0.009	0.185 ± 0.009
	0.6 < z < 0.8	1.250 ± 0.018	0.327 ± 0.024	12.846 ± 0.011	0.202 ± 0.010
	0.8 < z < 1.2	1.430 ± 0.047	0.391 ± 0.030	12.803 ± 0.001	0.174 ± 0.001


Red galaxies
		Galaxy bias b_g		Mean halo mass log ⟨ M_halo ⟩
	Redshift	a_bias	b_bias	a_h	b_h

	0.2 < z < 0.4	1.331 ± 0.011	0.162 ± 0.017	13.368 ± 0.001	0.073 ± 0.001
	0.4 < z < 0.6	1.421 ± 0.013	0.206 ± 0.014	13.246 ± 0.002	0.092 ± 0.002
	0.6 < z < 0.8	1.572 ± 0.016	0.243 ± 0.021	13.090 ± 0.011	0.129 ± 0.009
	0.8 < z < 1.2	1.679 ± 0.049	0.375 ± 0.027	12.971 ± 0.003	0.147 ± 0.002

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