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.6

Best-fitting parameters (from Eq. (25)) of M_min and M₁ as function of luminosity threshold corrected for passive redshift evolution to approximate stellar mass selected samples. Results are given for all and red samples, as function of redshift bins. Halo masses are given in h^-1 M_⊙.

All galaxies
		M_min			M₁
	Redshift	A	log (M_t)	α_M	A	log (M_t)	α_M

	0.2 < z < 0.4	0.203 ± 0.005	11.354 ± 0.012	0.503 ± 0.010	0.274 ± 0.017	12.756 ± 0.021	0.439 ± 0.035
	0.4 < z < 0.6	0.301 ± 0.195	11.570 ± 0.224	0.404 ± 0.149	0.269 ± 0.181	12.715 ± 0.211	0.399 ± 0.191
	0.6 < z < 0.8	0.377 ± 0.044	11.717 ± 0.063	0.352 ± 0.039	0.514 ± 0.002	12.898 ± 0.002	0.233 ± 0.002
	0.8 < z < 1.2	0.345 ± 0.006	11.731 ± 0.013	0.383 ± 0.006	0.334 ± 0.002	12.759 ± 0.005	0.335 ± 0.002


Red galaxies
		M_min			M₁
	Redshift	A	log (M_t)	α_M	A	log (M_t)	α_M

	0.2 < z < 0.4	0.706 ± 0.341	12.154 ± 0.129	0.307 ± 0.161	0.288 ± 0.009	12.930 ± 0.011	0.477 ± 0.020
	0.4 < z < 0.6	0.776 ± 0.531	12.209 ± 0.198	0.267 ± 0.241	0.552 ± 0.007	13.141 ± 0.004	0.268 ± 0.008
	0.6 < z < 0.8	0.761 ± 0.553	12.270 ± 0.233	0.302 ± 0.176	1.033 ± 0.114	13.435 ± 0.043	0.144 ± 0.036
	0.8 < z < 1.2	0.405 ± 0.429	12.037 ± 0.502	0.433 ± 0.187	0.839 ± 0.114	13.426 ± 0.083	0.188 ± 0.054

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