The VIMOS Public Extragalactic Redshift Survey (VIPERS) - Luminosity and stellar mass dependence of galaxy clustering at 0.5 < z < 1.1

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Volume 557 (September 2013)

A&A, 557 (2013) A17

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Table 1

Properties of the selected VIPERS sub-samples in threshold luminosity bins.

Redshift	Median	Magnitude range	Median magnitude	N _gal	r ₀	γ	Bias
range	redshift	M_B(z = 1.1) − 5log (h)	M_B − 5log (h)		[h^-1 Mpc ]

[0.5, 0.7]	0.62	< − 19.5	−19.87	17 473	4.45 ± 0.20	1.67 ± 0.05	1.36 ± 0.13
[0.5, 0.7]	0.62	< − 20.0	−20.15	12 432	4.81 ± 0.21	1.69 ± 0.05	1.44 ± 0.14
[0.5, 0.7]	0.62	< − 20.5	−20.49	7472	5.22 ± 0.29	1.73 ± 0.06	1.53 ± 0.17
[0.5, 0.7]	0.62	< − 21.0	−20.86	3599	5.58 ± 0.39	1.81 ± 0.08	1.60 ± 0.19
[0.5, 0.7]	0.62	< − 21.5	−21.28	1236	6.24 ± 0.56	1.79 ± 0.14	1.73 ± 0.24

[0.7, 0.9]	0.79	< − 20.0	−20.41	14 442	4.56 ± 0.22	1.65 ± 0.04	1.50 ± 0.12
[0.7, 0.9]	0.80	< − 20.5	−20.68	9469	4.95 ± 0.23	1.67 ± 0.04	1.59 ± 0.11
[0.7, 0.9]	0.80	< − 21.0	−21.05	4605	5.32 ± 0.30	1.70 ± 0.05	1.67 ± 0.12
[0.7, 0.9]	0.80	< − 21.5	−21.45	1619	5.95 ± 0.39	1.72 ± 0.10	1.79 ± 0.15

[0.9, 1.1]	0.97	< − 20.5	−21.00	5207	4.29 ± 0.19	1.63 ± 0.04	1.58 ± 0.11
[0.9, 1.1]	0.98	< − 21.0	−21.25	3477	5.08 ± 0.26	1.64 ± 0.05	1.79 ± 0.12
[0.9, 1.1]	0.99	< − 21.5	−21.65	1409	5.87 ± 0.43	1.68 ± 0.08	2.04 ± 0.19

Notes. The best-fit values of the clustering normalization, r₀, and slope, γ, have been obtained by fitting w_p(r_p) in 0.2 < r_p [h^-1 Mpc ] < 20. The errors are from the scatter among the HOD VIPERS mocks. The bias values assume a flat ΛCDM model with Ω_M = 0.25 and σ₈ = 0.8.

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