The VIMOS Public Extragalactic Redshift Survey (VIPERS) - Never mind the gaps: comparing techniques to restore homogeneous sky coverage

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Volume 565 (May 2014)

A&A, 565 (2014) A67

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Table 2

Values of the 16%, 50% and 84% of all the distributions of shown in Fig. 8 (ZADE), and the corresponding values obtained with LNP.


Redshift	Method	1st 20%			3rd 20%			5th 20%
		16%	50%	84%	16%	50%	84%	16%	50%	84%


R = 5 h^-1 Mpc

0.5 < z < 0.7	LNP	0.0	0.0	0.25	0.0	0.46	1.06	1.18	2.42	4.51
	ZADE	0.0	0.0	0.25	0.1	0.46	1.01	1.31	2.50	4.53

0.7 < z < 0.9	LNP	0.0	0.0	0.44	0.0	0.43	1.09	0.94	2.39	4.88
	ZADE	0.0	0.0	0.44	0.0	0.42	0.95	1.09	2.49	4.89

0.9 < z < 1.1	LNP	0.0	0.0	0.0	0.0	0.0	1.19	0.50	2.32	5.67
	ZADE	0.0	0.0	0.0	0.0	0.0	1.16	1.10	2.39	5.72


R = 8 h^-1 Mpc

0.5 < z < 0.7	LNP	0.0	0.14	0.34	0.38	0.66	1.05	1.44	2.20	3.50
	ZADE	0.0	0.14	0.31	0.41	0.67	1.01	1.54	2.24	3.53

0.7 < z < 0.9	LNP	0.0	0.11	0.35	0.30	0.62	1.12	1.36	2.25	3.57
	ZADE	0.0	0.10	0.32	0.32	0.62	1.07	1.47	2.29	3.61

0.9 < z < 1.1	LNP	0.0	0.0	0.37	0.01	0.52	1.19	1.18	2.31	4.10
	ZADE	0.0	0.0	0.30	0.13	0.52	1.11	1.30	2.37	4.14

Notes. These values are given as mean values among all the used mock catalogues. Their typical rms is on the order of 5–10% for R₅. For R₈, the typical rms is on the order of 5–10% for the first and third quintiles, and on the order of 2–3% in the highest density quintile.

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