Quenching of the star formation activity in cluster galaxies

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Table 2

Uncertainties in the different photometric and spectroscopic bands.

Band	Instrument	Uncertainty	Ref.

FUV	GALEX	15%	1
NUV	GALEX	15%	1
g	SDSS	15%	1
r	SDSS	15%	1
i	SDSS	15%	1
J	2MASS	15%	2
H	2MASS	15%	2
K	2MASS	15%	2
8 μm^a	IRAC/Spitzer	15%	3
11 μm	WISE	6%	3
22 μm	WISE	13%	3
24 μm^a	MIPS/Spitzer	4%	4
70 μm^a	MIPS/Spitzer	10%	4
100 μm	PACS/Herschel	16%	5
160 μm	PACS/Herschel	12%	5
250 μm	SPIRE/Herschel	6%	6
350 μm	SPIRE/Herschel	8%	6
500 μm	SPIRE/Herschel	11%	6
Hα	SPM	15%	7
Hβ	OHP	15%	8
Hγ	OHP	15%	8
Hδ	OHP	15%	8

Notes.

^(a)

Available only for a fraction of the analysed galaxies.

Reference. (1) Cortese et al. (2012b); (2) Jarrett et al. (2003); (3) Ciesla et al. (2014); (4) Bendo et al. (2012); (5) Cortese et al. (2014); (6) Ciesla et al. (2012); (7) Boselli et al. (2015); (8) Boselli et al. (2013).

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