Hidden starbursts and active galactic nuclei at 0 < z < 4 from the Herschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedback

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201323089e]

Table 3

Multiwavelength objects in the HerMES/SWIRE/CHFTLS overlap region.

Sample	N _tot ^a	N _AGN


Radio	567	316
IRAC	28394	172
4-Channel IRAC	1107	172
VVDS Type-1 AGN	77	77
X-ray	137	130
SPIRE^b	1753	181^c

Notes.

^(a)

Brighter than the 5σ completeness limit and matched to an optical counterpart with a well-defined redshift.

^(b)

Brighter than the 3σ completeness limit and matched to an optical counterpart with a well-defined redshift.

^(c)

These numbers reflect the number of unique galaxies in which an AGN is hosted, i.e., AGNs detected using multiple diagnostics are counted only once.

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