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 6

Fraction of galaxies and AGN hosts detected in SPIRE.

Sample	N	f _SB


All optical^a	⟨ 32 ⟩	⟨ 5.8 ⟩ ± 1.2%
Radio-starburst	146	58.2 ± 4.8%
4-channel IRAC	498	45.0 ± 2.0%
IR AGN	62	36.1 ± 4.6%
VVDS Type-1 AGN	10	13.0 ± 4.1%
X-ray AGN	26	20.0 ± 3.9%
Radio AGN	132	41.8 ± 3.6%
All AGN^b	181	32.3 ± 2.4%

Notes.

^(a)

The numbers here reflect the mean number and rate of SPIRE detections for hosts of (largely) dormant nuclei that were matched in sample size, ℳ_∗, and z to the “All AGN" sample, see Appendix B.

^(b)

This subsample is comprised of unique galaxies in which an AGN is hosted, i.e., AGNs detected using multiple diagnostics are counted only once.

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