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

Free Access

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

Table 4

Properties of the luminosity subsamples of the full SPIRE sample.

Sample	log (L_TIR) range	Equivalent L_TIR Class	N _total	N _spec ^a	⟨ log (L_TIR) ⟩	⟨ M_r′ ⟩	⟨ M_NUV − M_r′ ⟩

low-L_TIR	11 < log (L_TIR) < 11.5	low-lum LIRG	175	42	11.35	–21.90	3.74
moderate-L_TIR	11.5 < log (L_TIR) < 11.9	high-lum LIRG	266	52	11.70	–22.12	3.50
high-L_TIR	log (L_TIR) > 11.9	ULIRG	358	43	12.30	–22.67	3.14

Notes.

^(a)

Only VVDS galaxies are considered as ORELSE galaxies comprised ≲5% of each subsample.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.