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 5

Composite spectral properties of the luminosity subsamples of the full SPIRE sample.

Sample	⟨ EW( [ OII ]) ⟩	⟨ EW(Hδ) ⟩ ^a	⟨ D_n(4000) ⟩ ^b	⟨ A/K ⟩	⟨ E(B − V) ⟩


low-L_TIR	–8.63 ± 0.14 Å	4.11 (4.30) ± 0.11 Å	1.284 ± 0.003 (1.224 ± 0.004)	0.73	0.661 ± 0.005
moderate-L_TIR	–14.47 ± 0.13 Å	3.80 (4.12) ± 0.10 Å	1.137 ± 0.002 (1.081 ± 0.003)	1.65	0.703 ± 0.004
high-L_TIR	–14.99 ± 0.15 Å	6.77 (7.09) ± 0.14 Å	1.115 ± 0.003 (1.050 ± 0.004)	9.00	0.807 ± 0.005

Notes.

^(a)

The numbers given in parentheses are EW(Hδ) values corrected for emission infill (see text).

^(b)

The numbers given in parentheses are D_n(4000) values corrected for extinction (see text).

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