Herschel FIR counterparts of selected Lyα emitters at z ~ 2.2 - Fast evolution since z ~ 3 or missed obscured AGNs?

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Table B.2:

Number counts of LAEs redshifts 2.2 and 3.1, limited in Ly $\alpha$ luminosity and rest-frame EW.
Reference	Mean redshift	Total number	AGN-to-total fraction
Gronwall et al. (2007)	3.1	64	0.016¹
Ouchi et al. (2008)	3.1	40	0.075¹
Nilsson et al. (2009)	2.25	73	0.123¹
This work	2.2	16	0.75²

Notes. Only one AGN out of the six observed in this work is detected in X-rays (see main text).
⁽¹⁾ X-ray selected sample.
⁽²⁾ SED selected sample.

Source LaTeX | All tables | In the text

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