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Home All issues Volume 507 / No 2 (November IV 2009) A&A, 507 2 (2009) 747-756 Full HTML
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Table 3:

IR properties of the X-ray selected Compton-thick AGN.
ID z $3.6~\mu$m $4.5~\mu$m $5.8~\mu$m 8.0 $\mu $m $24~\mu$m R-[24] $\log L_{\rm IR} $ Comments
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
35 2.203 - - - - - - $12.95^{\dagger} $ sub-mm, oSFR
91 0.51 - - - - - - -  
92 0.91 17.82 17.07 16.64 16.27 160.6 14.16 11.15 irAGN
107 0.59 18.54 17.49 16.47 15.45 325.3 16.1 10.73 irSFR
121 0.520 - - - - - - - -
127 1.014 - - - - - - -  
135 2.466 17.91 17.05 16.31 15.97 376.4 13.88 11.6 sub-mm, oSFR, irSFR
171 1.993 17.86 17.09 15.92 14.38 801.1 7 13.60 12.96 sub-mm, oAGN, irAGN
190 2.005 16.60 15.64 14.53 13.33 1426.0 14.32 13.06 sub-mm, oAGN, irAGN
191 0.276 16.08 15.81 15.55 14.77 - - 10.96 irSFR

The columns are: (1) Alexander ID number; (2) redshift; three and two decimal numbers refer to spectroscopic and photometric redshift respectively; (3) 3.6 $\mu $m flux in units of $\mu $Jy; (4) 4.5 $\mu $m flux in units of $\mu $Jy; (5) 5.8 $\mu $m flux in units of $\mu $Jy; (6) 8.0 $\mu $m flux in units of $\mu $Jy; (7) 24 $\mu $m flux in units of $\mu $Jy; (8) R-[24] colour (Vega); (9) logarithm of the total IR luminosity in units of $L_\odot$; (10) comments: sub-mm denotes that the source is a sub-mm galaxy in the sample of Chapman et al. (2005); irAGN or irSFR denotes whether the source has been classified as a star-forming galaxy or an AGN according to the IR-SED fit; oAGN or oSFR denotes that the source has been classified as an AGN or a starburst according to the optical spectrum of Chapman et al. (2005); $\dagger$: luminosity from Chapman et al. (2005).


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