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Table E.2.

Summary of the properties of the AGN sample.

ID z log(Lbol/erg s−1) log(LFIR/erg s−1) log(M*/ M) log(LCO /K km s−1 pc2) SFR (M yr−1) sample
(1) (2) (3) (4) (5) (6) (7) (8)
J1333+1649* 2.089 47.91 ± 0.02 10.07 ± 0.14 2
X_N_102_35* 2.19 46.82 ± 0.02 < 9.94 2

Notes. This table is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/. Columns: (1) Source ID; (2) redshift; (3) bolometric luminosity; (4) FIR luminosity (8-1000 μm, star formation only); (5) stellar mass; (6) CO luminosity; (7) SFR derived from LFIR; (8) sample flag. Bolometric luminosity, FIR luminosity and stellar mass are derived from SED fitting (see Appendix D). SFRs are obtained from the FIR luminosity applying the Kennicutt (1998) relation corrected for a Chabrier (2003) IMF (i.e., reduced by 0.23 dex). CO luminosity LCO is derived from Eq. 1. Errors are given at 1σ. The sample flag indicates the parent sample of the targets: 1 for KASHz only, 2 for SUPER only, 3 for targets shared by the two surveys. The CO luminosity of SUPER targets (flag = 2 and 3) is taken from C21. The CO luminosity of SUPER targets shared with KASHz (flag = 3) and drawn from CDFS are from this work. The SED fitting parameters of SUPER targets (flag = 2 and 3) drawn from CDFS and COSMOS-Legacy are derived in this work (Appendix D), those of the other SUPER AGN are taken from C18 and C21. *: Bright broad-line AGN that are not considered in the analysis of Sect. 5 because missing one or more key parameters.

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