Connecting outflows with radio emission in active galactic nuclei at cosmic noon

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Table A.1.

Sample properties obtained from Circosta et al. (2018).

Name	RA[J2000]	Dec[J2000]	z_spec	log $\frac{L_{FIR}}{e r g s^{- 1}}$ $\frac{L_{FIR}}{erg s^{-1}}$	log $\frac{L_{bol}}{e r g s^{- 1}}$ $\frac{L_{bol}}{erg s^{-1}}$	log $\frac{L_{[2 - 10 k e V]}}{e r g s^{- 1}}$ $\frac{L_{[2-10 keV]}}{erg s^{-1}}$	log $\frac{P_{1.4 G H z}}{W H z^{- 1}}$ $\frac{P_{1.4GHz}}{W Hz^{-1}}$	q_24obs
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
J1333+1649	13:33:35.79	+16:49:03.96	2.089	-	47.91±0.02	45.81_−0.06^+0.07	28.15±0.01	-2.06
CID-346	09:59:43.41	+02:07:07.44	2.219	46.13±0.06	46.66±0.02	44.47 $_{- 0.09}^{+ 0.08}$ $^{+0.08}_{-0.09}$	24.86±0.07	0.05
XID-36	03:31:50.77	-27:47:03.41	2.259	45.84±0.02	45.70±0.06	43.84 $_{- 0.63}^{+ 0.31}$ $^{+0.31}_{-0.63}$	25.40±0.01	-1.00

Notes. (1) Target name; (2) Right ascension; (3) Declination; (4) Redshift; (5) FIR luminosity in the 8-1000 μm range; (6) AGN bolometric luminosity; (7) Absorption-corrected X-ray luminosity in the hard band (2-10 keV); (8) Radio power at 1.4 GHz; (9) q_24obs = log(S_24μm/S_r), where S_24μm and S_r are the observed 24 μm and 1.4 GHz flux densities.

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