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Table A.3.

Derived parameters for the H I 21 cm non-detections.

Source z Sν (int) Sν (peak) Δs τ NHI L1.4 GHz LUV Continuum
(mJy) (mJy beam−1) (mJy beam−1) (cm−2) W Hz−1 W Hz−1 morphology
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
SDSS J003058+011600 0.3748 416.3 189.0 1.0 0.017 20.22 25.92 - e
SDSS J075622+355442 0.3191 506.25 130.0 0.7 0.017 20.21 25.6 22.83 e
SDSS J083825+371037 0.3962 482.2 442.4 0.6 0.004 19.63 26.34 21.00 c
SDSS J102844+384437 0.3621 787.0 600.0 0.7 0.003 19.53 26.39 20.74 e
SDSS J110655+190912 0.3400 970.0 190.0 1.0 0.016 20.2 25.83 19.81 e
SDSS J112342+125214 0.3178 273.2 204.6 1.1 0.016 20.19 25.8 20.98 e
SDSS J112833+324323 0.3695 393.0 371.3 1.5 0.012 20.08 26.2 20.03 c
SDSS J114409+005436 0.2955 335.0 350.0 1.0 0.008 19.92 25.97 21.47 c
SDSS J115324+493109 0.3339 2060.0 1000.0 0.9 0.002 19.43 26.53 23.20 e
SDSS J123413+475351 0.3736 372.4 353.2 0.6 0.005 19.73 26.19 22.73 c
SDSS J140416+411749 0.3604 300.0 272.5 1.0 0.012 20.06 26.04 20.9 c
SDSS J140854+302103 0.2897 393.0 235.4 0.6 0.008 19.89 25.77 20.44 e
SDSS J145338+035933 0.3697 475.0 421.5 0.7 0.005 19.69 26.25 22.34 e
SDSS J145859+041614 0.3916 940.0 250.0 0.9 0.011 20.02 26.08 21.67 e
SDSS J150720+364245 0.3837 539.0 482.0 0.9 0.005 19.75 26.35 22.89 e
SDSS J152503+110744 0.3326 537.6 512.2 0.6 0.004 19.59 26.24 - c
SDSS J153617+462734 0.3696 308.7 198.4 0.4 0.007 19.86 25.93 20.86 e
SDSS J162214+090421 0.2917 356.3 256.5 0.5 0.006 19.81 25.81 20.49 e
SDSS J164734+270558 0.2822 650.0 470.0 0.5 0.003 19.51 26.04 21.10 e
SDSS J165547+232931 0.3931 318.7 312.3 0.7 0.006 19.82 26.18 20.6 c
SDSS J172109+354216 0.2832 228.4 212.11 0.6 0.008 19.91 25.7 22.59 c
SDSS J085451+621850 0.2673 RFI
SDSS J111141+355337 0.3048 RFI
SDSS J114539+442022 0.2997 RFI

Notes. The columns are: (1) Source name, (2) SDSS DR13 redshift, (3) Integrated radio continuum flux in mJy, (4) Peak flux density in mJy beam−1, (5) RMS noise on the spectrum in mJy beam−1 after Hanning smoothing it to a spectral resolution close to 50 km s−1, (6) 3σ optical depth limit, (7) 3σ limit on the H I column density in log scale estimated assuming a Tspin = 100 K and cf = 1, (8) Rest-frame 1.4GHz radio luminosity in log scale, (9) Rest-frame UV luminosity in log scale, (10) Continuum morphology as seen in our observations: e is extended; c is compact. Sources with the ratio Sν(peak)/Sν(int) > 0.9 were considered compact and the rest extended sources. The UV luminosity was estimated using the SDSS u- and g-band magnitudes. The values are left blank where the photometry was not available.

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