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Table 1.

Global properties of the galaxies studied in this work.

ID RA Dec z(a) (b) (c) M⋆(d) SFR(Hα) (e) sSFR (f) SFRB(g) sSFRB(g)
J0006+0255 00:06:06.53 02:55:04.13 0.09382828 1.59 2.85 8.48 1.118 −8.43 1.158 −8.42
J0028+3035 00:28:33.55 30:35:54.14 0.07451165 2.65 3.88 8.59 0.707 −8.74 0.660 −8.77
J0131+0210 01:31:38.15 02:10:14.58 0.05806014 2.12 2.44 6.66 0.564 −6.91 0.577 −6.90
J0138+1114 01:38:27.65 11:14:34.45 0.06219218 1.43 1.77 6.95 1.228 −6.86 1.271 −6.85
J0150+1643 01:50:46.25 16:43:26.43 0.05909079 1.65 1.94 7.82 1.316 −7.70 1.281 −7.71
J0744+1858 07:44:52.39 18:58:30.01 0.05227381 3.35 3.53 8.25 1.272 −8.14 1.265 −8.14
J0753+2820 07:53:25.26 28:20:12.74 0.06752457 3.94 5.24 8.35 0.867 −8.41 0.821 −8.43
J0809+4918 08:09:42.74 49:18:21.46 0.07809167 1.72 2.63 8.40 1.470 −8.23 1.447 −8.24
J1037+2325 10:37:28.61 23:25:29.81 0.01058074 5.27 1.21 7.10 0.009 −9.13 0.009 −9.13
J1109+3429 11:09:20.89 34:29:02.90 0.06697157 2.48 3.31 8.83 0.662 −9.01 0.649 −9.02
J1141+6059 11:41:46.74 60:59:43.13 0.01096911 6.93 1.46 6.88 0.027 −8.45 0.026 −8.47
J1311+3750 13:11:35.82 37:50:58.73 0.05381261 3.95 4.24 7.70 1.657 −7.48 1.643 −7.48
J1313+6044 13:13:31.26 60:44:54.52 0.07113630 2.52 3.52 8.11 3.104 −7.62 2.871 −7.65
J1338+4213 13:38:42.16 42:13:38.20 0.00863322 2.83 0.52 6.20 0.011 −8.16 0.011 −8.16
J1411+0550 14:11:13.40 05:50:35.07 0.04940260 1.61 1.58 7.99 1.715 −7.75 1.607 −7.78
J1528+2318 15:28:26.53 23:18:43.10 0.05948849 2.97 3.56 8.54 0.705 −8.69 0.665 −8.71
J1556+1818 15:56:47.51 18:18:25.57 0.09052273 2.28 3.94 7.82 1.964 −7.53 2.041 −7.51
J1608+0413 16:08:01.16 04:13:23.85 0.06322286 1.50 1.89 7.42 0.690 −7.58 0.640 −7.61

Notes.

(a)

Redshifts z adopted from the SDSS SkyServer at http://skyserver.sdss.org/.

(b)

r-band petrosian radii in arcsec taken from http://skyserver.sdss.org/.

(c)

r-band petrosian radii converted to linear scales (kpc).

(d)

Logarithm of the stellar mass in units of M⊙ as derived by FADO assuming a Kroupa (2001) IMF.

(e)

Star formation rate in units of M⊙ yr−1.

(f)

Logarithm of the sSFR, i.e. the SFR divided by stellar mass.

(g)

Based on corrected Hα values, see Sect. 4.4.

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