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Table 1.

Coordinates, redshifts, distances, and integrated characteristics of selected galaxies.

Name RA(2000.0) Dec.(2000.0) z DLa DAb 12+logO/H O32 log(M/M)c MFUVd SFRe
J0232+0025 02:32:29.50 +00:25:04.28 0.7641 4803 1543 8.13 5.8 9.41 −21.37 45
J0256+0122 02:56:58.26 +01:22:45.80 0.8867 5773 1622 7.95 2.8 8.84 −21.62 53
J0815+2942 08:15:53.71 +29:42:29.40 0.9141 5994 1636 8.36 1.9 10.01 −21.26 34
J0837+4512 08:37:58.69 +45:12:33.28 0.7816 4939 1556 7.93 3.6 8.18 −21.23 157
J0901+5111 09:01:38.28 +51:11:46.58 0.6374 3844 1434 7.99 6.4 9.20 −20.12 29
J0908+4626 09:08:25.75 +46:26:50.46 0.8148 5199 1579 8.16 4.0 9.55 −21.18 53
J0955+3935 09:55:28.37 +39:35:53.11 0.8293 5314 1588 7.83 2.7 10.09 −21.03 44
J1021+0436 10:21:40.54 +04:36:47.80 1.0053 6745 1677 8.42 5.1 10.67 −22.64 126
J1252+5237 12:52:31.39 +52:37:16.41 0.6225 3735 1419 7.98 4.3 8.43 −21.38 41
J1358+4611 13:58:06.75 +46:11:43.19 0.6195 3713 1416 8.06 2.8 9.22 −21.65 51
J1450+3913 14:50:29.88 +39:13:21.83 0.6145 3676 1410 8.11 3.5 9.85 −20.98 35

Notes. aLuminosity distance in Mpc (NED, Wright 2006). bAngular size distance in Mpc (NED, Wright 2006). cStellar mass M in solar units. dRest-frame absolute magnitude at λ = 1500 Å derived from an SED fitting of the SDSS spectrum and an extrapolation of the SED to the UV range. eStar-formation rate in units of M yr−1 derived from the extinction-corrected Hβ luminosity.

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