Table 1
Galaxy sample.
| Galaxy | Other designations | RA | Dec | m B | D | M B | Morph | A V |
| (2000) | (2000) | (Mpc) | (mag) | (mag) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
|
||||||||
| II Zw 33 | UGCA 102, Mrk 1094 | 05 10 48.1 | −02 40 54 | 14.57a | 37.4 | −18.29 | Ch | 0.288 |
| Haro 1 | NGC 2415, UGC 3930 | 07 36 56.7 | 35 14 31 | 12.61a | 52.9 | −21.00 | Ext | 0.117 |
| NGC 4670 | UGC 7930, Arp 163, Haro 9 | 12 45 17.2 | 27 07 32 | 13.02b | 22.4 | −18.73 | Nuc | 0.041 |
| Mrk 314 | NGC 7468, UGC 12329 | 23 02 59.2 | 16 36 19 | 13.78a | 29.0 | −18.53 | Ch | 0.234 |
| III Zw 102 | NGC 7625, UGC 12529, Arp 212 | 23 20 30.1 | 17 13 32 | 12.50a | 23.1 | −19.31 | Ext | 0.069 |
Notes. Columns (3) and (4): units of right ascension are hours, minutes, and seconds, and units of declination are degrees, arcminutes, and arcseconds. Column (5): B-band magnitudes: Column (6): distances, computed assuming a Hubble flow, with a Hubble constant H0 = 73 km s-1 Mpc-1, and taking into account the influence of the Virgo cluster, the Great Attractor and the Shapley supercluster, are taken from NED (http://nedwww.ipac.caltech.edu). Column (7): absolute magnitude in the B band, computed from the tabulated B-band magnitude and distance. Column (8): morphological classification following Cairós et al. (2001a). Column (9): galactic extinction, from the Schlafly & Finkbeiner (2011) recalibration, as listed in NED.
asymptotic photometry obtained by extrapolating the growth curves, and corrected for galactic extinction (Cairós et al. 2001a). The asymptotic magnitudes listed in Cairós et al. (2001a) were corrected for Galactic extinction following Burstein & Heiles (1982); here they were recomputed using the Schlafly & Finkbeiner (2011) extinction values;
integrated magnitudes from Gil de Paz et al. (2003), corrected for Galactic extinction.
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