Table 1
Galaxy sample.
| Galaxy | RA | Dec | m b | D | M B | Sampling | Classif. | Other names |
| (2000) | (2000) | (mag) | (Mpc) | (mag) | (pc ′′-1) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
|
||||||||
| Haro 11 | 00 36 52.5 | −33 33 19 | 14.31 ± 0.40 a | 84.0 | −20.31 | 407 | Ext | ESO 350-IG 038 |
| Haro 14 | 00 45 46.4 | −15 35 49 | 13.65 ± 0.05 b | 13.0 | −16.92 | 63 | Ext | NGC 0244 |
| Haro 15 | 00 48 35.4 | −12 43 07 | 13.93 ± 0.05 c | 85.9 | −20.73 | 416 | Ext | Mrk 960 |
| Tololo 0127-397 | 01 29 15.8 | −39 30 38 | 16.18 ± 0.06 c | 71.3d | −18.07 | 346 | Nuc | |
| Tololo 1924-416 | 19 27 58.2 | −41 34 32 | 13.97 ± 0.04 b | 42.4 | −19.16 | 206 | Ext | ESO 338-IG 004 |
| Tololo 1937-423 | 19 40 58.6 | −42 15 45 | 15.14 ± 0.04 b | 41.1 | −17.92 | 199 | Ext | |
| Mrk 900 | 21 29 59.6 | + 02 24 51 | 14.17 ± 0.03 b | 18.9 | −17.21 | 92 | Ext | NGC 7077, UGC 11755 |
| Mrk 1131 | 23 28 01.1 | −02 09 52 | 16.10 ± 0.40 d | 32.2 | −16.43 | 156 | Ext | |
Notes. Columns (2) and (3): units of right ascension are hours, minutes, and seconds, and units of declination are degrees, arcminutes, and arcseconds. Column (4): B-band magnitudes:
magnitudes taken from HyperLeda (http://leda.univ-lyon1.fr/; Paturel et al. 2003);
integrated magnitudes from Gil de Paz et al. (2003), corrected for Galactic extinction;
asymptotic magnitudes 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 have been recomputed using the Schlegel et al. (1998) extinction curve. Column (5): distance calculated using a Hubble constant of 73 km s-1 Mpc-1, and taking the influence of the Virgo Cluster, the Great Attractor, and the Shapley supercluster from NED into account (http://nedwww.ipac.caltech.edu/).
Distance, absolute magnitude, and sampling have been recomputed for Tololo 0127-397 using our measurement of its redshift (see Sect. 4.4). Column (6): absolute magnitude in the B-band computed from the tabulated B magnitude and distance. Column (8): morphological classification following Cairós et al. (2001a).
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