Table 1: The galaxy sample.

Galaxy	Other names	RA(J2000)	Dec (J2000)	D (Mpc)	AB (mag)	mB (mag)	MB (mag)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)
Tololo 0127-397		01 29 15.8	-39 30 37	61.0	0.067	16.18	-17.75
Mrk 370	NGC 1036, UGC 02160	02 40 29.0	19 17 50	10.9	0.399	13.19	-16.99
Mrk 5	UGCA 130	06 42 15.5	75 37 33	14.0	0.364	15.22	-15.51
Mrk 86	NGC 2537, UGC 04274	08 13 14.7	45 59 26	8.1	0.232	12.18	-17.37
Mrk 35	Haro 3, NGC 3353	10 45 22.4	55 57 37	15.6	0.031	13.18	-17.79
Mrk 36	Haro 4, UGCA 225	11 04 58.5	29 08 22	10.4	0.131	15.25	-14.84
I Zw 123	UGCA 410, Mrk 487	15 37 04.2	55 15 48	12.5	0.062	15.40	-15.09
Mrk 314	NGC 7468, UGC 12329	23 02 59.2	16 36 19	28.9	0.383	13.78	-18.53

Notes.- Columns: (1) name of the galaxy; (2) other designations of the galaxies; (3) right ascension in hours, minutes and seconds; (4) declination in degrees, arcminutes and arcseconds; (5) distance, computed assuming a Hubble flow with a Hubble constant H0 = 75 km s-1 Mpc-1, after correcting recession velocities relative to the centroid of the local group for Virgocentric infall; (6) extinction coefficient in the B band, from Schlegel, Finkbeiner, & Davis (1998); (7) asymptotic magnitude in the B band, from C01b. Notice that the asymptotic magnitudes listed in C01b were corrected for Galactic extinction following Burstein & Heiles (1984); here they have been recomputed using the Schlegel, Finkbeiner, & Davis (1998) extinction values; (8) absolute magnitude, obtained from the B asymptotic magnitudes using the distances tabulated in (5).