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Table 1:

Main parameters of the galaxy sample.
Galaxy RA(J2000) Dec.(J2000) D (Mpc) AB (mag) mB (mag) B-V MB (mag)
(1) (2) (3) (4) (5) (6) (7) (8)
Cam 0341-404 03 42 49.4 -40 35 56 56.69 0.068 16.62 0.36 -17.21
Haro 1 07 36 56.4 35 14 31 52.11 0.184 12.79 0.54 -20.98
Haro 15 00 48 35.9 -12 43 07 84.15 0.101 14.06 0.35 -20.67
Mrk 5 06 42 15.5 75 37 33 13.96 0.364 15.58 0.60 -15.51
Mrk 33 10 32 31.9 54 24 03 22.30 0.052 13.46 0.41 -18.33
Mrk 35 10 45 22.4 55 57 37 15.60 0.031 13.21 0.61 -17.79
Mrk 36 11 04 58.5 29 08 22 10.43 0.131 15.38 0.35 -14.84
Mrk 86 08 13 14.7 45 59 26 8.12 0.232 12.41 0.73 -17.37
Mrk 297 16 05 12.9 20 32 32 65.10 0.330 13.16 0.44 -21.24
Mrk 314 23 02 59.2 16 36 19 28.95 0.383 14.15 0.07 -18.53
Mrk 324 23 26 32.8 18 16 00 22.43 0.215 15.39 0.58 -16.58
Mrk 370 02 40 29.0 19 17 50 10.85 0.399 13.59 0.53 -16.99
Mrk 401 09 30 17.0 29 32 24 24.07 0.101 13.82 0.01 -18.19
Mrk 527 23 13 12.7 06 19 18 47.56 0.473 13.58 0.55 -20.28
Mrk 600 02 51 04.6 04 27 14 12.81 0.282 15.29 0.31 -15.53
Mrk 1089 05 01 37.8 -04 15 30 52.65 0.220 14.05 0.08 -19.78
Mrk 1090 05 01 44.1 -04 17 19 51.93 0.238 15.16 0.10 -18.65
PHL 0293 B 22 30 33.9 -00 07 35 21.39 0.302 17.65 0.51 -14.30
Tololo 0127-397 01 29 15.8 -39 30 37 61.05 0.067 16.18 0.51 -17.81
UM 417 02 19 30.2 -00 59 11 35.08 0.141 18.04 0.29 -14.83
UM 462 11 52 37.3 -02 28 10 14.12 0.083 14.69 0.47 -16.14
I Zw 123 15 37 04.2 55 15 48 12.52 0.062 15.46 0.55 -15.09
II Zw 33 05 10 48.1 -02 40 54 36.41 0.439 15.02 0.81 -18.22
II Zw 40 05 55 42.6 03 23 32 9.69 3.538 15.18 1.12 -18.29
II Zw 70 14 50 56.5 35 34 18 19.12 0.053 14.85 0.41 -16.61
II Zw 71 14 51 14.4 35 32 32 19.64 0.055 14.46 0.56 -17.06
III Zw 102 23 20 30.1 17 13 32 22.71 0.109 12.61 0.76 -19.28
III Zw 107 23 30 09.9 25 31 58 78.09 0.259 15.08 0.60 -19.64
Notes: Cols: (2) Right ascension in hours, minutes and seconds; (3) Declination in degrees, arcminutes and arcseconds; (4) 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; (5) Extinction coefficient in the B band, from Schlegel et al. (1998); (6) Asymptotic magnitude in the B band, from C01b. Note that the asymptotic magnitudes listed in C01b were corrected for Galactic extinction following Burstein & Heiles (1984); here they are presented uncorrected; (7) B-V colour from the asymptotic photometry of C01b, uncorrected for galactic extinction; (8) Absolute magnitude, obtained from the B asymptotic magnitudes of (6) recomputed using the Schlegel et al. (1998) extinction values, distances were taken from those tabulated in (5).

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