**Table 1:** Sample galaxies; see Sect. 2.
Object	RA(J2000)	t_J	t_H	t_K'	M_B	A_B	D	FWHM	Other
	Dec(J2000)				(ref.)		(ref.)	(final) $^{\ast}$	names
		[s]	[s]	[s]	[mag]	[mag]	[Mpc]	[ $^{\prime\prime}$ ]
	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)
Mkn 314	23 $^{\rm h}$ 02 $^{\rm m}$ 59 $.\!\!^{\rm s}$ 3	1440	1740	1920	-18.5	0.38	28.9	1.5	NGC 7468;
(iE)	$+16^{\circ}$ 36'18 $.\!\!^{\prime\prime}$ 9				(f)		(a)		UGC 12329
Mkn 209	12 $^{\rm h}$ 26 $^{\rm m}$ 16 $.\!\!^{\rm s}$ 0	1620	1440	1140	-14.2	0.07	5.8	1.5	UGCA 281; I Zw 36;
(iE)	$+48^{\circ}$ 29'36 $.\!\!^{\prime\prime}$ 6				(g)		(b)		Haro 29
Mkn 996	01 $^{\rm h}$ 27 $^{\rm m}$ 35 $.\!\!^{\rm s}$ 5	1260	1440	1200	-16.6	0.19	20.4	1.4
(nE)	$-06^{\circ}$ 19'36 $.\!\!^{\prime\prime}$ 1				(h)		(c)
Mkn 370	02 $^{\rm h}$ 40 $^{\rm m}$ 29 $.\!\!^{\rm s}$ 0	1140	1860	1640	-17.1	0.40	11.2	1.2	NGC 1036; IC 1828;
(nE)	$+19^{\circ}$ 17'49 $.\!\!^{\prime\prime}$ 6				(f)		(a)		UGC 2160
I Zw 115	15 $^{\rm h}$ 32 $^{\rm m}$ 57 $.\!\!^{\rm s}$ 0	672	672	480	-16.4	0.06	15.0	1.3	UGC 9893;
(iI)	$+46^{\circ}$ 27'06 $.\!\!^{\prime\prime}$ 5				(g)		(a)		VV 720
Mkn 5	06 $^{\rm h}$ 42 $^{\rm m}$ 15 $.\!\!^{\rm s}$ 5	1650	2100	2340	-15.7	0.36	15.3	1.5	UGCA 130
(iE/iI, C)	$+75^{\circ}$ 37'32 $.\!\!^{\prime\prime}$ 6				(f)		(a)
Mkn 600	02 $^{\rm h}$ 51 $^{\rm m}$ 04 $.\!\!^{\rm s}$ 6	1560	1320	1080	-15.5	0.28	12.6	1.1
(iE)	$+04^{\circ}$ 27'13 $.\!\!^{\prime\prime}$ 9				(f)		(a)
NGC 6789	19 $^{\rm h}$ 16 $^{\rm m}$ 41 $.\!\!^{\rm s}$ 9	1200	1680	1920	-14.3	0.30	3.6	1.4	UGC 11425
(iE)	$+63^{\circ}$ 58'18 $.\!\!^{\prime\prime}$ 0				(i)		(d)
Mkn 324	23 $^{\rm h}$ 26 $^{\rm m}$ 32 $.\!\!^{\rm s}$ 8	1680	600	1140	-16.5	0.22	21.8	1.4	UGCA 439
(iE)	$+18^{\circ}$ 15'59 $.\!\!^{\prime\prime}$ 8				(f)		(a)
Mkn 450	13 $^{\rm h}$ 14 $^{\rm m}$ 48 $.\!\!^{\rm s}$ 3	1200	1440	1920	-16.7	0.06	17.9	1.3	UGC 08323; VV 616;
(iE)	$+34^{\circ}$ 52'51 $.\!\!^{\prime\prime}$ 3				(j)		(a)		HS 1312+3508
NGC 5058	13 $^{\rm h}$ 16 $^{\rm m}$ 52 $.\!\!^{\rm s}$ 3	720	1680	1440	-15.9	0.13	11.6	1.1	UGC 08345; Mkn 786;
(iI?)	$+12^{\circ}$ 32'53 $.\!\!^{\prime\prime}$ 9				(i)		(c, e)		KPG 370

$^{\ast}$ Resolution of the best image set available for the respective galaxy, after reduction and combination; (a) Tully (1988); (b) Schulte-Ladbeck et al. (2001); (c) inferred from the heliocentric velocity $v_{\rm hel}$ listed in the NED, corrected for solar motion with respect to the center of the Virgo Cluster and adopting H₀=75 km s^-1 Mpc ^-1 (cf. N03); (d) Drozdovsky et al. (2001); (e) see Sect. 4.11; (f) m_B from Table 2 in Cairós et al. (2001a); (g) m_B from Papaderos et al. (1996a); (h) m_B from Thuan et al. (1996); (i) m_B from the RC3 (de Vaucouleurs et al. 1991); (j) m_B from Vennik et al. (2000).

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Surface photometry and profile decomposition
	4 Results and discussion of individual objects
	5 Summary
	References
	Online Material