Table 1: Sample galaxies.
Object RA(J2000) $t_{J, \rm NTT}$ $t_{H,\rm NTT}$ $t_{K_{\rm s},\rm NTT}$ MB AB D FWHM Other
  Dec(J2000) $t_{J,\rm CA}$ $t_{H,\rm CA}$ t $_{K',\rm CA} $ (ref.)   (ref.) (final) $^{\spadesuit}$ names
    [s] [s] [s] [mag] [mag] [Mpc] [ $^{\prime\prime}$]  
  (2) (3) (4) (5) (6) (7) (8) (9) (10)
Tol 3   10$^{\rm h}$06$^{\rm m}$33 $\hbox{$.\!\!^{\rm s}$ }$6 1440 1560 2100 -18.0 0.33 13.8 1.2 NGC 3125; ESO 435-G041;
(iE) $-29^{\circ}$56$^{\rm '}$09 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (a)   (a)   Tol1004-296
Haro 14   00$^{\rm h}$45$^{\rm m}$46 $\hbox{$.\!\!^{\rm s}$ }$4 - - - -17.0 0.09 12.5 1.6 NGC 0244; UGCA 010;
(iE/nE) $-15^{\circ}$35$^{\rm '}$49 $\hbox{$.\!\!^{\prime\prime}$ }$0 1440 1680 1920 (a)   (a)   VV 728
UM 461   11$^{\rm h}$51$^{\rm m}$33 $\hbox{$.\!\!^{\rm s}$ }$0 1500 1500 2100 -14.9 0.08 14.3 0.7 SCHG 1148-020
(iI) $-02^{\circ}$22$^{\rm '}$23 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (j)   (e)    
He 2-10   08$^{\rm h}$36$^{\rm m}$15 $\hbox{$.\!\!^{\rm s}$ }$0 1140 1500 2040 -18.7 0.48 8.7 0.9 ESO 495-G021
(iE/nE) $-26^{\circ}$24$^{\rm '}$34 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (k)   (f)    
Tol 1400-411   14$^{\rm h}$03$^{\rm m}$21 $\hbox{$.\!\!^{\rm s}$ }$0 1140 1500 2100 -16.5 0.30 4.8 0.9 NGC 5408; Tol 116;
(iI,C) $-41^{\circ}$22$^{\rm '}$44 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (l)   (c)   ESO 325-G047
Pox 4/Pox 4B   11$^{\rm h}$51$^{\rm m}$11 $\hbox{$.\!\!^{\rm s}$ }$6 1500 1500 2100 -18.8 0.17 46.7 0.6 CAM 1148-2020
(iI + comp.) $-20^{\circ}$36$^{\rm '}$02 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (m)   (b)    
Tol 65   12$^{\rm h}$25$^{\rm m}$46 $\hbox{$.\!\!^{\rm s}$ }$9 2100 2100 3000 -15.3 0.32 34.2 0.6 ESO 380-G027;
(i0/iI,C) $-36^{\circ}$14$^{\rm '}$01 $\hbox{$.\!\!^{\prime\prime}$ }$0s - - - (n)   (b)   Tol 1223-359
Tol 1214-277   12$^{\rm h}$17$^{\rm m}$17 $\hbox{$.\!\!^{\rm s}$ }$1 1200 1500 2100 -16.9 0.28 102.6 0.9 SCHG 1214-277;
(i0/iI,C) $-28^{\circ}$02$^{\rm '}$33 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (o)   (b)   Tol 21
Mkn 178   11$^{\rm h}$33$^{\rm m}$29 $\hbox{$.\!\!^{\rm s}$ }$1 240 1380 1380 -13.9 0.08 4.2 1.6 UGC 06541; HOLMBERG 263A;
(iE) $+49^{\circ}$14$^{\rm '}$17 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (p)   (h)   CGCG 242-046; SBS 1130+495
Mkn 1329   12$^{\rm h}$37$^{\rm m}$03 $\hbox{$.\!\!^{\rm s}$ }$0 300 360 480 -16.8 0.10 16.0 0.7 VCC 1699; IC 3589/91;
(iI,C) $+06^{\circ}$55$^{\rm '}$36 $\hbox{$.\!\!^{\prime\prime}$ }$0 1200 360 960 (i)   (i)   UGC 7790
IC 4662   17$^{\rm h}$47$^{\rm m}$06 $\hbox{$.\!\!^{\rm s}$ }$4 1980 1620 660 -14.9 0.30 2.0 0.8 ESO 102-G014;
(dI/iE) $-64^{\circ}$38$^{\rm '}$25 $\hbox{$.\!\!^{\prime\prime}$ }$0 - - - (l)   (g)   He 2-269
UM 448   11$^{\rm h}$42$^{\rm m}$12 $\hbox{$.\!\!^{\rm s}$ }$4 300 360 480 -19.8 0.11 76.1 0.7 UGC 06665; SCHG 1139+006;
(iI/BCG) $+00^{\circ}$20$^{\rm '}$03 $\hbox{$.\!\!^{\prime\prime}$ }$0 840 900 1200 (l)   (d)   Ark 312; ARP 161; Mkn 1304
$\spadesuit$: Resolution of the best image set available for the respective galaxy, after reduction and combination (a): Marlowe et al. (1999), (b): 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. Sect. 2.1). (c): Karachentsev et al. (2002), (d): Mirabel & Sanders (1988), (e): $v_{{\rm LG}}$ from Smoker et al. (2000), corrected for Local Group infall to the Virgo Cluster like b); (f): Tully (1988), (g): Heydari-Malayeri 1990, (h): Schulte-Ladbeck et al. (2000), (i): Yasuda et al. (1997), (j): mB from Méndez & Esteban (2000), (k): mB from Papaderos (1998), (l): mB from the RC3 (de Vaucouleurs et al. 1991), (m): mB for Pox 4 from Méndez & Esteban (1999); no published mB for Pox 4B (n): mB from P99, (o): mB from F01, (p): mB from Papaderos et al. (2002).


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