Table 2: Photometric parameters for the 2MASS sample (first group), CFHT 2004 sample (second group), and CTIO 2007 sample (third group).

Galaxya		 $\mu_{0K}$b r0Kc $m_{\rm SK}$d $m_{\rm TK}$e PAf eg W20h $\tau_1$i $A_{\rm KS}$j DMk Methodl Ref.m

IC 10		 17.75 97.8 6.13 6.51 -55 0.6 85 1.78 0.56 24.10 CEPH F00
NGC 1560 18.73 54.9 9.13 9.26 +23 0.8 157 0.21 0.07 27.56 TRGB K03a
Holmberg II 19.67 84.3 7.45 8.00 +20 0.0 72 0.04 0.01 27.48 TRGB K02a
NGC 2915 17.32 10.6 9.93 9.70 -50 0.3 153 0.31 0.10 27.76 TRGB K03b
NGC 3077 17.30 33.3 7.42 7.32 +40 0.3 91 0.08 0.02 27.75 TRGB S01
NGC 4214 17.64 33.6 8.11 8.14 -55 0.5 86 0.03 0.01 27.31 TRGB M02
NGC 6822 19.64 106.8 7.08 7.30 +10 0.2 75 0.27 0.09 23.50 CEPH V00
IC 5152 17.87 27.1 9.04 9.13 -70 0.6 100 0.03 0.01 26.41 TRGB K02b
UGC 3860 20.41 13.6 12.83 13.07 +30 0.5 51 0.07 0.02 28.85 HUB H03
UGC 5272 20.24 17.9 12.31 12.45 -65 0.6 108 0.02 0.01 29.15 HUB G04
UGC 5340 20.36 12.4 12.79 12.82 +30 0.4 97 0.02 0.01 29.00 HUB RC3
UGC 5764 20.41 14.5 13.26 13.41 +50 0.7 120 0.02 0.01 29.36 HUB RC3
UGC 7408 20.34 18.1 11.95 12.03 -75 0.4 51 0.01 0.00 29.29 HUB RC3
UGC 7490 20.03 17.5 11.91 11.33 +20 0.5 73 0.03 0.01 30.01 HUB UZC
NGC 4523 19.86 19.3 11.34 11.41 +30 0.4 144 0.04 0.01 29.03 3BS T00
UGCA 319 20.23 16.9 11.99 12.21 +30 0.4 108 0.09 0.03 29.11 HUB K04
WLM 21.30 98.1 9.68 9.91 +10 0.6 74 0.04 0.01 24.74 TRGB M98
ESO 349-031 21.21 12.3 13.34 13.28 0 0.2 29 0.01 0.00 27.36 TRGB K06
ESO 245-005 20.74 54.6 10.15 10.26 -60 0.5 85 0.02 0.01 28.07 TRGB K03c
ESO 320-14 20.28 10.9 13.00 12.90 +90 0.4 29 0.16 0.05 28.78 TRGB K07
ESO 321-014 21.22 23.0 12.13 12.52 +20 0.3 36 0.11 0.03 27.35 TRGB K05
KK98 200 20.53 8.7 13.55 13.42 -75 0.3 34 0.08 0.02 28.08 TRGB K05
ESO 325-11 21.43 32.8 11.75 12.20 -50 0.4 96 0.10 0.03 27.50 TRGB K05
ESO 223-09 19.30 34.5 9.34 9.44 -50 0.3 89 0.30 0.10 28.92 TRGB K07
ESO 461-036 20.62 13.1 13.13 13.30 +20 0.5 71 0.34 0.11 29.34 TRGB K06
a Galaxy Name. b Central surface brightness (from sech law) in mag/arcsec2. c Scale length (from sech law) in arcsec. d Apparent sech magnitude (from sech law) in mag. e Apparent isophotal magnitude in mag. f Position angle (from N to E) in deg. g Ellipticity (measured with the STSDAS/ELLIPSE task as a fixed parameter according to V05). h Width of the HI line profile measured in km s-1 at 20% of the peak. i Optical depth at 1 $\mu$ ($\tau_1$) calculated by YES. j Extinction in $K_{\rm s}$ band in mag. k Distance modulus. l Method for distance determination: CEPH - Cepheids, TRGB - Tip of the RGB, HUB - Hubble flow, 3BS - Brightest 3 blue stars. m Reference for distance determination (please see References section).

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