Table 3: Colors of the host galaxya.
Object J-H $H-K_{\rm s}$ B-J
  [mag] [mag] [mag]
Tol 3 0.55 $\pm$ 0.07 0.10 $\pm$ 0.06 -
Tol 65c 0.48 $\pm$ 0.17b - 1.3 $\pm$ 0.15b
Tol 1214-277c 0.39 $\pm$ 0.16b - 1.0 $\pm$ 0.13b
Tol 1400-411c 0.43 $\pm$ 0.08 0.26 $\pm$ 0.09 1.45 $\pm$ 0.16
Pox 4c 0.42 $\pm$ 0.13 0.12 $\pm$ 0.13 -
Pox 4B 0.43 $\pm$ 0.15b 0.1 $\pm$ 0.15b -
UM 448 0.69 $\pm$ 0.10b 0.14 $\pm$ 0.11b 2.09 $\pm$ 0.15
UM 461 0.50 $\pm$ 0.06 0.15 $\pm$ 0.06 1.92 $\pm$ 0.16
He 2-10 0.59 $\pm$ 0.06 0.11 $\pm$ 0.07 -
IC 4662c 0.57 $\pm$ 0.12b 0.03 $\pm$ 0.12b -
Mkn 178 0.53 $\pm$ 0.15 0.25 $\pm$ 0.16b 2.00 $\pm$ 0.15
Mkn 1329 0.65 $\pm$ 0.09 0.03 $\pm$ 0.10 -
Haro 14 0.69 $\pm$ 0.12b 0.20 $\pm$ 0.12b 2.02 $\pm$ 0.15
a Corrected for galactic extinction (see Sect. 2.4.2); NIR colors are transformed to the 2MASS system (cf. Sect. 2.4.1). The B band denotes the Johnson B. Errors include cumulative uncertainties in the determination of color profiles, the calibration and the transformation to the 2MASS system.
b Possible local instabilities in one SBP at low S/N levels.
c Possible contamination by gas emission over a large portion of the LSB host galaxy.

Source LaTeX | All tables | In the text