**Table 3:** Colors of the host galaxy^a.
Object	J-H	$H-K_{\rm s}$
	[mag]	[mag]
Mkn 314	0.77 $\pm$ 0.16^b	0.26 $\pm$ 0.18^b
Mkn 209	0.37 $\pm$ 0.13^b	0.19 $\pm$ 0.18^b
Mkn 996	0.56 $\pm$ 0.13	0.37 $\pm$ 0.16^b
Mkn 370	0.52 $\pm$ 0.14	0.16 $\pm$ 0.17
I Zw 115	0.46 $\pm$ 0.15^b	0.31 $\pm$ 0.26^b
Mkn 5	0.54 $\pm$ 0.15^b	0.45 $\pm$ 0.12^b
Mkn 600	0.50 $\pm$ 0.17^b,c	0.08 $\pm$ 0.29^b,c
NGC 6789	0.42 $\pm$ 0.12	0.31 $\pm$ 0.18^b
Mkn 324	0.55 $\pm$ 0.12	0.22 $\pm$ 0.18^b
Mkn 450	0.51 $\pm$ 0.16	0.19 $\pm$ 0.26^b
NGC 5058	0.41 $\pm$ 0.16	0.24 $\pm$ 0.25^b

Colors can be directly compared to data in the 2MASS photometric system; for details of the photometric system and the various error sources that are considered here, see Sects. 3.1 and 2.1.
^a Corrected for galactic extinction (see Sect. 2.1).
^b Possible local instabilities in one SBP at low S/N levels.
^c Possible contamination by nebular emission over a large portion of the LSB host galaxy.

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