Table 6: Diffused light model parameters. We considered an exponential model $\Delta m_\lambda = a\ {\rm e}^{b \theta } + c$ , where $\Delta m_\lambda$ is the surface magnitude per arcsec² of the sky background at an angular distance $\theta$ of a zero magnitude source, and (a,b,c) are the adjusted model parameters.
$\lambda$ J ( $\theta \ge 3''$ ) H ( $\theta \ge 3''$ ) $K_{\rm s}$ ( $\theta \ge 3''$ ) $K_{\rm s}$ ( $\theta \le 3''$ )

a -7.281 -7.969 -8.035 -9.068

b -0.163 -0.194 -0.228 -0.638

c 13.226 13.247 13.018 10.305

**Table 6:** Diffused light model parameters. We considered an exponential model $\Delta m_\lambda = a\ {\rm e}^{b \theta } + c$ , where $\Delta m_\lambda$ is the surface magnitude per arcsec² of the sky background at an angular distance $\theta$ of a zero magnitude source, and (a,b,c) are the adjusted model parameters.
$\lambda$	J ( $\theta \ge 3''$ )	H ( $\theta \ge 3''$ )	$K_{\rm s}$ ( $\theta \ge 3''$ )	$K_{\rm s}$ ( $\theta \le 3''$ )
a	-7.281	-7.969	-8.035	-9.068
b	-0.163	-0.194	-0.228	-0.638
c	13.226	13.247	13.018	10.305

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