**Table 3:** Measured IR fluxes in Jy (corresponding magnitudes in parenthesis) for the objects in the HMC region.
Band name	Object	Object	Object	Object
	F1	F2	F3	F4
J	-	$2.21\times10^{-4}$ (17.15)	-	-
H	$6.19\times10^{-5}$ (18.00)	$5.25\times10^{-4}$ (15.72)	-	-
$K_{\rm s}$	$2.25\times10^{-3}$ (13.60)	$6.57\times10^{-4}$ (15.00)	$1.67\times10^{-4}$ (16.49)	-
L'	$2.43\times10^{-2}$ (10.04)	-	$1.00\times10^{-3}$ (13.50)	$2.95\times10^{-3}$ (12.33)
nb_M	$3.10\times10^{-2}$ ( 9.21)	-	-	$1.49\times10^{-2}$ (10.01)
N1	$1.10\$ ( 3.90)^a	-	-	1.10 (3.90)^a
N	-	-	-	$6.00\times10^{-1}$ (4.55)
Q2	-	-	-	$2.28\times10^{1}$ (-0.85)^b

^a In the undeconvolved N1 band, the objects F1 and F4 merge into one entity, whose combined flux is reported.
^b Note that the Q2 flux is affected by a relatively large uncertainty of around 30% due to non-photometric sky conditions (see text).

Source LaTeX | All tables | In the text

	1 Introduction
	2 Infrared observations
	3 Results
	4 Discussion
	5 Conclusions
	References
	Online Material
	Appendix A: NIR astrometry
	Appendix B: Correct position of the compact MIR emission in G9.62+0.19-F
	Appendix C: MIR image restoration