Table 1: Instruments, filter properties and year of data acquisition of the high-resolution images of the IRS 13 field.
Filter Instrument/Telescope $\lambda$ / $\Delta\lambda$ Year

( $\mu$ m)

F110M NICMOS/HST 1.10/0.200 97-98

F145M NICMOS/HST 1.45/0.197 97-98

F160W NICMOS/HST 1.60/0.400 97-98

H Hokupa'a+Quirc/Gemini N 1.65/0.296 2000

Pa $\alpha$ NICMOS/HST 1.87/0.019 97-98

F190N NICMOS/HST 1.90/0.017 97-98

Kp Hokupa'a+Quirc/Gemini N 2.12/0.410 2000

K PUEO+KIR/CFHT 2.20/0.340 1998

F222M NICMOS/HST 2.22/0.143 97-98

L ADONIS+COMIC/3.6 m ESO 3.48/0.590 2000

**Table 1:** Instruments, filter properties and year of data acquisition of the high-resolution images of the IRS 13 field.
Filter	Instrument/Telescope	$\lambda$ / $\Delta\lambda$	Year
		( $\mu$ m)
F110M	NICMOS/HST	1.10/0.200	97-98
F145M	NICMOS/HST	1.45/0.197	97-98
F160W	NICMOS/HST	1.60/0.400	97-98
H	Hokupa'a+Quirc/Gemini N	1.65/0.296	2000
Pa $\alpha$	NICMOS/HST	1.87/0.019	97-98
F190N	NICMOS/HST	1.90/0.017	97-98
Kp	Hokupa'a+Quirc/Gemini N	2.12/0.410	2000
K	PUEO+KIR/CFHT	2.20/0.340	1998
F222M	NICMOS/HST	2.22/0.143	97-98
L	ADONIS+COMIC/3.6 m ESO	3.48/0.590	2000

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