Table 2: Photometric measurements in all the filters, in log (Jy), of all the stars detected by MCS deconvolution (Sect. 2.3) of the   IRS 13 field from the H and Kp Gemini AO images. Measurements in the NICMOS filters (F) were obtained by  StarFinder, and in the L band by MCS analysis. The sources are listed by order of decreasing brightness in the Kp band, except IRS 13W, which is listed first. Values preceded by < in the 1.1 m and the L bands are minima of detection, i.e. flux upper limits.

ID	F110M	F145M	F160W	H	F190N	Kp	F222M	L
W	<0.56	2.58	3.28	3.20	3.96	4.27	4.36	4.89
E1	1.76	3.40	3.82	3.93	4.27	4.40	4.49	5.03
E2	1.61	3.22	3.71	3.80	4.17	4.38	4.48	5.37
E4	0.93	2.68	3.17	3.28	3.69	4.11	4.18	<4.66
5	0.78	2.66	3.20	3.30	3.72	4.04	3.93
6	0.39	2.51	3.07	3.14	3.57	3.94	3.89
7	1.23	2.78	3.20	3.26	3.63	3.92	3.88
8	0.62	2.55	3.08	3.08	3.53	3.90	3.81
E3A	<0.45		2.29	2.43	3.11	3.81		5.46
10	0.11	1.88	2.63	2.81	3.23	3.68	3.55
E3B	<0.45		2.11	2.24		3.57		5.29
12	0.69	1.98	2.62	2.66	3.15	3.48	3.45
13	-0.09	2.02	2.58	2.65	3.14	3.46	3.40
14	-0.16	2.01	2.55	2.65	3.11	3.43	3.34
15	-0.06	1.75	2.25	2.37	2.82	3.12	3.23
16		1.57	2.18	2.36	2.71	3.11	2.92
E5	<-0.17	1.60		1.75	2.72	3.08	3.61	5.07
18	0.56	1.87	2.27	2.30	2.74	2.99	3.02
E6	<0.48		2.46	2.53		2.97		<4.68
20	0.86	1.42	2.01	2.11	2.57	2.88	2.89