Table 2: Photometric results for NB 1 and NB 2. The upper energy level of the transition is given in the third column. The x and y peak position offsets are relative to the 1-0 S(1) peak position.

line				T	total flux	peak flux	x offset	y offset
		(m)		(K)			(arcsec)	(arcsec)
NB 1
(1,0) S(7)		1.747		12817	12.9	5.7
(1,0) S(5)		1.835		10341	58.2	15.8
(1,0) S(4)		1.891		9286	18.9	8.3
(1,0) S(3)		1.957		8365	118.1	31.1	0.07	0.06
(1,0) S(2)		2.033		7584	33.3	7.9	0.0	0.04
(1,0) S(1)		2.121		6956	88.2	23.4	0.00	0.00
(1,0) S(0)		2.223		6471	13.7	6.0	0.13	0.05
(2,1) S(1)		2.247		12550	4.4	2.5	0.14	-0.13
(1,0) Q(1)		2.406		6149	51.9	20.9	0.08	-0.03
(1,0) Q(3)		2.423		6956	57.2	22.0	0.06	0.00
(1,0) Q(4)		2.437		7584	7.3	5.7	0.06	-0.16
(1,0) Q(5)		2.454		8365	13.3	10.3
NB 2
(1,0) S(7)		1.747		12817	6.7	3.6
(1,0) S(5)		1.835		10341	40.9	13.8
(1,0) S(4)		1.891		9286	10.8	5.2
(1,0) S(3)		1.957		8365	71.6	24.1	-0.07	0.06
(1,0) S(2)		2.033		7584	19.7	7.1	-0.10	0.05
(1,0) S(1)		2.121		6956	56.6	17.7	0.00	0.00
(1,0) S(0)		2.223		6471	8.8	3.5
(2,1) S(1)		2.247		12550	2.4	2.2	-0.16	0.18
(1,0) Q(1)		2.406		6149	30.1	15.5	0.01	0.05
(1,0) Q(3)		2.423		6956	31.7	16.8	0.01	0.00
(1,0) Q(4)		2.437		7584	4	5.1	0.02	0.14
(1,0) Q(5)		2.454		8365	3.1

Units of Units of 10-18 W m-2. The 1 flux measurement uncertainty is 3.1  10-18 W m-2. However, beyond 2.4 m this value increases to 6.2  10-18 W m-2. Units of 10-18 W m-2 arcsec-2. The 1 noise level is 1.6  10-18 Wm-2 arcsec-2.