Table 3: Photometric results for SB 1/SB 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		    $\lambda$    Ttotal flux $^{\ast}$ peak flux  $^{\dagger}$ x offset y offset
     ($\mu $m)    (K)    (arcsec) (arcsec)
(1,0) S(7)    1.747    1281713.4 2.9 -0.02 -0.07
(1,0) S(3)    1.957    8365103.8 17.5 -0.05 0.07
(1,0) S(2)    2.033    758428.1 4.9 0.04 0.08
(2,1) S(3)    2.073    1389010.1 2.8 $\cdot\cdot\cdot$ $\cdot\cdot\cdot$
(1,0) S(1)    2.121    695691.7 13.7 0.00 0.00
(1,0) S(0)    2.223    647113 3.0 $\cdot\cdot\cdot$ $\cdot\cdot\cdot$
(2,1) S(1)    2.247    125505.6 2.0 $\cdot\cdot\cdot$ $\cdot\cdot\cdot$
(1,0) Q(1)    2.406    614958.4 14.1 0.04 0.08
(1,0) Q(3)    2.423    695656.6 9.7 0.10 0.06
(1,0) Q(4)    2.437    758413.4 5.3 0.08 0.05
(1,0) Q(5)    2.454    836529.9 11.2 $\cdot\cdot\cdot$ $\cdot\cdot\cdot$
(1,0) Q(6)    2.475    92869.3 3.0 $\cdot\cdot\cdot$ $\cdot\cdot\cdot$
$\ast$ Units of Units of 10-18 W m-2. The 1$\sigma$ flux measurement uncertainty is 2.8 $\times $ 10-18 W m-2 and 5.6 $\times $ 10-18 W m-2 beyond 2.4 $\mu $m.
$\dagger$ Units of 10-18 Wm-2 arcsec-2. The 1$\sigma$ noise level is 1.0 $\times $ 10-18 W m-2 arcsec-2.


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