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Table 2:

Line identification of detected emissions.
(a) January 28, 2008; H2O
Transition Wavenumber Wavelength Flux g-factor1 Atmospheric transmittance
($\nu_{1}'$, $\nu_{2}'$, $\nu_{3}'$) J'Ka' Kc'-($\nu_{1}''$, $\nu_{2}''$,$\nu_{3}''$) J''Ka'' Kc'' [cm-1] [Å] [W m-2] [W molecule-1]  
(101)11 1-(001)20 2 3459.53 28 905.67 (8.60 $\pm $ 1.27) $\times$ 10-20 $2.48\times10^{-27}$ 0.81
(101)43 1-(100)53 2 3459.49 28 905.97 * $5.29\times10^{-28}$ 0.81
(101)42 2-(100)52 3 3456.45 28 931.44 (3.90 $\pm $ 1.08) $\times$ 10-20 $4.29\times10^{-27}$ 0.32
(101)30 3-(001)31 2 3455.43 28 939.99 (1.77 $\pm $ 0.82) $\times$ 10-20 $5.65\times10^{-28}$ 0.81
(101)21 1-(001)22 0 3454.69 28 946.17 (9.28 $\pm $ 0.81) $\times$ 10-20 $3.70\times10^{-27}$ 0.80
(200)11 0-(001)22 1 3453.30 28 957.81 (1.41 $\pm $ 0.08) $\times$ 10-19 $7.39\times10^{-27}$ 0.80
(101)20 2-(100)32 1 3453.15 28 959.03 (1.34 $\pm $ 0.09) $\times$ 10-19 $5.62\times10^{-27}$ 0.88
(200)11 0-(001)11 1 3450.29 28 983.04 (6.10 $\pm $ 0.87) $\times$ 10-20 $1.03\times10^{-26}$ 0.21
(110)32 1-(010)43 2 3449.78 28 987.36 (2.50 $\pm $ 0.77) $\times$ 10-20 $6.46\times10^{-28}$ 0.73
(200)22 0-(001)22 1 3445.89 29 020.12 (3.22 $\pm $ 0.90) $\times$ 10-20 $2.11\times10^{-27}$ 0.49
(200)21 2-(100)32 1 3412.92 29 300.39 (1.10 $\pm $ 0.08) $\times$ 10-19 $4.68\times10^{-27}$ 0.80
(101)31 3-(001)40 4 3411.62 29 311.61 (7.92 $\pm $ 0.66) $\times$ 10-20 $3.27\times10^{-27}$ 0.94
(201)11 1-(200)11 0 3405.42 29 364.95 (5.98 $\pm $ 0.72) $\times$ 10-20 $1.78\times10^{-27}$ 0.91
(201)22 1-(200)22 0 3405.39 29 365.21 * $1.78\times10^{-28}$ 0.90
(101)11 1-(001)22 1 3404.24 29 375.11 (3.82 $\pm $ 0.77) $\times$ 10-20 $1.65\times10^{-27}$ 0.42
(200)11 1-(001)21 2 3403.23 29 383.84 (1.26 $\pm $ 0.09) $\times$ 10-19 $4.29\times10^{-27}$ 0.76
(200)10 1-(001)20 2 3399.37 29 417.23 (4.01 $\pm $ 0.08) $\times$ 10-19 $1.36\times10^{-26}$ 0.82
(300)21 2-(101)11 1 3389.14 29 506.05 (1.71 $\pm $ 0.63) $\times$ 10-20 $2.44\times10^{-28}$ 0.94
(201)00 0-(200)10 1 3388.77 29 509.23 (8.34 $\pm $ 0.66) $\times$ 10-20 $2.65\times10^{-27}$ 0.94
(101)40 4-(001)51 5 3387.54 29 519.94 (4.28 $\pm $ 0.78) $\times$ 10-20 $1.47\times10^{-27}$ 0.89
(201)21 1-(101)20 2 3385.14 29 540.66 (2.62 $\pm $ 0.94) $\times$ 10-20 $7.16\times10^{-29}$ 0.58
(101)21 1-(001)32 2 3385.14 29 540.90 * $1.60\times10^{-27}$ 0.56
(200)21 2-(001)31 3 3382.10 29 567.43 (3.79 $\pm $ 0.07) $\times$ 10-19 $1.22\times10^{-26}$ 0.89
(200)20 2-(001)30 3 3378.48 29 599.08 (9.53 $\pm $ 0.76) $\times$ 10-20 $3.16\times10^{-27}$ 0.75
(101)31 3-(100) 42 22 3320.13 30 119.34 (6.44 $\pm $ 0.75) $\times$ 10-20 $1.38\times10^{-27}$ 0.97
(200)31 3-(001) 42 22 3319.47 30 125.29 (5.06 $\pm $ 0.71) $\times$ 10-20 $5.10\times10^{-28}$ 0.97
(101)32 2-(100) 43 12 3319.12 30 128.50 (2.79 $\pm $ 0.57) $\times$ 10-20 $1.21\times10^{-27}$ 0.96
(101)42 2-(001) 53 32 3308.06 30 229.17 (2.63 $\pm $ 0.82) $\times$ 10-20 $7.46\times10^{-28}$ 0.68
           
1 $T_{\rm rot}$ = 70 K. 2 In setting #2.          


(b) January 28, 2008; HCN $\nu _{3}$-band

Transition 		Wavenumber Wavelength Flux g-factor3 Atmospheric transmittance
  [cm-1] [Å] [W m-2] [W molecule-1]  
R6 3331.59 30 015.74 (5.08 $\pm $ 1.01) $\times$ 10-20 7.24 $\times$ 10-25 0.97
R5 3328.78 30 041.07 (4.22 $\pm $ 0.58) $\times$ 10-20 1.02 $\times$ 10-24 0.94
R4 3325.94 30 066.64 (5.77 $\pm $ 1.37) $\times$ 10-20 1.33 $\times$ 10-24 0.90
R3 3323.09 30 092.47 (2.68 $\pm $ 0.71) $\times$ 10-20 1.53 $\times$ 10-24 0.59
R2 3320.22 30 118.48 (4.71 $\pm $ 0.62) $\times$ 10-20 1.54 $\times$ 10-24 0.97
R1 3317.33 30 144.74 (3.43 $\pm $ 2.16) $\times$ 10-20 1.27 $\times$ 10-24 0.86
P2 3305.54 30 252.21 (7.12 $\pm $ 0.73) $\times$ 10-20 1.45 $\times$ 10-24 0.96
P3 3302.55 30 279.21 (7.85 $\pm $ 0.89) $\times$ 10-20 1.89 $\times$ 10-24 0.96
P4 3299.53 30 307.37 (7.40 $\pm $ 0.81) $\times$ 10-20 2.02 $\times$ 10-24 0.93
P7 3290.35 30 391.91 (3.20 $\pm $ 0.78) $\times$ 10-20 1.16 $\times$ 10-24 0.90
P8 3287.25 30 420.58 (2.90 $\pm $ 0.70) $\times$ 10-20 8.01 $\times$ 10-25 0.95

3 $T_{\rm rot} = 54$ K.
Flux values listed in the 4th column are calibrated but not corrected for the telluric absorption. The g-factors listed in the 5th
column are calculated for the observational conditions. Field of view of the aperture is $0.2\hbox {$^{\prime \prime }$ }\times \sim 0.8\hbox {$^{\prime \prime }$ }$. The * mark indicates
that the line is blended with the line above.

(c) January 28, 2008; C2H2 $\nu _{3}$-band
Transition Wavenumber Wavelength Flux g-factor4 Atmospheric transmittance
  [cm-1] [Å] [W m-2] [W molecule-1]  
R3 3304.17 30267.30 (1.73 $\pm $ 0.61) $\times$ 10-20 1.03 $\times$ 10-24 0.95
P3 3287.76 30418.40 (3.22 $\pm $ 0.82) $\times$ 10-20 1.05 $\times$ 10-24 0.92
P5 3282.99 30462.99 (2.25 $\pm $ 0.89) $\times$ 10-20 1.27 $\times$ 10-24 0.71
4 $T_{\rm rot} = 70$ K is assumed.          


(d) February 4, 2008; H2O
Transition Wavenumber Wavelength Flux g-factor5 Atmospheric transmittance
($\nu_{1}'$,$\nu_{2}'$,$\nu_{3}'$) J'Ka' Kc'-($\nu_{1}''$,$\nu_{2}''$,$\nu_{3}''$) J''Ka'' Kc'' [cm-1] [Å] [W m-2] [W molecule-1]  
(201)11 1-(200)11 0 3405.42 29 364.95 (4.07 $\pm $ 0.78) $\times$ 10-20 1.81 $\times$ 10-27 0.85
(201)22 1-(200)22 0 3405.39 29 365.21 * 1.58 $\times$ 10-28 0.82
(200)11 1-(001)21 2 3403.23 29 383.84 (6.84 $\pm $ 0.77) $\times$ 10-20 4.63 $\times$ 10-27 0.64
(200)10 1-(001)20 2 3399.37 29 417.23 (1.98 $\pm $ 0.06) $\times$ 10-19 1.37 $\times$ 10-26 0.74
(200)22 1-(100)33 0 3394.08 29 463.10 (1.00 $\pm $ 0.06) $\times$ 10-19 1.10 $\times$ 10-26 0.63
(200)41 4-(001)41 3 3390.04 29 498.19 (3.25 $\pm $ 0.62) $\times$ 10-20 2.08 $\times$ 10-28 0.74
(101)21 2-(100)33 1 3390.02 29 498.38 * 1.47 $\times$ 10-27 0.79
(201)00 0-(200)10 1 3388.77 29 509.23 (3.68 $\pm $ 0.72) $\times$ 10-20 2.81 $\times$ 10-27 0.90
(200)21 2-(001)31 3 3382.10 29 567.43 (1.63 $\pm $ 0.05) $\times$ 10-19 1.25 $\times$ 10-26 0.86
(200)20 2-(001)30 3 3378.48 29 599.08 (3.81 $\pm $ 0.53) $\times$ 10-20 3.09 $\times$ 10-27 0.77
(200)22 1-(001)32 2 3372.76 29649.35 (9.25 $\pm $ 0.53) $\times$ 10-20 7.13 $\times$ 10-27 0.89
(210)22 1-(110)33 0 3361.03 29752.74 (2.45 $\pm $ 0.55) $\times$ 10-20 5.19 $\times$ 10-28 0.66
(200)31 3-(001)41 4 3360.99 29753.14 * 1.77 $\times$ 10-27 0.62
(200)30 3-(001)40 4 3358.92 29771.45 (8.64 $\pm $ 0.61) $\times$ 10-20 4.83 $\times$ 10-27 0.78
(201)20 2-(200)30 3 3346.99 29877.58 (6.73 $\pm $ 0.63) $\times$ 10-20 2.60 $\times$ 10-27 0.94
(200)31 2-(001)41 3 3341.17 29929.64 (2.94 $\pm $ 0.54) $\times$ 10-20 2.22 $\times$ 10-27 0.90
(200)41 4-(001)51 5 3340.95 29931.63 (2.71 $\pm $ 0.53) $\times$ 10-20 2.13 $\times$ 10-27 0.88
(201)31 3-(200)41 4 3329.42 30035.28 (1.89 $\pm $ 0.66) $\times$ 10-20 1.07 $\times$ 10-27 0.85
5 $T_{\rm rot} = 65$ K.          


(e) February 4, 2008; CH4 $\nu _{3}$-band
Transition Wavenumber Wavelength Flux g-factor6 Atmospheric transmittance
  [cm-1] [Å] [W m-2] [W molecule-1]  
R1 3038.50 32 913.67 (2.03 $\pm $ 0.78) $\times$ 10-20 1.20 $\times$ 10-24 0.32
R0 3028.75 33 019.58 (3.44 $\pm $ 0.76) $\times$ 10-20 1.46 $\times$ 10-24 0.27
6 $T_{\rm rot}$ = 70 K is assumed.          


(f) February 4, 2008; C2H6 $\nu _{7}$-band
Transition Wavenumber Wavelength Flux g-factor7 Atmospheric transmittance
  [cm-1] [Å] [W m-2] [W molecule-1]  
RQ0 2986.73 33481.43 (4.23 $\pm $ 0.60) $\times$ 10-20 2.10 $\times$ 10-24 0.91
PQ1 2983.38 33519.03 (4.51 $\pm $ 0.60) $\times$ 10-20 1.89 $\times$ 10-24 0.94
PQ2 2980.07 33556.26 (5.01 $\pm $ 1.01) $\times$ 10-20 1.71 $\times$ 10-24 0.79
PQ3 2976.77 33593.46 (2.58 $\pm $ 0.71) $\times$ 10-20 1.22 $\times$ 10-24 0.91
7 $T_{\rm rot} = 70$ K is assumed, Dello Russo et al. (2001).

(g) February 4, 2008; CH3OH $\nu _{2}$-band
Transition Wavenumber Wavelength Flux g-factor8 Atmospheric transmittance
  [cm-1] [Å] [W m-2] [W molecule-1]  
  3001.10 33 323.83 (4.80 $\pm $ 0.88) $\times$ 10-20 2.86 $\times$ 10-25 0.95
  3001.04 33 324.49 *   0.94
  2997.16 33 367.63 (5.38 $\pm $ 0.70) $\times$ 10-20   0.89
  2997.15 33 367.75 *   0.85

8 The g-factor of the $\nu _{2}$ methanol line listed here is derived from the g-factor of the methanol $\nu _{3}$-band Q-branch by comparing the intensities of these lines in cometary spectra (see text). The g-factor of the methanol $\nu _{3}$-band Q-branch is taken equal to $5.80 \times 10^{-25}$ [W molecule-1] at $T_{\rm rot} = 70$ K (DiSanti, private comm.).

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