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Table A.2

Glycolaldehyde emission lines detected towards NGC 1333 SVS13-A (in TB scale).

Transitiona ν a Eu a S μ2 a TdV b Vpeak b FWHM b Tpeak b rms
(MHz) (K) (D2) (K km s-1) (km s-1) (km s-1) (mK) (mK)

1.4 mm

3310,23–339,24 217 053.668 374.45 104.58 0.6(0.2) +8.4(0.0) 3.5(0.0) 184(21) 65
95,4–84,5 217 830.692 40.20 25.16 5.2(0.5) +7.0(0.7) 4.0(1.4) 1096(36) 76
203,17–194,16 218 260.540 126.14 43.31 2.3(0.7) +7.1(0.7) 4.5(1.4) 455(70) 64
293,26–292,27 219 122.861 247.80 47.54 1.3(0.5) +7.4(1.0) 4.7(1.5) 270(18) 54
76,2–65,1 220 196.605 37.41 29.67 5.6(1.8) +8.5(0.0) 3.5(0.0) 1518(268) 149
76,1–65,2 220 196.800 37.41 29.67
114,7–103,8 220 204.039 46.61 18.68 2.5(1.7) +8.4(0.0) 3.5(0.0) 685(268) 149

1.3 mm

2810,18–289,19 230 767.152 287.09 81.84 3.9(1.2) +7.3(0.9) 5.7(1.9) 630(221) 167
212,19–203,18 230 898.536 131.19 71.15 3.9(1.5) +8.4(0.0) 4.0(0.0) 864(164) 236
222,21–211,20 232 335.395 134.52 94.55 8.5 (1.8) +9.3(0.3) 3.8 (1.5) 2097(45) 164
2710,18–279,19 232 522.255 271.37 77.57 3.0(0.9) +8.0(0.7) 4.3(1.5) 697(54) 130

Notes.

(a)

From the Jet Propulsion Laboratory database (Pickett et al. 1998).

(b)

The errors are the Gaussian fit uncertainties. For the weakest lines, the systemic velocity (see Table 1) and typical linewidths are assumed and consequently no error on these parameters is quoted.

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