Table 7: Measurements obtained toward Sgr B2(N) with the Australia Telescope Compact Array at 91 GHz.
Moleculea Conf.b $f_{{\rm min}}$c $f_{{\rm max}}$c $\sigma^d$ $F_{{\rm peak}}$e $\Delta\alpha$e $\Delta\delta$e $\theta_{{\rm maj}}^{{fwhm}}$ e $\theta_{{\rm min}}^{{fwhm}}$ e PAe $\Phi_{{\rm ATCA}}^f$ $\Phi_{{\rm 30~m}}^g$
    (MHz)) (MHz) (Jy/beam km s-1) ('') ('') ('') ('') ($^\circ $) (Jy km s-1) (Jy km s-1)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)
AAN F7 E 90 558.99 90 563.99 0.12 0.87 -2.32 $\pm$ 0.20 -0.22 $\pm$ 0.13 2.9 $\pm$ 0.4 2.2 $\pm$ 0.3 29.2 $\pm$ 0.1 1.12 3.06
AAN F7 I 90 559.05 90 564.05 0.15 1.47 -1.94 $\pm$ 0.20 0.58 $\pm$ 0.10 3.6 $\pm$ 0.4 2.7 $\pm$ 0.2 -79.8 $\pm$ 1.5 1.73 3.06
AAN F7 C 90 561.48 90 564.23 0.10 1.53 -0.96 $\pm$ 0.21 0.71 $\pm$ 0.17 7.0 $\pm$ 0.4 4.8 $\pm$ 0.3 -80.3 $\pm$ 0.0 1.37 1.79
AAN F7 M 90 559.13 90 563.96 0.12 1.19 -2.10 $\pm$ 0.16 0.25 $\pm$ 0.10 3.1 $\pm$ 0.3 2.7 $\pm$ 0.2 83.5 $\pm$ 0.0 1.71 2.96
AAN F7 A 90 562.03 90 563.96 0.06 0.61 -1.23 $\pm$ 0.15 0.26 $\pm$ 0.10 5.3 $\pm$ 0.3 3.3 $\pm$ 0.2 87.1 $\pm$ 22.5 1.37 1.00
AAN F8 E 90 781.27 90 786.77 0.21 1.22 -1.94 $\pm$ 0.24 -0.18 $\pm$ 0.16 3.8 $\pm$ 0.5 2.1 $\pm$ 0.3 45.0 $\pm$ 0.0 1.70 7.23
AAN F9 E 90 788.02 90 792.02 0.09 0.45 -1.70 $\pm$ 0.29 -0.06 $\pm$ 0.19 3.4 $\pm$ 0.6 1.9 $\pm$ 0.4 45.0 $\pm$ 0.1 0.49 2.14
AAN F9 I 90 788.11 90 792.11 0.13 0.97 -1.77 $\pm$ 0.26 0.23 $\pm$ 0.13 3.6 $\pm$ 0.5 2.2 $\pm$ 0.3 -84.0 $\pm$ 0.0 1.01 2.14
AAN F9 C 90 790.54 90 792.04 0.10 2.00 -1.25 $\pm$ 0.16 0.49 $\pm$ 0.13 6.1 $\pm$ 0.3 5.8 $\pm$ 0.3 -45.0 $\pm$ 0.0 1.86 1.59
AAN F9 M 90 788.04 90 792.16 0.10 0.85 -1.67 $\pm$ 0.17 0.02 $\pm$ 0.11 3.1 $\pm$ 0.3 2.4 $\pm$ 0.2 75.9 $\pm$ 0.1 1.07 2.14
AAN F9 A 90 790.95 90 792.16 0.05 0.63 -1.26 $\pm$ 0.14 0.23 $\pm$ 0.09 4.8 $\pm$ 0.3 3.9 $\pm$ 0.2 84.5 $\pm$ 0.0 1.51 1.31
AAN F10 E 90 796.52 90 800.77 0.16 1.17 -2.51 $\pm$ 0.20 0.02 $\pm$ 0.13 2.7 $\pm$ 0.4 2.2 $\pm$ 0.3 -81.2 $\pm$ 0.2 1.38 6.48
AAN F10 I 90 796.61 90 800.86 0.10 0.93 -1.81 $\pm$ 0.21 0.20 $\pm$ 0.11 3.3 $\pm$ 0.4 2.0 $\pm$ 0.2 82.3 $\pm$ 0.0 0.79 6.19
AAN F10 C 90 796.54 90 800.79 0.15 3.36 -1.08 $\pm$ 0.15 0.28 $\pm$ 0.12 6.6 $\pm$ 0.3 4.9 $\pm$ 0.2 -77.7 $\pm$ 0.0 2.78 6.48
AAN F10 M 90 796.52 90 800.88 0.13 1.32 -2.28 $\pm$ 0.15 0.03 $\pm$ 0.09 2.9 $\pm$ 0.3 2.2 $\pm$ 0.2 83.7 $\pm$ 22.5 1.42 6.48
AAN F10 A 90 796.52 90 800.88 0.13 1.82 -1.66 $\pm$ 0.12 0.12 $\pm$ 0.08 4.5 $\pm$ 0.2 3.1 $\pm$ 0.2 -89.3 $\pm$ 22.5 3.24 6.48
HC13CCN v7=1 HV I 90 804.36 90 805.36 0.05 0.49 -1.94 $\pm$ 0.20 5.16 $\pm$ 0.10 3.0 $\pm$ 0.4 2.0 $\pm$ 0.2 84.4 $\pm$ 0.0 0.41 2.39
HC13CCN v7=1 LV I 90 806.11 90 809.36 0.14 2.74 -1.56 $\pm$ 0.10 0.55 $\pm$ 0.05 3.7 $\pm$ 0.2 2.1 $\pm$ 0.1 83.6 $\pm$ 0.0 2.69 10.30
HC13CCN v7=1 LV C 90 806.04 90 809.29 0.15 4.98 -1.71 $\pm$ 0.10 0.25 $\pm$ 0.08 7.1 $\pm$ 0.2 4.4 $\pm$ 0.2 -83.8 $\pm$ 0.0 4.12 10.30
CH3OH $v_{{\rm t}}=1$ HV I 90 809.61 90 811.11 0.09 1.52 -1.85 $\pm$ 0.12 5.23 $\pm$ 0.06 3.7 $\pm$ 0.2 2.1 $\pm$ 0.1 -85.7 $\pm$ 0.1 1.54 6.55
CH3OH $v_{{\rm t}}=1$ LV I 90 812.36 90 814.11 0.11 1.60 -1.84 $\pm$ 0.13 0.44 $\pm$ 0.06 3.8 $\pm$ 0.3 3.6 $\pm$ 0.1 23.7 $\pm$ 22.5 2.72 10.40
CH3OH $v_{{\rm t}}=1$ LV C 90 812.29 90 814.29 0.12 5.22 -1.86 $\pm$ 0.08 -0.03 $\pm$ 0.06 7.1 $\pm$ 0.2 4.5 $\pm$ 0.1 -77.9 $\pm$ 0.0 4.29 10.40
a For amino acetonitrile (AAN), we give the feature number like in Col. 8 of Table 3. For the other molecules, HV and LV mean high and low velocity component, respectively.
b Interferometer configuration: E: extended (H 214), I: intermediate (H 168), C: compact (H 75), M: mixed (H 214 + H 168), A: all (H 214 + H 168 + H 75).
c Frequency range over which the intensity was integrated.
d Noise level in the integrated intensity map shown in Fig. 7.
e Peak flux, offsets in right ascension and declination with respect to the reference position of Fig. 7, major and minor diameters (FWHM), and position angle (East from North) derived by fitting an elliptical 2D Gaussian to the integrated intensity map shown in Fig. 7. The uncertainty in Col. 11 is the formal uncertainty given by the fitting routine GAUSS_2D, while the uncertainties correspond to the beam size divided by two times the signal-to-noise ratio in Cols. 7 and 8 and by the signal-to-noise ratio in Cols. 9 and 10.
f Flux spatially integrated over the region showing emission in the integrated intensity map of Fig. 7.
g Integrated flux of the 30 m spectrum computed over the frequency range given in Cols. 3 and 4.


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