Table A.1
Summary of NH3 (9, 6) maser observations.
Source | Telescope | Beam | Epoch | Channel | Sν | rms | ∫ Sνdv | VLSR | ΔV1∕2 |
---|---|---|---|---|---|---|---|---|---|
size | spacing | ||||||||
(km s−1) | (Jy) | (mJy) | (Jy km s−1) | (km s−1) | |||||
Cep A | Effelsberg | 49′′ | 2020, Jan. 04 | 0.62 | 0.67 | 3.41 | 1.19 ± 0.02 | -1.11 ± 0.02 | 1.67 ± 0.04 |
Effelsberg | 49′′ | 2021, Feb. 11 | 0.62 | 0.59 | 5.97 | 1.08 ± 0.02 | -0.74 ± 0.02 | 1.70 ± 0.04 | |
Effelsberg | 49′′ | 2021, Feb. 15 | 0.62 | 0.65 | 10.98 | 1.11 ± 0.03 | -0.75 ± 0.02 | 1.60 ± 0.05 | |
JVLAa | 1′′.47 × 0′′.99 | 2021, Jul. 13 | 0.13 | 1.13 | 144 | 0.89 ± 0.09 | -0.86 ± 0.03 | 0.74 ± 0.12 | |
Effelsberg | 49′′ | 2021, Aug. 11 | 0.07 | 0.98 | 13.36 | 0.49 ± 0.02 | -0.90 ± 0.01 | 0.47 ± 0.01 | |
0.35 | 0.26 ± 0.02 | -0.28 ± 0.02 | 0.69 ± 0.05 | ||||||
Effelsberg | 49′′ | 2021, Aug. 12 | 0.07 | 0.98 | 13.35 | 0.50 ± 0.01 | -0.89 ± 0.07 | 0.48 ± 0.07 | |
0.35 | 0.20 ± 0.01 | -0.29 ± 0.07 | 0.54 ± 0.07 | ||||||
0.06 | 0.07 ± 0.01 | 0.51 ± 0.07 | 1.09 ± 0.07 | ||||||
0.02 | 0.02 ± 0.01 | 2.15 ± 0.07 | 0.80 ± 0.07 | ||||||
0.07 | 0.06 ± 0.01 | 2.89 ± 0.07 | 0.92 ± 0.07 | ||||||
G34.26+0.15 | Effelsberg | 49′′ | 2020, Jan. 03 | 0.62 | 0.30 | 1.26 | 0.65 ± 0.03 | 62.50 ± 0.05 | 2.05 ± 0.13 |
Effelsberg | 49′′ | 2021, Feb. 11 | 0.62 | 0.24 | 2.42 | 0.40 ± 0.02 | 55.76 ± 0.04 | 1.60 ± 0.12 | |
Effelsberg | 49′′ | 2021, Feb. 15 | 0.62 | 0.20 | 4.86 | 0.38 ± 0.02 | 55.71 ± 0.05 | 1.80 ± 0.14 | |
JVLAb | 1′′.33 × 1′′.06 | 2021, Jul. 13 | 0.13 | 0.23 | 37.1 | 0.09 ± 0.02 | 54.41 ± 0.03 | 0.38 ± 0.09 | |
0.22 | 0.22 ± 0.02 | 55.82 ± 0.05 | 0.95 ± 0.12 | ||||||
0.15 | 0.06 ± 0.01 | 57.21 ± 0.04 | 0.35 ± 0.08 | ||||||
Effelsberg | 49′′ | 2021, Aug. 11 | 0.07 | 0.08 | 13.92 | 0.06 ± 0.007 | 54.10 ± 0.05 | 0.68 ± 0.12 | |
0.07 | 0.02 ± 0.006 | 54.82 ± 0.03 | 0.31 ± 0.09 | ||||||
0.12 | 0.10 ± 0.006 | 55.85 ± 0.02 | 0.75 ± 0.06 | ||||||
Effelsberg | 49′′ | 2021, Aug. 12 | 0.07 | 0.16 | 27.40 | 0.09 ± 0.008 | 55.83 ± 0.02 | 0.56 ± 0.05 |
Notes. The spectral parameters are obtained from Gaussian fitting. aThe JVLA spectrum toward Cep A is extracted from the Effelsberg-beam-sized region (FWHM 49′′). b For G34.26+0.15, the JVLA beam samples the NH3 (9,6) spectrum over a region of radius 3′′.5, which contains all detected NH3 (9,6) emissions.
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