Table C.1
Methanol masers toward Cygnus X reported in previous surveys.
| RA | Dec | Name | VLSR | Sν, Peak |
|---|---|---|---|---|
| (km s−1) | (Jy beam−1) | |||
| 20 29 24.937 | +40 11 19.29 | G078.886+0.708 | –7.02 | 0.54 |
| 20 30 50.685 | +41 02 27.50 | G079.735+0.990 | –5.44 | 23.17 |
| –3.86 | 5.00 | |||
| –3.16 | 1.91 | |||
| 20 37 00.980 | +41 34 55.05 | G080.861+0.383 | –11.06 | 2.53 |
| –4.04 | 8.52 | |||
| –1.93 | 1.17 | |||
| 20 39 00.879 | +42 22 48.93 | G081.721+0.571 | –3.51 | 0.86 |
| –2.63 | 2.96 | |||
| 20 39 00.378 | +42 24 36.92 | G081.744+0.590 | 3.86 | 3.82 |
| 4.57 | 5.53 | |||
| 20 39 01.573 | +42 24 59.09 | G081.752+0.590 | –8.60 | 8.35 |
| –6.67 | 3.43 | |||
| –5.80 | 3.87 | |||
| –2.81 | 1.51 | |||
| –2.28 | 0.90 | |||
| 20 39 02.274 | +42 25 50.81 | G081.765+0.597 | –1.23 | 2.54 |
| 20 38 36.423 | +42 37 35.01 | G081.871+0.780 | 3.51 | 42.91 |
| 4.04 | 99.94 | |||
| 4.74 | 166.73 | |||
| 5.27 | 76.09 | |||
| 5.80 | 67.27 | |||
| 7.20 | 174.93 | |||
| 9.48 | 17.48 | |||
| VLSR, ΔV | Sν, Peak | |||
| (km s−1) | (Jy) | |||
| 20 23 23.65 | +37 35 34.3 | G76.093+0.158 | 4.92 (4.27, 6.90) | 0.49 |
| 20 29 20.35 | +40 11 37.5 | G78.882+0.723 | –6.94 (–7.41, –6.51) | 0.95 |
| 20 30 22.77 | +40 09 23.2 | G78.969+0.541 | 4.74 (4.01, 5.48) | 1.24 |
| 20 30 50.70 | +41 02 28.8 | G79.736+0.991 | –5.51 (–6.63, –2.84) | 19.4 |
| 20 37 01.02 | +41 34 56.9 | G80.862+0.383 | –4.01 (–4.57, –1.77) | 9.67 |
| 20 39 02.01 | +42 24 59.3 | G81.752+0.591 | –8.57 (–9.39, 5.04) | 15.4 |
| 20 37 47.39 | +42 38 39.0 | G81.794+0.911(a) | 7.19 (–4.73, 7.54) | 0.59 |
| 20 38 36.67 | +42 37 30.6 | G81.871+0.779 | 4.53 (2.55, 9.87) | 225.7 |
| 20 40 16.72 | +42 56 28.6 | G82.308+0.729 | 10.3 (10.0, 11.3) | 58.4 |
Notes. The top table lists maser components reported in the catalog of Hu et al. (2016) and gives the LSR velocity of the component and the flux density. The bottom table lists masers in the catalog of Yang et al. (2019) and gives LSR velocity of peak emission, the LSR velocity interval of the maser emission in parentheses, and peak flux density. (a) Not detected in GLOSTAR.
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