Table A.2
Data used to create Fig. 5.
| Source (l b) | 6.7 GHz | 12.2 GHz | ||||||
|---|---|---|---|---|---|---|---|---|
| Speak 2010 | Speak 2019 | Speak 2010 | Speak 2019 | Vpeak 2010 | Vpeak 2019 | Nfeat. 2010 | Nfeat. 2019 | |
| (° °) | (Jy) | (Jy) | (Jy) | (Jy) | (km s−1) | (km s−1) | ||
| G32.744−0.075 | 56.0 | 38.3 | 7.2 | 3.7 | 30.5 | 30.6 | 3 | 3 |
| G33.641−0.228 | 140.0 | 145.0 | 29.3 | 37.8 | 58.8 | 60.3 | 3 | 2 |
| G35.200−1.736 | 500.0 | 37.0 | 46.0 | 11.9 | 44.6 | 45.2 | 8 | 1 |
| G36.115+0.552 | 40.0 | 13.7 | 4.9 | 2.4 | 74.6 | 75.1 | 1 | 1 |
| G37.430+1.518 | 400.0 | 293.0 | 90.0 | 73.8 | 41.2 | 41.3 | 1 | 1 |
| G37.546−0.112 | 4.0 | 4.0 | 1.4 | 1.1 | 50.0 | 50.0 | 1 | 1 |
| G40.282−0.219 | 22.0 | 25.5 | 3.7 | 1.7 | 74.3 | 74.4 | 3 | 3 |
| G40.425+0.700 | 22.0 | 24.7 | 8.2 | 7.9 | 6.7 | 6.6 | 2 | 2 |
| G42.034+0.190 | 22.0 | 14.1 | 2.6 | 4.6 | 11.5 | 11.5 | 4 | 4 |
| G43.890−0.784 | 9.0 | 9.1 | 4.2 | 2.4 | 47.9 | 51.7 | 2 | 2 |
| G45.804−0.356 | 12.0 | 12.3 | 2.8 | 1.3 | 60.0 | 60.0 | 1 | 1 |
| G49.043−1.079 | 33.0 | 12.1 | 7.1 | 0.9 | 37.4 | 36.3 | 2 | 1 |
| G49.265+0.311 | 7.0 | 6.5 | 1.2 | 1.4 | –4.2 | –4.6 | 1 | 2 |
| G49.349+0.413 | 8.0 | 7.3 | 2.8 | 2.0 | 68.3 | 68.1 | 2 | 2 |
| G49.416+0.324 | 8.0 | 9.6 | 0.9 | 0.8 | –10.5 | -10.2 | 1 | 1 |
| G52.199+0.723 | 6.0 | 9.8 | 5.4 | 2.8 | 3.7 | 3.3 | 2 | 2 |
| G52.663−1.092 | 4.5 | 5.9 | 2.2 | 2.6 | 65.2 | 65.2 | 1 | 1 |
Notes. Column 2 presents crude estimation of the 6.7 GHz maser peak flux density from Breen et al. (2015), Col. 3 presents peak flux densities from unpublished 6.7 GHz line survey. Data for Cols. 4 and 6 is taken from Breen et al. (2016), Table 2. Columns 5 and 7 present the same data, as in Table 1. Last two columns present number of visible features on 12 GHz spectra from Breen et al. (2016) and this survey, respectively.
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