Table 3
Estimated distances and maser luminosities from D-conflguration maps for the maser sources listed in Table 2.
| Name (glon, glat) (1) | ΔVD (km s−1) (2) | Dist. (kpc) (3) | Note (4) | SInt (Jy km s−1) (5) | Lmaser,D (L⊙) (6) |
|---|---|---|---|---|---|
| G35.2260–0.3544 | 0.72 | 9.43 ± 0.36 | В | 0.96 ±0.07 | 5.8 × 10−7 |
| G35.2476–0.2365 | 0.90 | 4.84 ± 0.61 | В | 3.26 ±0.08 | 5.2 × 10−7 |
| G35.3974+0.0252 | 0.90 | 5.90 ± 0.54 | A | 1.22 ± 0.07 | 2.86 × 10−7 |
| G35.4166–0.2839 | 0.90 | 3.20 + 0.37 | A | 4.53 ± 0.07 | 3.13 × 10−7 |
| G35.4571–0.1782 | 1.80 | 4.10 ±0.38 | A | 2.27 ± 0.13 | 2.58 × 10−7 |
Notes. Refer to the online table for a complete list of sources. Column (1) is the GLOSTAR source name. Column (2) gives the total velocity extent of maser emission above the local 4σ level. Column (3) gives the distance obtained from the Bayesian distance estimator (Reid et al. 2019) or from the ATLASGAL compact source catalogue (CSC) (Urquhart et al. 2018, 2022) as marked in Col. (4) with а В or A respectively. Columns (5) and (6) give the maser integrated flux and luminosity, respectively.
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