Table 4
Statistics of the matches between GLOSTAR VLA D-configuration and other published surveys.
| Survey | Ref. | Wavelength | Resolution (″) | rms level mJy beam−1 | Num. of sources in GLOSTAR region | Num. of matches (10″) | Num. of matches (6″) |
|---|---|---|---|---|---|---|---|
| THOR | (1) | 20 cm | 25 | 0.3–1 | 6337 | 5179 | 5092 |
| RMS | (2) | 6 cm | 1.0–2.0 | 0.22 | 737 | 150 | 145 |
| CORNISH | (3) | 6 cm | 1.5 | 0.33 | 1754 | 1231 | 1221 |
| GLOSTAR B configuration | (4) | 6 cm | 1.0 | 0.08 | 5437 | 2496 | 2473 |
| ATLASGAL | (5) | 870 μm | 19.2 | 50–70 | 3096 | 198 | 109 |
| HiGAL | (6) | 70–500 μm | 5.8–35 | ... | 35 344 | 1096 | 918 |
| WISE | (7) | 3.4–22 μm | 6–12 | ... | 2 426 781 | 5473 | 3034 |
| GLIMPSE | (8,9) | 3.6–8.0 μm | 1.4–2 | ... | 18 100 849 | 7326 | 5525 |
Notes. A match radius of 10″ and 6″ has been used, centered on the peak of the GLOSTAR emission. References are: (1) Wang et al. (2018), (2) Urquhart et al. (2009), (3) Hoare et al. (2012), (4) Yang et al. (2023), (5) Schuller et al. (2009), (6) Molinari et al. (2016), (7) Wright et al. (2010), (8) Churchwell et al. (2009) and (9) (Fazio et al. 2004).
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