Table 6
GLOSTAR source catalog for the observed region.
GLOSTAR name | ℓ | b | S/N | Speak | σSpeak | Sint | σSint | Yfactor | Radius | Spectral index | Radio | submm | IR | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(°) | (°) | (mJy beam−1) | (mJy) | (″) | α | Δα | α* | Δα* | GB | C | R | T | MM | A | H | W | G | Class | Ref. | Method | |||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) | (16) | (17) | (18) | (19) | (20) | (21) | (22) | (23) | (24) | (25) | (26) |
G002.005+00.348 | 02.0047 | +0.3479 | 09.2 | 1.29 | 0.16 | 1.34 | 0.16 | 1.0 | 13.10 | ... | ... | ... | ... | EgC | 1 | No SMM or IR counterpart | |||||||||
G002.007–00.681 | 02.0072 | −0.6806 | 170.3 | 26.07 | 1.41 | 121.27 | 6.07 | 4.7 | 52.00 | ... | ... | ... | ... | Y | HII | 1 | Only FIR counterpart | ||||||||
G002.011+00.108 | 02.0111 | +0.1076 | 05.4 | 0.75 | 0.14 | 1.10 | 0.15 | 1.5 | 12.50 | ... | ... | ... | ... | Y | EgC | 1 | No SMM or IR counterpart | ||||||||
G002.012+00.744 | 02.0120 | +0.7438 | 178.3 | 15.20 | 0.82 | 13.67 | 0.69 | 0.9 | 21.10 | ... | ... | −0.16 | 0.05 | Y | Y | Y | PN | 2 | Previously known source | ||||||
G002.013+00.896 | 02.0125 | +0.8959 | 05.3 | 0.46 | 0.09 | 0.57 | 0.09 | 1.2 | 11.10 | ... | ... | ... | ... | Y | EgC | 1 | Color-magnitude constrain | ||||||||
G002.018+00.669 | 02.0177 | +0.6688 | 32.2 | 3.12 | 0.19 | 3.52 | 0.20 | 1.1 | 20.20 | ... | ... | −0.33 | 0.25 | Y | Y | Other | 2 | Previously known source | |||||||
G002.021–00.824 | 02.0210 | −0.8243 | 19.0 | 1.92 | 0.14 | 1.65 | 0.13 | 0.9 | 14.40 | ... | ... | 0.07 | 0.18 | Y | Y | HII | 1 | Color-magnitude constrain | |||||||
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
G021.103–00.976 | 21.1032 | −0.9757 | 15.3 | 2.89 | 0.24 | 2.67 | 0.23 | 0.9 | 14.20 | 0.26 | 0.15 | 0.04 | 0.24 | Y | Y | Y | Radio-star | 2 | Previously known source | ||||||
G021.103+00.664 | 21.1034 | +0.6639 | 07.4 | 0.60 | 0.09 | 0.51 | 0.09 | 0.8 | 10.60 | ... | ... | ... | Y | Y | Y | EgC | 2 | Previously known source | |||||||
G021.114+00.872 | 21.1137 | +0.8723 | 05.1 | 0.43 | 0.09 | 0.44 | 0.09 | 1.0 | 9.70 | −0.96 | 0.20 | Y | Y | Y | Y | Radio-star | 2 | Previously known source | |||||||
G021.121–00.956 | 21.1206 | −0.9563 | 05.6 | 0.91 | 0.17 | 1.29 | 0.17 | 1.4 | 12.10 | ... | ... | ... | ... | Y | Y | EgC | 2 | Previously known source | |||||||
G021.126–00.294 | 21.1258 | −0.2944 | 17.2 | 5.42 | 0.43 | 204.65 | 10.24 | 37.7 | 106.60 | 0.11 | 0.12 | ... | ... | Y | LSS | 1 | Visual Inspection | ||||||||
G021.130–00.247 | 21.1300 | −0.2465 | 05.4 | 1.63 | 0.31 | 17.96 | 0.95 | 11.0 | 31.80 | ... | ... | ... | ... | LSS | 1 | Visual Inspection | |||||||||
G021.145+00.585 | 21.1445 | +0.5854 | 05.9 | 0.49 | 0.09 | 0.68 | 0.09 | 1.4 | 12.60 | ... | ... | ... | ... | EgC | 1 | No SMM or IR counterpart | |||||||||
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
G047.145–00.166 | 47.1451 | −0.1660 | 04.1 | 0.25 | 0.06 | 0.23 | 0.06 | 0.9 | 7.70 | ... | ... | ... | ... | Y | EgC | 1 | Only MIR counterparts | ||||||||
G047.147+00.730 | 47.1471 | +0.7299 | 20.1 | 1.36 | 0.10 | 11.02 | 0.56 | 8.1 | 46.90 | ... | ... | ... | ... | SNR | 7 | Previously known SNR | |||||||||
G047.147–00.113 | 47.1472 | −0.1132 | 05.1 | 0.31 | 0.06 | 0.28 | 0.06 | 0.9 | 9.00 | ... | ... | ... | ... | Y | EgC | 1 | Only MIR counterparts | ||||||||
G047.154+00.890 | 47.1540 | +0.8903 | 24.6 | 1.52 | 0.10 | 1.72 | 0.11 | 1.1 | 18.90 | −0.22 | 0.07 | −0.64 | 0.30 | Y | Y | EgC | 1 | Only MIR counterparts | |||||||
G047.162–00.513 | 47.1617 | −0.5132 | 04.5 | 0.28 | 0.06 | 0.21 | 0.06 | 0.8 | 7.50 | −0.55 | 0.22 | ... | ... | Y | EgC | 1 | No SMM or IR counterpart | ||||||||
G047.171–00.621 | 47.1708 | −0.6208 | 04.0 | 0.24 | 0.06 | 0.16 | 0.06 | 0.6 | 6.30 | ... | ... | ... | ... | Y | Y | EgC | 1 | Color-magnitude constrain | |||||||
G047.172–00.481 | 47.1722 | −0.4806 | 08.5 | 0.52 | 0.07 | 0.39 | 0.06 | 0.8 | 10.60 | −0.52 | 0.13 | ... | ... | Y | Y | EgC | 1 | Only MIR counterparts | |||||||
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
· | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · | · |
G059.932+00.837 | 59.9320 | +0.8368 | 55.7 | 5.88 | 0.33 | 7.02 | 0.37 | 1.2 | 21.60 | −0.47 | 0.04 | −0.66 | 0.11 | Y | EgC | 1 | No SMM or IR counterpart | ||||||||
G059.937–00.353 | 59.9365 | −0.3528 | 05.2 | 0.88 | 0.18 | 0.93 | 0.18 | 1.1 | 10.00 | −0.43 | 0.16 | ... | ... | Y | Y | Y | SNR | 7 | Previously known SNR | ||||||
G059.940–00.157 | 59.9399 | −0.1569 | 39.4 | 6.92 | 0.41 | 7.06 | 0.39 | 1.0 | 18.60 | −0.03 | 0.05 | 0.36 | 0.12 | Y | Y | EgC | 3 | Previously known source | |||||||
G059.941–00.042 | 59.9413 | −0.0417 | 28.6 | 4.86 | 0.31 | 5.58 | 0.33 | 1.1 | 18.80 | −0.52 | 0.05 | −0.88 | 0.23 | Y | EgC | 1 | No SMM or IR counterpart | ||||||||
G059.948+00.555 | 59.9478 | +0.5549 | 14.6 | 1.83 | 0.16 | 1.67 | 0.15 | 0.9 | 14.00 | −0.13 | 0.09 | −0.28 | 0.28 | Y | Y | Y | EgC | 1 | Color-magnitude constrain | ||||||
G059.963+00.036 | 59.9629 | +0.0361 | 04.6 | 0.94 | 0.21 | 1.26 | 0.21 | 1.3 | 10.20 | ... | ... | ... | ... | Y | Y | EgC | 1 | Color-magnitude constrain | |||||||
G059.968+00.660 | 59.9680 | +0.6597 | 07.1 | 1.17 | 0.18 | 0.89 | 0.17 | 0.8 | 11.00 | −0.04 | 0.14 | ... | ... | Y | Y | Y | EgC | 1 | Color-magnitude constrain |
Notes. The columns are, from left to right, the source name, Galactic coordinates, the S/N, the peak and integrated flux densities and their errors, the Y-factor, the effective radius, the estimated spectral indices determined from the GLOSTAR and THOR flux densities and from only the in-band GLOSTAR sub-images (*). Columns 15 to 23 list if the source has a counterpart in other surveys. Radio: GB for GLOSTAR B-configuration catalog (Yang et al. 2023), C for CORNISH (Hoare et al. 2012; Purcell et al. 2013), R for RMS (Urquhart et al. 2009), T for THOR (Beuther et al. 2016; Wang et al. 2020), and MM for methanol masers surveys (Nguyen et al. 2022; Green et al. 2009). Submillimeter/FIR: A for ATLASGAL (Urquhart et al. 2018). Infrared: H for HiGAL (Molinari et al. 2016), W for WISE (Wright et al. 2010), and G for GLIMPSE (Churchwell et al. 2009). Column 24 lists the final classification of the radio sources. References in column 25 are as follows: (1) This work, (2) Yang et al. (2023), (3) Purcell et al. (2013), (4) Urquhart et al. (2009), (5) Anderson et al. (2014), (6) Wang et al. (2020), (7) SNR remnants catalogs by Dokara et al. (2021) or Green (2019), and (8) Methanol maser catalogs by Nguyen et al. (2022) or Green et al. (2009). Finally, column 27 lists the method used for the source classification. Only a small portion of the data is provided here, and the full table is available at the CDS and through the dedicated GLOSTAR webpage at https://glostar.mpifr-bonn.mpg.de/glostar//
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