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Table 6

GLOSTAR source catalog for the observed region.

GLOSTAR name 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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