Table 7.
GLOSTAR source catalog.
GLOSTAR name | ℓ | b | SNR | Speak | ΔSpeak | Sint | ΔSint | Y-factor | Radius | Spectral index | Classification | ||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(°) | (°) | (mJy beam−1) | (mJy) | (″) | α | Δα | α(*) | Δα(*) | Type | Ref. | |||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) | (16) |
G028.091−00.092 | 28.091 | −0.093 | 11.4 | 3.12 | 0.32 | 4.26 | 0.35 | 1.1 | 16 | ⋯ | ⋯ | −0.07 | 0.25 | ⋯ | ⋯ |
G028.097−00.951 | 28.097 | −0.951 | 6.1 | 0.54 | 0.09 | 0.45 | 0.09 | 0.6 | 10 | ⋯ | ⋯ | −0.36 | 0.69 | ⋯ | ⋯ |
G028.098−00.781 | 28.098 | −0.781 | 186.9 | 17.80 | 0.96 | 22.06 | 1.11 | 1.2 | 25 | −0.91 | 0.01 | −1.08 | 0.03 | Radio star | 8 |
G028.100+00.644 | 28.099 | 0.644 | 6.5 | 0.87 | 0.14 | 0.76 | 0.14 | 0.6 | 10 | ⋯ | ⋯ | −0.57 | 0.28 | ⋯ | ⋯ |
G028.107−00.301 | 28.109 | −0.300 | 5.6 | 0.81 | 0.15 | 1.89 | 0.17 | 1.3 | 16 | ⋯ | ⋯ | −0.57 | 0.62 | ⋯ | ⋯ |
G028.109−00.490 | 28.108 | −0.490 | 20.0 | 2.84 | 0.21 | 2.70 | 0.20 | 0.9 | 15 | 0.06 | 0.09 | −0.18 | 0.1 | ⋯ | ⋯ |
G028.116−00.368 | 28.116 | −0.368 | 44.0 | 5.77 | 0.34 | 5.82 | 0.32 | 1.0 | 18 | −0.1 | 0.04 | −0.12 | 0.05 | ⋯ | ⋯ |
G028.120+00.419 | 28.120 | 0.419 | 4.9 | 0.87 | 0.19 | 0.64 | 0.18 | 0.4 | 8 | ⋯ | ⋯ | 0.15 | 0.43 | ⋯ | ⋯ |
G028.126+00.742 | 28.126 | 0.742 | 33.6 | 4.26 | 0.26 | 3.86 | 0.23 | 0.9 | 17 | −0.28 | 0.04 | −0.81 | 0.1 | ⋯ | ⋯ |
G028.127+00.341(‡) | 28.127 | 0.341 | 58.2 | 12.98 | 0.22 | 51.78 | 0.45 | 4.0 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
G028.137−00.194 | 28.138 | −0.194 | 4.2 | 0.77 | 0.19 | 0.68 | 0.19 | 0.4 | 8 | ⋯ | ⋯ | 0.53 | 0.37 | ⋯ | ⋯ |
G028.137−00.567 | 28.137 | −0.566 | 5.7 | 1.15 | 0.21 | 1.29 | 0.21 | 0.7 | 11 | −0.58 | 0.15 | −1.14 | 0.48 | ⋯ | ⋯ |
G028.140+00.329(‡) | 28.140 | 0.329 | 11.0 | 4.50 | 0.43 | 7.30 | 1.00 | 1.6 | ⋯ | 0.23 | 0.12 | −0.52 | 0.19 | HII region | 3 |
G028.144−00.378 | 28.144 | −0.379 | 8.0 | 1.08 | 0.15 | 1.11 | 0.15 | 0.8 | 12 | ⋯ | ⋯ | −0.46 | 0.55 | ⋯ | ⋯ |
G028.146+00.517 | 28.145 | 0.517 | 8.7 | 1.21 | 0.15 | 1.86 | 0.17 | 1.2 | 16 | ⋯ | ⋯ | −0.66 | 0.27 | ⋯ | ⋯ |
G028.149−00.998 | 28.149 | −0.997 | 76.9 | 11.93 | 0.66 | 19.71 | 1.00 | 1.6 | 25 | ⋯ | ⋯ | −1.05 | 0.05 | ⋯ | ⋯ |
G028.151+00.164 | 28.148 | 0.149 | 38.6 | 10.38 | 0.62 | 194.53 | 9.73 | 18.0 | 95 | ⋯ | ⋯ | ⋯ | ⋯ | HII region | 1 |
G028.151−00.958 | 28.151 | −0.957 | 16.0 | 2.00 | 0.16 | 2.25 | 0.17 | 1.0 | 17 | −0.37 | 0.09 | −0.4 | 0.28 | ⋯ | ⋯ |
G028.159−00.024 | 28.157 | −0.020 | 8.0 | 2.91 | 0.40 | 28.85 | 1.49 | 6.6 | 38 | ⋯ | ⋯ | ⋯ | ⋯ | Extended/Diffuse | 1 |
G028.159−00.798 | 28.159 | −0.798 | 29.1 | 2.97 | 0.19 | 2.67 | 0.17 | 0.9 | 16 | −0.35 | 0.05 | −0.36 | 0.23 | ⋯ | ⋯ |
G028.160−00.046 | 28.160 | −0.046 | 4.8 | 1.68 | 0.36 | 1.59 | 0.36 | 0.5 | 9 | ⋯ | ⋯ | −0.15 | 0.52 | HII region | 3 |
G028.163−00.163(†) | 28.163 | −0.163 | 7.0 | 0.50 | 0.07 | 2.00 | 0.34 | 4.0 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | HII region | 3 |
G028.172−00.605 | 28.173 | −0.606 | 4.9 | 1.13 | 0.24 | 14.55 | 0.76 | 5.5 | 32 | ⋯ | ⋯ | ⋯ | ⋯ | Ionization Front | 1 |
G028.178+00.074 | 28.178 | 0.072 | 4.3 | 1.49 | 0.35 | 9.56 | 0.59 | 2.5 | 21 | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ |
G028.187+00.583 | 28.187 | 0.583 | 22.3 | 3.02 | 0.21 | 2.75 | 0.19 | 0.9 | 15 | −0.01 | 0.06 | −0.71 | 0.11 | ⋯ | ⋯ |
G028.189−00.744 | 28.189 | −0.744 | 17.0 | 1.74 | 0.14 | 1.36 | 0.12 | 0.7 | 13 | −0.33 | 0.08 | −1.09 | 0.2 | ⋯ | ⋯ |
G028.193−00.785 | 28.193 | −0.785 | 8.6 | 0.87 | 0.11 | 1.29 | 0.12 | 1.1 | 16 | −0.68 | 0.12 | −0.22 | 0.26 | Pulsar | 5 |
G028.197−00.891 | 28.198 | −0.892 | 4.6 | 0.48 | 0.11 | 0.96 | 0.11 | 1.0 | 13 | ⋯ | ⋯ | −0.94 | 0.47 | ⋯ | ⋯ |
G028.200−00.050 | 28.191 | −0.050 | 771.1 | 332.67 | 17.92 | 396.10 | 19.81 | 1.2 | 48 | ⋯ | ⋯ | ⋯ | ⋯ | HII region | 3 |
G028.209+00.226 | 28.209 | 0.226 | 5.8 | 1.07 | 0.19 | 0.95 | 0.19 | 0.6 | 10 | ⋯ | ⋯ | 0.22 | 0.4 | ⋯ | ⋯ |
Notes. The source names are appended with a (‡) to indicate if a source has been split (as described in Sect. 3.2.1) and a (†) if the source has been recovered (as described in Sect. 3.2.2). (*)Values calculated using the 8 sub images are described in Sect. 2. Only a small portion of the data is provided here, the full table is available in electronic form at the CDS.
References. (1) This work, (2) Kalcheva et al. 2018, (3) Anderson et al. (2014), (4) Giveon et al. (2005a), (5) SIMBAD, (6) Irabor et al. (2018), (7) Ortega et al. (2010), (8) Purcell et al. 2013.
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