Table 1
ATLASGAL compact source catalogue for sources located in the 280° <ℓ< 330° and 21° <ℓ< 60° region.
ℓmax | bmax | ℓ | b | σ maj | σmin | PA | θR | Speak | ΔSpeak | Sint | ΔSint | Flag | S/N | |
Catalogue name | (°) | (°) | (°) | (°) | (′′) | (′′) | (°) | (′′) | (Jy beam-1) | (Jy) | ||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
|
||||||||||||||
AGAL300.164−00.087 | 300.164 | −0.087 | 300.164 | −0.089 | 11 | 7 | 10 | ··· | 1.39 | 0.26 | 5.09 | 1.02 | 0 | 8.9 |
AGAL300.218−00.111 | 300.218 | −0.111 | 300.218 | −0.113 | 19 | 12 | 122 | 30 | 1.17 | 0.26 | 5.68 | 1.11 | 0 | 6.2 |
AGAL300.323−00.199 | 300.323 | −0.199 | 300.323 | −0.199 | 8 | 6 | 138 | ··· | 0.71 | 0.38 | 2.28 | 0.57 | 16 | 1.9 |
AGAL300.341−00.214 | 300.341 | −0.214 | 300.340 | −0.213 | 13 | 9 | 140 | 16 | 0.76 | 0.30 | 5.30 | 1.05 | 2 | 2.7 |
AGAL300.381−00.287 | 300.381 | −0.287 | 300.379 | −0.286 | 25 | 13 | 141 | 37 | 0.90 | 0.14 | 7.11 | 1.33 | 0 | 97.4 |
AGAL300.403+00.544 | 300.403 | 0.544 | 300.404 | 0.544 | 13 | 10 | 129 | 19 | 1.02 | 0.61 | 3.38 | 0.75 | 0 | 1.7 |
AGAL300.456−00.189 | 300.456 | −0.189 | 300.455 | −0.191 | 14 | 9 | 15 | 17 | 0.94 | 0.17 | 4.29 | 0.89 | 0 | 9.9 |
AGAL300.491−00.176 | 300.491 | −0.176 | 300.489 | −0.175 | 20 | 12 | 172 | 31 | 0.68 | 0.15 | 6.12 | 1.18 | 3 | 6.5 |
AGAL300.499−00.212 | 300.499 | −0.212 | 300.500 | −0.211 | 17 | 7 | 7 | ··· | 0.58 | 0.12 | 2.52 | 0.61 | 3 | 6.5 |
Notes. The columns are as follows: (1) name derived from Galactic coordinates of the maximum intensity in the source; (2)−(3) Galactic coordinates of maximum intensity in the catalogue source; (4)−(5) Galactic coordinates of emission centroid; (6)−(8) semi-major and semi-minor size and source position angle measured anti-clockwise from Galactic north; (9) effective radius of source; (10)−(13) peak and integrated flux densities and their associated uncertainties; (14) SExtractor detection flag (see Bertin & Arnouts 1996 notes on these flags); (15) signal-to-noise ratio (S/N) – values for sources with peak flux below 6σ detection should not be used blindly. Only a small portion of the data is provided here, the full table is only available in electronic form at the CDS.
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