Table 1.
Catalogue of the COSMOS VLBA+GBT detected sources (1.4 GHz).
ID | COSMOSVLADP | Si,VLA [μJy] | M | RA [deg] | Dec [deg] | rms [μJy/beam] | Sp,V+G [μJy/beam] | ΔSp,V+G [μJy/beam] | Si,V+G [μJy] | ΔSi,V+G [μJy] |
---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
C1886 | J100048.89+023127.5 | 234 | 0 | 150.20371 | 2.524278 | 12.5 | 100 | 16 | 100 | 16 |
C1903 | J100050.45+023356.1 | 610 | 0 | 150.210224 | 2.565571 | 10.3 | 253 | 27 | 277 | 30 |
C1975 | J100057.06+022942.9 | 123 | 0 | 150.237772 | 2.495213 | 10.3 | 103 | 15 | 103 | 15 |
C1977 | J100057.11+023451.7 | 347 | 0 | 150.237968 | 2.581037 | 7.6 | 185 | 20 | 186 | 20 |
C2010 | J100059.05+023508.9 | 237 | 0 | 150.246091 | 2.585823 | 7.2 | 162 | 18 | 162 | 17 |
C2049 | J100101.81+024111.7 | 169 | 0 | 150.257517 | 2.686597 | 10.4 | 75 | 13 | 110 | 15 |
C2053* | J100102.27+023034.5 | 82 | 0 | 150.259458 | 2.509566 | 8.0 | 41 | 9 | 66 | 10 |
C2078* | J100104.26+023307.7 | 79 | 0 | 150.267716 | 2.552051 | 6.6 | 44 | 8 | 46 | 8 |
C2096* | J100105.55+023309.8 | 158 | 1 | 150.273142 | 2.55273 | 6.3 | – | – | 77 | 11 |
C2096a | J100105.55+023309.8 | 158 | 0 | 150.273147 | 2.552731 | 6.7 | 37 | 8 | 39 | 8 |
C2096b | J100105.55+023309.8 | 158 | 0 | 150.273136 | 2.552728 | 6.6 | 30 | 7 | 38 | 8 |
C2136 | J100108.99+022815.9 | 669 | 0 | 150.287493 | 2.471066 | 10.3 | 389 | 40 | 390 | 40 |
C2184 | J100112.06+024106.7 | 2464 | 1 | 150.300291 | 2.685168 | 8.7 | – | – | 611 | 47 |
C2184a | J100112.06+024106.7 | 2464 | 0 | 150.300296 | 2.685171 | 9.5 | 158 | 19 | 221 | 24 |
C2184b | J100112.06+024106.7 | 2464 | 0 | 150.300288 | 2.685166 | 9.4 | 143 | 17 | 390 | 40 |
C2231* | J100116.17+023241.8 | 133 | 0 | 150.317413 | 2.544883 | 5.3 | 26 | 6 | 33 | 6 |
C2259 | J100118.04+023610.3 | 77 | 0 | 150.325164 | 2.602793 | 5.6 | 60 | 8 | 67 | 9 |
C2283 | J100119.92+023856.2 | 326 | 0 | 150.332979 | 2.648923 | 6.6 | 38 | 8 | 43 | 8 |
C2284 | J100120.06+023443.7 | 10 590 | 0 | 150.3336 | 2.578797 | 13.2 | 8860 | 891 | 9215 | 922 |
C2290 | J100120.45+023834.2 | 183 | 0 | 150.335177 | 2.642863 | 6.3 | 41 | 8 | 45 | 8 |
C2302 | J100121.29+023535.8 | 228 | 0 | 150.33873 | 2.593252 | 5.3 | 42 | 7 | 57 | 8 |
C2313 | J100122.02+023724.3 | 224 | 0 | 150.341768 | 2.623411 | 5.8 | 139 | 15 | 140 | 15 |
C2315* | J100122.07+023405.5 | 235 | 0 | 150.341957 | 2.568208 | 5.2 | 36 | 6 | 82 | 10 |
C2361* | J100125.31+023527.5 | 131 | 0 | 150.355530 | 2.590917 | 5.2 | 20 | 6 | 27 | 6 |
C2362 | J100125.36+023851.7 | 134 | 0 | 150.355690 | 2.647704 | 6.1 | 78 | 10 | 80 | 10 |
C2374* | J100126.28+023934.1 | 57 | 0 | 150.359571 | 2.659473 | 7.6 | 39 | 9 | 42 | 9 |
C2383* | J100127.97+024029.3 | 1502 | 0 | 150.366624 | 2.674827 | 8.1 | 42 | 9 | 57 | 10 |
C2407 | J100129.83+023239.0 | 159 | 0 | 150.374252 | 2.544137 | 6.1 | 63 | 9 | 76 | 10 |
C2436 | J100131.14+022924.7 | 5377 | 0 | 150.379782 | 2.490183 | 9.9 | 923 | 93 | 1184 | 119 |
C2443 | J100131.36+022639.2 | 16 120 | 0 | 150.380641 | 2.444316 | 11.4 | 70 | 13 | 83 | 14 |
C2470 | J100133.58+022749.6 | 127 | 0 | 150.389932 | 2.463782 | 10.1 | 59 | 12 | 60 | 12 |
C2512 | J100136.93+023834.3 | 264 | 0 | 150.403918 | 2.642866 | 7.6 | 166 | 18 | 173 | 19 |
C2517 | J100137.85+023710.4 | 80 | 0 | 150.407764 | 2.619514 | 7.2 | 56 | 9 | 56 | 9 |
C2535 | J100139.36+023432.0 | 154 | 0 | 150.41403 | 2.575519 | 7.2 | 68 | 10 | 79 | 11 |
C2541* | J100139.85+023329.3 | 166 | 0 | 150.416043 | 2.558077 | 7.3 | 39 | 8 | 43 | 8 |
C2566* | J100141.42+023523.9 | 84 | 0 | 150.422577 | 2.589912 | 7.2 | 48 | 9 | 50 | 9 |
C2627 | J100145.97+023948.0 | 262 | 0 | 150.441538 | 2.663279 | 11.8 | 110 | 16 | 166 | 20 |
C2631 | J100146.69+023251.6 | 122 | 0 | 150.444606 | 2.547659 | 9.2 | 77 | 12 | 86 | 13 |
C2662 | J100149.61+023334.8 | 2202 | 1 | 150.456723 | 2.559672 | 10.3 | – | – | 1178 | 96 |
C2662a | J100149.61+023334.8 | 2202 | 0 | 150.456724 | 2.559673 | 13.3 | 838 | 85 | 891 | 90 |
C2662b | J100149.61+023334.8 | 2202 | 0 | 150.456718 | 2.55967 | 13.1 | 232 | 27 | 287 | 32 |
Notes.Column 1: Source name used in the present project. An asterisk (*) represents those sources that were detected with the VLBA+GBT but not with the VLBA. A lower-case letter added to the ID refers to each component of a multi-component source; Col. 2: source name from Schinnerer et al. (2010); Col. 3: integrated VLA flux density of the source (1.4 GHz) from Schinnerer et al. (2010); Col. 4: classification between single- and multi-component source, 0: single-component source, 1: multi-component source; Cols. 5, 6: right ascension and declination (J2000) of the source, measured with the VLBA+GBT (uniform weighting); Col. 7: local noise rms measured with the VLBA+GBT (uniform weighting); Cols. 8, 9: peak flux density of the source and its error, measured with the VLBA+GBT (uniform weighting); Cols. 10, 11: integrated flux density of the source and its error, measured with the VLBA+GBT (uniform weighting).
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