Table B.2.
Continumm fluxes of centimeter sources in G035.02+0.35.
Component | Band | RA (J2000) | Dec (J2000) | ![]() |
---|---|---|---|---|
(h m s) | (° ′ ″) | (mJy) | ||
CM1 | C | 18:54:00.492 | 02:01:18.34 | 12.092/12.747 |
Ku | 18:54:00.492 | 02:01:18.34 | 12.432 | |
K | 18:54:00.492 | 02:01:18.34 | 11.837 | |
CM2a | C | 18:54:00.648 | 02:01:19.36 | 0.825 |
Ku | 18:54:00.649 | 02:01:19.42 | 1.584 | |
K | 18:54:00.648 | 02:01:19.42 | 2.036 | |
CM3 | C | 18:54:00.764 | 02:01:22.96 | 0.474/0.337 |
Ku | 18:54:00.764 | 02:01:22.90 | 0.276 | |
K | 18:54:00.764 | 02:01:22.96 | 0.264 | |
CM4b | C | 18:54:00.528 | 02:01:15.46 | 0.061/0.054 |
Ku | 18:54:00.532 | 02:01:15.52 | 0.035 | |
K | 18:54:00.536 | 02:01:15.40 | 0.032 | |
CM5 | C | 18:54:00.508 | 02:01:21.10 | 0.061/0.049 |
Ku | 18:54:00.508 | 02:01:21.10 | 0.042 | |
K | 18:54:00.508 | 02:01:21.04 | 0.046 | |
CM6 | C | 18:54:00.592 | 02:01:17.74 | 0.262/0.290 |
Ku | 18:54:00.592 | 02:01:17.74 | 0.257 | |
K | 18:54:00.596 | 02:01:17.68 | 0.199 | |
CM7 | C | 18:54:00.252 | 02:01:10.96 | 0.031/0.024 |
Ku | 18:54:00.252 | 02:01:10.90 | 0.017 | |
K | 18:54:00.252 | 02:01:10.90 | 0.026 | |
CM8 | C | 18:54:01.657 | 02:01:54.04 | 0.055/0.068 |
Ku | 18:54:01.657 | 02:01:53.98 | 0.049 | |
K | … | … | <0.045 |
Notes. Column 1: centimeter continuum components detected at multiple bands, as indicated in Col. 2. Columns 3 and 4: peak pixel positions of the continuum sources at each band. Based on the absolute position differences at different frequencies, we estimate an absolute position uncertainty of approximately . Column 5: radio continuum flux densities measured at each frequency within a common uv-distance range, as described in Sanna et al. (2018, their Sect. 3). The two fluxes at C band refer to the central frequencies of 5.0 (left) and 7.0 GHz (right). The rms and beam size are ∼10 μJy beam−1 and
at each band, respectively. Estimates of the positional uncertainties for the centimeter sources are discussed in Appendix A.
Values obtained from Table A.1 of Sanna et al. (2018).
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