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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.

(a)

Values obtained from Table A.1 of Sanna et al. (2018).

(b)

Flux densities of component CM4 refer to the main peak.

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