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Table B.4

Physical properties of the radio sources not classified as H II regions.

ID npix l [°] b [°] Name σnoisepMathematical equation: $\[\sigma_{\text {noise}}^{p}\]$ [mJy/b] SNR SOBSpMathematical equation: $\[\mathrm{S}_{\text {OBS}}^{\mathrm{p}}\]$ [mJy/b] F5.8GHz [mJy] Y-factor
2 746 358.917 +0.072 G358.917+0.072 0.467 149.0 69.10 87.10 1.26
7 215 358.696 +0.263 G358.696+0.263 0.194 109.0 21.10 19.60 0.93
11 126 358.592 +0.046 G358.592+0.046 0.448 53.9 23.90 18.10 0.76
12 272 358.849 +0.161 G358.849+0.161 0.293 39.8 11.70 17.10 1.46
13 281 358.710 +0.136 G358.710+0.136 0.428 36.4 15.50 19.20 1.24
27 165 358.614 −0.034 G358.614–0.034 0.553 12.2 6.69 8.97 1.34
28 75 358.823 −0.118 G358.823–0.118 0.290 11.8 3.36 2.42 0.72
32 96 358.533 −0.100 G358.553–0.100 0.416 10.3 4.27 3.89 0.91
36 403 358.622 +0.093 G358.622+0.093 0.433 7.6 3.56 13.70 3.85
38 1382 358.557 +0.243 G358.557+0.243 0.345 5.1 2.37 35.20 14.85
39 89 358.510 +0.178 G358.510+0.178 0.450 6.1 2.85 2.97 1.04
42 43 358.631 −0.122 G358.631–0.122 0.613 5.5 3.36 1.82 0.54
44 44 358.633 +0.240 G358.633+0.240 0.342 5.4 1.82 1.05 0.58
46 54 358.688 +0.182 G358.688+0.182 0.360 5.1 1.81 1.27 0.70

References. The columns represent the source ID, number of pixels (npix), Galactic coordinates (l, b), the source name, rms noise at position of peak pixel (σnoisepMathematical equation: $\[\sigma_{\text {noise}}^{p}\]$), observed SNR, peak surface brightness (SOBSpMathematical equation: $\[\mathrm{S}_{\text {OBS}}^{\mathrm{p}}\]$), flux density derived using the VLA-D 5.8 GHz radio continuum data and the Y-factor.

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