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Table 3:

Parameters of the continuum sources detected in the IRAS 00213+6530 region.
  Position$^{\rm a}$ Flux Density Flux Density Spectral
  $\alpha$ (J2000) $\delta$ (J2000) at 6 cm at 3.6 cm Index
Source (h m s) ( $\hbox{$^\circ$ }$ ' '') (mJy) (mJy) 6 cm-3.6 cm

1
00 23 21.01 +65 43 46.5 0.87 $\pm$ 0.07 ...b ...
2 00 23 45.65 +65 48 36.1 0.17 $\pm$ 0.03 <0.18c <0.10
3 00 23 46.41 +65 49 12.7 1.66 $\pm$ 0.04 0.38 $\pm$ 0.07d -2.7 $\pm$ 0.3
4 00 23 49.01 +65 46 14.7 0.69 $\pm$ 0.03 0.42 $\pm$ 0.02 -0.9 $\pm$ 0.1
5 00 23 52.06 +65 39 58.9 4.20 $\pm$ 0.60 ...b ...
6 00 23 53.70 +65 49 41.6 0.86 $\pm$ 0.03 <0.25c, d <-2.1
7 00 24 09.11 +65 46 58.0 0.57 $\pm$ 0.03 0.24 $\pm$ 0.02 -1.6 $\pm$ 0.2
8 00 24 11.39 +65 47 09.6 0.16 $\pm$ 0.03 0.21 $\pm$ 0.02 0.5 $\pm$ 0.4
9 00 24 24.46 +65 49 05.9 0.13 $\pm$ 0.03 0.27 $\pm$ 0.02 1.3 $\pm$ 0.4
10 00 24 36.71 +65 48 27.5 0.55 $\pm$ 0.03 0.22 $\pm$ 0.03 -1.7 $\pm$ 0.3
11 00 24 56.70 +65 49 10.3 0.63 $\pm$ 0.05 ...b ...
12 00 25 24.75 +65 45 48.3 4.90 $\pm$ 1.10 ...b ...

a
 Positions taken from the 3.6 cm map, except for non-detected sources at this band, for which positions correspond to the 6 cm map. b Source well outside the primary beam at this wavelength. Primary beam correction greater than 12, and the uncertainty in the corrected flux is very large. c The upper limit for non-detected sources is 4$\sigma$. d Flux density measured in 2000 September 23. Source highly variable, so to compute the spectral index we used observations carried out at the same epoch.


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