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Table 3.

Average flux densities for all sources from the TELAMON sample as observed during the first 2.5 yr.

ID S20 mm(a) D-Rate (b) Nobs(c) S14 mm(a) D-Rate (b) Nobs(c) S7 mm(a) D-Rate (b) Nobs(c) α(d)
(J2000) [Jy] [%] [Jy] [%] [Jy] [%]
J0035+5950 0.0725 ± 0.0074 88 18 0.0676 ± 0.0055 85 14 – 0 4 −0.35
J0112+2244 – – 0 1.47 ± 0.36 95 48 1.57 ± 0.42 93 47 0.10
J0136+3906 0.0413 ± 0.0051 83 6 0.0397 ± 0.0022 100 1 – – 0 −
J0152+0146 (e) – 0 3 – – 0 – – 0 −
J0214+5144 0.167 ± 0.012 93 15 0.151 ± 0.015 82 23 0.162 ± 0.014 12 8 −0.42
J0221+3556 – – 0 0.609 ± 0.043 95 21 0.465 ± 0.063 100 21 −0.44
J0222+4302 – – 0 0.94 ± 0.12 100 30 0.82 ± 0.17 86 29 −0.18
J0232+2017 0.0413 ± 0.0051 79 24 0.0377 ± 0.0074 52 25 – 0 4 0.32
J0316+4119 0.1386 ± 0.0070 94 17 0.135 ± 0.013 86 30 – 0 12 −0.15
J0319+1845 0.0202 ± 0.0021 50 2 – 0 1 – – 0 −
J0416+0105 0.0535 ± 0.0081 85 20 0.051 ± 0.010 68 19 – 0 6 −0.16
J0507+6737 0.0278 ± 0.0013 25 4 0.0277 ± 0.0016 22 9 – 0 2 −
J0509+0541 – – 0 1.33 ± 0.43 97 40 1.17 ± 0.41 89 39 −0.12
J0521+2112 – – 0 0.373 ± 0.029 97 33 0.366 ± 0.048 74 31 0.01
J0648+1516 0.0324 ± 0.0064 100 1 0.0312 ± 0.0024 100 1 – – 0 −
J0650+2502 0.0879 ± 0.0082 77 18 0.0860 ± 0.0099 85 21 – 0 4 −0.13
J0710+5909 0.05440 ± 0.00042 20 10 0.0452 ± 0.0022 100 1 – – 0 −
J0721+7120 – – 0 0.83 ± 0.17 100 8 0.79 ± 0.19 87 8 −0.04
J0733+5153 (f) – 0 9 – – 0 – – 0 −
J0739+0136 – – 0 1.55 ± 0.34 100 10 1.70 ± 0.35 70 10 0.03
J0809+5219 0.146 ± 0.011 80 10 0.135 ± 0.014 90 10 – 0 1 −0.02
J0812+0237 0.0403 ± 0.0050 70 17 0.0438 ± 0.0095 50 6 – – 0 −
J0847+1133 (e) – 0 2 – 0 1 – – 0 −
J0854+2006 – – 0 6.03 ± 0.93 100 9 5.6 ± 1.1 88 9 −0.12
J0958+6533 – – 0 1.90 ± 0.30 80 10 2.49 ± 0.61 88 9 0.43
J1015+4926 0.243 ± 0.014 92 14 0.224 ± 0.014 90 22 0.215 ± 0.041 33 6 −0.24
J1058+2817 0.095 ± 0.011 83 18 0.100 ± 0.011 77 18 – 0 1 0.19
J1104+3812 0.465 ± 0.021 100 2 0.424 ± 0.046 95 45 0.419 ± 0.062 67 40 −0.05
J1136+7009 0.1628 ± 0.0057 86 15 0.151 ± 0.020 88 25 – 0 7 −0.23
J1136+6737 0.0350 ± 0.0040 77 9 – 0 1 – – 0 −
J1159+2914 – – 0 4.5 ± 2.1 100 10 4.9 ± 2.2 80 10 −0.07
J1217+3007 0.374 ± 0.024 100 2 0.404 ± 0.050 96 32 0.410 ± 0.059 89 29 −0.05
J1221+3010 0.0555 ± 0.0064 93 16 0.065 ± 0.016 75 12 – 0 2 0.28
J1221+2813 0.521 ± 0.052 50 2 0.490 ± 0.056 94 39 0.458 ± 0.065 75 36 −0.10
J1224+2122 – – 0 0.89 ± 0.15 90 10 0.624 ± 0.078 88 9 −0.49
J1224+2436 0.0324 ± 0.0087 90 10 – – 0 – – 0 −
J1230+2518 0.2639 ± 0.0049 100 1 0.342 ± 0.063 93 30 0.369 ± 0.092 84 26 0.05
J1415+1320 0.657 ± 0.021 100 2 0.564 ± 0.066 87 16 0.54 ± 0.12 80 15 −0.13
J1422+3223 0.675 ± 0.023 100 2 0.73 ± 0.18 94 39 0.81 ± 0.22 91 37 0.21
J1427+2348 0.416 ± 0.042 100 1 0.362 ± 0.051 100 32 0.335 ± 0.073 60 30 −0.11
J1428+4240 0.0304 ± 0.0046 33 6 0.0225 ± 0.0021 7 14 – 0 2 −
J1443+1200 0.0403 ± 0.0035 77 9 0.0417 ± 0.0060 100 1 – – 0 −
J1443+2501 0.260 ± 0.057 86 29 0.221 ± 0.057 97 34 – 0 4 −0.26
J1555+1111 0.368 ± 0.035 92 27 0.339 ± 0.043 97 42 0.313 ± 0.061 50 14 −0.01
J1653+3945 1.187 ± 0.034 100 2 1.057 ± 0.051 100 35 0.885 ± 0.085 84 32 −0.27
J1725+1152 0.116 ± 0.015 90 10 0.125 ± 0.028 90 10 – – 0 0.18
J1728+5013 0.127 ± 0.010 90 21 0.123 ± 0.015 91 34 – 0 11 −0.11
J1743+1935 0.208 ± 0.015 90 20 0.191 ± 0.015 100 33 – 0 11 −0.19
J1751+0938 2.25 ± 0.33 100 6 2.35 ± 0.39 100 13 2.43 ± 0.51 100 13 0.07
J1813+3144 0.106 ± 0.010 83 18 0.1070 ± 0.0099 92 27 – 0 4 −0.21
J1943+2118 0.0377 ± 0.0076 61 18 0.0316 ± 0.0022 11 9 – – 0 −
J1959+6508 0.204 ± 0.019 90 21 0.197 ± 0.017 86 36 0.2122 ± 0.0091 18 11 −0.15
J2001+4352 0.223 ± 0.056 100 14 0.230 ± 0.053 100 14 – – 0 0.05
J2039+5219 0.0285 ± 0.0039 100 1 – 0 1 – – 0 −
J2056+4940 0.117 ± 0.018 77 9 0.111 ± 0.017 66 9 – – 0 −0.13
J2202+4216 – – 0 5.8 ± 2.3 90 11 7.1 ± 2.7 90 11 0.27
J2250+3825 (e) – 0 2 – – 0 – – 0 −
J2243+2021 0.0987 ± 0.0058 70 20 0.0988 ± 0.0087 78 19 – – 0 0.04
J2347+5142 0.1615 ± 0.0097 90 20 0.151 ± 0.014 87 33 – 0 12 −0.29

Notes.

(a)

Average flux density and standard deviation at the given wavelength taken over all observed epochs.

(b)

Detection rate (i.e., number of epochs with detection divided by the number of epochs where the source was observed) at the given wavelength.

(c)

Number of epochs where the source was observed at the given wavelength.

(d)

Median spectral index across all observed epochs with at least three sub-band detections.

(e)

Source was observed but not detected at 20 mm and 14 mm. We have confirmed with independent 45 mm observations that the source is indeed very faint, i.e., a successful detection at wavelengths < 20 mm is unlikely. For these faint sources we have defined a new observing category and are now monitoring them with high detection rates at 45 mm.

(f)

Affected by source confusion with a brighter neighbouring source, therefore no detection was possible.

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