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Table 7

Example of the data file, available at the CDS, containing Metsähovi, RATAN-600, and Planck observations.

Source name Frequency Time Flux density Error
(GHz) (decimal year) (Jy) (Jy)
1H0323+342 4.8 2013.810959 0.49 0.03
1H0323+342 4.8 2014.197260 0.52 0.03
1H0323+342 4.8 2014.780822 0.46 0.02
1H0323+342 4.8 2015.010959 0.35 0.02
1H0323+342 8.2 2013.810959 0.47 0.03
1H0323+342 8.2 2014.197260 0.49 0.05
1H0323+342 8.2 2014.780822 0.42 0.03
1H0323+342 8.2 2015.010959 0.33 0.03
1H0323+342 11.2 2013.810959 0.44 0.05
1H0323+342 11.2 2014.197260 0.45 0.05
1H0323+342 11.2 2014.780822 0.41 0.04
1H0323+342 11.2 2015.010959 0.30 0.03
1H0323+342 21.7 2013.810959 0.31 0.05
1H0323+342 21.7 2014.197260 0.38 0.06
1H0323+342 21.7 2014.780822 0.39 0.06
1H0323+342 21.7 2015.010959 0.28 0.04
1H0323+342 37 2012.103123 nd
1H0323+342 37 2012.103250 nd
1H0323+342 37 2012.108219 nd
1H0323+342 37 2013.228524 0.64 0.08
1H0323+342 37 2013.234888 0.46 0.07
1H0323+342 37 2013.515495 0.46 0.07
1H0323+342 37 2013.526617 0.60 0.06
1H0323+342 37 2013.647215 0.40 0.06
1H0323+342 37 2013.781315 0.67 0.13
1H0323+342 37 2013.783215 nd
1H0323+342 37 2013.837960 nd
1H0323+342 37 2013.849637 1.05 0.15
1H0323+342 37 2013.871182 0.56 0.08
1H0323+342 37 2014.078259 0.80 0.07
1H0323+342 37 2014.207397 0.59 0.07
1H0323+342 37 2014.592094 nd
1H0323+342 37 2014.695785 0.39 0.07
1H0323+342 37 2014.739778 0.50 0.07
1H0323+342 37 2014.887168 nd
1H0323+342 37 2015.125504 0.53 0.06
1H0323+342 37 2015.160275 nd
1H0323+342 37 2015.199265 0.45 0.06
1H0323+342 70 2010.654795 1.19 0.26
1H0323+342 70 2011.128767 1.12 0.28
1H0323+342 143 2009.893200* 0.75 0.15
1H0323+342 143 2010.893200* 0.82 0.18
1H0323+342 217 2009.660274 0.46 0.10
1H0323+342 217 2010.660274 0.70 0.13

Notes. Non-detections are shown only for Metsähovi data. Column 1: source name; Col. 2: frequency; Col. 3: date. For RATAN-600 this is the average date of the observations stacked together. This also applies to those Planck observations marked with an asterisk. Column 4: flux density. RATAN-600 flux densities are averages of multiple observations. This also applies to those Planck observations marked with an asterisk in Col. 3. Column 5: error in the flux density.

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