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Table 6.

Integrated radio fluxes and luminosities.

Source Resolution Frequency Flux Density Luminosity
Θ [″] ν [GHz] Sν [mJy] log(Lν [W Hz−1])
R1 12 3.0 0.78 ± 0.04 24.44 ± 0.02
12 1.5 1.7 ± 0.1 24.78 ± 0.03
12 0.650 4.3 ± 0.3 25.18 ± 0.03
12 0.400 5.8 ± 0.5 25.31 ± 0.04
12 0.144 30.8 ± 4.7 26.04 ± 0.07
R2 12 3.0 4.2 ± 0.2 25.2 ± 0.02
12 1.5 14.2 ± 0.6 25.73 ± 0.02
12 0.650 30.3 ± 2.0 26.06 ± 0.03
12 0.400 60.7 ± 3.9 26.36 ± 0.02
12 0.144 218.0 ± 41.2 26.91 ± 0.09
RELIC ( † ) 12 3.0 5.0 ± 0.2 25.27 ± 0.02
12 1.5 15.9 ± 0.6 25.77 ± 0.02
12 0.650 34.6 ± 2.0 26.11 ± 0.02
12 0.400 66.5 ± 3.9 26.39 ± 0.03
12 0.144 248.8 ± 40.9 26.97 ± 0.07
HALO 19 3.0 3.1 ± 0.1 25.0 ± 0.02
19 1.5 6.1 ± 0.2 25.31 ± 0.02
19 0.650 17.9 ± 1.0 25.77 ± 0.02
19 0.400 28.3 ± 1.7 25.97 ± 0.03
19 0.144 73.8 ± 11.1 26.39 ± 0.06

Notes. ( † )With “relic” we refer to the sum of R1 and R2. The LOFAR and uGMRT images (i.e. ν = 0.144, 0.400, and 0.650 GHz) were obtained with a robust=-0.5. The map noises at 12″ are 6.2, 17.3, 41.6, 98.7, and 137.0 μJy beam−1 for the 3.0 GHz, 1.5 GHz, 650 MHz, 400 MHz, and 144 MHz observations, respectively. The map noises at 19″ are 9.6, 26.6, 70.3, 156.2, and 178.5 μJy beam−1 for the 3.0 GHz, 1.5 GHz, 650 MHz, 400 MHz, and 144 MHz observations, respectively.

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