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Table 2

Flux densities at WMAP Ka, Q, V, and W band for the 198 extragalactic radio sources selected from the ERCSC.

Namea GLON GLAT Type Band WMAP1 WMAP2 WMAP3 WMAP4 WMAP5 WMAP6 WMAP7 ERCSCb Vrmsc Notesd
[deg] [deg] [Jy] [Jy] [Jy] [Jy] [Jy] [Jy] [Jy] [Jy]
J0006−0623 93.503  −66.636 BLL Ka 1.44 ± 0.33 1.88 ± 0.30 1.86 ± 0.29 1.54 ± 0.29 1.26 ± 0.29 1.05 ± 0.30 0.77 ± 0.30 1.46 ± 0.08 17.24
(0003−066) Q 1.69 ± 0.37 1.32 ± 0.34 2.31 ± 0.34 1.74 ± 0.35 1.50 ± 0.35 0.67 ± 0.41 1.20 ± 0.36 1.43 ± 0.07 10.96
V 1.72 ± 0.58 1.23 ± 0.54 1.19 ± 0.63 1.14 ± 0.56 1.49 ± 0.59 0.90 ± 0.56 1.27 ± 0.63 1.35 ± 0.09
W  −0.04 ± 0.93 0.45 ± 0.84 0.48 ± 0.91 1.17 ± 0.85 3.95 ± 1.09  −0.37 ± 0.72 1.25 ± 0.84 1.22 ± 0.08
J0010+1058 106.981  −50.622 AGN Ka 0.65 ± 0.29 1.31 ± 0.30 1.60 ± 0.32 2.09 ± 0.30 0.90 ± 0.29 0.92 ± 0.30 0.20 ± 0.30 2.51 ± 0.10 29.68 v
(Mrk 1501) Q 0.38 ± 0.37 0.70 ± 0.37 1.54 ± 0.34 2.11 ± 0.37 1.04 ± 0.36 0.53 ± 0.37 1.75 ± 0.36 2.68 ± 0.16
V  −0.13 ± 0.63 0.75 ± 0.56 1.73 ± 0.63 0.75 ± 0.60 0.90 ± 0.61 0.54 ± 0.64 1.93 ± 0.60 2.27 ± 0.17
W 0.69 ± 0.99 1.07 ± 0.97 2.20 ± 1.12 3.54 ± 0.75 2.01 ± 0.93  −1.11 ± 0.91 0.98 ± 1.01 1.89 ± 0.10
J0050−5738 303.285  −59.481 FSRQ Ka 0.97 ± 0.23 0.94 ± 0.22 0.92 ± 0.23 1.61 ± 0.22 1.38 ± 0.23 1.64 ± 0.22 1.55 ± 0.23 1.33 ± 0.09 18.85 v
(0047−579) Q 1.30 ± 0.27 1.21 ± 0.25 1.77 ± 0.26 1.62 ± 0.27 1.27 ± 0.26 1.14 ± 0.27 1.45 ± 0.27 1.36 ± 0.18  −9.43
V 1.46 ± 0.42 1.03 ± 0.45 1.21 ± 0.45 1.40 ± 0.46 0.57 ± 0.43 0.42 ± 0.44 2.08 ± 0.45 1.25 ± 0.15
W 0.24 ± 0.72 1.53 ± 0.73 0.94 ± 0.57 1.71 ± 0.81 1.24 ± 0.69 0.52 ± 0.68 0.04 ± 0.68 0.81 ± 0.08
J0051−0650 122.730  −69.711 FSRQ Ka 1.53 ± 0.30 1.11 ± 0.30 1.44 ± 0.31 1.36 ± 0.30 1.16 ± 0.29 1.24 ± 0.30 2.01 ± 0.30 1.38 ± 0.08 5.43
(0048−071) Q 1.70 ± 0.38 0.77 ± 0.36 1.06 ± 0.37 1.17 ± 0.38  −0.41 ± 0.38 0.76 ± 0.38 1.38 ± 0.35 1.49 ± 0.09
V 2.25 ± 0.60 1.25 ± 0.63 1.58 ± 0.57 0.44 ± 0.58 2.32 ± 0.59 2.62 ± 0.60 3.78 ± 0.68 1.55 ± 0.11 12.76
W 2.09 ± 0.90 0.66 ± 0.94 1.94 ± 0.90 2.70 ± 0.83 1.94 ± 0.85  −0.89 ± 0.92 2.05 ± 1.16 1.39 ± 0.09
J0106−4034 290.673  −76.187 FSRQ Ka 2.37 ± 0.22 1.42 ± 0.22 1.90 ± 0.22 2.64 ± 0.22 3.77 ± 0.22 3.51 ± 0.22 3.40 ± 0.22 1.30 ± 0.07 31.75 V
(0104−408) Q 2.34 ± 0.28 1.67 ± 0.28 2.10 ± 0.29 2.60 ± 0.28 3.55 ± 0.28 3.39 ± 0.28 3.17 ± 0.29 1.33 ± 0.08 24.00 V
V 1.47 ± 0.45 1.78 ± 0.47 2.24 ± 0.49 1.26 ± 0.49 3.39 ± 0.44 3.50 ± 0.46 2.47 ± 0.45 1.23 ± 0.11 30.58 V
W 3.27 ± 0.60 1.57 ± 0.62 1.57 ± 0.75 3.22 ± 0.67 2.74 ± 0.63 2.67 ± 0.73 2.51 ± 0.76 0.97 ± 0.08  −15.32
J0108+0135 131.817  −60.985 FSRQ Ka 2.33 ± 0.30 3.32 ± 0.31 2.43 ± 0.30 1.12 ± 0.31 1.45 ± 0.32 1.05 ± 0.30 1.56 ± 0.31 3.13 ± 0.10 40.77 V
(0106+013) Q 2.05 ± 0.36 3.06 ± 0.37 1.39 ± 0.36 1.87 ± 0.36 0.21 ± 0.34 0.47 ± 0.37 0.09 ± 0.39 2.85 ± 0.08 37.99 V
V 2.13 ± 0.56 2.36 ± 0.62 2.31 ± 0.61 1.64 ± 0.63 0.46 ± 0.63 0.67 ± 0.62 1.68 ± 0.57 2.38 ± 0.06
W  −1.17 ± 1.15 1.89 ± 1.06  −1.34 ± 1.17  −1.63 ± 1.20  −0.34 ± 0.73 1.49 ± 0.91 0.07 ± 1.20 1.97 ± 0.05
J0121+1149 134.577  −50.354 FSRQ Ka 0.94 ± 0.32 0.82 ± 0.31 0.66 ± 0.32 0.99 ± 0.31 0.39 ± 0.33 1.77 ± 0.31 1.81 ± 0.31 1.75 ± 0.08
(0119+115) Q 0.38 ± 0.39 0.92 ± 0.36 1.03 ± 0.36 0.83 ± 0.37 0.81 ± 0.35 1.57 ± 0.35 2.65 ± 0.37 1.56 ± 0.07
V 0.74 ± 0.63  −0.16 ± 0.60 0.95 ± 0.66 0.63 ± 0.63 1.14 ± 0.59 1.03 ± 0.59 0.30 ± 0.58 1.26 ± 0.05
W 0.65 ± 0.81  −0.79 ± 0.94 0.15 ± 0.89  −1.63 ± 0.89 0.27 ± 0.77  −0.40 ± 0.93 0.84 ± 1.07 1.00 ± 0.05
J0132−1655 168.145  −76.020 FSRQ Ka 2.10 ± 0.28 2.56 ± 0.30 2.38 ± 0.30 2.47 ± 0.30 2.18 ± 0.29 1.82 ± 0.29 1.87 ± 0.29 1.71 ± 0.08  −3.11
(0130−171) Q 1.66 ± 0.33 2.09 ± 0.33 2.20 ± 0.36 1.76 ± 0.36 2.16 ± 0.35 1.54 ± 0.34 1.29 ± 0.34 1.53 ± 0.06 0.73
V 0.95 ± 0.51 2.71 ± 0.55 2.28 ± 0.54 2.77 ± 0.56 1.60 ± 0.58 2.21 ± 0.58 1.24 ± 0.52 1.24 ± 0.04  −7.05
W 1.56 ± 0.84 4.50 ± 0.77 0.38 ± 0.78 1.54 ± 0.98 0.73 ± 1.01 1.49 ± 0.75 2.62 ± 0.89 0.99 ± 0.04
J0136+4751 130.788  −14.316 FSRQ Ka 4.33 ± 0.28 4.86 ± 0.28 4.61 ± 0.28 4.13 ± 0.29 3.50 ± 0.28 3.66 ± 0.29 4.32 ± 0.29 4.68 ± 0.12 9.59 V
(0133+476) Q 5.02 ± 0.37 5.42 ± 0.38 4.86 ± 0.36 4.24 ± 0.39 2.42 ± 0.35 4.10 ± 0.36 4.01 ± 0.36 4.42 ± 0.11 21.99 V
V 4.15 ± 0.58 6.32 ± 0.56 3.89 ± 0.57 3.39 ± 0.60 2.98 ± 0.56 3.44 ± 0.61 3.33 ± 0.63 3.92 ± 0.12 25.29 V
W 3.15 ± 0.90 2.49 ± 0.69 1.73 ± 0.85 1.80 ± 0.93 0.07 ± 0.95 0.66 ± 1.09 3.56 ± 0.90 3.40 ± 0.11
J0137−2431 201.403  −79.286 FSRQ Ka 0.53 ± 0.28 1.44 ± 0.26 1.43 ± 0.28 1.07 ± 0.24 1.23 ± 0.27 1.05 ± 0.27 0.57 ± 0.27 2.45 ± 0.09  −8.72
(0135−247) Q 0.82 ± 0.33 1.72 ± 0.32 1.37 ± 0.31 1.64 ± 0.31 1.27 ± 0.33 1.20 ± 0.33 1.41 ± 0.33 2.49 ± 0.15  −14.46
V 0.80 ± 0.53 1.12 ± 0.50 3.21 ± 0.56 1.72 ± 0.52 1.52 ± 0.50 0.98 ± 0.52 1.69 ± 0.54 2.73 ± 0.14 14.00
W  −1.96 ± 0.81 2.39 ± 0.82 2.73 ± 1.01 1.47 ± 0.81 1.30 ± 0.81  −1.11 ± 0.75  −0.23 ± 0.83 2.25 ± 0.09

Notes. Example, full table is available at the CDS.

(a)

The J2000 name for each source is given. For easy reference, we have also included in parentheses the commonly known name or its B1950 name.

(b)

These are the ERCSC flux densities extrapolated to the center frequencies of WMAP Ka, Q, V, and W-band.

(c)

This field is left blank when a timeline is not included in the variability analysis. Negative values indicate that the flux density fluctuation level is less than the noise level (see Sect. 4.1).

(d)

“V” denotes strongly variable sources (>99% confidence), and “v” denotes moderately variable sources (>95% confidence) at a given frequency.

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