Giant lobes of Centaurus A as seen in radio and γ-ray images obtained with the Fermi-LAT and Planck satellites

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Table 3

Flux density measurements of the regions of Cen A at low frequencies.

Frequency				Flux density [Jy]
[GHz]	N1	N2	N3	core	S1	S2	S3

0.118^a	362.65 ± 48.26	517.63 ± 61.86	620.58 ± 70.84	2877.38 ± 295.91	479.99 ± 60.31	849.74 ± 95.37	764.29 ± 86.30
0.408^a	165.07 ± 18.78	265.98 ± 28.95	291.83 ± 31.21	1103.06 ± 112.19	368.12 ± 39.64	495.86 ± 52.01	382.24 ± 40.48
1.4^b	72.25 ± 1.55	97.56 ± 2.04	107.22 ± 2.22	483.45 ± 9.74	81.13 ± 1.73	163.92 ± 3.37	162.55 ± 3.34
30	9.63 ± 0.01	11.19 ± 0.01	12.41 ± 0.01	82.48 ± 0.01	9.29 ± 0.01	19.26 ± 0.01	24.36 ± 0.01
44	5.43 ± 0.03	8.03 ± 0.03	8.67 ± 0.02	55.09 ± 0.02	–	10.82 ± 0.03	16.63 ± 0.02
70	2.37 ± 0.07	11.70 ± 0.06	7.92 ± 0.05	39.89 ± 0.05	–	15.67 ± 0.06	12.58 ± 0.05
100	–	4.45 ± 0.05	–	23.21 ± 0.03	–	9.11 ± 0.04	–
143	–	–	–	9.16 ± 0.04	–	3.92 ± 0.04	–

Notes. Blanks indicate the signal that was not detected in that region.

^(a)

10% of the flux is considered as systematic error.

^(b)

2% of the flux is considered as systematic error.

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