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Table 3.

Flux densities and spectral indices for the A1775 radio sources.

Source Frequency Flux density Spectral index
[MHz] 1[mJy]
Head 144 1249 ± 125 α 144 400 = 0.63 ± 0.14 $ \alpha_{144}^{400}=0.63 \pm 0.14 $
400 653 ± 65 α 400 650 = 0.77 ± 0.23 $ \alpha_{400}^{650}=0.77 \pm 0.23 $
650 448 ± 22
Inner Tail 144 1253 ± 125 α 144 400 = 1.06 ± 0.14 $ \alpha_{144}^{400}=1.06 \pm 0.14 $
400 424 ± 42 α 400 650 = 1.44 ± 0.23 $ \alpha_{400}^{650}=1.44 \pm 0.23 $
650 211 ± 10
Outer Tail 144 372 ± 37 α 144 400 = 1.55 ± 0.14 $ \alpha_{144}^{400}=1.55 \pm 0.14 $
400 76 ± 7.6 α 400 650 = 2.23 ± 0.23 $ \alpha_{400}^{650}=2.23 \pm 0.23 $
650 26 ± 1.3
F1 144 466 ± 46 α 144 400 = 2.56 ± 0.14 $ \alpha_{144}^{400}=2.56 \pm 0.14 $
400 34 ± 3.4 α 400 650 > 5.59 $ \alpha_{400}^{650} > 5.59 $
650 < 2.2
F2 144 375 ± 37 α 144 400 = 2.70 ± 0.14 $ \alpha_{144}^{400}=2.70 \pm 0.14 $
400 23 ± 2.3 α 400 650 = 4.98 ± 0.23 $ \alpha_{400}^{650}=4.98 \pm 0.23 $
650 2.1 ± 0.11

Notes. These measurements were performed at the three frequencies 144, 400, and 650 MHz, across the ‘head’, ‘inner’ tail, and ‘outer’ tail of the head-tail radio galaxy, as well as filaments F1 and F2. Spectral index values at high and low frequencies were derived from the integrated spectrum.

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