Table 4.
Properties of the radio sources for Abell S1063 and Abell 370, labeled in Figs. 1 and 8.
| Name | RA | Dec | S325 MHz | S1.5 GHz | S3 GHz |
 |
 |
|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (mJy) | (mJy) | (mJy) | |||
| AS1063 Halo(a) | 22 48 43.5 | −44 31 44.0 | 24.3 ± 2.5 | 5.8 ± 0.4 | 1.7 ± 0.2 | −0.94 ± 0.08 | −1.77 ± 0.20 |
| AS1063 Source A | 22 48 44.0 | −44 31 51.85 | 8.5 ± 1.1 | 2.1 ± 0.2 | 1.0 ± 0.1 | −0.93 ± 0.10 | −1.03 ± 0.15 |
| AS1063 Source B | 22 48 41.8 | −44 31 56.48 | 2.2 ± 0.3 | 0.7 ± 0.1 | 0.3 ± 0.1 | −0.80 ± 0.12 | −1.07 ± 0.23 |
| AS1063 Source C | 22 48 44.6 | −44 30 09.59 | 40.7 ± 4.2 | 10.0 ± 0.5 | 4.5 ± 0.2 | −0.92 ± 0.08 | −1.16 ± 0.10 |
| AS1063 Source D | 22 48 49.3 | −44 30 44.58 | 37.8 ± 3.8 | 5.6 ± 0.3 | 1.8 ± 0.1 | −1.24 ± 0.07 | −1.61 ± 0.11 |
| A370 Halo(a) | 02 39 52.0 | −01 35 12.0 | 20.0 ± 2.3 | 3.7 ± 0.3 | <1.3 | −1.10 ± 0.09 | < − 1.51 |
| A370 Source A | 02 39 52.7 | −01 34 19.8 | 0.9 ± 0.1 | 0.2 ± 0.1 | – | −1.06 ± 0.18 | – |
| A370 Source B | 02 39 53.1 | −01 34 56.0 | – | 0.11 ± 0.01 (b) | – | – | – |
| A370 Source C | 02 39 50.9 | −01 35 42.4 | 3.1 ± 0.3 | 1.5 ± 0.1 | 0.8 ± 0.1 | −0.48 ± 0.09 | −0.91 ± 0.16 |
| A370 Source D | 02 39 52.1 | −01 35 56.8 | 1.2 ± 0.6 | 0.3 ± 0.1 | 0.2 ± 0.1 | −0.86 ± 0.34 | −0.91 ± 0.75 |
| A370 Source E | 02 39 55.4 | −01 34 07.9 | 15.5 ± 2.0 | 7.1 ± 0.7 | 4.4 ± 0.4 | −0.51 ± 0.10 | −0.70 ± 0.19 |
| A370 Source F | 02 39 56.5 | −01 34 29.0 | 4.5 ± 1.0 | 2.0 ± 0.4 | 1.3 ± 0.1 | −0.53 ± 0.19 | −0.64 ± 0.28 |
Notes.
Alternative flux densities by manually subtraction the contribution of compact sources. For AS1063: S325 MHz = 25.3 ± 2.7 mJy, S1.5 GHz = 5.1 ± 0.5 mJy, S3 GHz = 1.4 ± 0.2 mJy; for A370: S325 MHz = 23.9 ± 2.9 mJy, S1.5 GHz = 2.7 ± 0.8 mJy, S3 GHz < 1.7 mJy.
The southern BCG is blended with other sources. Here we adopt the 1.4 GHz flux density from Wold et al. (2012).
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