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Table 6.

Flux measurements for the sample of the tailed galaxies.

Radio Cluster Telescope ν Stot Sc Sdiff Ref.
galaxy name (MHz) (mJy) (mJy) (mJy)
J 1254-2901a A 3528 N GMRT 235 349.4 ± 28.0 239.9 ± 19.2 109.5 ± 34.0 This work
GMRT 610 186.6 ± 9.3 140.0 ± 7.0 46.6 ± 11.6 This work
ATCA 1380 110.5 ± 3.3 (Venturi et al. 2001)
ATCA 2380 57.9 ± 1.7 (Venturi et al. 2001)
VLA 8400 22.1 ± 0.7 This work
J 1254-2901b A 3528 N GMRT 235 22.7 ± 1.8 This work
GMRT 610 13.1 ± 0.7 This work
J 1254-2904 A 3528 N GMRT 150 1463.7 ± 292.7 607.4 ± 121.5 856.3 ± 316.9 TGSS image
GMRT 235 926.6 ± 74.1 416.1 ± 33.3 510.6 ± 81.2 This work
GMRT 610 342.8 ± 17.1 221.4 ± 11.1 121.4 ± 20.4 This work
MOST 843 519.0 ± 15.6 SUMSS image
ATCA 1380 295.9 ± 8.9 (Venturi et al. 2001)
VLA 1400 311.7 ± 9.4 NVSS image
ATCA 2380 142.8 ± 4.3 126.2±3.8 16.6±5.7 (Venturi et al. 2001)
VLA 8400 30.0±1.0 This work
J 1254-2916 A 3528 S GMRT 235 259.3 ± 20.7 132.8 ± 10.6 126.5 ± 23.3 This work
GMRT 610 149.1 ± 7.5 76.5 ± 3.8 72.6 ± 8.4 This work
MOST 843 124.0 ± 3.7 SUMSS image
ATCA 1380 62.1 ± 1.9 (Venturi et al. 2001)
VLA 1400 85.8 ± 2.6 23.7 ± 3.2a NVSS image
ATCA 2380 49.6 ± 1.5 (Venturi et al. 2001)
VLA 8400 15.3 ± 0.5 This work
J 1324-3138 A 3556 GMRT 235 278.3 ± 22.3 9.1 ± 0.7 269.2 ± 22.3 This work
VLA 327 230 ± 11.5 (Venturi et al. 1998)
GMRT 325 254 ± 12.7 8.1 ± 0.4 245.9 ± 12.7 This work
GMRT 610 122.7 ± 6.1 6.2 ± 0.2 119.5 ± 6.1 This work
MOST 843 80.2 ± 2.4 (Venturi et al. 1998)
ATCA 1380 41 ± 1.2 2.1 ± 0.1 38.9 ± 1.2 (Venturi et al. 1997)
ATCA 1400 43.1 ± 1.3 2.7 ± 0.1 40.4 ± 1.3 ATCA archive image
ATCA 2380 21.0 ± 0.6 1.7 ± 0.1 19.3 ± 0.6 (Venturi et al. 1997)
ATCA 4790 7.3 ± 0.3 0.5 ± 0.03 6.8 ± 0.3 (Venturi et al. 1998)
ATCA 5000 6.8 ± 0.2 0.4 ± 0.01 6.5 ± 0.2 ATCA archive image
ATCA 8640 2.2 ± 0.1 0.1 ± 0.01 2.1 ± 0.1 (Venturi et al. 1998)

Notes. The information on the observations (e.g. beam and literature references) are provided in Tables 2 and 3. The diffuse emission is the difference between the total flux density and the emission from the central components.

(a)

The diffuse emission was calculated by difference between the VLA (total region) and the ATCA (central region) observation.

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