Cosmic dance in the Shapley Concentration Core - I. A study of the radio emission of the BCGs and tailed radio galaxies

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Table 3.

Observational parameters of the literature images.

Array	ν	Resolution	PA	rms
	(MHz)	(′′×′′)	(°)	(mJy beam⁻¹)
TGSS-GMRT^a	150	24.0 × 15.0	30	9
ATCA^b	1380	10.0 × 6.0	0	0.14
ATCA^c	1400	11.8 × 6.2	−0.31	0.56
NVSS-VLA-D^d	1400	45.0 × 45.0	61	0.13
ATCA^b	2380	6.0 × 3.5	2	0.15
ATCA^c	2400	6.2 × 4.2	0.15	0.39
VLA^g	327	59.0 × 45.0	80.5	1.9
SUMSS-MOST^e	843	82.0 × 43.0	0	1.4
ATCA^e	1380	6.0 × 10.0	0	0.2
ATCA^g	1376	10.2 × 6.0	0.26	0.16
ATCA^e	2380	5.3 × 3.4	0	0.15
ATCA^g	4790	20.2 × 10.0	0	0.04
VLA^g	8640	20.0 × 10.0	0	0.04

Notes. The information refers to the A 3528 and A 3558 cluster complexes, on the top and on the bottom, respectively.

References.

^(a)

TGSS image (Intema et al. 2017);

^(b)

Venturi et al. (2001);

^(c)

Reid et al. (1998);

^(d)

NVSS image (http://www.cv.nrao.edu/nvss/);

^(e)

SUMSS catalogue (http://www.physics.usyd.edu.au/sifa/Main/SUMSS);

^(f)

Venturi et al. (1997);

^(g)

Venturi et al. (1998).

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