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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Volume 620 (December 2018)

A&A, 620 (2018) A25

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Table 1.

Logs of the observations.

Cluster	RA, Dec (J2000)	Array	Project	Observing date	ν	Δν	Total time
					(MHz)	(MHz)	on source (h)
A 3528 N	12 54 20, –29 02 30	GMRT	05TVa01	5/6-Apr.-2004	235	8	4^a
	12 54 20, –29 02 30	GMRT	05TVa01	5/6-Apr.-2004	610	16	4^a
	12 54 22, –29 01 02	VLA-CnB	AV246	13-Mar.-2000	8460	100	0.25^b
	12 54 21, –29 04 16	VLA-CnB	AV246	13-Mar.-2000	8460	100	0.25^b
A 3528 S	12 55 00, –29 40 00	GMRT	05TVa01	5/6-Apr.-2004	235	8	4^a
	12 55 00, –29 40 00	GMRT	05TVa01	5/6-Apr.-2004	610	16	4^a
	12 54 51, –29 16 20	VLA-CnB	AV246	3-Mar.-2000	8460	100	0.25^b
A 3532	12 56 30, –30 30 00	GMRT	05TVa01	5/6-Apr.-2004	235	8	4^a
	12 56 30, –30 30 00	GMRT	05TVa01	5/6-Apr.-2004	610	16	4^a
A 3556	13 24 00, –31 38 00	GMRT	05TVa01	5/6-Apr.-2004	235	8	4^a
	13 24 00, –31 38 00	GMRT	05TVa01	5/6-Apr.-2004	610	16	4^a
A 3558	13 27 54, –31 29 32	GMRT	22_039	30-Aug.-2012	325	32	8^c
	13 27 54, –31 29 32	GMRT	22_039	02-May-2015	610	32	7^c

Notes.

^(a)

Observations of project 05TVa01 were carried out on two consecutive days with the dual 235/610 MHz receiver, for a total of 8 h each day. We cycled among the four pointing centres every 20 min.

^(b)

The total duration of project AV246 was one hour, and the observations were carried out switching among the three pointing centres every 10 min.

^(c)

Full track observations.

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