A search for diffuse radio emission in the relaxed, cool-core galaxy clusters A1068, A1413, A1650, A1835, A2029, and Ophiuchus

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Table 2:

Details of the VLA observations.
Cluster	RA	Dec	Frequency	Bandwidth	Config.	Obs. Time	Date	Note
	J2000	J2000	MHz	MHz		h
A1068	10 40 47.0	+39 57 18.0	1465/1415	25	C	3.4, 1.0, 5.7	2006 Oct. 21, 23, 28
A1413	11 55 19.0	+23 24 30.0	1465/1415	25	C	8.0	2006 Oct. 23
A1650	12 58 41.0	-01 45 25.0	1465/1415	25	C	7.0	2006 Oct. 22
A1835	14 01 02.0	+02 51 30.0	1465/1385	50	D	4.2	2003 March 10
A1835	$\hbox{$^{\prime\prime}$ }$	$\hbox{$^{\prime\prime}$ }$	1465/1415	25	C	0.7, 4.7	2006 Oct. 23,28
A1835	14 01 02.1	+02 52 42.7	1465/1665	25	A	2	1998 Apr. 23	archive (AT211)
A2029	15 10 58.0	+05 45 42.0	1465/1385	50	D	4.7	2003 March 09
A2029	$\hbox{$^{\prime\prime}$ }$	$\hbox{$^{\prime\prime}$ }$	1465/1415	50	C	6.3	2006 Dec. 26
A2029	15 10 56.1	05 44 42.6	1465/1515	25	A	0.1	1993 Jan. 14	archive (AL252)
Ophiuchus	17 12 31.9	-23 20 32.6	1452/1502	25	D	0.5	1990 Jan. 25	archive (AC261)

Column 1: Cluster Name; Cols. 2, 3: observation pointing (RAJ2000, DecJ2000); Col. 4: observing frequency; Col. 5: bandwidth; Col. 6: VLA configuration; Col. 7: total integration time on source; Col. 8: observing dates; Col. 9: notes on archival observations.

Source LaTeX | All tables | In the text

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