Radio counterpart of the lensed submm emission in the cluster MS0451.6-0305: new evidence for the merger scenario

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Volume 509 (January 2010)

A&A, 509 (2010) A54

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Table 4:

Conunterparts of the radio detections.
Radio	Optical/IR	$d_{\rm obs}$	$r_{\rm src}$	$P_{\rm assoc.}$
source	source	(arcsecs)	(arcsecs)	( $\%$ )
E1	B1 $^\ast$	0.38	0.6	67.8
CR1	ARC 1.1	1.12	0.15	<1
	ARC 2.1	1.40	0.25	<1
	ARC 3.1	1.60	0.20	<1
CR2	G2	1.39	0.70	<1
	C2 $^\ast$	1.82	0.60	<1
	ARC 1.2	1.92	0.15	<1
E2	B2 $^\ast$	0.26	0.60	79.29
	G10	0.74	0.23	<1
E3	4.3 $^\ast$	0.77	0.60	20.7
	5.3 $^\ast$	1.22	0.30	<1
	G23	1.54	0.35	<1
RJ	G8	1.91	0.30	<1
	G11	2.40	0.26	<1
	G14	1.39	0.60	<1

The columns show: possible counterparts of the radio detections (Optical/IR source), mesured offset between the radio source and the optical/IR source ( $d_{\rm obs}$ ), radius of the optical/IR source ( $r_{\rm src}$ ) and probability that the centroid of the radio source lies inside the area of the optical/IR source ( $P_{\rm assoc.}$ ). The coordinates of the counterpart sources can be found in Tables 5 and 6. Sources which positions were taken from the K' band image are indicated with an asterisk (otherwise we used the HST coordinates). The positions of the radio sources used to calculate $d_{\rm obs}$ correspond to the values derived with MAXFIT in the aligned radio map.

Source LaTeX | All tables | In the text

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