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

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Table 6:

Constraints for the new lens model of MS0451.
Source name	ID	RA ( $+4^{\rm h}$ $54^{\rm m}$ )	Dec ( $- 3^{\circ}$ )	Band
		J2000 (s)	J2000 ( $\hbox{$^\prime$ }$ , $\hbox{$^{\prime\prime}$ }$ )
	1.1 $^\ast$	12.956	0:53.379	F814W
ARC1	1.2 $^\ast$	12.931	0:58.029
	1.3 $^\ast$	11.124	1:26.641
	2.1	12.958	0:54.869	F814W
ARC1	2.2	12.938	0:57.446
	2.3	11.124	1:26.641
	3.1	12.958	0:55.147	F814W
ARC1	3.2	12.945	0:56.710
	3.3	11.124	1:26.641
B1	4.1 $^\ast$	12.806	0:44.344	K' band
B2	4.2 $^\ast$	12.684	1:01.488
B3	4.3 $^\ast$	10.927	1:24.795
C1	5.1	12.822	0:47.834	K' band
C2	5.2	12.747	0:59.481
C3	5.3	10.897	1:25.627
RC1	6.1	12.890	0:53.907	1.4 GHz
RC2	6.2	12.868	0:59.696

Sources used as constraints in the lens model presented by Borys et al. (2004) are indicated with an asterisk in their ID number.

Source LaTeX | All tables | In the text

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