The 400d Galaxy Cluster Survey weak lensing programme - I. MMT/Megacam analysis of CL0030+2618 at z = 0.50

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Table 2:

Notable galaxies in the field of CL0030+2618.
Galaxy	$\alpha_{{\rm J2000}}$	$\delta_{{\rm J2000}}$	$r'^{{\rm MMT}}_{{\rm AUTO}}$	$g'^{{\rm MMT}}_{{\rm AUTO}}$	$i'^{{\rm MMT}}_{{\rm AUTO}}$	z	Note	See figure
G1	$00^{{\rm h}}30^{{\rm m}}34\hbox{$.\!\!^{\rm s}$ }0$	$26\degr18\hbox{$^\prime$ }09\hbox{$^{\prime\prime}$ }$	19.20	21.14	18.31	0.516 $^{\dagger}$	dominant in CL0030+2618	Fig. 1
G2	$00^{{\rm h}}30^{{\rm m}}37\hbox{$.\!\!^{\rm s}$ }9$	$26\degr18\hbox{$^\prime$ }18\hbox{$^{\prime\prime}$ }$	18.82	20.23	18.27	n.a.	dominant in foreground group	Fig. 1
G3	$00^{{\rm h}}30^{{\rm m}}36\hbox{$.\!\!^{\rm s}$ }3$	$26\degr19\hbox{$^\prime$ }20\hbox{$^{\prime\prime}$ }$	19.46	20.76	18.95	n.a.	strong lensing feature	Fig. 1
G4	$00^{{\rm h}}30^{{\rm m}}39\hbox{$.\!\!^{\rm s}$ }5$	$26\degr20\hbox{$^\prime$ }56\hbox{$^{\prime\prime}$ }$	17.23	17.98	16.94	0.493 $^{\dagger}$	QSO	Fig. 9

Notes. $^{(\dagger)}$ Redshift taken from Boyle et al. (1997).

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