Searching for strong galaxy-scale lenses in galaxy clusters with deep networks - I. Methodology and network performance

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Table 3.

Description of the cluster sample used in the non-GGSL selection.

Cluster		z_cluster	N
Abell 383	A383	0.188	70
Abell 209	A209	0.209	75
RX J2129+0005	R2129	0.234	51
Abell 2744	A2744	0.308	126
MS 2137–2353	MS2137	0.316	52
RX J2248–4431 ^(a)	R2248	0.346	178
MACS J1931–2635	M1931	0.352	28
MACS 1115+0129	M1115	0.352	96
Abell 370	A370	0.375	172
MACS J0416–2403	M0416	0.397	120
MACS J1206–0847	M1206	0.439	147
MACS J0329–0211	M0329	0.450	66
RX J1347–1145	R1347	0.451	44
MACS J1311–0310	M1311	0.494	53
MACS J1149+2223	M1149	0.542	130
MACS J2129–0741	M2129	0.587	45

Notes. The cluster name, short name, and redshift are listed in the first three columns. The fourth column shows the number of non-GGSLs identified through visual inspection.

^(a)

The cluster RX J2248−4431 is also known as Abell S1063.

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