Multiply imaged time-varying sources behind galaxy clusters - Comparing fast radio bursts to QSOs, SNe, and GRBs

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Table 1.

Grale models used for the lens reconstructions as shown in Figs. 5, 6, and 7 (from top left to bottom right).

Model	Mass sheet	τ₁₂	τ₁₃	τ₂₃
1	–	–	–	–
2	✓	–	–	–
3	–	✓	✓	✓
4	✓	✓	✓	✓
5	–	✓	–	–
6	✓	✓	–	–
7	–	–	–	✓
8	✓	–	–	✓

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Model	Mass sheet	τ₁₂	τ₁₃	τ₂₃
1	–	–	–	–
2	✓	–	–	–
3	–	✓	✓	✓
4	✓	✓	✓	✓
5	–	✓	–	–
6	✓	✓	–	–
7	–	–	–	✓
8	✓	–	–	✓

Model	Mass sheet	τ₁₂	τ₁₃	τ₂₃
1	–	–	–	–
2	✓	–	–	–
3	–	✓	✓	✓
4	✓	✓	✓	✓
5	–	✓	–	–
6	✓	✓	–	–
7	–	–	–	✓
8	✓	–	–	✓

Model	Mass sheet	τ₁₂	τ₁₃	τ₂₃
1	–	–	–	–
2	✓	–	–	–
3	–	✓	✓	✓
4	✓	✓	✓	✓
5	–	✓	–	–
6	✓	✓	–	–
7	–	–	–	✓
8	✓	–	–	✓