Rates of strongly lensed tidal disruption events - A comprehensive investigation of black hole, luminosity, and temperature dependencies

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Table 3.

Rate of double and quad lensed TDEs, the ratio of double to quad lenses, and the fraction of quad to total lenses.

Model	Band	Doubles	Quads	$\frac{N_{doubles}}{N_{quads}}$ $\frac{N_{\mathrm{doubles}}}{N_{\mathrm{quads}}}$	$\frac{N_{quads}}{N_{TDE, lensed}}$ $\frac{N_{\mathrm{quads}}}{N_{\mathrm{TDE, lensed}}}$
		Rate	Rate		[%]
L₁,	u	0.63	0.2	3.18	23.91
TRINITY,	g	3.86	0.77	5.03	16.58
20 000 K	r	2.82	0.69	4.12	19.54
	i	1.26	0.41	3.07	24.58

L₂,	u	0.97	0.26	3.78	20.92
TRINITY,	g	6.15	1.14	5.41	15.6
20 000 K	r	4.61	1.15	4.02	19.92
	i	1.98	0.67	2.94	25.4

L₂,	u	1.7	0.6	2.81	26.22
TRINITY	g	8.63	1.8	4.81	17.22

T-dep.	r	4.98	1.28	3.89	20.43
	i	2.06	0.67	3.09	24.46

L₂,	u	0.22	0.14	1.56	39.13
TRINITY,	g	2.26	0.85	2.65	27.41
40 000 K	r	0.56	0.35	1.58	38.71
	i	0.08	0.09	0.96	50.9

L₂,	u	0.9	0.24	3.75	21.04
COSMOS2015,	g	5.92	1.38	4.29	18.91
20 000 K	r	4.42	1.37	3.24	23.59
	i	1.78	0.78	2.28	30.5

Notes. The rates are given in per year and 20 000 deg². We expect to find a few doubles for every quad. This table is calculated for LSST magnitude limits.

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