Polarimetric diversity in tidal disruption events: Comparative study of low-polarised sources with AT2020mot

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Table 2.

Peak bolometric luminosities and blackbody temperatures.

Name	log L_bol	T_bb
	[erg s⁻¹]	[K]
(1)	(2)	(3)
AT2020mot	$44 . 10_{- 0.03}^{+ 0.03}$ $44.10^{+0.03}_{-0.03}$	$31706_{- 2319}^{+ 2861}$ $31706^{+2861}_{-2319}$
AT2020afhd	$44 . 03_{- 0.02}^{+ 0.01}$ $44.03^{+0.01}_{-0.02}$	$47698_{- 2599}^{+ 1641}$ $47698^{+1641}_{-2599}$
AT2022dbl	$43 . 81_{- 0.02}^{+ 0.02}$ $43.81^{+0.02}_{-0.02}$	$35413_{- 1812}^{+ 2055}$ $35413^{+2055}_{-1812}$
AT2022dbl₂	$43 . 36_{- 0.04}^{+ 0.03}$ $43.36^{+0.03}_{-0.04}$	$36158_{- 3194}^{+ 4013}$ $36158^{+4013}_{-3194}$
AT2022fpx	$43 . 77_{- 0.01}^{+ 0.01}$ $43.77^{+0.01}_{-0.01}$	$15187_{- 323}^{+ 341}$ $15187^{+341}_{-323}$
AT2022gri	$43 . 42_{- 0.02}^{+ 0.02}$ $43.42^{+0.02}_{-0.02}$	$22209_{- 1135}^{+ 1331}$ $22209^{+1331}_{-1135}$
AT2022hvp	$45 . 29_{- 0.01}^{+ 0.01}$ $45.29^{+0.01}_{-0.01}$	$39734_{- 1013}^{+ 1051}$ $39734^{+1051}_{-1013}$
AT2022upj	$43 . 73_{- 0.03}^{+ 0.03}$ $43.73^{+0.03}_{-0.03}$	$29632_{- 2114}^{+ 2610}$ $29632^{+2610}_{-2114}$
AT2022wtn	$43 . 35_{- 0.01}^{+ 0.01}$ $43.35^{+0.01}_{-0.01}$	$14912_{- 459}^{+ 503}$ $14912^{+503}_{-459}$
AT2023clx	$42 . 66_{- 0.01}^{+ 0.01}$ $42.66^{+0.01}_{-0.01}$	$15280_{- 400}^{+ 427}$ $15280^{+427}_{-400}$
AT2023ugy	$44 . 54_{- 0.02}^{+ 0.02}$ $44.54^{+0.02}_{-0.02}$	$47987_{- 2800}^{+ 1473}$ $47987^{+1473}_{-2800}$
AT2023lli	$43 . 67_{- 0.04}^{+ 0.04}$ $43.67^{+0.04}_{-0.04}$	$37242_{- 4854}^{+ 6097}$ $37242^{+6097}_{-4854}$
AT2024bgz	$43 . 89_{- 0.01}^{+ 0.01}$ $43.89^{+0.01}_{-0.01}$	$16880_{- 396}^{+ 421}$ $16880^{+421}_{-396}$
AT2024gre	$44 . 13_{- 0.01}^{+ 0.01}$ $44.13^{+0.01}_{-0.01}$	$17125_{- 341}^{+ 356}$ $17125^{+356}_{-341}$

Notes. (1) TDE name. (2) Logarithm of the bolometric luminosity at the peak. (3) Blackbody temperature fit to the photometric data of the source at the peak.

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