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Table 4.

Comparison of different properties of AT 2020wey with three well-studied faint and fast TDEs (iPTF16fnl, AT 2019qiz, and AT 2020neh).

AT 2020wey iPTF16fnl AT 2019qiz AT 2020neh
(a)log(MBH/ M)
(b)log(MBH/ M)
M/ M
b
LX < 6.1 < 0.24 5.1 < 45
(1040 erg s−1)
Spectral type H+He H+He+N III H+He+N III H+He+N III
Host galaxy QBS QBS Spiral Dwarf

Notes.

(a)

Based on the M − σ relation.

(b)

Based on MOSFIT fit.

(c)

There is a range in the BH masses because three different relations are used (Nicholl et al. 2020).

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