Panning for gold, but finding helium: Discovery of the ultra-stripped supernova SN 2019wxt from gravitational-wave follow-up observations

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Table 3.

Input parameters used to generate the various TARDIS models presented in this work.

	Phase (days)
	+0.9	+6.5	+8.4	+15.6
t_exp (days)	4.1	9.7	11.6	18.8
L_ph (10⁴¹ erg s⁻¹)	17.0	6.71	5.75	2.52
v_min (km s⁻¹)	17 000	9300	7700	3500
T_ph (10³ K)	8.99	6.51	6.26	5.84
M_TARDIS (10⁻³ M_⊙) ^(a)	1.35	13.1	15.4	19.6

Notes.

^(a)

M_TARDIS is a derived property of our models, but is included here for reference. It represents the mass bound by the TARDIS computational domain, and so it represents a lower limit for a model’s total ejecta mass.

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