Sample of hydrogen-rich superluminous supernovae from the Zwicky Transient Facility

Open Access

Fig. 15.

Mass loss rate (Ṁ) of the SLSNe II for which we can approximate a pseudo-bolometric light curve (see Sect. 3.4) considering a RSG, LBV and WR progenitor. The different mass loss rate ranges are shown in consecutive horizontal axis. The left panel considers v_SN = 2500 km s⁻¹ and the right panel v_SN = 10 000 km s⁻¹.

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