Abstract:
We present high-cadence photometric and spectroscopic observations of SN 2020jfo in ultraviolet and optical/near-infrared bands
starting from ∼3 to ∼434 d after the explosion, including the earliest data with the 10.4-m GTC. SN 2020jfo is a hydrogen-rich
Type II SN with a relatively short plateau duration (67.0 ± 0.6 d). When compared to other Type IIsupernovae (SNe) ofsimilar or
shorter plateau lengths, SN 2020jfo exhibits a fainter peak absolute V-band magnitude (MV = −16.90 ± 0.34 mag). SN 2020jfo
shows significant Hα absorption in the plateau phase similar to that of typical SNe II. The emission line of stable [Ni II] λ7378,
mostly seen in low-luminosity SNe II, is very prominent in the nebular-phase spectra of SN 2020jfo. Using the relative strengths
of [Ni II] λ7378 and [Fe II] λ7155, we derive the Ni/Fe production (abundance) ratio of 0.08–0.10, which is ∼1.5 times the solar
value. The progenitor mass of SN 2020jfo from nebular-phase spectral modelling and semi-analytical modelling falls in the
range of 12–15 M . Furthermore, semi-analytical modelling suggests a massive H envelope in the progenitor of SN 2020jfo,
which is unlikely for SNe II having short plateaus.
