21 citations · 24 across the 4 of their papers we have counts for
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astro-ph.HE2024
On the Formation of the W-shaped O II Lines in Spectra of Type I Superluminous Supernovae
Sei Saito, Masaomi Tanaka, Paolo A. Mazzali +2
H-poor superluminous supernovae (SLSNe-I) are characterized by O II lines around 4,000 - 4,500 A in pre-/near-maximum spectra, so-called W-shaped O II lines. As these lines are fro…
astro-ph.HE2024
Intermediate-luminosity Type IIP SN 2021gmj: a low-energy explosion with signatures of circumstellar material
Yuta Murai, Masaomi Tanaka, Miho Kawabata +28
We present photometric, spectroscopic and polarimetric observations of the intermediate-luminosity Type IIP supernova (SN) 2021gmj from 1 to 386 days after the explosion. The peak…