activity
20032025
most citedSupernova rates from the SUDARE VST-Omegacam search. I

109 citations · 257 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2025

Continuous Wide-Field Optical Monitoring for Very Early-Phase Transient Discovery

Massimo Della Valle, Maria Teresa Botticella, Enrico Cappellaro +40

The study of transient phenomena in a multimessenger context is expected to remain a major pillar of astrophysical discovery in the decades ahead. Supernovae, Kilonovae, Black-Hole…

astro-ph.HE2025★ 4 cited

Possible evidence for the 478 keV emission line from Be decay during the outburst phases of V1369 Cen

L. Izzo, T. Siegert, P. Jean +4

After decades of uncertainty about the origin of lithium, recent evidence suggests Galactic novae as its main astrophysical source. In this work, we present possible evidence for t…

astro-ph.HE2022

Euclid: Searching for pair-instability supernovae with the Deep Survey

T. J. Moriya, C. Inserra, M. Tanaka +106

Pair-instability supernovae are theorized supernovae that have not yet been observationally confirmed. They are predicted to exist in low-metallicity environments. Because overall…

astro-ph.HE2022★ 1 cited

Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja

Griffin Hosseinzadeh, Charles D. Kilpatrick, Yize Dong +56

We present high-cadence optical, ultraviolet (UV), and near-infrared data of the nearby ( Mpc) Type II supernova (SN) 2021yja. Many Type II SNe show signs of interactio…

astro-ph.HE2021★ 102 cited

The peculiar short-duration GRB 200826A and its supernova

A. Rossi, B. Rothberg, E. Palazzi +31

Gamma-ray bursts (GRBs) are classified as long and short events. Long GRBs (LGRBs) are associated with the end states of very massive stars, while short GRBs (SGRBs) are linked to…

astro-ph.HE2016★ 8 cited

Optical photometry and spectroscopy of the low-luminosity, broad-lined Ic supernova iPTF15dld

E. Pian, L. Tomasella, E. Cappellaro +37

Core-collapse stripped-envelope supernova (SN) explosions reflect the diversity of physical parameters and evolutionary paths of their massive star progenitors. We have observed th…