activity
20052025
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 9.6k across the 93 of their papers we have counts for

collaborators

93 papers

astro-ph.HE2025★ 8 cited

SN 2024bfu, SN 2025qe, and the early light curves of type Iax supernovae

M. R. Magee, T. L. Killestein, M. Pursiainen +39

Type Iax supernovae (SNe Iax) are one of the most common subclasses of thermonuclear supernova and yet their sample size, particularly those observed shortly after explosion, remai…

astro-ph.SR2024★ 10 cited

SN 2020pvb: a Type IIn-P supernova with a precursor outburst

Nancy Elias-Rosa, Seán J. Brennan, Stefano Benetti +37

We present photometric and spectroscopic data sets for SN 2020pvb, a Type IIn-P supernova (SN) similar to SNe 1994W, 2005cl, 2009kn and 2011ht, with a precursor outburst detected (…

astro-ph.EP2023

UV to near-IR observations of the DART-Dimorphos collision

E. O. Ofek, D. Kushnir, D. Polishook +15

The impact of the Double Asteroid Redirection Test (DART) spacecraft with Dimorphos allows us to study asteroid collision physics, including momentum transfer, the ejecta propertie…

astro-ph.HE2023★ 4 cited

The Early Ultraviolet Light-Curves of Type II Supernovae and the Radii of Their Progenitor Stars

Ido Irani, Jonathan Morag, Avishay Gal-Yam +18

We present a sample of 34 normal SNe II detected with the Zwicky Transient Facility, with multi-band UV light-curves starting at days after explosion, as well as X-ray d…

astro-ph.HE2023★ 1 cited

Resolving the explosion of supernova 2023ixf in Messier 101 within its complex circumstellar environment

E. A. Zimmerman, I. Irani, P. Chen +54

Observing a supernova explosion shortly after it occurs can reveal important information about the physics of stellar explosions and the nature of the progenitor stars of supernova…

astro-ph.HE2023★ 8 cited

1100 days in the life of the supernova 2018ibb -- The best pair-instability supernova candidate, to date

Steve Schulze, Claes Fransson, Alexandra Kozyreva +63

Abridged - Stars with ZAMS masses between 140 and are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce…