activity
20162020
most citedEarly Blue Excess from the Type Ia Supernova 2017cbv and Implications for Its Progenitor

140 citations · 279 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.HE202029 cited

SN 2018gjx reveals that some SNe Ibn are SNe IIb exploding in dense circumstellar material

S. J. Prentice, K. Maguire, I. Boian +27

We present the data and analysis of SN 2018gjx, an unusual low-luminosity transient with three distinct spectroscopic phases. Phase I shows a hot blue spectrum with signatures of i…

astro-ph.HE202024 cited

SN 2017ivv: two years of evolution of a transitional Type II supernova

C. P. Gutiérrez, A. Pastorello, A. Jerkstrand +39

We present the photometric and spectroscopic evolution of the Type II supernova (SN II) SN 2017ivv (also known as ASASSN-17qp). Located in an extremely faint galaxy (M ma…

astro-ph.HE2019

Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068

K. A. Bostroem, S. Valenti, D. J. Sand +44

We present the discovery and high-cadence follow-up observations of SN 2018ivc, an unusual Type II supernova that exploded in NGC 1068 (D=10.1 Mpc). The light curve of SN 2018ivc d…

astro-ph.HE2019

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…

astro-ph.HE201986 cited

The Type II-P Supernova 2017eaw: from explosion to the nebular phase

Tamás Szalai, József Vinkó, Réka Könyves-Tóth +36

The nearby SN 2017eaw is a Type II-P (``plateau') supernova showing early-time, moderate CSM interaction. We present a comprehensive study of this SN including the analysis of high…

astro-ph.SR2019

Signatures of Circumstellar Interaction in the Type IIL Supernova ASASSN-15oz

K. Azalee Bostroem, Stefano Valenti, Assaf Horesh +27

Hydrogen-rich, core-collapse supernovae are typically divided into four classes: IIP, IIL, IIn, and IIb. In general, interaction with circumstellar material is only considered for…