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20132026
most citedObservation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

1.2k citations · 14.7k across the 149 of their papers we have counts for

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Showing 2022Show all

5 papers · 1 filter

astro-ph.HE2022★ 96 cited

The prevalence and influence of circumstellar material around hydrogen-rich supernova progenitors

Rachel J. Bruch, Avishay Gal-Yam, Ofer Yaron +44

Narrow transient emission lines (flash-ionization features) in early supernova (SN) spectra trace the presence of circumstellar material (CSM) around the massive progenitor stars o…

astro-ph.HE2022★ 41 cited

A radio-detected Type Ia supernova with helium-rich circumstellar material

Erik C. Kool, Joel Johansson, Jesper Sollerman +34

Type Ia supernovae (SNe Ia) are thermonuclear explosions of degenerate white dwarf (WD) stars destabilized by mass accretion from a companion star, but the nature of their progenit…

astro-ph.HE2022★ 3 cited

SN 2022oqm -- a Ca-rich explosion of a compact progenitor embedded in C/O circumstellar material

I. Irani, Ping Chen, Jonathan Morag +27

We present the discovery and analysis of SN\,2022oqm, a Type Ic supernova (SN) detected \,day after explosion. The SN rises to a blue and short-lived (2\,days) initial peak. Ea…

astro-ph.HE2022★ 17 cited

SN 2019zrk, a bright SN 2009ip analog with a precursor

Claes Fransson, Jesper Sollerman, Nora L. Strotjohann +12

We present photometric and spectroscopic observations of the Type IIn supernova SN 2019zrk (also known as ZTF20aacbyec). The SN shows a 100 day precursor, with a slow ris…

astro-ph.HE2022★ 21 cited

SN2020qlb: A hydrogen-poor superluminous supernova with well-characterized light curve undulations

S. L. West, R. Lunnan, C. M. B. Omand +21

SN\,2020qlb (ZTF20abobpcb) is a hydrogen-poor superluminous supernova (SLSN-I) that is among the most luminous (maximum M mag) and that has one of the longest rise t…