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20162025
most citedThe X-ray counterpart to the gravitational wave event GW 170817

888 citations · 2.4k across the 36 of their papers we have counts for

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astro-ph.SR202260 cited

Nested Dust Shells around the Wolf-Rayet Binary WR 140 observed with JWST

Ryan M. Lau, Matthew J. Hankins, Yinuo Han +29

Massive colliding-wind binaries that host a Wolf-Rayet (WR) star present a potentially important source of dust and chemical enrichment in the interstellar medium (ISM). However, t…

astro-ph.SR202011 cited

SN 2014ab: An Aspherical Type IIn Supernova with Low Polarization

Christopher Bilinski, Nathan Smith, G. Grant Williams +20

We present photometry, spectra, and spectropolarimetry of supernova (SN) 2014ab, obtained through days after peak brightness. SN 2014ab was a luminous Type IIn SN ($M_V…

astro-ph.SR202042 cited

Berkeley Supernova Ia Program: Data Release of 637 Spectra from 247 Type Ia Supernovae

Benjamin E. Stahl, WeiKang Zheng, Thomas de Jaeger +18

We present 637 low-redshift optical spectra collected by the Berkeley Supernova Ia Program (BSNIP) between 2009 and 2018, almost entirely with the Kast double spectrograph on the S…

astro-ph.SR2019

Supernova 2014C: ongoing interaction with extended circumstellar material with silicate dust

Samaporn Tinyanont, Ryan M Lau, Mansi M Kasliwal +8

Supernova (SN) 2014C is a unique explosion where a seemingly typical hydrogen-poor stripped envelope SN started to interact with a dense, hydrogen-rich circumstellar medium (CSM) a…

astro-ph.SR2018

Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the 2 Observations

W. Li, X. Wang, J. Vinkó +160

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the field. The data revealed an excess emission…

astro-ph.SR2018

The Type IIn Supernova 2010bt: The Explosion of a Star in Outburst

N. Elias-Rosa, S. D. Van Dyk, S. Benetti +12

It is well known that massive stars (M > 8 M_sun) evolve up to the collapse of the stellar core, resulting in most cases as a supernova (SN) explosion. Their heterogeneity is relat…