activity
19972023
most citedThe unusual afterglow of GRB 980326: evidence for the gamma-ray burst/supernova connection

487 citations · 11.9k across the 114 of their papers we have counts for

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19 papers · 1 filter

astro-ph.HE2023

Multi-Epoch Spectropolarimetry for a Sample of Type IIn Supernovae: Persistent Asymmetry in Dusty Circumstellar Material

Christopher Bilinski, Nathan Smith, G. Grant Williams +5

We present multi-epoch spectropolarimetry and spectra for a sample of 14 Type IIn supernovae (SNe IIn). We find that after correcting for likely interstellar polarization, SNe IIn…

astro-ph.HE2021

Making Sense of Nothing

Douglas C. Leonard

A model of the optical light detected following the merger of two neutron stars reveals polarization to be a unique probe of the geometry of the kilonova explosion that accompanied…

astro-ph.HE2021

A High-Velocity Scatterer Revealed in the Thinning Ejecta of a Type II Supernova

Douglas C. Leonard, Luc Dessart, D. John Hillier +7

We present deep, nebular-phase spectropolarimetry of the Type II-P/L SN 2013ej, obtained 167 days after explosion with the European Southern Observatory's Very Large Telescope. The…

astro-ph.HE2021★ 7 cited

Polarization signatures of a high-velocity scatterer in nebular-phase spectra of Type II supernovae

Luc Dessart, D. John Hillier, Douglas C. Leonard

Type II supernovae (SNe) often exhibit a linear polarization, arising from free-electron scattering, with complicated optical signatures, both in the continuum and in lines. Focusi…

astro-ph.HE2021★ 20 cited

Multiepoch VLT-FORS spectro-polarimetric observations of supernova 2012aw reveal an asymmetric explosion

Luc Dessart, Douglas C. Leonard, D. John Hillier +1

We present VLT-FORS spectropolarimetric observations of the type II supernova (SN) 2012aw taken at seven epochs during the photospheric phase, from 16 to 120d after explosion. We c…

astro-ph.HE2019★ 84 cited

The Type II-Plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor

Schuyler D. Van Dyk, WeiKang Zheng, Justyn R. Maund +31

We present extensive optical photometric and spectroscopic observations, from 4 to 482 days after explosion, of the Type II-plateau (II-P) supernova (SN) 2017eaw in NGC 6946. SN 20…

astro-ph.HE2019★ 36 cited

Supernova 2017eaw: molecule and dust formation from infrared observations

Samaporn Tinyanont, Mansi M Kasliwal, Kelsie Krafton +15

We present infrared (IR) photometry and spectroscopy of the Type II-P SN 2017eaw and its progenitor in the nearby galaxy NGC 6946. Progenitor observations in the Ks band in 4 epoch…

astro-ph.HE2017★ 150 cited

Swift monitoring of NGC 4151: Evidence for a Second X-ray/UV Reprocessing

R. Edelson, J. Gelbord, E. Cackett +41

Swift monitoring of NGC 4151 with ~6 hr sampling over a total of 69 days in early 2016 is used to construct light curves covering five bands in the X-rays (0.3-50 keV) and six in t…

astro-ph.HE2016★ 21 cited

Asymmetries in SN 2014J Near Maximum Light Revealed Through Spectropolarimetry

Amber L. Porter, Mark D. Leising, G. Grant Williams +7

We present spectropolarimetric observations of the nearby Type Ia SN 2014J in M82 over six epochs: +0, +7, +23, +51, +77, +109, and +111 days with respect to B-band maximum. The st…

astro-ph.HE2016★ 55 cited

Long-rising Type II supernovae from PTF and CCCP

F. Taddia, J. Sollerman, C. Fremling +17

Supernova (SN) 1987A was a peculiar H-rich event with a long-rising (LR) light curve (LC), stemming from a compact blue supergiant star (BSG). Only a few similar events have been p…

astro-ph.HE2015★ 94 cited

Type II supernova energetics and comparison of light curves to shock-cooling models

Adam Rubin, Avishay Gal-Yam, Annalisa De Cia +37

During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding early-time SN light curves in the…

astro-ph.HE2015★ 169 cited

PTF11iqb: Cool supergiant mass loss that bridges the gap between Type IIn and normal supernovae

Nathan Smith, Jon C. Mauerhan, S. Bradley Cenko +16

PTF11iqb was initially classified as a TypeIIn event caught very early after explosion. It showed narrow Wolf-Rayet (WR) spectral features on day 2, but the narrow emission weakene…

astro-ph.HE2014★ 156 cited

A Sample of Type II-L Supernovae

T. Faran, D. Poznanski, A. V. Filippenko +8

What are Type II-Linear supernovae (SNe II-L)? This class, which has been ill defined for decades, now receives significant attention -- both theoretically, in order to understand…

astro-ph.HE2014★ 101 cited

Early Emission from the Type IIn Supernova 1998S at High Resolution

Isaac Shivvers, Jose H. Groh, Jon C. Mauerhan +3

The well-studied Type IIn supernova (SN) 1998S is often dubbed the prototypical SN IIn, and it provides a unique opportunity to study its progenitor star from within as the SN ligh…

astro-ph.HE2014★ 179 cited

Photometric and Spectroscopic Properties of Type II-P Supernovae

Tamar Faran, Dovi Poznanski, Alexei V. Filippenko +9

We study a sample of 23 Type II Plateau supernovae (SNe II-P), all observed with the same set of instruments. Analysis of their photometric evolution confirms that their typical pl…

astro-ph.HE2011★ 241 cited

Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features

Assaf Sternberg, Avishay Gal-Yam, Josh D. Simon +17

Type Ia supernovae are key tools for measuring distances on a cosmic scale. They are generally thought to be the thermonuclear explosion of an accreting white dwarf in a close bina…

astro-ph.HE2011★ 44 cited

The old environment of the faint calcium-rich supernova SN 2005cz

Hagai B. Perets, Avishay Gal-yam, R. Mark Crockett +5

The supernova SN 2005cz has recently attracted some attention, due to the fact that it was spectroscopically similar to type Ib supernovae (SNe), a class that is presumed to result…

astro-ph.HE2009★ 349 cited

A faint type of supernova from a white dwarf with a helium-rich companion

H. B. Perets, A. Gal-Yam, P. Mazzali +25

Supernovae (SNe) are thought to arise from two different physical processes. The cores of massive, short-lived stars undergo gravitational core collapse and typically eject a few s…

astro-ph.HE2009★ 154 cited

An Intermediate Luminosity Transient in NGC300: The Eruption of a Dust-Enshrouded Massive Star

E. Berger, A. M. Soderberg, R. A. Chevalier +10

[abridged] We present multi-epoch high-resolution optical spectroscopy, UV/radio/X-ray imaging, and archival Hubble and Spitzer observations of an intermediate luminosity optical t…