activity
20072026
most citedRapidly-Evolving and Luminous Transients from Pan-STARRS1

364 citations · 9.9k across the 203 of their papers we have counts for

collaborators
Showing 2018Show all

10 papers · 1 filter

astro-ph.HE2018★ 4 cited

Target of Opportunity Observations of Gravitational Wave Events with LSST

R. Margutti, P. Cowperthwaite, Z. Doctor +79

The discovery of the electromagnetic counterparts to the binary neutron star merger GW170817 has opened the era of GW+EM multi-messenger astronomy. Exploiting this breakthrough req…

astro-ph.HE2018★ 30 cited

A Hydrogen-Poor Superluminous Supernova with Enhanced Iron-Group Absorption: A New Link Between SLSNe and Broad-Lined Type Ic SNe

P. K. Blanchard, M. Nicholl, E. Berger +4

We present optical observations of the Type I superluminous supernova (SLSN-I) SN2017dwh at , which reached mag at peak. Spectra taken a few…

astro-ph.HE2018★ 267 cited

An embedded X-ray source shines through the aspherical AT2018cow: revealing the inner workings of the most luminous fast-evolving optical transients

Raffaella Margutti, B. D. Metzger, R. Chornock +41

We present the first extensive radio to gamma-ray observations of a fast-rising blue optical transient (FBOT), AT2018cow, over its first ~100 days. AT2018cow rose over a few days t…

astro-ph.GA2018★ 20 cited

The Temperature and Ionization of Unshocked Ejecta in Cas A

J. C. Raymond, B. -C. Koo, Y. -H. Lee +3

The supernova remnant Cassiopeia A (Cas A) is one of the few remnants in which it is possible to observe unshocked ejecta. A deep 1.64 micron image of Cas A shows a patch of diffus…

astro-ph.HE2018★ 18 cited

Where is the engine hiding its missing energy? Constraints from a deep X-ray non-detection of the Superluminous SN 2015bn

Kornpob Bhirombhakdi, Ryan Chornock, Raffaella Margutti +5

SN 2015bn is a nearby hydrogen-poor superluminous supernova (SLSN-I) that has been intensively observed in X-rays with the goal to detect the spin-down powered emission from a magn…

astro-ph.HE2018★ 46 cited

Evidence for a pulsar wind nebula in the Type Ib-peculiar supernova SN 2012au

Dan Milisavljevic, Daniel J. Patnaude, Roger A. Chevalier +5

We present an optical spectrum of the energetic Type Ib supernova (SN) 2012au obtained at an unprecedented epoch of 6.2 years after explosion. Forbidden transition emission lines o…

astro-ph.HE2018★ 27 cited

The Type I Superluminous Supernova PS16aqv: Lightcurve Complexity and Deep Limits on Radioactive Ejecta in a Fast Event

P. K. Blanchard, M. Nicholl, E. Berger +6

[Abridged] We present UV/optical observations of PS16aqv (SN 2016ard), a Type I superluminous supernova (SLSN-I) classified as part of our search for low- SLSNe. PS16aqv is a fa…

astro-ph.HE2018★ 9 cited

Peculiar Supernovae

Dan Milisavljevic, Raffaella Margutti

What makes a supernova truly `peculiar?' In this chapter we attempt to address this question by tracing the history of the use of `peculiar' as a descriptor of non-standard superno…

astro-ph.SR2018★ 71 cited

SN 2017ein and the Possible First Identification of a Type Ic Supernova Progenitor

Schuyler D. Van Dyk, WeiKang Zheng, Thomas G. Brink +11

We have identified a progenitor candidate in archival Hubble Space Telescope (HST) images for the Type Ic SN 2017ein in NGC 3938, pinpointing the candidate's location via HST Targe…

astro-ph.GA2018★ 38 cited

MMT Spectroscopy of Supernova Remnant Candidates in M33

Knox S. Long, William P. Blair, Dan Milisavljevic +2

To date, over 220 emission nebulae in M33 have been identified as supernova remnants (SNRs) or SNR candidates, principally through [SII]:Halpha line ratios that are elevated compar…