activity
20132026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 6.4k across the 167 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★ 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.HE2018★ 44 cited

One thousand days of SN 2015bn: HST imaging shows a light curve flattening consistent with magnetar predictions

Matt Nicholl, Peter K. Blanchard, Edo Berger +9

We present the first observations of a Type I superluminous supernova (SLSN) at days after maximum light. We observed SN 2015bn using the Hubble Space Telescope Adva…

astro-ph.HE2018★ 18 cited

Strongly Bipolar Inner Ejecta of the Normal Type IIP Supernova ASASSN-16at

Subhash Bose, Subo Dong, N. Elias-Rosa +24

We report distinctly double-peakedH-alpha and H-beta emission lines in the late-time, nebular-phase spectra (>~200 d) of the otherwise normal at early phases (<~ 100 d) Type IIP su…

astro-ph.SR2018★ 5 cited

SN 2014J in M82: New Insights On the Spectral Diversity of Type Ia Supernovae

Kaicheng Zhang, Xiaofeng Wang, JuJia Zhang +25

We present extensive spectroscopic observations for one of the closest type Ia supernovae (SNe Ia), SN 2014J discovered in M82, ranging from 10.4 days before to 473.2 days after B-…

astro-ph.HE2018★ 17 cited

AT 2017be - a new member of the class of Intermediate-Luminosity Red Transients

Y-Z. Cai, A. Pastorello, M. Fraser +20

We report the results of our spectrophotometric monitoring campaign for AT~2017be in NGC~2537. Its lightcurve reveals a fast rise to an optical maximum, followed by a plateau lasti…

astro-ph.HE2018★ 40 cited

Type II supernovae in low luminosity host galaxies

C. P. Gutiérrez, J. P. Anderson, M. Sullivan +29

We present an analysis of a new sample of type II core-collapse supernovae (SNe II) occurring within low-luminosity galaxies, comparing these with a sample of events in brighter ho…

astro-ph.HE2018★ 36 cited

Late-time observations of the extraordinary Type II supernova iPTF14hls

J. Sollerman, F. Taddia, I. Arcavi +22

We study iPTF14hls, a luminous and extraordinary long-lived Type II supernova, which lately has attracted much attention and disparate interpretation. We present new optical photom…

astro-ph.SR2018★ 15 cited

ASASSN-15no: The Supernova that plays hide-and-seek

S. Benetti, L. Zampieri, A. Pastorello +11

We report the results of our follow-up campaign of the peculiar supernova ASASSN-15no, based on optical data covering ~300 days of its evolution. Initially the spectra show a pure…

astro-ph.SR2018★ 12 cited

SNhunt151: an explosive event inside a dense cocoon

N. Elias-Rosa, S. Benetti, E. Cappellaro +20

SNhunt151 was initially classified as a supernova (SN) impostor (nonterminal outburst of a massive star). It exhibited a slow increase in luminosity, lasting about 450 d, followed…