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 2019Show all

15 papers · 1 filter

astro-ph.HE2019★ 33 cited

AT 2018cow VLBI: No Long-Lived Relativistic Outflow

Michael F. Bietenholz, Raffaella Margutti, Deanne Coppejans +7

We report on VLBI observations of the fast and blue optical transient (FBOT), AT 2018cow. At ~62 Mpc, AT 2018cow is the first relatively nearby FBOT. The nature of AT 2018cow is no…

astro-ph.HE2019★ 146 cited

Two years of non-thermal emission from the binary neutron star merger GW170817: rapid fading of the jet afterglow and first constraints on the kilonova fastest ejecta

A. Hajela, R. Margutti, K. D. Alexander +27

We present Chandra and VLA observations of GW170817 at ~521-743 days post merger, and a homogeneous analysis of the entire Chandra data set. We find that the late-time non-thermal…

astro-ph.HE2019★ 102 cited

The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin

Wen-fai Fong, P. K. Blanchard, K. D. Alexander +25

We present a revised and complete optical afterglow light curve of the binary neutron star merger GW170817, enabled by deep Hubble Space Telescope (HST) F606W observations at $\app…

astro-ph.HE2019★ 36 cited

Optical follow-up of the tidal disruption event iPTF16fnl: new insights from X-shooter observations

F. Onori, G. Cannizzaro, P. G. Jonker +11

We present the results from Nordic Optical Telescope and X-shooter follow-up campaigns of the tidal disruption event (TDE) iPTF16fnl, covering the first 100 days after the tr…

astro-ph.HE2019★ 53 cited

The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell

L. Tartaglia, A. Pastorello, J. Sollerman +41

In this paper we report the results of the first four years of spectroscopic and photometric monitoring of the Type IIn supernova SN 2015da (also known as PSN J13522411+39412…

astro-ph.SR2019★ 18 cited

Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System

Wenxiong Li, Xiaofeng Wang, Maokai Hu +18

We present extensive ground-based and () photometry of the highly reddened, very nearby type Ia supernova (SN Ia) 2014J in M82, covering the phases fr…

astro-ph.SR2019★ 129 cited

Luminous Red Novae: Stellar Mergers or Giant Eruptions?

A. Pastorello, E. Mason, S. Taubenberger +36

We present extensive datasets for a class of intermediate-luminosity optical transients known as "luminous red novae" (LRNe). They show double-peaked light curves, with an initial…

astro-ph.HE2019★ 36 cited

SN 2016coi (ASASSN-16fp): an energetic H-stripped core-collapse supernova from a massive stellar progenitor with large mass loss

G. Terreran, R. Margutti, D. Bersier +25

We present comprehensive observations and analysis of the energetic H-stripped SN 2016coi (a.k.a. ASASSN-16fp), spanning the -ray through optical and radio wavelengths, acquired…

astro-ph.HE2019★ 97 cited

Follow-up of the Neutron Star Bearing Gravitational Wave Candidate Events S190425z and S190426c with MMT and SOAR

G. Hosseinzadeh, P. S. Cowperthwaite, S. Gomez +23

On 2019 April 25.346 and 26.640 UT the LIGO and Virgo gravitational wave (GW) observatories announced the detection of the first candidate events in Observing Run 3 that contain at…

astro-ph.GA2019

Astro2020 Science White Paper: Are Supernovae the Dust Producer in the Early Universe?

Jeonghee Rho, Danny Milisavljevic, Arkaprabha Sarangi +23

Whether supernovae are a significant source of dust has been a long-standing debate. The large quantities of dust observed in high-redshift galaxies raise a fundamental question as…

astro-ph.HE2019★ 3 cited

Astro2020 Science White Paper: Discovery Frontiers of Explosive Transients - An ELT & LSST Perspective

Melissa L. Graham, Danny Milisavljevic, Armin Rest +17

The Large Synoptic Survey Telescope (LSST) will open a discovery frontier for faint and fast transients with its ability to detect variable flux components down to 24.5 mag i…

astro-ph.HE2019★ 1 cited

Achieving Transformative Understanding of Extreme Stellar Explosions with ELT-enabled Late-time Spectroscopy

D. Milisavljevic, R. Margutti, R. Chornock +35

Supernovae are among the most powerful and influential explosions in the universe. They are also ideal multi-messenger laboratories to study extreme astrophysics. However, many fun…

astro-ph.HE2019★ 7 cited

SN 2016B a.k.a ASASSN-16ab: a transitional type II supernova

Raya Dastidar, Kuntal Misra, Mridweeka Singh +12

We present photometry, polarimetry and spectroscopy of the Type II supernova ASASSN-16ab/SN 2016B in PGC 037392. The photometric and spectroscopic follow-up commenced about two wee…

astro-ph.HE2019★ 3 cited

Multi-Messenger Astronomy with Extremely Large Telescopes

Ryan Chornock, Philip S. Cowperthwaite, Raffaella Margutti +82

The field of time-domain astrophysics has entered the era of Multi-messenger Astronomy (MMA). One key science goal for the next decade (and beyond) will be to characterize gravitat…

astro-ph.HE2019

Gravity and Light: Combining Gravitational Wave and Electromagnetic Observations in the 2020s

R. J. Foley, K. D. Alexander, I. Andreoni +110

As of today, we have directly detected exactly one source in both gravitational waves (GWs) and electromagnetic (EM) radiation, the binary neutron star merger GW170817, its associa…