activity
20142025
most citedSwope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source

1.2k citations · 3.7k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2025

Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption

Rewa Clark Bush, Samantha C. Wu, Rosa Wallace Everson +3

Once per 10,000-100,000 years, an unlucky star may experience a close encounter with a supermassive black hole (SMBH), partially or fully tearing apart the star in an exceedingly b…

astro-ph.SR2024★ 7 cited

The Evolution of Binaries Embedded Within Common Envelopes

Alejandra Rosselli-Calderon, Ricardo Yarza, Ariadna Murguia-Berthier +5

Triple stellar systems allow us to study stellar processes that cannot be attained in binary stars. The evolutionary phases in which the stellar members undergo mass exchanges can…

astro-ph.HE2024★ 1 cited

The Dynamics of Debris Disk Creation in Neutron Star Mergers

Yossef Zenati, Julian Krolik, Leonardo Werneck +4

The detection of GW170817/AT2017gfo inaugurated an era of multimessenger astrophysics, in which gravitational wave and multiwavelength photon observations complement one another to…

astro-ph.HE2023

From Feast to Famine: A Systematic Study of Accretion onto Oblique Pulsars with 3D GRMHD Simulations

Ariadna Murguia-Berthier, Kyle Parfrey, Alexander Tchekhovskoy +1

Disk-fed accretion onto neutron stars can power a wide range of astrophysical sources ranging from X-ray binaries, to accretion powered millisecond pulsars, ultra-luminous X-ray so…

astro-ph.HE2023★ 2 cited

Bound Debris Expulsion from Neutron Star Merger Remnants

Yossef Zenati, Julian H. Krolik, Leonardo R. Werneck +4

Many studies have found that neutron star mergers leave a fraction of the stars' mass in bound orbits surrounding the resulting massive neutron star or black hole. This mass is a s…

gr-qc2022★ 21 cited

Addition of tabulated equation of state and neutrino leakage support to IllinoisGRMHD

Leonardo R. Werneck, Zachariah B. Etienne, Ariadna Murguia-Berthier +11

We have added support for realistic, microphysical, finite-temperature equations of state (EOS) and neutrino physics via a leakage scheme to IllinoisGRMHD, an open-source GRMHD cod…

astro-ph.HE2022★ 41 cited

On the jet-ejecta interaction in 3D GRMHD simulations of binary neutron star merger aftermath

Ore Gottlieb, Serena Moseley, Teresita Ramirez-Aguilar +3

Short -ray burst (sGRB) jets form in the aftermath of a neutron star merger, drill through disk winds and dynamical ejecta, and extend over four to five orders of magnitude in d…

astro-ph.SR2022★ 19 cited

Hydrodynamics and survivability during post-main-sequence planetary engulfment

Ricardo Yarza, Naela Razo Lopez, Ariadna Murguia-Berthier +6

The engulfment of substellar bodies (SBs, such as brown dwarfs and planets) by giant stars is a possible explanation for rapidly rotating giants, lithium-rich giants, and the prese…

astro-ph.HE2022★ 40 cited

Jet Formation in 3D GRMHD Simulations of Bondi-Hoyle-Lyttleton Accretion

Nicholas Kaaz, Ariadna Murguia-Berthier, Koushik Chatterjee +2

A black hole (BH) travelling through a uniform, gaseous medium is described by Bondi-Hoyle-Lyttleton (BHL) accretion. If the medium is magnetized, then the black hole can produce r…

astro-ph.HE2021★ 11 cited

Handing off the outcome of binary neutron star mergers for accurate and long-term post-merger simulations

Federico G. Lopez Armengol, Zachariah B. Etienne, Scott C. Noble +20

We perform binary neutron star (BNS) merger simulations in full dynamical general relativity with IllinoisGRMHD, on a Cartesian grid with adaptive-mesh refinement. After the remnan…

astro-ph.HE2021★ 25 cited

HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage

Ariadna Murguia-Berthier, Scott C. Noble, Luke F. Roberts +25

The first binary neutron star merger has already been detected in gravitational waves. The signal was accompanied by an electromagnetic counterpart including a kilonova component p…

astro-ph.HE2020★ 45 cited

What determines the structure of short gamma-ray burst jets?

Gerardo Urrutia, Fabio De Colle, Ariadna Murguia-Berthier +1

The discovery of GRB 170817A, the first unambiguous off-axis short gamma-ray burst arising from a neutron star merger, has challenged our understanding of the angular structure of…

astro-ph.HE2020★ 63 cited

The Fate of the Merger Remnant in GW170817 and its Imprint on the Jet Structure

Ariadna Murguia-Berthier, Enrico Ramirez-Ruiz, Fabio De Colle +3

The first neutron star binary merger detected in gravitational waves, GW170817 and the subsequent detection of its emission across the electromagnetic spectrum showed that these sy…

astro-ph.HE2020★ 19 cited

On the maximum stellar rotation to form a black hole without an accompanying luminous transient

Ariadna Murguia-Berthier, Aldo Batta, Agnieszka Janiuk +4

The collapse of a massive star with low angular momentum content is commonly argued to result in the formation of a black hole without an accompanying bright transient. Our goal in…

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…

astro-ph.HE2018★ 83 cited

A luminosity distribution for kilonovae based on short gamma-ray burst afterglows

Stefano Ascenzi, Michael W. Coughlin, Tim Dietrich +8

The combined detection of a gravitational-wave signal, kilonova, and short gamma-ray burst (sGRB) from GW170817 marked a scientific breakthrough in the field of multi-messenger ast…

astro-ph.HE2017★ 115 cited

A Neutron Star Binary Merger Model for GW170817/GRB170817a/SSS17a

Ariadna Murguia-Berthier, Enrico Ramirez-Ruiz, Charles D. Kilpatrick +14

The merging neutron star gravitational wave event GW170817 has been observed throughout the entire electromagnetic spectrum from radio waves to -rays. The resulting energetics,…

astro-ph.HE2017★ 1.2k cited

Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source

D. A. Coulter, R. J. Foley, C. D. Kilpatrick +14

On 2017 August 17, the Laser Interferometer Gravitational-wave Observatory (LIGO) and the Virgo interferometer detected gravitational waves emanating from a binary neutron star mer…

astro-ph.HE2017★ 839 cited

Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

M. R. Drout, A. L. Piro, B. J. Shappee +41

On 2017 August 17, gravitational waves were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB170817A. An optical transient so…

astro-ph.HE2017★ 35 cited

The Unprecedented Properties of the First Electromagnetic Counterpart to a Gravitational Wave Source

Matthew R. Siebert, Ryan J. Foley, Maria R. Drout +15

We discovered Swope Supernova Survey 2017a (SSS17a) in the LIGO/Virgo Collaboration (LVC) localization volume of GW170817, the first detected binary neutron star (BNS) merger, only…

astro-ph.GA2017★ 67 cited

The Old Host-Galaxy Environment of SSS17a, the First Electromagnetic Counterpart to a Gravitational Wave Source

Y. -C. Pan, C. D. Kilpatrick, J. D. Simon +16

We present an analysis of the host-galaxy environment of Swope Supernova Survey 2017a (SSS17a), the discovery of an electromagnetic counterpart to a gravitational wave source, GW17…

astro-ph.HE2017★ 272 cited

Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger

Charles D. Kilpatrick, Ryan J. Foley, Daniel Kasen +18

11 hours after the detection of gravitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers, an associated optical trans…

astro-ph.HE2017★ 342 cited

Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger

B. J. Shappee, J. D. Simon, M. R. Drout +33

On 2017 August 17, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event GW170817. We report time-seri…