activity
20092023
most citedThe X-ray counterpart to the gravitational wave event GW 170817

888 citations · 4.6k across the 59 of their papers we have counts for

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48 papers · 1 filter

astro-ph.HE2023★ 3 cited

Energy-dependent polarization of Gamma-Ray Bursts' prompt emission with the POLAR and POLAR-2 instruments

Nicolas De Angelis, J. Michael Burgess, Franck Cadoux +10

Gamma-Ray Bursts are among the most powerful events in the Universe. Despite half a century of observations of these transient sources, many open questions remain about their natur…

astro-ph.HE2023★ 12 cited

A helium-burning white dwarf binary as a supersoft X-ray source

J. Greiner, C. Maitra, F. Haberl +12

Type Ia supernovae are cosmic distance indicators, and the main source of iron in the Universe, but their formation paths are still debated. Several dozen supersoft X-ray sources,…

astro-ph.HE2023★ 1 cited

Misidentification of Short GRBs as Magnetars in Nearby Galaxies

E. C. Schösser, J. M. Burgess, J. Greiner

Context. Recent observations of GRB 200415A, a short and very bright pulse of -rays, have been claimed to be an extragalactic magnetar giant flare (MGF) whose proposed host gala…

astro-ph.HE2022★ 10 cited

Advancing the Landscape of Multimessenger Science in the Next Decade

Kristi Engel, Tiffany Lewis, Marco Stein Muzio +91

The last decade has brought about a profound transformation in multimessenger science. Ten years ago, facilities had been built or were under construction that would eventually dis…

astro-ph.HE2022

The Future of Gamma-Ray Experiments in the MeV-EeV Range

Kristi Engel, Jordan Goodman, Petra Huentemeyer +95

Gamma-rays, the most energetic photons, carry information from the far reaches of extragalactic space with minimal interaction or loss of information. They bring messages about par…

astro-ph.HE2022★ 1 cited

Improving INTEGRAL/SPI data analysis of GRBs

Björn Biltzinger, Jochen Greiner, J. Michael Burgess +1

INTEGRAL/SPI is a coded mask instrument observing since 2002 in the keV to MeV energy range, which covers the peak of the spectrum of most Gamma-Ray Bursts (GRBs). Since its…

astro-ph.HE2022★ 5 cited

Assessing coincident neutrino detections using population models

F. Capel, J. M. Burgess, D. J. Mortlock +1

Several tentative associations between high-energy neutrinos and astrophysical sources have been recently reported, but a conclusive identification of these potential neutrino emit…

astro-ph.HE2021★ 1 cited

Gamma-Ray Polarization Results of the POLAR Mission and Future Prospects

M. Kole, N. de Angelis, J. M. Burgess +14

Despite over 50 years of Gamma-Ray Burst (GRB) observations many open questions remain about their nature and the environments in which the emission takes place. Polarization measu…

astro-ph.HE2020★ 79 cited

The POLAR Gamma-Ray Burst Polarization Catalog

Merlin Kole, Nicolas De Angelis, Francesco Berlato +18

Despite over 50 years of research, many open questions remain about the origin and nature of GRBs. Polarization measurements of the prompt emission of these extreme phenomena have…

astro-ph.HE2019★ 26 cited

Improved Fermi-GBM GRB localizations using BALROG

F. Berlato, J. Greiner, J. Michael Burgess

The localizations of gamma-ray bursts (GRBs) detected with the Gamma-ray Burst Monitor (GBM) onboard the Fermi satellite are known to be affected by significant systematic errors o…

astro-ph.HE2019★ 59 cited

Time-Resolved GRB Polarization with POLAR and GBM

J. Michael Burgess, M. Kole, F. Berlato +5

Simultaneous -ray measurements of gamma-ray burst (GRB) spectra and polarization offer a unique way to determine the underlying emission mechanism(s) in these objects as well as…

astro-ph.HE2018★ 115 cited

Gamma-ray bursts as cool synchrotron sources

J. Michael Burgess, Damien Bégué, Ana Bacelj +3

Gamma-ray bursts are the most energetic electromagnetic sources in the Universe. Their prompt gamma-ray radiation corresponds to an energy release of 1E42-1E47J. Fifty years after…

astro-ph.HE2017★ 8 cited

The peculiar physics of GRB 170817A and their implications for short GRBs

D. Bégué, J. Michael Burgess, J. Greiner

The unexpected nearby gamma-ray burst GRB 170817A associated with the LIGO binary neutron star merger event GW170817 presents a challenge to the current understanding of the emissi…

astro-ph.HE2017

Viewing short Gamma-ray Bursts from a different angle

J. Michael Burgess, Jochen Greiner, Damien Begue +3

The recent coincident detection of gravitational waves (GW) from a binary neutron star merger with aLIGO/Virgo and short-lived gamma-ray emission with Fermi/GBM (called GW 170817)…

astro-ph.HE2017★ 888 cited

The X-ray counterpart to the gravitational wave event GW 170817

E. Troja, L. Piro, H. van Eerten +31

A long-standing paradigm in astrophysics is that collisions- or mergers- of two neutron stars (NSs) form highly relativistic and collimated outflows (jets) powering gamma-ray burst…

astro-ph.HE2017★ 26 cited

Is Spectral Width a Reliable Measure of GRB Emission Physics?

J. Michael Burgess

The spectral width and sharpness of unfolded, observed GRB spectra have been presented as a new tool to infer physical properties about GRB emission via spectral fitting of empiric…

astro-ph.HE2016★ 99 cited

On the GBM event seen 0.4 sec after GW 150914

J. Greiner, J. M. Burgess, V. Savchenko +1

In view of the recent report by Connaughton we analyse continuous TTE data of Fermi-GBM around the time of the gravitational wave event GW 150914. We find that after proper account…

astro-ph.HE2016★ 9 cited

The anatomy of a long gamma-ray burst: a simple classification scheme for the emission mechanism(s)

Damien Bégué, J. Michael Burgess

Ultra-relativistic motion and efficient conversion of kinetic energy to radiation are required by gamma-ray burst (GRB) observations, yet they are difficult to simultaneously achie…

astro-ph.HE2015★ 32 cited

Synchrotron emission in GRBs observed by Fermi: Its limitations and the role of the photosphere

S. Iyyani, F. Ryde, J. M. Burgess +2

It has been suggested that the prompt emission in gamma-ray bursts consists of several components giving rise to the observed spectral shape. Here we examine a sample of the 8 brig…

astro-ph.HE2015★ 90 cited

The Multi-Mission Maximum Likelihood framework (3ML)

Giacomo Vianello, Robert J. Lauer, Patrick Younk +7

Astrophysical sources are now observed by many different instruments at different wavelengths, from radio to high-energy gamma-rays, with an unprecedented quality. Putting all thes…

astro-ph.HE2015★ 27 cited

An External Shock Origin of GRB

J. Michael Burgess, Damien Bégué, Felix Ryde +4

The prompt emission of the long, smooth, and single-pulsed gamma-ray burst, GRB , is analyzed under the guise of an external shock model. First, we fit the -ra…

astro-ph.HE2015

Extremely narrow spectrum of GRB110920A: further evidence for localised, subphotospheric dissipation

S. Iyyani, F. Ryde, B. Ahlgren +6

Much evidence points towards that the photosphere in the relativistic outflow in GRBs plays an important role in shaping the observed MeV spectrum. However, it is unclear whether t…

astro-ph.HE2015★ 46 cited

Evidence for jet launching close to the black hole in GRB 101219B - a Fermi GRB dominated by thermal emission

J. Larsson, J. L. Racusin, J. M. Burgess

We present observations by the Fermi Gamma-Ray Space Telescope Gamma-Ray Burst Monitor (GBM) of the nearby (z=0.55) GRB 101219B. This burst is a long GRB, with an associated supern…

astro-ph.HE2014★ 28 cited

Swift and Fermi observations of X-ray flares: the case of Late Internal Shock

E. Troja, L. Piro, V. Vasileiou +5

Simultaneous Swift and Fermi observations of gamma-ray bursts (GRBs) offer a unique broadband view of their afterglow emission, spanning more than ten decades in energy. We present…