activity
20072026
most citedSearch for dark matter annihilations towards the inner Galactic halo from 10 years of observations with H.E.S.S

314 citations · 4.9k across the 151 of their papers we have counts for

collaborators
Showing 2022Show all

17 papers · 1 filter

astro-ph.HE2022★ 24 cited

Pulsar revival in neutron star mergers: multi-messenger prospects for the discovery of pre-merger coherent radio emission

A. J. Cooper, O. Gupta, Z. Wadiasingh +5

We investigate pre-merger coherent radio emission from neutron star mergers arising due to the magnetospheric interaction between compact objects. We consider two plausible radiati…

astro-ph.HE2022★ 1 cited

Magnetar spin-down glitch clearing the way for FRB-like bursts and a pulsed radio episode

G. Younes, M. G. Baring, A. K. Harding +16

Magnetars are a special subset of the isolated neutron star family, with X-ray and radio emission mainly powered by the decay of their immense magnetic fields. Many attributes of m…

astro-ph.HE2022★ 58 cited

Evidence for an abundant old population of Galactic ultra long period magnetars and implications for fast radio bursts

P. Beniamini, Z. Wadiasingh, J. Hare +3

Two recent discoveries, namely PSR J0901-4046 and GLEAM-X J162759.5-523504.3 (hereafter GLEAM-X J1627), have corroborated an extant population of radio-loud periodic sources with l…

astro-ph.HE2022★ 12 cited

High-Energy Photon Opacity in the Twisted Magnetospheres of Magnetars

Kun Hu, Matthew G. Baring, Alice K. Harding +1

Magnetars are neutron stars characterized by strong surface magnetic fields generally exceeding the quantum critical value of 44.1 TeraGauss. High-energy photons propagating in the…

astro-ph.HE2022★ 1 cited

Snowmass 2021 Cosmic Frontier White Paper: The Dense Matter Equation of State and QCD Phase Transitions

Slavko Bogdanov, Emmanuel Fonseca, Rahul Kashyap +26

Our limited understanding of the physical properties of matter at ultra-high density, high proton/neutron number asymmetry, and low temperature is presently one of the major outsta…

astro-ph.HE2022★ 117 cited

The Radius of PSR J0740+6620 from NICER with NICER Background Estimates

Tuomo Salmi, Serena Vinciguerra, Devarshi Choudhury +15

We report a revised analysis for the radius, mass, and hot surface regions of the massive millisecond pulsar PSR J0740+6620, studied previously with joint fits to NICER and XMM-New…

astro-ph.HE2022★ 27 cited

The discovery of the 528.6 Hz accreting millisecond X-ray pulsar MAXI J1816-195

Peter Bult, Diego Altamirano, Zaven Arzoumanian +15

We present the discovery of 528.6 Hz pulsations in the new X-ray transient MAXI J1816-195. Using NICER, we observed the first recorded transient outburst from the neutron star low-…

astro-ph.IM2022★ 96 cited

The All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) Mission Concept

Regina Caputo, Marco Ajello, Carolyn Kierans +52

The All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) is designed to identify and characterize gamma rays from extreme explosions and accelerators. The main science th…

astro-ph.HE2022★ 11 cited

Search for new cosmic-ray acceleration sites within the 4FGL catalog Galactic plane sources

LAT Collaboration, S. Abdollahi, F. Acero +117

Cosmic rays are mostly composed of protons accelerated to relativistic speeds. When those protons encounter interstellar material, they produce neutral pions which in turn decay in…

astro-ph.HE2022★ 50 cited

A Gamma-ray Pulsar Timing Array Constrains the Nanohertz Gravitational Wave Background

M. Ajello, W. B. Atwood, L. Baldini +129

After large galaxies merge, their central supermassive black holes are expected to form binary systems whose orbital motion generates a gravitational wave background (GWB) at nanoh…

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

Limits on the hard X-ray emission from the periodic fast radio burst FRB 180916.J0158+65

Sibasish Laha, Zorawar Wadiasingh, Tyler Parsotan +11

FRB 180916.J0158+65 is one of the nearest, periodically repeating, and actively bursting fast radio burst (FRB) which has been localized to the outskirts of a spiral galaxy. In thi…

astro-ph.HE2022★ 1 cited

Simultaneous view of the FRB~180301 with FAST and NICER during a bursting phase

Sibasish Laha, George Younes, Zorawar Wadiasingh +16

FRB180301 is one of the most actively repeating fast radio bursts (FRBs) which has shown polarization angle changes in its radio burst emission, an indication for their likely orig…

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★ 17 cited

The Fundamental Plane Relation for Gamma-Ray Pulsars Implied by 4FGL

Constantinos Kalapotharakos, Zorawar Wadiasingh, Alice K. Harding +1

We explore the validity of the recently reported fundamental plane (FP) relation of gamma-ray pulsars using 190 pulsars included in the latest 4FGL-DR3 catalog. This sample number…

astro-ph.HE2022★ 28 cited

Pulse Peak Migration during the Outburst Decay of the Magnetar SGR 1830-0645: Crustal Motion and Magnetospheric Untwisting

G. Younes, S. K. Lander, M. G. Baring +12

Magnetars, isolated neutron stars with magnetic field strengths typically ~G, exhibit distinctive months-long outburst epochs during which strong evolution of soft…

astro-ph.HE2022★ 8 cited

X-ray burst and persistent emission properties of the magnetar SGR 1830-0645 in outburst

G. Younes, C. -P. Hu, K. Bansal +18

We report on NICER X-ray monitoring of the magnetar SGR 1830-0645 covering 223 days following its October 2020 outburst, as well as Chandra and radio observations. We present the m…