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

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19 papers · 1 filter

astro-ph.HE2025

Future Space-based Gamma-ray Pulsar Timing Arrays

Matthew Kerr, Zorawar Wadiasingh, Adrien Laviron +3

Radio pulsar timing array (PTA) experiments using millisecond pulsars (MSPs) are beginning to detect nHz gravitational waves (GWs). MSPs are bright GeV gamma-ray emitters, and all-…

astro-ph.HE2025★ 8 cited

The Radius of PSR J0437-4715 from NICER Data

M. C. Miller, A. J. Dittmann, I. M. Holt +12

Neutron star Interior Composition Explorer (NICER) data have been used to estimate the masses and radii of the rotation-powered millisecond pulsars PSR J00300451, PSR J074066…

astro-ph.HE2025

NICER Magnetar Burst Catalog

Che-Yen Chu, Chin-Ping Hu, Teruaki Enoto +13

In this paper, we present a comprehensive catalog of short bursts from magnetars based on eight years of NICER observations. A total of 1130 bursts were identified from 14 sources,…

astro-ph.HE2025

Searching for Long-Period Radio Transients in ASKAP EMU Data with 10-Second Imaging

Yu Wing Joshua Lee, Yuanming Wang, Manisha Caleb +10

Long-period radio transients (LPTs) are a recently identified phenomenon that challenge our current understanding of compact objects and coherent radio emission mechanisms. These o…

astro-ph.HE2025★ 3 cited

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.HE2025

Fast X-ray Transient Detection with AXIS: application to Magnetar Giant Flares

Michela Negro, Zorawar Wadiasingh, George Younes +6

Magnetar giant flares (MGFs) are among the most luminous high-energy transients in the local universe, consisting of a short, intense MeV gamma-ray spike followed by a softer, puls…

astro-ph.HE2025★ 4 cited

Vacuum birefringence and the polarized X-ray emission from a radio magnetar

Rachael E. Stewart, Hoa Dinh Thi, George Younes +13

Magnetars are isolated neutron stars with exceptionally strong surface fields exceeding G. Their bright X-ray emission probes physical regimes in which quantum electrodyn…

astro-ph.HE2025

Testing Magnetic Field Configurations in Spider Pulsar PSR J1723-2837 with IXPE

Michela Negro, Haocheng Zhang, Niccolò Di Lalla +4

We present the first X-ray polarimetry observations of a redback millisecond pulsar binary, PSR J1723-2837, with the Imaging X-ray Polarimetry Explorer (IXPE). We conduct a spectro…

astro-ph.HE2025

Pair Cascades in Magnetar Magnetospheres

Alice K. Harding, Zorawar Wadiasingh, Matthew G. Baring

Resonant inverse Compton scattering (RICS) of soft thermal photons by relativistic particles on closed magnetic field loops has been proposed to explain the hard emission observed…

astro-ph.HE2025

Towards Modelling AR Sco: Calibration -- Reproducing High-Energy Pulsar Emission and Testing Convergence to Aristotelian Electrodynamics

Louis Du Plessis, Christo Venter, Alice K. Harding +2

In recent years, kinetic simulations have been crucial to further our understanding of pulsar electrodynamics. Yet, due to the large-scale separation between the gyro-period vs the…

astro-ph.HE2025

A coherent radio burst from an X-ray neutron star in the Carina Nebula

K. M. Rajwade, J. Tian, G. Younes +10

The neutron star zoo comprises several sub-populations that range from energetic magnetars and thermally emitting X-ray neutron stars to radio-emitting pulsars. Despite studies ove…

astro-ph.HE2025★ 2 cited

Puzzling Variation of Gamma Rays from the Sun over the Solar Cycle Revealed with Fermi-LAT

A. Acharyya, A. Adelfio, M. Ajello +100

The steady-state gamma-ray emission from the Sun is thought to consist of two emission components due to interactions with Galactic cosmic rays: (1) a hadronic disk component, and…

astro-ph.HE2025★ 1 cited

Multidisciplinary Science in the Multimessenger Era

Eric Burns, Christopher L. Fryer, Ivan Agullo +82

Astrophysical observations of the cosmos allow us to probe extreme physics and answer foundational questions on our universe. Modern astronomy is increasingly operating under a hol…

astro-ph.HE2025

Rapid Spectral Evolution of SGR 1935+2154 During its 2022 Outburst

Chin-Ping Hu, Zorawar Wadiasingh, Wynn C. G. Ho +9

During the 2022 outburst of SGR 1935+2154, a Fast-Radio-Burst-like event (FRB 20221014A) and X-ray activities occurred between two spin-up glitches, suggesting these glitches may c…

astro-ph.HE2025★ 6 cited

Magnetosphere Evolution and Precursor-Driven Electromagnetic Signals in Merging Binary Neutron Stars

Dimitrios Skiathas, Constantinos Kalapotharakos, Zorawar Wadiasingh +3

We detail new force-free simulations to investigate magnetosphere evolution and precursor electromagnetic (EM) signals from binary neutron stars. Our simulations fully follow a rep…

astro-ph.HE2025

Irradiated Pulsar Planets and Companions as 511 keV Positron Annihilation Line Sources

Zachary Metzler, Zorawar Wadiasingh

Millisecond pulsars (MSPs) are prolific GeV emitters, and nearly 80\% of Fermi-LAT MSPs reside in compact binaries. We demonstrate that the companions in these compa…

astro-ph.HE2025

Timing and Spectral Evolution of the Magnetar 1E 1841-045 in Outburst

G. Younes, S. K. Lander, M. G. Baring +19

We present the timing and spectral analyses of the NICER, NuSTAR, and IXPE observations of the magnetar 1E 1841-045 covering 82 days following its August 2024 bursting activity as…

astro-ph.HE2025★ 34 cited

The emission of interpulses by a 6.45-hour period coherent radio transient

Y. W. J. Lee, M. Caleb, Tara Murphy +29

Long-period radio transients are a novel class of astronomical objects characterised by prolonged periods ranging from 18 minutes to 54 minutes. They exhibit highly polarised, cohe…

astro-ph.HE2025★ 2 cited

Pioneering High-Speed Pulsar Parameter Estimation Using Convolutional Neural Networks

Greg Olmschenk, Emily Broadbent, Constantinos Kalapotharakos +5

Accurate thermal emission models of neutron stars are essential for constraining the dense matter equation of state. However, incorporating realistic magnetic field structures is c…