activity
20142026
most citedChromatic periodic activity down to 120 MHz in a Fast Radio Burst

131 citations · 458 across the 18 of their papers we have counts for

collaborators

19 papers

astro-ph.HE2026

Fermi-LAT Gamma-ray Emission Discovered from the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud

Jordan Eagle

A second extragalactic pulsar wind nebula (PWN) is discovered in the MeV-GeV band using the Fermi-LAT. Faint, point-like gamma-ray emission is detected at the location of the compo…

astro-ph.HE2025

Low-energy Radio Bursts from Magnetar XTE J1810197: Implications for Fast Radio Bursts

Banshi Lal, Yogesh Maan, Moaz Abdelmaguid +3

Magnetars are the leading candidate sources of fast radio bursts (FRBs). However, the observational probes of the connections between magnetars and FRBs are severely limited by the…

astro-ph.HE2025

The Timing Evolution of the Magnetar Swift J1818.0-1607 During a Period of Reduced Activity

Moaz Abdelmaguid, Paulo C. C. Freire, Joseph D. Gelfand +3

We report results from an observational campaign of the radio-loud magnetar Swift J1818.0-1607 using the Green Bank Telescope (GBT) at 2.0 GHz, which began in November 2021 during…

astro-ph.HE2023★ 8 cited

Broadband X-ray Spectroscopy of the Pulsar Wind Nebula in HESS J1640-465

Moaz Abdelmaguid, Joseph D Gelfand, Eric Gotthelf +1

We present updated measurements of the X-ray properties of the pulsar wind nebula associated with the TeV -ray source HESS J1640-465 derived from Chandra & NuSTAR data. We repor…

astro-ph.HE2023★ 6 cited

Fermi-LAT Gamma-ray Emission Discovered from the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud

Jordan Eagle, Daniel Castro, Peter Mahhov +7

We report the second extragalactic pulsar wind nebula (PWN) to be detected in the MeV-GeV band by the Fermi-LAT, located within the Large Magellanic Cloud (LMC). The only other kno…

astro-ph.HE2023★ 5 cited

New upper limits on low-frequency radio emission from isolated neutron stars with LOFAR

Inés Pastor-Marazuela, Samayra M. Straal, Joeri van Leeuwen +1

Neutron stars that show X-ray and -ray pulsed emission must, somewhere in the magnetosphere, generate electron-positron pairs. Such pairs are also required for radio emission, b…