activity
20052026
most citedThe Spectral Energy Distribution of Fermi bright blazars

1k citations · 1.7k across the 17 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE2026

GRB 220706A: a gamma-ray burst with a month-long engine and a luminous supernova

Benjamin P. Gompertz, Nusrin Habeeb, Dheeraj R. Pasham +30

While the progenitors of many long gamma-ray bursts (GRBs) are well established as the core collapse of very massive, envelope-stripped, rapidly-rotating stars, it has been suggest…

astro-ph.HE2025

X-ray Observations of Nova Scorpii 2023 (V1716 Sco) in Outburst

John Worley, Marina Orio, Andrej Dobrotka +5

Nova Scorpii 2023 was first detected as a luminous supersoft X-ray source (SSS) 93 days after outburst and continued emitting soft X-rays for over two months, until it was too clos…

astro-ph.HE2025

Constraints on diffuse X-ray Emission from the TeV halo Candidate HESS J1813-126

David Guevel, Kim L Page, Kaya Mori +2

Extended regions of very high energy -ray emission associated with middle-aged pulsars have been found by -ray observatories. These regions, called TeV halos or pulsar halos,…

astro-ph.HE2025

Prompt Periodicity in the GRB 211211A Precursor: Black-hole or magnetar engine?

Gavin P. Lamb, Thomas Baxter, Conor M. B. Omand +18

The merger origin long GRB 211211A was a class (re-)defining event. A precursor was identified with a s separation from the main burst, as well as a claimed candidate quas…

astro-ph.HE2024★ 9 cited

Mixing of hot shocked plasma with cold gas in Nova YZ Ret 2020

Sharon Mitrani, Ehud Behar, Jeremy J. Drake +5

The origin of bright X-ray emission lines that appear late in a nova eruption remains largely a puzzle. We present two high-resolution X-ray grating spectra of the classical nova Y…

astro-ph.HE2024

Simultaneous multi-wavelength observations of the repeating fast radio burst FRB 20190520B with Swift and FAST

Zhen Yan, Wenfei Yu, Kim L. Page +8

Among several dozen known repeating Fast radio bursts (FRBs), those precisely localized offer the best opportunities to explore their multi-wavelength counterparts, which are key t…

astro-ph.HE2023★ 1 cited

Observing the launch of an Eddington wind in the luminous Seyfert galaxy PG1211+143

Ken Pounds, Kim Page

The luminous narrow line Seyfert galaxy PG1211+143 was the first non-BAL AGN to reveal a powerful ionized wind, based on early observations with ESA's XMM-Newton X-ray Observatory.…

astro-ph.HE2020★ 27 cited

Chandra High Energy Transmission Gratings Spectra of V3890 Sgr

Marina Orio, Jeremy J. Drake, Jan-Uwe Ness +13

The recurrent nova (RN) V3890 Sgr was observed during the 7th day after the onset of its most recent outburst, with the Chandra ACIS-S camera and High Energy Transmission Gratings…

astro-ph.HE2010★ 243 cited

The unusual X-ray emission of the short Swift GRB 090515: Evidence for the formation of a magnetar?

A. Rowlinson, P. T. O'Brien, N. R. Tanvir +16

The majority of short gamma-ray bursts (SGRBs) are thought to originate from the merger of compact binary systems collapsing directly to form a black hole. However, it has been pro…

astro-ph.HE2010★ 32 cited

GRB 090926A and Bright Late-time Fermi LAT GRB Afterglows

C. A. Swenson, A. Maxham, P. W. A. Roming +10

GRB 090926A was detected by both the GBM and LAT instruments on-board the Fermi Gamma-Ray Space Telescope. Swift follow-up observations began ~13 hours after the initial trigger. T…