activity
20152026
most citedThe First Fermi-LAT Solar Flare Catalog

59 citations · 213 across the 13 of their papers we have counts for

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Showing 2019Show all

11 papers · 1 filter

astro-ph.GA201915 cited

Localizing the -ray emitting region in the blazar TXS 2013+370

E. Traianou, T. P. Krichbaum, B. Boccardi +9

The -ray production mechanism and its localization in blazars are still a matter of debate. The main goal of this paper is to constrain the location of the high-energy emission…

astro-ph.GA201919 cited

Exploring the Morphology and Origins of the 4C 38.41 Jet

Juan Carlos Algaba, Bindu Rani, Sang-Sung Lee +3

We study the properties of the innermost jet of the flat spectrum radio quasar 1633+382 (4C~38.41) based on VLBI data from the radio monitoring observations of the Boston Universit…

astro-ph.HE2019

Fermi and Swift Observations of GRB 190114C: Tracing the Evolution of High-Energy Emission from Prompt to Afterglow

M. Ajello, M. Arimoto, M. Axelsson +147

We report on the observations of gamma-ray burst (GRB) 190114C by the Fermi Gamma-ray Space Telescope and the Neil Gehrels Swift Observatory. The early-time observations reveal mul…

astro-ph.IM2019

All-sky Medium Energy Gamma-ray Observatory: Exploring the Extreme Multimessenger Universe

Julie McEnery, Juan Abel Barrio, Ivan Agudo +182

The All-sky Medium Energy Gamma-ray Observatory (AMEGO) is a probe class mission concept that will provide essential contributions to multimessenger astrophysics in the late 2020s…

astro-ph.GA20191 cited

Origin and Evolution of the Multi-band Variability in the Flat Spectrum Radio Source 4C 38.41

Juan Carlos Algaba, Sang Sung Lee, Bindu Rani +13

The flat spectrum radio quasar 4C 38.41 showed a significant increase of its radio flux density during the period 2012 March - 2015 August which correlates with gamma-ray flaring a…

astro-ph.HE2019

Prospects for AGN Studies at Hard X-ray through MeV Energies

Eileen Meyer, Justin Finke, George Younes +7

This White Paper explores advances in the study of Active Galaxies which will be enabled by new observing capabilities at MeV energies (hard X-rays to gamma-rays; 0.1-1000 MeV), wi…