activity
20122026
most citedThe All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) Mission Concept

96 citations · 395 across the 26 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

12 papers · 1 filter

astro-ph.HE2026

Detectability of Polarized Gamma-ray Emission from Blazar Flares with COSI

Garrett A. Latiolais, Jorge Otero-Santos, Michela Negro +18

We investigate the detectability of polarized gamma-ray emission from blazar flares with the Compton Spectrometer and Imager (COSI). Using 17 years of Fermi Large Area Telescope ob…

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

Characterizing Candidate Blazar Counterparts of the Ultra-High-Energy Event KM3-230213A

KM3NeT Collaboration, MessMapp Group, LAT Collaboration +13

High-energy astrophysical neutrinos serve as crucial messengers for understanding hadronic acceleration processes and identifying the origins of cosmic rays, with blazars among the…

astro-ph.HE2023★ 19 cited

The Compton Spectrometer and Imager

John A. Tomsick, Steven E. Boggs, Andreas Zoglauer +72

The Compton Spectrometer and Imager (COSI) is a NASA Small Explorer (SMEX) satellite mission in development with a planned launch in 2027. COSI is a wide-field gamma-ray telescope…

astro-ph.HE2023★ 7 cited

The cosipy library: COSI's high-level analysis software

Israel Martinez-Castellanos, Savitri Gallego, Chien-You Huang +72

The Compton Spectrometer and Imager (COSI) is a selected Small Explorer (SMEX) mission launching in 2027. It consists of a large field-of-view Compton telescope that will probe wit…

astro-ph.HE2023★ 40 cited

UV/Optical disk reverberation lags despite a faint X-ray corona in the AGN Mrk 335

Erin Kara, Aaron J. Barth, Edward M. Cackett +37

We present the first results from a 100-day Swift, NICER and ground-based X-ray/UV/optical reverberation mapping campaign of the Narrow-Line Seyfert 1 Mrk 335, when it was in an un…

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

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.HE2021★ 1 cited

Modeling and Simulations of TXS 0506+056 Neutrino Events in the MeV Band

Tiffany R. Lewis, Christopher M. Karwin, Tonia M. Venters +5

Neutrino detections identified with multiwavelength blazar spectra represent the first $\g$-ray-neutrino multimessenger signals. The blazar, TXS 0506+056 is also unusual in its spe…

astro-ph.HE2021

Radiation and Polarization Signatures from Magnetic Reconnection in Relativistic Jets--II. Connection with -rays

Haocheng Zhang, Xiaocan Li, Dimitrios Giannios +5

It is commonly believed that blazar jets are relativistic magnetized plasma outflows from supermassive black holes. One key question is how the jets dissipate magnetic energy to ac…

astro-ph.HE2016★ 29 cited

Time-Dependent Electron Acceleration in Blazar Transients: X-Ray Time Lags and Spectral Formation

Tiffany R. Lewis, Peter A. Becker, Justin D. Finke

Electromagnetic radiation from blazar jets often displays strong variability, extending from radio to -ray frequencies. In a few cases, this variability has been characterized u…

astro-ph.HE2012

Infrahumps detected in Kepler light curve of V1504 Cygni

Robert Coyne, Ashwin Shenoy, Glen MacLachlan +6

We present a power spectral density analysis of the short cadence Kepler data for the cataclysmic variable V1504 Cygni. We identify three distinct periods: the orbital period (1.66…