activity
19932026
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 8.6k across the 105 of their papers we have counts for

collaborators

107 papers

astro-ph.IM2026★ 14 cited

The Vera C. Rubin Observatory Data Preview 1

Vera C Rubin Observatory Team, Tatiana Acero Cuellar, Emily Acosta +325

We present Rubin Data Preview 1 DP1, the first data from the NSF DOE Vera C Rubin Observatory, comprising raw and calibrated single epoch images, coadds, difference images, detecti…

astro-ph.HE2025

High-energy variability of the gravitationally lensed blazar PKS 1830-211

Sarah M. Wagner, Jeffrey D. Scargle, Greg Madejski +4

The production site and process responsible for the highly variable high-energy emission observed from blazar jets are still debated. Gravitational lenses can be used as microscope…

astro-ph.IM2025★ 1 cited

The GammaTPC Gamma-Ray Telescope Concept

Tom Shutt, Bahrudin Trbalic, Eric Charles +8

We present GammaTPC, a transformative 0.1-10 MeV -ray instrument concept featuring a tracker using a liquid argon time projection chamber (LAr TPC) technology with the novel GAM…

astro-ph.HE2023★ 3 cited

The High Energy X-ray Probe (HEX-P): the most powerful jets through the lens of a superb X-ray eye

Lea Marcotulli, Marco Ajello, Markus Böttcher +20

A fraction of the active supermassive black holes at the centers of galaxies in our Universe are capable of launching extreme kiloparsec-long relativistic jets. These jets are know…

astro-ph.HE2022★ 8 cited

New Identifications and Multi-wavelength Properties of Extragalactic Fermi Gamma-Ray Sources in the SPT-SZ Survey Field

Lizhong Zhang, Joaquin D. Vieira, Marco Ajello +5

The fourth Fermi Large Area Telescope (LAT) catalog (4FGL) contains 5064 -ray sources detected at high significance, but 26% of them still lack associations at other wavelengths…

astro-ph.HE2021★ 10 cited

Statistical properties of flux variations in blazar light curves at GeV and TeV energies

Sarah M. Wagner, Paul R. Burd, Daniela Dorner +23

Despite numerous detections of individual flares, the physical origin of the rapid variability observed from blazars remains uncertain. Using Bayesian blocks and the Eisenstein-Hut…