activity
19972023
most citedRadioactive 26Al and massive stars in the Galaxy

768 citations · 5.3k across the 81 of their papers we have counts for

collaborators

83 papers

astro-ph.HE2023★ 25 cited

The multi-wavelength view of shocks in the fastest nova V1674 Her

K. V. Sokolovsky, T. J. Johnson, S. Buson +41

Classical novae are shock-powered multi-wavelength transients triggered by a thermonuclear runaway on an accreting white dwarf. V1674 Her is the fastest nova ever recorded (time to…

astro-ph.IM2023★ 5 cited

The NectarCAM Timing System

F. Bradascio, H. Rueda, J. A. Barrio +14

NectarCAM is a Cherenkov camera which is going to equip the Medium-Sized Telescopes (MST) of the northern site of the Cherenkov Telescope Array Observatory (CTAO). NectarCAM is equ…

astro-ph.HE2022★ 44 cited

Fermi-LAT Gamma-ray Detection of the Recurrent Nova RS Ophiuchi during its 2021 Outburst

C. C. Cheung, T. J. Johnson, P. Jean +15

We report the Fermi-LAT gamma-ray detection of the 2021 outburst of the symbiotic recurrent nova RS Ophiuchi. In this system, unlike classical novae from cataclysmic binaries, the…

astro-ph.HE2022

Search for gamma-ray emission from a galactic supernova with the anticoincidence system of SPI

Mariona Caixach, Pierre Jean, Jordi Isern +1

The detection of the very early gamma-emission of a Type Ia supernova (SNIa) could provide a deep insight on the explosion mechanism and nature of the progenitor. However this has…

astro-ph.HE2022★ 13 cited

Measurement of Galactic Al with the Compton Spectrometer and Imager

Jacqueline Beechert, Thomas Siegert, John A. Tomsick +11

The Compton Spectrometer and Imager (COSI) is a balloon-borne compact Compton telescope designed to survey the 0.2-5 MeV sky. COSI's energy resolution of 0.2% at 1.8 MeV, sin…

astro-ph.IM2021★ 11 cited

The Compton Spectrometer and Imager Project for MeV Astronomy

John A. Tomsick, Steven E. Boggs, Andreas Zoglauer +33

The Compton Spectrometer and Imager (COSI) is a 0.2-5 MeV Compton telescope capable of imaging, spectroscopy, and polarimetry of astrophysical sources. Such capabilities are made p…