activity
20162022
most citedDemonstration of stellar intensity interferometry with the four VERITAS telescopes

63 citations · 228 across the 16 of their papers we have counts for

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Showing astro-ph.HEShow all

24 papers · 1 filter

astro-ph.HE2021

VERITAS contributions to the 37th International Cosmic Ray Conference

C. B. Adams, A. Archer, W. Benbow +58

Compilation of papers presented by the VERITAS Collaboration at the 37th International Cosmic Ray Conference (ICRC), held July 12 through July 23, 2021 (online) in Berlin, Germany.

astro-ph.HE20211 cited

VTSCat - The VERITAS Catalog of Gamma Ray Observations

Sameer Patel, Gernot Maier, Philip Kaaret

We present a catalog of results of gamma-ray observations made by VERITAS, published from 2008 to 2020. VERITAS is a ground based imaging atmospheric Cherenkov telescope observator…

astro-ph.HE202128 cited

ASASSN-15hy: an under-luminous, red 03fg-like type Ia supernova

J. Lu, C. Ashall, E. Y. Hsiao +33

We present photometric and spectroscopic observations of the 03fg-like type Ia supernova (SN Ia) ASASSN-15hy from the ultraviolet (UV) to the near-infrared (NIR). ASASSN-15hy share…

astro-ph.HE20213 cited

An Archival Search for Neutron-Star Mergers in Gravitational Waves and Very-High-Energy Gamma Rays

C. B. Adams, W. Benbow, A. Brill +59

The recent discovery of electromagnetic signals in coincidence with neutron-star mergers has solidified the importance of multimessenger campaigns in studying the most energetic as…

astro-ph.HE2021

VERITAS Observations of the Galactic Center Region at Multi-TeV Gamma-Ray Energies

C. B. Adams, W. Benbow, A. Brill +56

The Galactic Center (GC) region hosts a variety of powerful astronomical sources and rare astrophysical processes that emit a large flux of non-thermal radiation. The inner 375 pc…

astro-ph.HE20219 cited

SN 2013ai: a link between hydrogen-rich and hydrogen-poor core-collapse supernovae

S. Davis, P. J. Pessi, M. Fraser +33

We present a study of optical and near-infrared (NIR) spectra along with the light curves of SN 2013ai. These data range from discovery until 380 days after explosion. SN 2013ai is…