
VERITAS
SMITHSONIAN ASTROPHYSICAL OBSERVATORY
The VERITAS Collaboration (Very Energetic Radiation Imaging Telescope Array System) is a leading gamma-ray astronomy research facility located at the Fred Lawrence Whipple Observatory.
DOTI designs and manufactures precision optical mirrors and advanced optical coatings used in the facility’s four 12-meter telescope mirror arrays. These tessellated mirror systems play a critical role in enabling high-sensitivity observations for gamma-ray telescopes and astrophysics research.
The VERITAS team utilizes these high-performance optical components to study a wide range of cosmic phenomena, including black holes, pulsars, X-ray binaries, supernova remnants, globular clusters, galaxies and galaxy clusters, dark matter, and gamma-ray bursts. DOTI’s expertise in optical fabrication, mirror polishing, and coating technologies supports ongoing advancements in astroparticle physics and astronomical instrumentation.
Displays & Optical Technologies, Inc. has been a trusted supplier of precision optical mirrors for the VERITAS project for over two decades. Below are selected articles and journals highlighting the groundbreaking research conducted by the VERITAS team.

Articles

Mirror Facets for VERITAS Telescopes
E. Roache, R. Irvin, J. S. Perkins, K. Harris, A. Falcone, J. Finley, and T. Weekes
Smithsonian Astrophysical Observatory

VERITAS, 1ES 1218 + 30.4 and the Extragalactic Background Light
Luis Valcarcel
Centre for High-Energy Physics
McGill University
Welcome to VERTIAS
University of Arizona
Mirrors and Lasers in Astroparticle Physics Infrastructures
Center for Astrophysics | Harvard & Smithsonian
The First VERITAS Telescope
Harvard
VERITAS Telescopes Help Solve 100-Year-Old Mystery: The Origin of Cosmic Rays
Center for Astrophysics | Harvard & Smithsonian
VERITAS and OSG Explore Extreme Window into the Universe
The OSG Consortium

Mirrors and Lasers in Astroparticle Physics Infrastructures
2nd ASPERA Technology Forum
EGO/Virgo Site (Cascina), Pisa





