An image-based array trigger for imaging atmospheric Cherenkov telescope arrays

0538358 - FZÚ 2021 RIV NL eng J - Journal Article
Dickinson, H. … Total 7 authors
An image-based array trigger for imaging atmospheric Cherenkov telescope arrays.
Nuclear Instruments & Methods in Physics Research Section A. Roč. 891, May (2018), s. 6-17. ISSN 0168-9002. E-ISSN 1872-9576
Research Infrastructure: CTA-CZ - 90046
Keywords : gamma-ray astronomy * array trigger * gamma-hadron separation
OECD category: Particles and field physics
Impact factor: 1.433, year: 2018
Method of publishing: Limited access
https://doi.org/10.1016/j.nima.2018.02.048

It is anticipated that forthcoming, next generation, atmospheric Cherenkov telescope arrays will include a number of medium-sized telescopes that are constructed using a dual-mirror Schwarzschild-Couder configuration. These telescopes will sample a wide (8 degrees) field of view using a densely pixelated camera comprising over 10(4) individual readout channels. A readout frequency congruent with the expected single-telescope trigger rates would result in substantial data rates. To ameliorate these data rates, a novel, hardware-level Distributed Intelligent Array Trigger (DIAT) is envisioned. A copy of the DIAT operates autonomously at each telescope and uses reduced resolution imaging data from a limited subset of nearby telescopes to veto events prior to camera readout and any subsequent network transmission of camera data that is required for centralized storage or aggregation. We present the results of Monte-Carlo simulations that evaluate the efficacy of a 'Parallax width' discriminator that can be used by the DIAT to efficiently distinguish between genuine gamma-ray initiated events and unwanted background events that are initiated by hadronic cosmic rays.
Permanent Link: http://hdl.handle.net/11104/0316779