Characterisation and Testing of CHEC-M - a camera prototype for the Small-Sized Telescopes of the Cherenkov Telescope Array
arXiv:1806.11308 · doi:10.1016/j.nima.2018.06.078
Abstract
The Compact High Energy Camera (CHEC) is a camera design for the Small-Sized Telescopes (SSTs; 4 m diameter mirror) of the Cherenkov Telescope Array (CTA). The SSTs are focused on very-high-energy -ray detection via atmospheric Cherenkov light detection over a very large area. This implies many individual units and hence cost-effective implementation. CHEC relies on dual-mirror optics to reduce the plate-scale and make use of 6 6 mm pixels, leading to a low-cost (150 kEuro), compact (0.5 m 0.5 m), and light (45 kg) camera with 2048 pixels providing a camera FoV of 9 degrees. The electronics are based on custom TARGET (TeV array readout with GSa/s sampling and event trigger) ASICs and FPGAs sampling incoming signals at a gigasample per second, with flexible camera-level triggering within a single backplane FPGA. CHEC is designed to observe in the -ray energy range of 1300 TeV, and at impact distances up to 500 m. To accommodate this and provide full flexibility for later data analysis, full waveforms with 96 samples for all 2048 pixels can be read out at rates up to 900 Hz. The first prototype, CHEC-M, based on multi-anode photomultipliers (MAPMs) as photosensors, was commissioned and characterised in the laboratory and during two measurement campaigns on a telescope structure at the Paris Observatory in Meudon. In this paper, the results and conclusions from the laboratory and on-site testing of CHEC-M are presented. They have provided essential input on the system design and on operational and data analysis procedures for a camera of this type. A second full-camera prototype based on Silicon photomultipliers (SiPMs), addressing the drawbacks of CHEC-M identified during the first prototype phase, has already been built and is currently being commissioned and tested in the laboratory.
References in corpus (16)
- Design Concepts for the Cherenkov Telescope Array
- The Status of the H.E.S.S. Project
- VERITAS: the Very Energetic Radiation Imaging Telescope Array System
- Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory
- Monte Carlo design studies for the Cherenkov Telescope Array
- Characterization of Three High Efficiency and Blue Sensitive Silicon Photomultipliers
- Wide field aplanatic two-mirror telescopes for ground-based gamma-ray astronomy
- The optical system of the H.E.S.S. imaging atmospheric Cherenkov telescopes, Part II: mirror alignment and point spread function
- TARGET: A multi-channel digitizer chip for very-high-energy gamma-ray telescopes
- Performance Verification of the FlashCam Prototype Camera for the Cherenkov Telescope Array
- TARGET: A Digitizing And Trigger ASIC For The Cherenkov Telescope Array
- TARGET 5: a new multi-channel digitizer with triggering capabilities for gamma-ray atmospheric Cherenkov telescopes
- The first GCT camera for the Cherenkov Telescope Array
- Extending the Sensitivity of Air Cerenkov Telescopes
- Calibration Techniques for VERITAS
- Inauguration and First Light of the GCT-M Prototype for the Cherenkov Telescope Array