Speaker
Nepomuk Otte
(Georgia Institute of Technology)
Description
We present a development of a novel 11328 pixel silicon photomultiplier (SiPM) camera for use with a ground-based Cherenkov telescope with Schwarzschild-Couder optics as a possible mid-size telescope for the Cherenkov Telescope Array (CTA), which is the next generation very-high-energy gamma-ray observatory. . The finely pixelated camera samples air-shower images with more than twice the optical resolution of cameras that are used in current Cherenkov telescopes. Advantages of the higher resolution will be a better event reconstruction yielding improved background suppression and angular resolution of the reconstructed gamma-ray events, which is crucial in morphology studies of, for example, Galactic particle accelerators and the search for gamma-ray halos around extragalactic sources. Packing such a large number of pixels into an area of only half a square meter and having a fast readout directly attached to the back of the sensors is a challenging task. For the prototype camera development SiPMs from Hamamatsu with through silicon via (TSV) technology are used. We give a status report of the camera design and highlight a number of technological advancements that made this development possible.
Registration number following "ICRC2015-I/" | 731 |
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Collaboration | CTA |
Primary author
Nepomuk Otte
(Georgia Institute of Technology)
Co-authors
Akira Okumura
(Nagoya University)
Amanda Weinstein
(Iowa State University)
Caitlin Johson
(UCSC)
David Williams
(UCSC)
Hidaka Naoya
(Nagoya University)
Hiroyasu TAJIMA
(SLAC)
Hugh Dickinson
(Iowa State University)
Jonathan Biteau
(UC Santa Cruz)
Justin Vandenbroucke
(University of Wisconsin)
Kevin Meagher
(Georgia Tech)
Mr
Leonid Sapozhnikov
(SLAC)
Luigi Tibaldo
(SLAC)
Dr
Marcos Santander
(Barnard College, Columbia University)
Peter Karn
(University of Wisconsin - Madison)
Stefan Funk
(University Erlangen)
Thanh Nguyen
Dr
Tobias Jogler
(SLAC)