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4 September 2015 Toward the construction of a medium size prototype Schwarzschild-Couder telescope for CTA
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The construction of a prototype Schwarzschild-Couder telescope (pSCT) started in early June 2015 at the Fred Lawrence Whipple Observatory in Southern Arizona, as a candidate medium-sized telescope for the Cherenkov Telescope Array (CTA). Compared to current Davies-Cotton telescopes, this novel instrument with an aplanatic two-mirror optical system will offer a wider field-of-view and improved angular resolution. In addition, the reduced plate scale of the camera allows the use of highly-integrated photon detectors such as silicon photo multipliers. As part of CTA, this design has the potential to greatly improve the performance of the next generation ground-based observatory for very high-energy (E>60 GeV) gamma-ray astronomy. In this contribution we present the design and performance of both optical and alignment systems of the pSCT.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. Rousselle, K. Byrum, R. Cameron, V. Connaughton, M. Errando, S. Griffiths, V. Guarino, T. B. Humensky, P. Jenke, P. Kaaret, D. Kieda, M. Limon, I. Mognet, R. Mukherjee, D. Nieto, A. Okumura, A. Peck, A. Petrashyk, D. Ribeiro, B. Stevenson, V. Vassiliev, and P. Yu "Toward the construction of a medium size prototype Schwarzschild-Couder telescope for CTA", Proc. SPIE 9603, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VII, 960305 (4 September 2015);

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