Given TeV emission similar to GRB 090510, CTA could detect short-GRB counterparts of gravitational-wave mergers even when follow-up starts more than an hour after the event.
The small size telescope projects for the Cherenkov Telescope Array
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abstract
The small size telescopes (SSTs), spread over an area of several square km, dominate the CTA sensitivity in the photon energy range from a few TeV to over 100 TeV, enabling for the detailed exploration of the very high energy gamma-ray sky. The proposed telescopes are innovative designs providing a wide field of view. Two of them, the ASTRI (Astrophysics con Specchi a Tecnologia Replicante Italiana) and the GCT (Gamma-ray Cherenkov Telescope) telescopes, are based on dual mirror Schwarzschild-Couder optics, with primary mirror diameters of 4 m. The third, SST-1M, is a Davies-Cotton design with a 4 m diameter mirror. Progress with the construction and testing of prototypes of these telescopes is presented. The SST cameras use silicon photomultipliers, with preamplifier and readout/trigger electronics designed to optimize the performance of these sensors for (atmospheric) Cherenkov light. The status of the camera developments is discussed. The SST sub-array will consist of about 70 telescopes at the CTA southern site. Current plans for the implementation of the array are presented.
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Gravitational-wave follow-up with CTA after the detection of GRBs in the TeV energy domain
Given TeV emission similar to GRB 090510, CTA could detect short-GRB counterparts of gravitational-wave mergers even when follow-up starts more than an hour after the event.