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2016

Large Size Telescope Report

Mazin, D., Cortina, J., Teshima, M. et al.

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The Cherenkov Telescope Array (CTA) observatory will be deployed over two sites in the two hemispheres.

Both sites will be equipped with four Large Size Telescopes (LSTs), which are crucial to achieve the science goals of CTA in the 20-200 GeV energy range.
Each LST is equipped with a primary tessellated mirror dish of 23 m diameter, supported by a structure made mainly of carbon fibre reinforced plastic tubes and aluminum joints.
This solution guarantees light weight (around 100 tons), essential for fast repositioning to any position in the sky in <20 seconds.

Large Size Telescope Report · Around

Built on

S. Funk, J. A. Hinton, and CTA Consortium, “Comparison of Fermi-LAT and CTA in the region between 10-100 GeV,” Astroparticle Physics
2013
Earlier work this paper cites.
J. Cortina, M. Teshima, and f. t. CTA Consortium, “Status of the Cherenkov Telescope Array’s Large Size Telescopes,” In Proc. of the 34th International Cosmic Ray Conference (ICRC2015), The Hague, The Netherlands
2015
Earlier work this paper cites.

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M. Hayashida, K. Noda, M. Teshima, et al
2015
Cited alongside, same era.
J. Glicenstein, O. Abril, J. Barrio, et al
2015
Cited alongside, same era.

Then

LST team for the CTA Consortium, “Large Size Telescope Technical Design Report, v3.0,” Tech. Rep. LST-TDR/140408, available at http://cta-observatory.org/, Feb. 2016
2016
Closest in time.
J. Aleksić, S. Ansoldi, L. A. Antonelli, et al
2016
Closest in time.

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