Science with the Cherenkov Telescope Array by Acharya, B, Agudo, I, Batista, R, Armstrong, T, Cotter, G, Franco, A, Morris, P, Sarkar, S, Watson, J, Consortium, TCTA

“…The Cherenkov Telescope Array, CTA, will be the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond. …”

FRAM for the Cherenkov Telescope Array: an update by Janeček Petr, Ebr Jan, Blažek Jiří, Prouza Michael, Mašek Martin, Eliášek Jiří

“…The Cherenkov Telescope Array (CTA) is a project to build a new generation ground-based gammaray observatory. …”
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Design Concepts for the Cherenkov Telescope Array by Consortium, TCTA

The GCT camera for the Cherenkov Telescope Array by Lapington, J, Abchiche, A, Allan, D, Amans, J, Armstrong, T, Balzer, A, Berge, D, Boisson, C, Bousquet, J, Bose, R, Brown, A, Bryan, M, Buchholtz, G, Buckley, J, Chadwick, P, Costantini, H, Cotter, G, Daniel, M, De Franco, A, De Frondat, F, Dournaux, J, Dumas, D, Ernenwein, J, Fasola, G, Funk, S, Gironnet, J, Graham, J, Greenshaw, T, Hervet, O, Hidaka, N, Hinton, J, Huet, J, Jankowsky, D, Jegouzo, I, Jogler, T, Kawashima, T, Kraus, M, Laporte, P, Leach, S, Lefaucheur, J, Markoff, S, Melse, T, Minaya, I, Mohrmann, L, Molyneux, P, Moore, P, Nolan, S, Okumura, A, Osborne, J, Parsons, R, Rosen, S, Ross, D, Rowell, G, Rulten, C, Sato, Y, Sayede, F, Schmoll, J, Schoorlemmer, H, Servillat, M, Sol, H, Stamatescu, V, Stephan, M, Stuik, R, Sykes, J, Tajima, H, Thornhill, J, Tibaldo, L, Trichard, C, Varner, G, Vink, J, Watson, J, White, R, Yamane, N, Zech, A, Zink, A, Zorn, J

“… The Gamma Cherenkov Telescope (GCT) is one of the designs proposed for the Small Sized Telescope (SST) section of the Cherenkov Telescope Array (CTA). The GCT uses dual-mirror optics, resulting in a compact telescope with good image quality and a large field of view with a smaller, more economical, camera than is achievable with conventional single mirror solutions. …”

The Cherenkov Telescope Array Observatory workflow management system by Arrabito Luisa, Bregeon Johan, Faure Alice, Gueta Orel, Pigoux Natthan, Tsaregorodtsev Andrei

“…The Cherenkov Telescope Array Observatory (CTAO) is the next generation ground-based observatory for gamma-ray astronomy at very high energies. …”
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The Cherenkov Telescope Array Science Goals and Current Status by The CTA Consortium, Ong Rene A.

“…The Cherenkov Telescope Array (CTA) is the major ground-based gamma-ray observatory planned for the next decade and beyond. …”
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Site Characterization of the Northern Site of the Cherenkov Telescope Array by Gaug Markus, Font Lluís, Maggio Camilla

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Calibration and analysis of the GCT camera for the Cherenkov Telescope Array by Watson, J

“…The Imaging Atmospheric Cherenkov Telescope (IACT) technique enables the probing of the universe at TeV energies through the detection of these Cherenkov showers. The Cherenkov Telescope Array (CTA) will represent the next leap forward in gamma-ray astronomy, improving on the sensitivity of current IACTs by a factor of 10, encompassing energies from 20 GeV to 300TeV, and operating as the first open observatory in this field. …”

Optical spectroscopy of blazars for the Cherenkov Telescope Array – II by Kasai, E, Goldoni, P, Pita, S, Williams, DA, Max-Moerbeck, W, Hervet, O, Cotter, G, Backes, M, Boisson, C, Becerra González, J, Barres de Almeida, U, D’Ammando, F, Fallah Ramazani, V, Lindfors, E

The gamma-ray Cherenkov telescope for the Cherenkov telescope array by Tibaldo, L, Abchiche, A, Allan, D, Amans, J, Armstrong, T, Balzer, A, Bergey, D, Boisson, C, Bousquet, J, Brown, A, Bryan, M, Buchholtz, G, Chadwick, P, Costantini, H, Cotter, G, Daniels, M, De Franco, A, De Frondat, F, Dournaux, J, Dumas, D, Ernenwein, J, Fasola, G, Funk, S, Gironnet, J, Graham, J, Greenshaws, T, Hervet, O, Hidaka, N, Hintoni, J, Huet, J, Jankowsky, D, Jegouzo, I, Jogler, T, Kraus, M, Lapington, J, Laporte, P, Lefaucheur, J, Markoff, S, Melse, T, Mohrmann, L, Molyneux, P, Nolan, S, Okumura, A, Osborne, J, Parsons, R, Rosen, S, Ross, D, Rowell, G, Rulten, C, Sato, Y, Sayede, F, Schmoll, J, Schoorlemmer, H, Servillat, M, Sol, H, Stamatescu, V, Stephan, M, Stuik, R, Sykes, J, Tajima, H, Thornhill, J, Trichard, C, Vink, J, Watson, J, White, R, Yamane, N, Zech, A, Zink, A, Zorn, J, Consortium, CTA

“…The Cherenkov Telescope Array (CTA) is a forthcoming ground-based observatory for very-high-energy gamma rays. …”

Dark matter line searches with the Cherenkov Telescope Array by Abe, S, Abhir, J, Abhishek, A, Acero, F, Acharyya, A, Adam, R, Aguasca-Cabot, A, Agudo, I, Aguirre-Santaella, A, Alfaro, J, Alfaro, R, Alvarez-Crespo, N, Alves Batista, R, Amans, J, Amato, E, Ambrosi, G, Angel, L, Aramo, C, Arcaro, C, Arnesen, T, Arrabito, L, Asano, K, Ascasibar, Y, Aschersleben, J, Cotter, G, Sarkar, S, Spencer, S

“…We provide an updated assessment of the sensitivity of the Cherenkov Telescope Array (CTA) to such signals, based on observations of the Galactic centre region as well as of selected dwarf spheroidal galaxies. …”

Prospects for Gamma-Ray Burst detection by the Cherenkov Telescope Array by Bissaldi E., Di Girolamo T., Di Pierro F., Gasparetto T., Longo F., Vallania P., Vigorito C.

“…This work aims at revising the prospects for GRB alerts with the Cherenkov Telescope Array (CTA) based on the new LAT results. …”
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Secluded dark matter in light of the Cherenkov Telescope Array (CTA) by Clarissa Siqueira

“…Taking into account 1% level of systematics, in this work we show that the Cherenkov Telescope Array (CTA) will place the most stringent bounds on the dark matter annihilation cross section, surpassing existing probes based on H.E.S.S., Fermi-LAT, and Planck data, for dark matter masses above 400GeV, independently of the channel and choosing the Einasto profile. …”
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The ASTRI mini-array within the future Cherenkov Telescope Array by Vercellone Stefano

“…The Cherenkov Telescope Array (CTA) is a large collaborative effort aimed at the design and operation of an observatory dedicated to very high-energy gamma-ray astrophysics in the energy range from a few tens of GeV to above 100 TeV, which will yield about an order of magnitude improvement in sensitivity with respect to the current major arrays (H.E.S.S., MAGIC, and VERITAS). …”
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The Raman LIDAR for the pre-production phase of Cherenkov Telescope Array by Iarlori Marco, Pietropaolo Ermanno, Rizi Vincenzo, Aramo Carla, Valore Laura, Silvestri Valerio, Cirella Alberto, Dughera Giovanni, Galli Stefano, Marengo Marco

“…The ARCADE Raman lidar has been tested and validated at L'Aquila before the deployment at CTA (Cherenkov Telescope Array) North site. Some modifications have been done on the original ARCADE system to improve its performances, and an extensive programme of measurements has been performed. …”
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Studying molecular profiles above the Cherenkov Telescope Array sites by Munar-Adrover Pere, Gaug Markus

“…The Cherenkov Telescope Array (CTA) will bring a whole new insight to the gamma-ray Universe. …”
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Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout by Acharyya, A, Agudo, I, Angüner, E, Alfaro, R, Alfaro, J, Alispach, C, Aloisio, R, Alves Batista, R, Amans, J, Amati, L, Amato, E, Ambrosi, G, Antonelli, L, Aramo, C, Armstrong, T, Arqueros, F, Arrabito, L, Asano, K, Ashkar, H, Balazs, C, Balbo, M, Balmaverde, B, Barai, P, Barbano, A, Barkov, M, Barres De Almeida, U, Barrio, J, Bastieri, D, Becerra González, J, Becker Tjus, J, Bellizzi, L, Benbow, W, Bernardini, E, Bernardos, M, Bernlöhr, K, Berti, A, Berton, M, Bertucci, B, Beshley, V, Biasuzzi, B, Bigongiari, C, Bird, R, Bissaldi, E, Biteau, J, Blanch, O, Blazek, J, Boisson, C, Bonanno, G, Bonardi, A, Bonavolontá, C, Bonnoli, G, Bordas, P, Böttcher, M, Bregeon, J, Brill, A, Brown, A, Brügge, K, Brun, P, Bruno, P, Bulgarelli, A, Bulik, T, Burton, M, Burtovoi, A, Busetto, G, Cameron, R, Canestrari, R, Capalbi, M, Caproni, A, Capuzzo-Dolcetta, R, Caraveo, P, Caroff, S, Carosi, R, Casanova, S, Cascone, E, Cassol, F, Catalani, F, Catalano, O, Cauz, D, Cerruti, M, Chaty, S, Chen, A, Chernyakova, M, Chiaro, G, Cieślar, M, Colak, S, Conforti, V, Congiu, E, Contreras, J, Cortina, J, Costa, A, Costantini, H, Cotter, G, Cristofari, P, Cumani, P, Spencer, S

“…The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. …”

The quest for dark matter in dwarf spheroidal galaxies with the Cherenkov Telescope Array by Saturni Francesco G., Rodríguez-Fernández Gonzalo, Morselli Aldo

“…Such factors are of great importance to test the performances of the next-generation γ-ray instruments such as the Cherenkov Telescope Array in detecting dark-matter signals from astronomical environments, or constraining the limits to dark-matter physics parameters (particle mass and lifetime, annihilation cross section).…”
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Atmospheric monitoring using the Cherenkov Transparency Coefficient for the Cherenkov Telescope Array by Stefanik Stanislav, Nosek Dalibor

“…The future ground-based gamma-ray observatory, the Cherenkov Telescope Array (CTA) will require reliable monitoring of the atmosphere which is an inherent part of the detector. …”
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Inauguration and first light of the GCT-M prototype for the Cherenkov Telescope Array by Watson, J, De Franco, A, Abchiche, A, Allan, D, Amans, J, Armstrong, T, Balzer, A, Berge, D, Boisson, C, Bousquet, J, Brown, A, Bryan, M, Buchholtz, G, Chadwick, P, Costantini, H, Cotter, G, Daniel, M, De Frondat, F, Dournaux, J, Dumas, D, Ernenwein, J, Fasola, G, Funk, S, Gironnet, J, Graham, J, Greenshaw, T, Hervet, O, Hidaka, N, Hinton, J, Huet, J, Jegouzo, I, Jogler, T, Kraus, M, Lapington, J, Laporte, P, Lefaucheur, J, Markoff, S, Melse, T, Mohrmann, L, Molyneux, P, Nolan, S, Okumura, A, Osborne, J, Parsons, R, Rosen, S, Ross, D, Rowell, G, Rulten, C, Sato, Y, Sayede, F, Schmoll, J, Schoorlemmer, H, Servillat, M, Sol, H, Stamatescu, V, Stephan, M, Stuik, R, Sykes, J, Tajima, H, Thornhill, J, Tibaldo, L, Trichard, C, Vink, J, White, R, Yamane, N, Zech, A, Zink, A, Zorn, J, Consortium, CTA

“…The Gamma-ray Cherenkov Telescope (GCT) is a candidate for the Small Size Telescopes (SSTs) of the Cherenkov Telescope Array (CTA). Its purpose is to extend the sensitivity of CTA to gamma-ray energies reaching 300 TeV. …”