Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA

C. B. Adams; G. Ambrosi; M. Ambrosio; C. Aramo; P. I. Batista; W. Benbow; B. Bertucci; E. Bissaldi; M. Bitossi; A. Boiano; C. Bonavolontà; R. Bose; A. Brill; A. M. Brown; J. H. Buckley; R. Canestrari; M. Capasso; M. Caprai; C. E. Covault; D. Depaoli; L. Di Venere; M. Errando; S. Fegan; Q. Feng; E. Fiandrini; A. Furniss; A. Gent; N. Giglietto; F. Giordano; E. Giro; R. Halliday; O. Hervet; J. Holder; T. B. Humensky; S. Incardona; M. Ionica; W. Jin; D. Kieda; F. Licciulli; S. Loporchio; G. Marsella; V. Masone; K. Meagher; T. Meures; B. A.W. Mode; S. A.I. Mognet; R. Mukherjee; D. Nieto; A. Okumura; N. Otte; F. R. Pantaleo; R. Paoletti; G. Pareschi; F. Di Pierro; E. Pueschel; D. Ribeiro; L. Riitano; E. Roache; D. Ross; J. Rousselle; A. Rugliancich; M. Santander; R. Shang; L. Stiaccini; H. Tajima; L. P. Taylor; L. Tosti; G. Tovmassian; G. Tripodo; V. Vagelli; M. Valentino; J. Vandenbroucke; V. V. Vassiliev; J. J. Watson; R. White; D. A. Williams; P. Yu; A. Zink

doi:10.1117/12.2594580

Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA

C. B. Adams
, G. Ambrosi
, M. Ambrosio
, C. Aramo
, P. I. Batista
, W. Benbow
, B. Bertucci
, E. Bissaldi
, M. Bitossi
, A. Boiano
, C. Bonavolontà
, R. Bose
, A. Brill
, A. M. Brown
, J. H. Buckley
, R. Canestrari
, M. Capasso
, M. Caprai
, C. E. Covault
, D. Depaoli

L. Di Venere, M. Errando, S. Fegan, Q. Feng, E. Fiandrini, A. Furniss, A. Gent, N. Giglietto, F. Giordano, E. Giro, R. Halliday, O. Hervet, J. Holder, T. B. Humensky, S. Incardona, M. Ionica, W. Jin, D. Kieda, F. Licciulli, S. Loporchio, G. Marsella, V. Masone, K. Meagher, T. Meures, B. A.W. Mode, S. A.I. Mognet, R. Mukherjee, D. Nieto, A. Okumura, N. Otte, F. R. Pantaleo, R. Paoletti, G. Pareschi, F. Di Pierro, E. Pueschel, D. Ribeiro, L. Riitano, E. Roache, D. Ross, J. Rousselle, A. Rugliancich, M. Santander, R. Shang, L. Stiaccini, H. Tajima, L. P. Taylor, L. Tosti, G. Tovmassian, G. Tripodo, V. Vagelli, M. Valentino, J. Vandenbroucke, V. V. Vassiliev, J. J. Watson, R. White, D. A. Williams, P. Yu, A. Zink

Columbia University
INFN Sezione di Perugia
INFN Sezione di Napoli
c/o DESY
Center for Astrophysics | Harvard & Smithsonian
University of Perugia
Politecnico di Bari
INFN Sezione di Bari
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
ISASI
Washington University in St. Louis
Durham University
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
Barnard College
Case Western Reserve University
University of Turin
INFN Sezione di Torino
California State University - East Bay
College of Computing
INAF Osservatorio Astronomico di Padova
Michigan State University
University of California at Santa Cruz
The Bartol Research Institute
SUNY Maritime College
University of Palermo
INFN Sezione di Catania
University of Alabama
University of Utah
University of Wisconsin-Madison
Pennsylvania State University
IPARCOS-UCM (Instituto de Física de Partículas y del Cosmos)
Complutense University
Nagoya University
University of Siena
INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
University of Leicester
National Astronomical Observatory
University of California, Los Angeles
Universidad Nacional Autónoma de México
Science and Research Directorate
Max-Planck-Institut für Kernphysik
Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen

Résultats de recherche: Le chapitre dans un livre, un rapport, une anthologie ou une collection › Contribution à une conférence › Revue par des pairs

2 Citations (Scopus)

Résumé

The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high-energy gamma rays. One candidate design for CTA’s medium-sized telescopes consists of the Schwarzschild-Couder Telescope (SCT), featuring innovative dual-mirror optics. The SCT project has built and is currently operating a 9.7-m prototype SCT (pSCT) at the Fred Lawrence Whipple Observatory (FLWO); such optical design enables the use of a compact camera with state-of-the art silicon photomultiplier detectors. A partially-equipped camera has recently successfully detected the Crab Nebula with a statistical significance of 8.6 standard deviations. A funded upgrade of the pSCT focal plane sensors and electronics is currently ongoing, which will bring the total number of channels from 1600 to 11328 and the telescope field of view from about 2.7^◦ to 8^◦. In this work, we will describe the technical and scientific performance of the pSCT.

langue originale	Anglais
titre	Astronomical Optics
Sous-titre	Design, Manufacture, and Test of Space and Ground Systems III
rédacteurs en chef	Tony B. Hull, Daewook Kim, Pascal Hallibert, Fanny Keller
Editeur	SPIE
ISBN (Electronique)	9781510644786
Les DOIs	https://doi.org/10.1117/12.2594580
état	Publié - 1 janv. 2021
Evénement	Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III 2021 - San Diego, États-Unis Durée: 1 août 2021 → 5 août 2021

Série de publications

Nom	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11820
ISSN (imprimé)	0277-786X
ISSN (Electronique)	1996-756X

Une conférence

Une conférence	Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III 2021
Pays/Territoire	États-Unis
La ville	San Diego
période	1/08/21 → 5/08/21

Accès au document

10.1117/12.2594580

Contient cette citation

Adams, C. B., Ambrosi, G., Ambrosio, M., Aramo, C., Batista, P. I., Benbow, W., Bertucci, B., Bissaldi, E., Bitossi, M., Boiano, A., Bonavolontà, C., Bose, R., Brill, A., Brown, A. M., Buckley, J. H., Canestrari, R., Capasso, M., Caprai, M., Covault, C. E., ... Zink, A. (2021). Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA. Dans T. B. Hull, D. Kim, P. Hallibert, & F. Keller (eds.), Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III Article 118200E (Proceedings of SPIE - The International Society for Optical Engineering; Vol 11820). SPIE. https://doi.org/10.1117/12.2594580

Adams, C. B. ; Ambrosi, G. ; Ambrosio, M. et al. / Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA. Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III. Editeur / Tony B. Hull ; Daewook Kim ; Pascal Hallibert ; Fanny Keller. SPIE, 2021. (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{d2de18e237534d39b099082a6a9f9752,

title = "Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA",

abstract = "The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high-energy gamma rays. One candidate design for CTA{\textquoteright}s medium-sized telescopes consists of the Schwarzschild-Couder Telescope (SCT), featuring innovative dual-mirror optics. The SCT project has built and is currently operating a 9.7-m prototype SCT (pSCT) at the Fred Lawrence Whipple Observatory (FLWO); such optical design enables the use of a compact camera with state-of-the art silicon photomultiplier detectors. A partially-equipped camera has recently successfully detected the Crab Nebula with a statistical significance of 8.6 standard deviations. A funded upgrade of the pSCT focal plane sensors and electronics is currently ongoing, which will bring the total number of channels from 1600 to 11328 and the telescope field of view from about 2.7◦ to 8◦. In this work, we will describe the technical and scientific performance of the pSCT.",

keywords = "Aplanatic optical system, Gamma rays, Imaging Cherenkov telescopes, Schwarzschild-Couder telescope, Silicon photomultipliers",

author = "Adams, \{C. B.\} and G. Ambrosi and M. Ambrosio and C. Aramo and Batista, \{P. I.\} and W. Benbow and B. Bertucci and E. Bissaldi and M. Bitossi and A. Boiano and C. Bonavolont{\`a} and R. Bose and A. Brill and Brown, \{A. M.\} and Buckley, \{J. H.\} and R. Canestrari and M. Capasso and M. Caprai and Covault, \{C. E.\} and D. Depaoli and \{Di Venere\}, L. and M. Errando and S. Fegan and Q. Feng and E. Fiandrini and A. Furniss and A. Gent and N. Giglietto and F. Giordano and E. Giro and R. Halliday and O. Hervet and J. Holder and Humensky, \{T. B.\} and S. Incardona and M. Ionica and W. Jin and D. Kieda and F. Licciulli and S. Loporchio and G. Marsella and V. Masone and K. Meagher and T. Meures and Mode, \{B. A.W.\} and Mognet, \{S. A.I.\} and R. Mukherjee and D. Nieto and A. Okumura and N. Otte and Pantaleo, \{F. R.\} and R. Paoletti and G. Pareschi and \{Di Pierro\}, F. and E. Pueschel and D. Ribeiro and L. Riitano and E. Roache and D. Ross and J. Rousselle and A. Rugliancich and M. Santander and R. Shang and L. Stiaccini and H. Tajima and Taylor, \{L. P.\} and L. Tosti and G. Tovmassian and G. Tripodo and V. Vagelli and M. Valentino and J. Vandenbroucke and Vassiliev, \{V. V.\} and Watson, \{J. J.\} and R. White and Williams, \{D. A.\} and P. Yu and A. Zink",

note = "Publisher Copyright: {\textcopyright} 2021 SPIE.; Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III 2021 ; Conference date: 01-08-2021 Through 05-08-2021",

year = "2021",

month = jan,

day = "1",

doi = "10.1117/12.2594580",

language = "English",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Hull, \{Tony B.\} and Daewook Kim and Pascal Hallibert and Fanny Keller",

booktitle = "Astronomical Optics",

}

Adams, CB, Ambrosi, G, Ambrosio, M, Aramo, C, Batista, PI, Benbow, W, Bertucci, B, Bissaldi, E, Bitossi, M, Boiano, A, Bonavolontà, C, Bose, R, Brill, A, Brown, AM, Buckley, JH, Canestrari, R, Capasso, M, Caprai, M, Covault, CE, Depaoli, D, Di Venere, L, Errando, M, Fegan, S, Feng, Q, Fiandrini, E, Furniss, A, Gent, A, Giglietto, N, Giordano, F, Giro, E, Halliday, R, Hervet, O, Holder, J, Humensky, TB, Incardona, S, Ionica, M, Jin, W, Kieda, D, Licciulli, F, Loporchio, S, Marsella, G, Masone, V, Meagher, K, Meures, T, Mode, BAW, Mognet, SAI, Mukherjee, R, Nieto, D, Okumura, A, Otte, N, Pantaleo, FR, Paoletti, R, Pareschi, G, Di Pierro, F, Pueschel, E, Ribeiro, D, Riitano, L, Roache, E, Ross, D, Rousselle, J, Rugliancich, A, Santander, M, Shang, R, Stiaccini, L, Tajima, H, Taylor, LP, Tosti, L, Tovmassian, G, Tripodo, G, Vagelli, V, Valentino, M, Vandenbroucke, J, Vassiliev, VV, Watson, JJ, White, R, Williams, DA, Yu, P & Zink, A 2021, Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA. Dans TB Hull, D Kim, P Hallibert & F Keller (eds), Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III., 118200E, Proceedings of SPIE - The International Society for Optical Engineering, VOL. 11820, SPIE, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III 2021, San Diego, États-Unis, 1/08/21. https://doi.org/10.1117/12.2594580

Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA. / Adams, C. B.; Ambrosi, G.; Ambrosio, M. et al.
Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III. Ed. / Tony B. Hull; Daewook Kim; Pascal Hallibert; Fanny Keller. SPIE, 2021. 118200E (Proceedings of SPIE - The International Society for Optical Engineering; Vol 11820).

Résultats de recherche: Le chapitre dans un livre, un rapport, une anthologie ou une collection › Contribution à une conférence › Revue par des pairs

TY - GEN

T1 - Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA

AU - Adams, C. B.

AU - Ambrosi, G.

AU - Ambrosio, M.

AU - Aramo, C.

AU - Batista, P. I.

AU - Benbow, W.

AU - Bertucci, B.

AU - Bissaldi, E.

AU - Bitossi, M.

AU - Boiano, A.

AU - Bonavolontà, C.

AU - Bose, R.

AU - Brill, A.

AU - Brown, A. M.

AU - Buckley, J. H.

AU - Canestrari, R.

AU - Capasso, M.

AU - Caprai, M.

AU - Covault, C. E.

AU - Depaoli, D.

AU - Di Venere, L.

AU - Errando, M.

AU - Fegan, S.

AU - Feng, Q.

AU - Fiandrini, E.

AU - Furniss, A.

AU - Gent, A.

AU - Giglietto, N.

AU - Giordano, F.

AU - Giro, E.

AU - Halliday, R.

AU - Hervet, O.

AU - Holder, J.

AU - Humensky, T. B.

AU - Incardona, S.

AU - Ionica, M.

AU - Jin, W.

AU - Kieda, D.

AU - Licciulli, F.

AU - Loporchio, S.

AU - Marsella, G.

AU - Masone, V.

AU - Meagher, K.

AU - Meures, T.

AU - Mode, B. A.W.

AU - Mognet, S. A.I.

AU - Mukherjee, R.

AU - Nieto, D.

AU - Okumura, A.

AU - Otte, N.

AU - Pantaleo, F. R.

AU - Paoletti, R.

AU - Pareschi, G.

AU - Di Pierro, F.

AU - Pueschel, E.

AU - Ribeiro, D.

AU - Riitano, L.

AU - Roache, E.

AU - Ross, D.

AU - Rousselle, J.

AU - Rugliancich, A.

AU - Santander, M.

AU - Shang, R.

AU - Stiaccini, L.

AU - Tajima, H.

AU - Taylor, L. P.

AU - Tosti, L.

AU - Tovmassian, G.

AU - Tripodo, G.

AU - Vagelli, V.

AU - Valentino, M.

AU - Vandenbroucke, J.

AU - Vassiliev, V. V.

AU - Watson, J. J.

AU - White, R.

AU - Williams, D. A.

AU - Yu, P.

AU - Zink, A.

PY - 2021/1/1

Y1 - 2021/1/1

N2 - The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high-energy gamma rays. One candidate design for CTA’s medium-sized telescopes consists of the Schwarzschild-Couder Telescope (SCT), featuring innovative dual-mirror optics. The SCT project has built and is currently operating a 9.7-m prototype SCT (pSCT) at the Fred Lawrence Whipple Observatory (FLWO); such optical design enables the use of a compact camera with state-of-the art silicon photomultiplier detectors. A partially-equipped camera has recently successfully detected the Crab Nebula with a statistical significance of 8.6 standard deviations. A funded upgrade of the pSCT focal plane sensors and electronics is currently ongoing, which will bring the total number of channels from 1600 to 11328 and the telescope field of view from about 2.7◦ to 8◦. In this work, we will describe the technical and scientific performance of the pSCT.

AB - The Cherenkov Telescope Array (CTA) is the next-generation ground-based observatory for very-high-energy gamma rays. One candidate design for CTA’s medium-sized telescopes consists of the Schwarzschild-Couder Telescope (SCT), featuring innovative dual-mirror optics. The SCT project has built and is currently operating a 9.7-m prototype SCT (pSCT) at the Fred Lawrence Whipple Observatory (FLWO); such optical design enables the use of a compact camera with state-of-the art silicon photomultiplier detectors. A partially-equipped camera has recently successfully detected the Crab Nebula with a statistical significance of 8.6 standard deviations. A funded upgrade of the pSCT focal plane sensors and electronics is currently ongoing, which will bring the total number of channels from 1600 to 11328 and the telescope field of view from about 2.7◦ to 8◦. In this work, we will describe the technical and scientific performance of the pSCT.

KW - Aplanatic optical system

KW - Gamma rays

KW - Imaging Cherenkov telescopes

KW - Schwarzschild-Couder telescope

KW - Silicon photomultipliers

U2 - 10.1117/12.2594580

DO - 10.1117/12.2594580

M3 - Conference contribution

AN - SCOPUS:85117121879

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Astronomical Optics

A2 - Hull, Tony B.

A2 - Kim, Daewook

A2 - Hallibert, Pascal

A2 - Keller, Fanny

PB - SPIE

T2 - Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III 2021

Y2 - 1 August 2021 through 5 August 2021

ER -

Adams CB, Ambrosi G, Ambrosio M, Aramo C, Batista PI, Benbow W et al. Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA. Dans Hull TB, Kim D, Hallibert P, Keller F, rédacteurs en chef, Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems III. SPIE. 2021. 118200E. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2594580

Technical and scientific performance of the prototype Schwarzschild-Couder Telescope for CTA

Résumé

Série de publications

Une conférence

Accès au document

Empreinte digitale

Contient cette citation