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CTA : the World's largest ground-based gamma-ray observatory
Journal
POS Proceedings of Science
Alternative title
Cherenkov Telescope Array : the World’s largest VHE gamma-ray observatory
Author
Jamrozy Marek
Ostrowski Michał
Stawarz Łukasz
Ziętara Krzysztof
Volume
395
Other author
Współautorami artykułu są członkowie CTA Observatory CTA Consortium i LST Collaboration w liczbie 1139
Title of volume
37th International Cosmic Ray Conference (ICRC2021)
Article ID
005
eISSN
1824-8039
Remarks
1143 - łączna liczba autorów publikacji
Language
English
Journal language
English
Abstract in English
Very-High Energy (VHE) gamma-ray astroparticle physics is a relatively young field, and observations over the past decade have surprisingly revealed almost two hundred VHE emitters which appear to act as cosmic particle accelerators. These sources are an important component of the Universe, influencing the evolution of stars and galaxies. At the same time, they also act as a probe of physics in the most extreme environments known - such as in supernova explosions, and around or after the merging of black holes and neutron stars. However, the existing experiments have provided exciting glimpses, but often falling short of supplying the full answer. A deeper understanding of the TeV sky requires a significant improvement in sensitivity at TeV energies, a wider energy coverage from tens of GeV to hundreds of TeV and a much better angular and energy resolution with respect to the currently running facilities. The next generation gamma-ray observatory, the Cherenkov Telescope Array Observatory (CTAO), is the answer to this need. In this talk I will present this upcoming observatory from its design to the construction, and its potential science exploitation. CTAO will allow the entire astronomical community to explore a new discovery space that will likely lead to paradigm changing breakthroughs. In particular, CTA has an unprecedented sensitivity to short (sub-minute) timescale phenomena, placing it as a key instrument in the future of multi-messenger and multi-wavelength time domain astronomy. I will conclude the talk presenting the first scientific results obtained by the LST-1, the prototype of one CTA telescope type - the Large Sized Telescope, that is currently under commission.
Conference
37th International Cosmic Ray Conference (ICRC2021)
Conference start date
2021-07-12
End date conference
2021-07-23
Conference city
Berlin
Conference country
Niemcy
Conference type
international
Affiliation
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne
| dc.abstract.en | Very-High Energy (VHE) gamma-ray astroparticle physics is a relatively young field, and observations over the past decade have surprisingly revealed almost two hundred VHE emitters which appear to act as cosmic particle accelerators. These sources are an important component of the Universe, influencing the evolution of stars and galaxies. At the same time, they also act as a probe of physics in the most extreme environments known - such as in supernova explosions, and around or after the merging of black holes and neutron stars. However, the existing experiments have provided exciting glimpses, but often falling short of supplying the full answer. A deeper understanding of the TeV sky requires a significant improvement in sensitivity at TeV energies, a wider energy coverage from tens of GeV to hundreds of TeV and a much better angular and energy resolution with respect to the currently running facilities. The next generation gamma-ray observatory, the Cherenkov Telescope Array Observatory (CTAO), is the answer to this need. In this talk I will present this upcoming observatory from its design to the construction, and its potential science exploitation. CTAO will allow the entire astronomical community to explore a new discovery space that will likely lead to paradigm changing breakthroughs. In particular, CTA has an unprecedented sensitivity to short (sub-minute) timescale phenomena, placing it as a key instrument in the future of multi-messenger and multi-wavelength time domain astronomy. I will conclude the talk presenting the first scientific results obtained by the LST-1, the prototype of one CTA telescope type - the Large Sized Telescope, that is currently under commission. | pl |
| dc.affiliation | Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne | pl |
| dc.conference | 37th International Cosmic Ray Conference (ICRC2021) | |
| dc.conference.city | Berlin | |
| dc.conference.country | Niemcy | |
| dc.conference.datefinish | 2021-07-23 | |
| dc.conference.datestart | 2021-07-12 | |
| dc.contributor.author | Jamrozy, Marek - 128434 | pl |
| dc.contributor.author | Ostrowski, Michał - 100042 | pl |
| dc.contributor.author | Stawarz, Łukasz - 132081 | pl |
| dc.contributor.author | Ziętara, Krzysztof - 174018 | pl |
| dc.contributor.other | Współautorami artykułu są członkowie CTA Observatory, CTA Consortium i LST Collaboration w liczbie 1139 | pl |
| dc.date.accessioned | 2022-12-05T12:51:57Z | |
| dc.date.available | 2022-12-05T12:51:57Z | |
| dc.date.issued | 2022 | pl |
| dc.date.openaccess | 0 | |
| dc.description.accesstime | w momencie opublikowania | |
| dc.description.additional | 1143 - łączna liczba autorów publikacji | pl |
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Wijers—M. Wilkinson—M. Will—J. Williams—T.J. Williamson—A. Wolter—Y.W. Wong—M. Wood—T. Yamamoto—H. Yamamoto—Y. Yamane—R. Yamazaki—S. Yanagita—L. Yang—S. Yoo—T. Yoshida—T. Yoshikoshi—P. Yu—A. Yusafzai—M. Zacharias—B. Zaldivar—L. Zampieri—R. Zanin—R. Zanmar Sanchez—D. Zaric—M. Zavrtanik—D. Zavrtanik—A. Zdziarski—A. Zech—H. Zechlin—A. Zenin—A. Zerwekh—A. Zink—J. Ziolkowski—M. Zivec—A. Zmija | pl |
| dc.description.conftype | international | pl |
| dc.description.publication | 1 | pl |
| dc.description.version | ostateczna wersja wydawcy | |
| dc.description.volume | 395 | pl |
| dc.identifier.articleid | 005 | pl |
| dc.identifier.doi | 10.22323/1.395.0005 | pl |
| dc.identifier.eissn | 1824-8039 | pl |
| dc.identifier.uri | https://ruj.uj.edu.pl/xmlui/handle/item/304390 | |
| dc.language | eng | pl |
| dc.language.container | eng | pl |
| dc.rights | Udzielam licencji. Uznanie autorstwa - Użycie niekomercyjne - Bez utworów zależnych 4.0 Międzynarodowa | * |
| dc.rights.licence | CC-BY-NC-ND | |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/legalcode.pl | * |
| dc.share.type | otwarte czasopismo | |
| dc.subtype | ConferenceProceedings | pl |
| dc.title | CTA : the World's largest ground-based gamma-ray observatory | pl |
| dc.title.alternative | Cherenkov Telescope Array : the World’s largest VHE gamma-ray observatory | pl |
| dc.title.journal | POS Proceedings of Science | pl |
| dc.title.volume | 37th International Cosmic Ray Conference (ICRC2021) | pl |
| dc.type | JournalArticle | pl |
| dspace.entity.type | Publication |
dc.abstract.enpl
Very-High Energy (VHE) gamma-ray astroparticle physics is a relatively young field, and observations over the past decade have surprisingly revealed almost two hundred VHE emitters which appear to act as cosmic particle accelerators. These sources are an important component of the Universe, influencing the evolution of stars and galaxies. At the same time, they also act as a probe of physics in the most extreme environments known - such as in supernova explosions, and around or after the merging of black holes and neutron stars. However, the existing experiments have provided exciting glimpses, but often falling short of supplying the full answer. A deeper understanding of the TeV sky requires a significant improvement in sensitivity at TeV energies, a wider energy coverage from tens of GeV to hundreds of TeV and a much better angular and energy resolution with respect to the currently running facilities. The next generation gamma-ray observatory, the Cherenkov Telescope Array Observatory (CTAO), is the answer to this need. In this talk I will present this upcoming observatory from its design to the construction, and its potential science exploitation. CTAO will allow the entire astronomical community to explore a new discovery space that will likely lead to paradigm changing breakthroughs. In particular, CTA has an unprecedented sensitivity to short (sub-minute) timescale phenomena, placing it as a key instrument in the future of multi-messenger and multi-wavelength time domain astronomy. I will conclude the talk presenting the first scientific results obtained by the LST-1, the prototype of one CTA telescope type - the Large Sized Telescope, that is currently under commission. dc.affiliationpl
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne dc.conference
37th International Cosmic Ray Conference (ICRC2021) dc.conference.city
Berlin dc.conference.country
Niemcy dc.conference.datefinish
2021-07-23 dc.conference.datestart
2021-07-12 dc.contributor.authorpl
Jamrozy, Marek - 128434 dc.contributor.authorpl
Ostrowski, Michał - 100042 dc.contributor.authorpl
Stawarz, Łukasz - 132081 dc.contributor.authorpl
Ziętara, Krzysztof - 174018 dc.contributor.otherpl
Współautorami artykułu są członkowie CTA Observatory, CTA Consortium i LST Collaboration w liczbie 1139 dc.date.accessioned
2022-12-05T12:51:57Z dc.date.available
2022-12-05T12:51:57Z dc.date.issuedpl
2022 dc.date.openaccess
0 dc.description.accesstime
w momencie opublikowania dc.description.additionalpl
1143 - łączna liczba autorów publikacji dc.description.adminpl
[AT]R. Zanin—H. Abdalla—H. Abe—S. Abe—A. Abusleme—F. Acero—A. Acharyya—V. Acin Portella—K. Ackley—R. Adam—C. Adams—S.S. Adhikari—I. Aguado Ruesga—I. Agudo—R. Aguilera—A. Aguirre Santaella—F. Aharonian—A. Alberdi—R. Alfaro—J. Alfaro—C. Alispach—R. Aloisio—R. Alves Batista—J.P. Amans—L. Amati—E. Amato—L. Ambrogi—G. Ambrosi—M. Ambrosio—R. Ammendola—J. Anderson—M. Anduze—E.O. Anguner—L.A. Antonelli—V. Antonuccio—P. Antoranz—R. Anutarawiramkul—J. Aragunde Gutierrez—C. Aramo—A. Araudo—M. Araya—A. Arbet Engels—C. Arcaro—V. Arendt—C. Armand—T. Armstrong—F. Arqueros—L. Arrabito—B. Arsioli—M. Artero—K. Asano—Y. Ascasibar—J. Aschersleben—M. Ashley—P. Attina—P. Aubert—C. B. Singh—D. Baack—A. Babic—M. Backes—V. Baena—S. Bajtlik—A. Baktash—C. Balazs—M. Balbo—O. Ballester—J. Ballet—B. Balmaverde—A. Bamba—R. Bandiera—A. Baquero Larriva—P. Barai—C. Barbier—V. Barbosa Martins—M. Barcelo—M. Barkov—M. Barnard—L. Baroncelli—U. Barres de Almeida—J.A. Barrio—D. Bastieri—P.I. Batista—I. Batkovic—C. Bauer—R. 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Todero Peixoto—K. Toma—L. Tomankova—J. Tomastik—M. Tornikoski—D.F. Torres—E. Torresi—G. Tosti—L. Tosti—N. Tothill—F. Toussenel—G. Tovmassian—C. Trichard—M. Trifoglio—A. Trois—S. Truzzi—A. Tsiahina—B. Turk—A. Tutone—Y. Uchiyama—P. Utayarat—L. Vaclavek—M. Vacula—V. Vagelli—F. Vagnetti—J.A. Valdivia—M. Valentino—A. Valio—B. Vallage—P. Vallania Quispe—A.M. van den Berg—W. van Driel—C. van Eldik—C. van Rensburg—B. van Soelen—J. Vandenbroucke—G. Vasileiadis—V. Vassiliev—M. Vazquez Acosta—M. Vecchi—A. Vega—J. Veh—P. Veitch—C. Venter—S. Ventura—S. Vercellone—V. Verguilov—G. Verna—S. Vernetto—V. Verzi—G.P. Vettolani—C. Veyssiere—I. Viale—A. Viana—N. Viaux—J. Vignatti—C.F. Vigorito—J. Villanueva—V. Vitale—V. Vittorini—V. Vodeb—N. Vogel—V. Voisin—S. Vorobiov—M. Vrastil—T. Vuillaume—S.J. Wagner—P. Wagner—K. Wakazono—S.P. Wakely—M. Ward—D. Warren—J. Watson—M. Wechakama—P. Wegner—A. Weinstein—C. Weniger—F. Werner—H. Wetteskind—M.L. White—A. Wierzcholska—S. Wiesand—R. Wijers—M. Wilkinson—M. Will—J. Williams—T.J. Williamson—A. Wolter—Y.W. Wong—M. Wood—T. Yamamoto—H. Yamamoto—Y. Yamane—R. Yamazaki—S. Yanagita—L. Yang—S. Yoo—T. Yoshida—T. Yoshikoshi—P. Yu—A. Yusafzai—M. Zacharias—B. Zaldivar—L. Zampieri—R. Zanin—R. Zanmar Sanchez—D. Zaric—M. Zavrtanik—D. Zavrtanik—A. Zdziarski—A. Zech—H. Zechlin—A. Zenin—A. Zerwekh—A. Zink—J. Ziolkowski—M. Zivec—A. Zmija dc.description.conftypepl
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395 dc.identifier.articleidpl
005 dc.identifier.doipl
10.22323/1.395.0005 dc.identifier.eissnpl
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CTA : the World's largest ground-based gamma-ray observatory dc.title.alternativepl
Cherenkov Telescope Array : the World’s largest VHE gamma-ray observatory dc.title.journalpl
POS Proceedings of Science dc.title.volumepl
37th International Cosmic Ray Conference (ICRC2021) dc.typepl
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Publication Affiliations
Wydział Fizyki, Astronomii i Informatyki Stosowanej
Jamrozy, Marek
Ostrowski, Michał
Stawarz, Łukasz
Ziętara, Krzysztof
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