The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era

Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Caraveo, Patrizia A. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2020

Schlagwörter:	Gamma-ray astronomy Gamma-ray sources Cherenkov telescopes Gamma-ray missions Multi-messenger astronomy

Übergeordnetes Werk:	Enthalten in: Rivista del nuovo cimento - Bologna : SIF, 1969, 43(2020), 6 vom: 27. Apr., Seite 281-318
Übergeordnetes Werk:	volume:43 ; year:2020 ; number:6 ; day:27 ; month:04 ; pages:281-318

Links:	Volltext

DOI / URN:	10.1007/s40766-020-00006-3

Katalog-ID:	SPR039754936

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allfields	10.1007/s40766-020-00006-3 doi (DE-627)SPR039754936 (SPR)s40766-020-00006-3-e DE-627 ger DE-627 rakwb eng 530 ASE Caraveo, Patrizia A. verfasserin aut The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky. Gamma-ray astronomy (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov telescopes (dpeaa)DE-He213 Gamma-ray missions (dpeaa)DE-He213 Multi-messenger astronomy (dpeaa)DE-He213 Enthalten in Rivista del nuovo cimento Bologna : SIF, 1969 43(2020), 6 vom: 27. Apr., Seite 281-318 (DE-627)385985711 (DE-600)2143515-7 1826-9850 nnns volume:43 year:2020 number:6 day:27 month:04 pages:281-318 https://dx.doi.org/10.1007/s40766-020-00006-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_165 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 43 2020 6 27 04 281-318
spelling	10.1007/s40766-020-00006-3 doi (DE-627)SPR039754936 (SPR)s40766-020-00006-3-e DE-627 ger DE-627 rakwb eng 530 ASE Caraveo, Patrizia A. verfasserin aut The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky. Gamma-ray astronomy (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov telescopes (dpeaa)DE-He213 Gamma-ray missions (dpeaa)DE-He213 Multi-messenger astronomy (dpeaa)DE-He213 Enthalten in Rivista del nuovo cimento Bologna : SIF, 1969 43(2020), 6 vom: 27. Apr., Seite 281-318 (DE-627)385985711 (DE-600)2143515-7 1826-9850 nnns volume:43 year:2020 number:6 day:27 month:04 pages:281-318 https://dx.doi.org/10.1007/s40766-020-00006-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_165 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 43 2020 6 27 04 281-318
allfields_unstemmed	10.1007/s40766-020-00006-3 doi (DE-627)SPR039754936 (SPR)s40766-020-00006-3-e DE-627 ger DE-627 rakwb eng 530 ASE Caraveo, Patrizia A. verfasserin aut The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky. Gamma-ray astronomy (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov telescopes (dpeaa)DE-He213 Gamma-ray missions (dpeaa)DE-He213 Multi-messenger astronomy (dpeaa)DE-He213 Enthalten in Rivista del nuovo cimento Bologna : SIF, 1969 43(2020), 6 vom: 27. Apr., Seite 281-318 (DE-627)385985711 (DE-600)2143515-7 1826-9850 nnns volume:43 year:2020 number:6 day:27 month:04 pages:281-318 https://dx.doi.org/10.1007/s40766-020-00006-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_165 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 43 2020 6 27 04 281-318
allfieldsGer	10.1007/s40766-020-00006-3 doi (DE-627)SPR039754936 (SPR)s40766-020-00006-3-e DE-627 ger DE-627 rakwb eng 530 ASE Caraveo, Patrizia A. verfasserin aut The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky. Gamma-ray astronomy (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov telescopes (dpeaa)DE-He213 Gamma-ray missions (dpeaa)DE-He213 Multi-messenger astronomy (dpeaa)DE-He213 Enthalten in Rivista del nuovo cimento Bologna : SIF, 1969 43(2020), 6 vom: 27. Apr., Seite 281-318 (DE-627)385985711 (DE-600)2143515-7 1826-9850 nnns volume:43 year:2020 number:6 day:27 month:04 pages:281-318 https://dx.doi.org/10.1007/s40766-020-00006-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_165 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 43 2020 6 27 04 281-318
allfieldsSound	10.1007/s40766-020-00006-3 doi (DE-627)SPR039754936 (SPR)s40766-020-00006-3-e DE-627 ger DE-627 rakwb eng 530 ASE Caraveo, Patrizia A. verfasserin aut The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era 2020 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky. Gamma-ray astronomy (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov telescopes (dpeaa)DE-He213 Gamma-ray missions (dpeaa)DE-He213 Multi-messenger astronomy (dpeaa)DE-He213 Enthalten in Rivista del nuovo cimento Bologna : SIF, 1969 43(2020), 6 vom: 27. Apr., Seite 281-318 (DE-627)385985711 (DE-600)2143515-7 1826-9850 nnns volume:43 year:2020 number:6 day:27 month:04 pages:281-318 https://dx.doi.org/10.1007/s40766-020-00006-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_165 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 43 2020 6 27 04 281-318
language	English
source	Enthalten in Rivista del nuovo cimento 43(2020), 6 vom: 27. Apr., Seite 281-318 volume:43 year:2020 number:6 day:27 month:04 pages:281-318
sourceStr	Enthalten in Rivista del nuovo cimento 43(2020), 6 vom: 27. Apr., Seite 281-318 volume:43 year:2020 number:6 day:27 month:04 pages:281-318
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Gamma-ray astronomy Gamma-ray sources Cherenkov telescopes Gamma-ray missions Multi-messenger astronomy
dewey-raw	530
isfreeaccess_bool	false
container_title	Rivista del nuovo cimento
authorswithroles_txt_mv	Caraveo, Patrizia A. @@aut@@
publishDateDaySort_date	2020-04-27T00:00:00Z
hierarchy_top_id	385985711
dewey-sort	3530
id	SPR039754936
language_de	englisch
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author	Caraveo, Patrizia A.
spellingShingle	Caraveo, Patrizia A. ddc 530 misc Gamma-ray astronomy misc Gamma-ray sources misc Cherenkov telescopes misc Gamma-ray missions misc Multi-messenger astronomy The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era
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topic_title	530 ASE The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era Gamma-ray astronomy (dpeaa)DE-He213 Gamma-ray sources (dpeaa)DE-He213 Cherenkov telescopes (dpeaa)DE-He213 Gamma-ray missions (dpeaa)DE-He213 Multi-messenger astronomy (dpeaa)DE-He213
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title	The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era
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title_full	The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era
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title_sort	golden age of high-energy gamma-ray astronomy: the cherenkov telescope array in the multimessenger era
title_auth	The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era
abstract	Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky.
abstractGer	Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky.
abstract_unstemmed	Abstract High-energy photons are a powerful tool to understand the most violent phenomena in our Universe. However, detecting gamma-ray photons is a daunting task both owing to the overwhelming presence of cosmic rays and to the opacity of our atmosphere. Thus, direct detection of gamma-ray photons must be done in space, while instruments on the ground can see very high-energy photons through the secondary particles they produce in the atmosphere. Mastering space instruments as well as ground-based ones required decades of relentless efforts implying hardware and software developments as well as theoretical studies and extensive simulations. Space instruments, as well as ground-based ones, are now producing a steady flow of important results often in conjunction with observatories working at different wavelengths. Multi-messenger astronomy, which combines the electromagnetic channel with gravitational waves and neutrinos, is the newly born discipline to which high-energy gamma-ray detectors provide an essential contribution. Building instruments to continuously cover the gamma-ray sky is, thus, a priority for the astronomical community which is looking forward for the Cherenkov Telescope Array, a new generation ground based gamma-ray observatory designed to monitor, to study and to unveil the mysteries hidden in the very high energy sky.
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title_short	The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era
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The golden age of high-energy gamma-ray astronomy: the Cherenkov Telescope Array in the multimessenger era

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