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相关论文: Status of the CANGAROO-III Project

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We report on the status of the construction of an array of four 10 m atmospheric Cherenkov telescopes for gamma-ray astronomy, near Woomera, in South Australia -- the CANGAROO-III project. The first telescope of this array is the upgraded…

The CANGAROO-III project,which consists of an array of four 10 m imaging Cherenkov telescopes,has just started being constructed in Woomera, South Australia,in a collaboration between Australia and Japan. The first stereoscopic observation…

Preliminary results from CANGAROO-II, a 10 m imaging Cherenkov telescope, in Woomera, South Australia are presented. They include the confirmation of detections of TeV gamma-ray sources we have reported using a 3.8 m telescope, CANGAROO-I.…

天体物理学 · 物理学 2015-06-24 Masaki Mori , the CANGAROO collaboration

CANGAROO group constructed an imaging air Cherenkov telescope (CANGAROO-II) in March 1999 atWoomera, South Australia to observe celestial gamma-rays in hundreds GeV region. It has a 7m parabolic mirror consisting of 60 small plastic…

CANGAROO group has constructed the new large imaging Air \v Cerenkov telescope to exploit hundred GeV region gamma-ray astronomy in March 1999 at Woomera, South Australia. It has a 7m parabolic mirror consisting of 60 small plastic…

CANGAROO-III is an Imaging Atmospheric Cherenkov Telescope (IACT) array of four 10 m telescopes for very high energy (sub-TeV) gamma-ray astronomy. A design study of the CANGAROO-III telescope system was carried out using the Monte Carlo…

天体物理学 · 物理学 2014-10-13 R. Enomoto , S. Hara , CANGAROO collaboration

We have observed the giant radio galaxy Centaurus A and the globular cluster $\omega$ Centauri in the TeV energy region using the CANGAROO-III stereoscopic system. The system has been in operation since 2004 withan array of four Imaging…

天体物理学 · 物理学 2009-11-13 S. Kabuki , R. Enomoto , CANGAROO-III collaboration

KAGRA is a 3-km interferometric gravitational wave telescope located in the Kamioka mine in Japan. It is the first km-class gravitational wave telescope constructed underground to reduce seismic noise, and the first km-class telescope to…

广义相对论与量子宇宙学 · 物理学 2020-08-20 KAGRA Collaboration , T. Akutsu , M. Ando , A. Araya , N. Aritomi , H. Asada , Y. Aso , S. Atsuta , K. Awai , M. A. Barton , K. Cannon , K. Craig , W. Creus , K. Doi , K. Eda , Y. Enomoto , R. Flaminio , Y. Fujii , M. -K. Fujimoto , T. Furuhata , S. Haino , K. Hasegawa , K. Hashino , K. Hayama , S. Hirobayashi , E. Hirose , B. H. Hsieh , Y. Inoue , K. Ioka , Y. Itoh , T. Kaji , T. Kajita , M. Kakizaki , M. Kamiizumi , S. Kambara , N. Kanda , S. Kanemura , M. Kaneyama , G. Kang , J. Kasuya , Y. Kataoka , N. Kawai , S. Kawamura , C. Kim , H. Kim , J. Kim , Y. Kim , N. Kimura , T. Kinugawa , S. Kirii , Y. Kitaoka , Y. Kojima , K. Kokeyama , K. Komori , K. Kotake , R. Kumar , H. Lee , H. Lee , Y. Liu , N. Luca , E. Majorana , S. Mano , M. Marchio , T. Matsui , F. Matsushima , Y. Michimura , O. Miyakawa , T. Miyamoto , A. Miyamoto , K. Miyo , S. Miyoki , W. Morii , S. Morisaki , Y. Moriwaki , T. Morozumi , M. Musha , S. Nagano , K. Nagano , K. Nakamura , T. Nakamura , H. Nakano , M. Nakano , K. Nakao , T. Narikawa , L. Nguyen Quynh , W. -T. Ni , T. Ochi , J. Oh , S. Oh , M. Ohashi , N. Ohishi , M. Ohkawa , K. Okutomi , K. Oohara , F. E. Peña Alleano , I. Pinto , N. Sago , M. Saijo , Y. Saito , K. Sakai , Y. Sakai , Y. Sasaki , M. Sasaki , S. Sato , T. Sato , Y. Sekiguchi , N. Seto , M. Shibata , T. Shimoda , H. Shinkai , A. Shoda , K. Somiya , E. Son , A. Suemasa , T. Suzuki , T. Suzuki , H. Tagoshi , H. Takahashi , R. Takahashi , A. Takamori , H. Takeda , H. Tanaka , K. Tanaka , T. Tanaka , D. Tatsumi , T. Tomaru , T. Tomura , F. Travasso , K. Tsubono , S. Tsuchida , N. Uchikata , T. Uchiyama , T. Uehara , S. Ueki , K. Ueno , T. Ushiba , M. H. P. M. van Putten , H. Vocca , S. Wada , T. Wakamatsu , T. Yamada , S. Yamamoto , T. Yamamoto , K. Yamamoto , A. Yamamoto , J. Yokoyama , T. Yokozawa , T. H. Yoon , H. Yuzurihara , S. Zeidler , Z. -H. Zhu

A Cherenkov imaging camera for the CANGAROO-III experiment has been developed for observations of gamma-ray induced air-showers at energies from 10$^{11}$ to 10$^{14}$ eV. The camera consists of 427 pixels, arranged in a hexagonal shape at…

We discuss preliminary studies concerning a large-diameter gamma-ray telescope, to be part of an array of telescopes installed at the existing observation site on the Canary island of La Palma. One of the telescopes in the array will be…

天体物理学 · 物理学 2007-05-23 Carmen Baixeras

The Square Kilometre Array telescopes have recently started their construction phase, after years of pre-construction effort. The new SKA Observatory (SKAO) intergovernmental organisation has been created, and the start of construction…

天体物理仪器与方法 · 物理学 2021-10-27 J. Santander-Vela , M. Bartolini , and , M. Miccolis , N. Rees

Kepler's supernova, discovered in October 1604, produced a remnant that has been well studied observationally in the radio, infrared, optical, and X-ray bands, and theoretically. Some models have predicted a TeV gamma-ray flux that is…

天体物理学 · 物理学 2009-11-13 R. Enomoto , Y. Higashi , T. Yoshida , T. Tanimori

LHAASO is expected to be the most sensitive project to face the open problems in Galactic cosmic ray physics through a combined study of photon- and charged particle-induced extensive air showers in the energy range 10$^{11}$ - 10$^{17}$…

高能天体物理现象 · 物理学 2019-08-13 G. Di Sciascio

The Zadko Telescope is a 1 m f/4 Cassegrain telescope, situated in the state of Western Australia about 80 km north of Perth. The facility plays a niche role in Australian astronomy, as it is the only meter class facility in Australia…

KAGRA is a newly build gravitational-wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper in the series of KAGRA-featured articles, we discuss the science targets of KAGRA projects,…

广义相对论与量子宇宙学 · 物理学 2020-08-10 KAGRA Collaboration , T. Akutsu , M. Ando , K. Arai , Y. Arai , S. Araki , A. Araya , N. Aritomi , H. Asada , Y. Aso , S. Bae , Y. Bae , L. Baiotti , R. Bajpai , M. A. Barton , K. Cannon , Z. Cao , E. Capocasa , M. Chan , C. Chen , K. Chen , Y. Chen , C-Y. Chiang , H. Chu , Y-K. Chu , S. Eguchi , Y. Enomoto , R. Flaminio , Y. Fujii , F. Fujikawa , M. Fukunaga , M. Fukushima , D. Gao , G. Ge , S. Ha , A. Hagiwara , S. Haino , W. -B. Han , K. Hasegawa , K. Hattori , H. Hayakawa , K. Hayama , Y. Himemoto , Y. Hiranuma , N. Hirata , E. Hirose , Z. Hong , B. H. Hsieh , C-Z. Huang , H-Y Huang , P. Huang , Y-C. Huang , Y. Huang , D. C. Y. Hui , S. Ide , B. Ikenoue , S. Imam , K. Inayoshi , Y. Inoue , K. Ioka , K. Ito , Y. Itoh , K. Izumi , C. Jeon , H-B. Jin , K. Jung , P. Jung , K. Kaihotsu , T. Kajita , M. Kakizaki , M. Kamiizumi , N. Kanda , G. Kang , K. Kashiyama , K. Kawaguchi , N. Kawai , T. Kawasaki , C. Kim , J. Kim , J. C. Kim , W. S. Kim , Y. -M. Kim , N. Kimura , N. Kita , H. Kitazawa , Y. Kojima , K. Kokeyama , K. Komori , A. K. H. Kong , K. Kotake , C. Kozakai , R. Kozu , R. Kumar , J. Kume , C. Kuo , H-S. Kuo , Y. Kuromiya , S. Kuroyanagi , K. Kusayanagi , K. Kwak , H. K. Lee , H. W. Lee , R. Lee , M. Leonardi , T. G. F. Li , K. L. Li , L. C. -C. Lin , C-Y. Lin , F-K. Lin , F-L. Lin , H. L. Lin , G. C. Liu , L. -W. Luo , E. Majorana , M. Marchio , Y. Michimura , N. Mio , O. Miyakawa , A. Miyamoto , Y. Miyazaki , K. Miyo , S. Miyoki , Y. Mori , S. Morisaki , Y. Moriwaki , K. Nagano , S. Nagano , K. Nakamura , H. Nakano , M. Nakano , R. Nakashima , Y. Nakayama , T. Narikawa , L. Naticchioni , R. Negishi , L. Nguyen Quynh , W. -T. Ni , A. Nishizawa , S. Nozaki , Y. Obuchi , W. Ogaki , J. J. Oh , K. Oh , S. H. Oh , M. Ohashi , N. Ohishi , M. Ohkawa , H. Ohta , Y. Okutani , K. Okutomi , K. Oohara , C. P. Ooi , S. Oshino , S. Otabe , K. Pan , H. Pang , A. Parisi , J. Park , F. E. Pena Arellano , I. Pinto , N. Sago , S. Saito , Y. Saito , K. Sakai , Y. Sakai , Y. Sakuno , S. Sato , T. Sato , T. Sawada , T. Sekiguchi , Y. Sekiguchi , L. Shao , S. Shibagaki , R. Shimizu , T. Shimoda , K. Shimode , H. Shinkai , T. Shishido , A. Shoda , K. Somiya , E. J. Son , H. Sotani , R. Sugimoto , J. Suresh , T. Suzuki , T. Suzuki , H. Tagoshi , H. Takahashi , R. Takahashi , A. Takamori , S. Takano , H. Takeda , M. Takeda , H. Tanaka , K. Tanaka , K. Tanaka , T. Tanaka , T. Tanaka , S. Tanioka , E. N. Tapia San Martin , S. Telada , T. Tomaru , Y. Tomigami , T. Tomura , F. Travasso , L. Trozzo , T. Tsang , J-S. Tsao , K. Tsubono , S. Tsuchida , D. Tsuna , T. Tsutsui , T. Tsuzuki , D. Tuyenbayev , N. Uchikata , T. Uchiyama , A. Ueda , T. Uehara , K. Ueno , G. Ueshima , F. Uraguchi , T. Ushiba , M. H. P. M. van Putten , H. Vocca , J. Wang , T. Washimi , C. Wu , H. Wu , S. Wu , W-R. Xu , T. Yamada , K. Yamamoto , K. Yamamoto , T. Yamamoto , K. Yamashita , R. Yamazaki , Y. Yang , K. Yokogawa , J. Yokoyama , T. Yokozawa , T. Yoshioka , H. Yuzurihara , S. Zeidler , M. Zhan , H. Zhang , Y. Zhao , Z. -H. Zhu

The ANTARES project aims at the construction of an underwater neutrino telescope at the scale of 0.1 km^2 2400 m deep in the Mediterranean Sea. After a 4-year R&D program, the ANTARES project has entered the construction phase which will be…

高能物理 - 实验 · 物理学 2015-06-25 T. Montaruli , for ANTARES Collaboration

The 17 m MAGIC Cherenkov telescope for gamma ray astronomy between 30 and 300 GeV started operations in its final configuration in October 2003 and is currently well into its calibration phase. Here I report on its present status and its…

天体物理学 · 物理学 2019-08-14 J. Cortina

The new 1-m f/4 fast-slew Zadko Telescope was installed in June 2008 about 70 km north of Perth, Western Australia. It is the only metre-class optical facility at this southern latitude between the east coast of Australia and South Africa,…

The Subaru Telescope is an 8.2 m optical/infrared telescope constructed during 1991--1999 and has been operational since 2000 on the summit area of Maunakea, Hawaii, by the National Astronomical Observatory of Japan (NAOJ). This paper…

天体物理仪器与方法 · 物理学 2021-09-01 Masanori Iye
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