| 書目名稱 | Focusing Telescopes in Nuclear Astrophysics | | 編輯 | Peter Ballmoos | | 視頻video | http://file.papertrans.cn/345/344847/344847.mp4 | | 概述 | The first book of its kind on focusing gamma-ray telescopes | | 圖書封面 |  | | 描述 | HESS (High Energy Stereoscopic System), a ground-based Cerenkov array telescopes has been operated since a few years and in 2004 has performed the ?rst Galactic plane scan with a sensitivity of a few percent of the Crab at energies above 100 GeV, resulting in the discoveryofeightsources,mostofwhichwithoutanycounterpartatdifferentenergies[1,2]. ParticularattentionwasdevotedtoHESSJ1813-178,notidenti?edwithanyknownX/gamma ray emitter and hypothesised to be a dark particle accelerator. Independently, and at the same time, INTEGRAL discovered a new soft gamma-ray source, namely IGR J18135-1751, identi?edasthecounterpartofHESSJ1813-178.Thishighenergyemitter,whosenaturewas still mysterious at the time of the discovery was then associated with the supernova remnant (SNR) G12.82 0.02 [6, 10, 18]. Even if a chance coincidence cannot be completely ruled out in view of the 2 arcmin INTEGRAL error box and the possible angular extension in the high energy,theoverallcharacteristicsofthisstarformingregion[7]comprisingSNRG12.82 0.02 areconsistentwithsupernova/plerionorigin.Morerecently,theMAGIC(MajorAtmospheric Gamma Imaging Cerenkov telescope) collaboration has reported a positive observations of | | 出版日期 | Book 2006 | | 關鍵詞 | Experimental Astrophysics; Flight systems for focusing telescopes; Focal plane instrumentation; Gamma-r | | 版次 | 1 | | doi | https://doi.org/10.1007/978-1-4020-5304-7 | | isbn_softcover | 978-94-017-8313-2 | | isbn_ebook | 978-1-4020-5304-7 | | copyright | Springer Science+Business Media B.V. 2006 |
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