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The project of all-sky hard X-ray and soft gamma-ray monitoring on-board international space stationстатья
Информация о цитировании статьи получена из
Web of Science,
Scopus
Дата последнего поиска статьи во внешних источниках: 29 мая 2015 г.
- Авторы: Kudryavtsev M.I., Svertilov S.I., Bogomolov V.V., Bogomolov A.V.
- Сборник: X-RAY TIMING AND COSMIC GAMMA RAY BURSTS
- Серия: ADVANCES IN SPACE RESEARCH
- Том: 22
- Год издания: 1998
- Первая страница: 1057
- Последняя страница: 1060
- DOI: 10.1016/S0273-1177(98)00143-4
- Аннотация: Further progress in hard X-ray and soft gamma-ray observations can be achieved in the experiments with wide-field code-aperture instruments, which allow, due to long exposure times, to achieve the timing of different astrophysical objects (possible even in the near-Earth missions). The deep all-sky survey at the level of registration similar to 100 new sources (mainly Active Galactic Nuclei) in the energy range similar to 0.3-1 MeV is possible in the observations made during similar to 10 years with the instrument with similar to 2 pi FOV, similar to 1000-3000 cm(2) effective area and similar to 3 degrees-5 degrees angular resolution. The gamma-telescope "Gammascope" with such characteristics is now being elaborated. It is proposed for the experiment on the International Orbital Station "Alpha". The instrument is based on a combination of the quasi-spherical coding-mask and NaI-CsI position-sensitive detector (PSD). (C) 1998 COSPAR. Published by Elsevier Science Ltd.
- Добавил в систему: Свертилов Сергей Игоревич