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عنوان
Science with e-ASTROGAM:
پدید آورنده
De Angelis, A; Tatischeff, V; Grenier, IA; McEnery, J; Mallamaci, M; Tavani, M; Oberlack, U; Hanlon, L; Walter, R; Argan, A; Von Ballmoos, P; Bulgarelli, A; Bykov, A; Hernanz, M; Kanbach, G; Kuvvetli, I; Pearce, M; Zdziarski, A; Conrad, J; Ghisellini, G; Harding, A; Isern, J; Leising, M; Longo, F; Madejski, G; Martinez, M; et al.
موضوع
رده
کتابخانه
مرکز و کتابخانه مطالعات اسلامی به زبانهای اروپایی
محل استقرار
استان:
قم
ـ شهر:
قم
تماس با کتابخانه :
32910706
-
025
شماره کتابشناسی ملی
شماره
LA0zq3338p
عنوان و نام پديدآور
عنوان اصلي
Science with e-ASTROGAM:
نام عام مواد
[Article]
نام نخستين پديدآور
De Angelis, A; Tatischeff, V; Grenier, IA; McEnery, J; Mallamaci, M; Tavani, M; Oberlack, U; Hanlon, L; Walter, R; Argan, A; Von Ballmoos, P; Bulgarelli, A; Bykov, A; Hernanz, M; Kanbach, G; Kuvvetli, I; Pearce, M; Zdziarski, A; Conrad, J; Ghisellini, G; Harding, A; Isern, J; Leising, M; Longo, F; Madejski, G; Martinez, M; et al.
عنوان اصلي به قلم نويسنده ديگر
A space mission for MeV-GeV gamma-ray astrophysics
یادداشتهای مربوط به خلاصه یا چکیده
متن يادداشت
© 2018 Elsevier B.V. e-ASTROGAM ('enhanced ASTROGAM') is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated to the study of the non-thermal Universe in the photon energy range from 0.3 MeV to 3 GeV - the lower energy limit can be pushed to energies as low as 150 keV for the tracker, and to 30 keV for calorimetric detection. The mission is based on an advanced space-proven detector technology, with unprecedented sensitivity, angular and energy resolution, combined with polarimetric capability. Thanks to its performance in the MeV-GeV domain, substantially improving its predecessors, e-ASTROGAM will open a new window on the non-thermal Universe, making pioneering observations of the most powerful Galactic and extragalactic sources, elucidating the nature of their relativistic outflows and their effects on the surroundings. With a line sensitivity in the MeV energy range one to two orders of magnitude better than previous generation instruments, e-ASTROGAM will determine the origin of key isotopes fundamental for the understanding of supernova explosion and the chemical evolution of our Galaxy. The mission will provide unique data of significant interest to a broad astronomical community, complementary to powerful observatories such as LIGO-Virgo-GEO600-KAGRA, SKA, ALMA, E-ELT, TMT, LSST, JWST, Athena, CTA, IceCube, KM3NeT, and LISA.
مجموعه
تاريخ نشر
2018
عنوان
UC Santa Cruz
دسترسی و محل الکترونیکی
نام الکترونيکي
مطالعه متن کتاب
اطلاعات رکورد کتابشناسی
نوع ماده
[Article]
کد کاربرگه
275578
اطلاعات دسترسی رکورد
سطح دسترسي
a
تكميل شده
Y
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