Pith. sign in

REVIEW

The GAMMA-400 space observatory: status and perspectives

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1412.4239 v1 pith:ZQFCOZ7K submitted 2014-12-13 physics.ins-det astro-ph.HEastro-ph.IM

The GAMMA-400 space observatory: status and perspectives

A.M. Galper , V. Bonvicini , N.P. Topchiev , O. Adriani , R.L. Aptekar , I.V. Arkhangelskaja , A.I. Arkhangelskiy , L. Bergstrom
show 59 more authors
E. Berti G. Bigongiari S.G. Bobkov M. Boezio E.A. Bogomolov S. Bonechi M. Bongi S. Bottai K.A. Boyarchuk G. Castellini P.W. Cattaneo P. Cumani G.L. Dedenko C. De Donato V.A. Dogiel M.S. Gorbunov Yu.V. Gusakov B.I. Hnatyk V.V. Kadilin V.A. Kaplin A.A. Kaplun M.D. Kheymits V.E. Korepanov J. Larsson A.A. Leonov V.A. Loginov F. Longo P. Maestro P.S. Marrocchesi V.V. Mikhailov E. Mocchiutti A.A. Moiseev N. Mori I.V. Moskalenko P.Yu. Naumov P. Papini M. Pearce P. Picozza A.V. Popov A. Rappoldi S. Ricciarini M.F. Runtso F. Ryde O.V. Serdin R. Sparvoli P. Spillantini S.I. Suchkov M. Tavani A.A. Taraskin A. Tiberio E.M. Tyurin M.V. Ulanov A. Vacchi E. Vannuccini G.I. Vasilyev Yu.T. Yurkin N. Zampa V.N. Zirakashvili V.G. Zverev
This is my paper
classification physics.ins-det astro-ph.HEastro-ph.IM
keywords observatorygamma-400raysallowbroadcosmicenergyextragalactic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The present design of the new space observatory GAMMA-400 is presented in this paper. The instrument has been designed for the optimal detection of gamma rays in a broad energy range (from ~100 MeV up to 3 TeV), with excellent angular and energy resolution. The observatory will also allow precise and high statistic studies of the electron component in the cosmic rays up to the multi TeV region, as well as protons and nuclei spectra up to the knee region. The GAMMA-400 observatory will allow to address a broad range of science topics, like search for signatures of dark matter, studies of Galactic and extragalactic gamma-ray sources, Galactic and extragalactic diffuse emission, gamma-ray bursts and charged cosmic rays acceleration and diffusion mechanism up to the knee.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.