Pith. sign in

REVIEW

GAMMA-400 gamma-ray observatory

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 1507.06246 v3 pith:GVNYES6F submitted 2015-07-22 astro-ph.IM

GAMMA-400 gamma-ray observatory

N.P. Topchiev , A.M. Galper , V. Bonvicini , O. Adriani , R.L. Aptekar , I.V. Arkhangelskaja , A.I. Arkhangelskiy , A.V. Bakaldin
show 66 more authors
L. Bergstrom E. Berti G. Bigongiari S.G. Bobkov M. Boezio E.A. Bogomolov L. Bonechi M. Bongi S. Bottai G. Castellini P.W. Cattaneo P. Cumani O.D. Dalkarov G.L. Dedenko C. De Donato V.A. Dogiel N. Finetti D. Gascon 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 M. Martinez A.L. Menshenin V.V. Mikhailov E. Mocchiutti A.A. Moiseev N. Mori I.V. Moskalenko P.Yu. Naumov P. Papini J.M. Paredes M. Pearce P. Picozza A. Rappoldi S. Ricciarini M.F. Runtso F. Ryde O.V. Serdin R. Sparvoli P. Spillantini Yu.I. Stozhkov S.I. Suchkov A.A. Taraskin M. Tavani A. Tiberio E.M. Tyurin M.V. Ulanov A. Vacchi E. Vannuccini G.I. Vasilyev J.E. Ward Yu.T. Yurkin N. Zampa V.N. Zirakashvili V.G. Zverev
This is my paper
classification astro-ph.IM
keywords gamma-raygamma-400emissionenergywillangularelectronsfluxes
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electrons + positrons. Precision investigations of gamma-ray emission from Galactic Center, Crab, Vela, Cygnus, Geminga, and other regions will be performed, as well as diffuse gamma-ray emission, along with measurements of high-energy electron + positron and nuclei fluxes. Furthermore, it will study gamma-ray bursts and gamma-ray emission from the Sun during periods of solar activity. The energy range of GAMMA-400 is expected to be from ~20 MeV up to TeV energies for gamma rays, up to 20 TeV for electrons + positrons, and up to 10E15 eV for cosmic-ray nuclei. For high-energy gamma rays with energy from 10 to 100 GeV, the GAMMA-400 angular resolution improves from 0.1{\deg} to ~0.01{\deg} and energy resolution from 3% to ~1%; the proton rejection factor is ~5x10E5. GAMMA-400 will be installed onboard the Russian space observatory.

discussion (0)

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