activity
20122020
most citedStatus of the GAMMA-400 Project

85 citations · 156 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2020★ 28 cited

Dark matter searches by the planned gamma-ray telescope GAMMA-400

Andrey E. Egorov, Nikolay P. Topchiev, Arkadiy M. Galper +4

Our paper reviews the planned space-based gamma-ray telescope GAMMA-400 and evaluates in details its opportunities in the field of dark matter (DM) indirect searches. We estimated…

astro-ph.IM2017

The high-performance data acquisition system for the GAMMA-400 satellite-borne gamma-ray telescope

A. V. Bakaldin, S. G. Bobkov, O. V. Serdin +4

The future GAMMA-400 space mission is aimed for the study of gamma rays in the energy range from ~20 MeV up to ~1 TeV. The observations will carry out with GAMMA-400 gamma-ray tele…

astro-ph.IM2015

Study of the Gamma-ray performance of the GAMMA-400 Calorimeter

P. Cumani, A. M. Galper, V. Bonvicini +73

GAMMA-400 is a new space mission, designed as a dual experiment, capable to study both high energy gamma rays (from 100 MeV to few TeV) and cosmic rays (electrons up to 20 Te…

astro-ph.IM2013★ 9 cited

The Space-Based Gamma-Ray Telescope GAMMA-400 and Its Scientific Goals

A. M. Galper, O. Adriani, R. L. Aptekar +46

The design of the new space-based gamma-ray telescope GAMMA-400 is presented. GAMMA-400 is optimized for the energy 100 GeV with the best parameters: the angular resolution ~0.01 d…

astro-ph.IM2012★ 34 cited

Design and Performance of the GAMMA-400 Gamma-Ray Telescope for the Dark Matter Searches

A. M. Galper, O. Adriani, R. L. Aptekar +37

The GAMMA-400 gamma-ray telescope is designed to measure the fluxes of gamma rays and cosmic-ray electrons + positrons, which can be produced by annihilation or decay of the dark m…

astro-ph.IM2012★ 85 cited

Status of the GAMMA-400 Project

A. M. Galper, O. Adriani, R. L. Aptekar +35

The preliminary design of the new space gamma-ray telescope GAMMA-400 for the energy range 100 MeV - 3 TeV is presented. The angular resolution of the instrument, 1-2° at Eγ ~100 M…