A System for Generating the Trigger Signals of the Spaceborne GAMMA-400 Telescope


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The GAMMA-400 space project is one of the new generation of space observatories designed to search for signs of dark matter in the cosmic gamma emission, and to measure the characteristics of diffuse gamma-ray emission and gamma-rays from the Sun during periods of solar activity; gamma-ray bursts; extended and point gamma-ray sources; and electron, positron, and cosmic-ray nuclei fluxes with energies in the TeV ranges. The GAMMA-400 γ-ray telescope constitutes the core of the scientific instrumentation. The nature of the intended experiments imposes stringent requirements on the gamma telescope’s system of trigger signal formation, now being developed using the state-of-the-art logic devices and fast data links. The design concept of the system is discussed, along with the chosen engineering solutions and some experimental results obtained during the operation of the system prototype using a positron beam with energies of 100–300 MeV from the PAKHRA S-25R synchrotron at the Lebedev Physical Institute.

Sobre autores

A. Arkhangelskiy

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Autor responsável pela correspondência
Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991; Moscow, 115409

A. Galper

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991; Moscow, 115409

I. Arkhangelskaja

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 115409

A. Bakaldin

Lebedev Physical Institute, Russian Academy of Sciences; Scientific Research Institute of System Analysis, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991; Moscow, 117218

Yu. Gusakov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

O. Dalkarov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

A. Egorov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

V. Zverev

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

A. Leonov

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991; Moscow, 115409

N. Pappe

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

M. Runtso

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 115409

Yu. Stozhkov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

S. Suchkov

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

N. Topchiev

Lebedev Physical Institute, Russian Academy of Sciences

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991

M. Kheymits

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 115409

E. Chasovikov

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 115409

I. Chernysheva

Lebedev Physical Institute, Russian Academy of Sciences; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 119991; Moscow, 115409

Yu. Yurkin

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: AIArkhangelskij@mephi.ru
Rússia, Moscow, 115409

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