Estimation of the detected background by the future gamma ray transient mission CAMELOT-Reference-Cited by-同舟云学术

Estimation of the detected background by the future gamma ray transient mission CAMELOT

Published:2019-08 Issue:7 Volume:340 Page:666-673
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr

Author:

Řípa Jakub¹²³,Galgóczi Gábor²,Werner Norbert¹⁴⁵,Pál András⁶,Ohno Masanori¹²⁵⁶,Mészáros László⁶,Mizuno Tsunefumi⁷,Tarcai Norbert⁸,Torigoe Kento⁵,Uchida Nagomi⁵,Fukazawa Yasushi⁵,Takahashi Hiromitsu⁵,Nakazawa Kazuhiro⁹,Hirade Naoyoshi⁵,Hirose Kengo⁵,Hisadomi Syohei⁹,Enoto Teruaki¹⁰,Odaka Hirokazu¹¹,Ichinohe Yuto¹²,Frei Zsolt²,Kiss László⁶

Affiliation:

1. MTA‐Eötvös University Lendület Hot Universe Research Group Budapest Hungary

2. Institute of PhysicsEötvös University Budapest Hungary

3. Astronomical InstituteCharles University Prague Czech Republic

4. Department of Theoretical Physics and Astrophysics, Faculty of ScienceMasaryk University Brno Czech Republic

5. School of ScienceHiroshima University Higashi‐Hiroshima Japan

6. Konkoly Observatory of the Hungarian Academy of Sciences Budapest Hungary

7. Hiroshima Astrophysical Science CenterHiroshima University Higashi‐Hiroshima Japan

8. C3S Electronics Development LLC Budapest Hungary

9. Department of PhysicsNagoya University Nagoya Japan

10. The Hakubi Center for Advanced Research and Department of AstronomyKyoto University Kyoto Japan

11. Department of PhysicsUniversity of Tokyo Tokyo Japan

12. Department of PhysicsRikkyo University Tokyo Japan

Funder

European Social Fund

Magyar Tudományos Akadémia

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.201913673

Reference53 articles.

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4. Protons in near earth orbit

5. Leptons in near earth orbit

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