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All-sky Medium Energy Gamma-ray Observatory: Exploring the Extreme Multimessenger Universe

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Ivan Agudo
  • Function : Author
Marco Ajello
  • Function : Author
Stefano Ansoldi
  • Function : Author
Sonia Anton
  • Function : Author
  • PersonId : 1050319
Natalia Auricchio
  • Function : Author
John B. Stephen
  • Function : Author
John Beacom
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Wlodek Bednarek
  • Function : Author
Denis Bernard
  • Function : Author
  • PersonId : 1082751
Eugenio Bottacini
  • Function : Author
Sara Buson
  • Function : Author
Riccardo Campana
  • Function : Author
Martina Cardillo
  • Function : Author
Ezio Caroli
  • Function : Author
Stefano del Sordo
  • Function : Author
Mattia Di Mauro
  • Function : Author
Seth W. Digel
  • Function : Author
  • PersonId : 839141
Michele Doro
  • Function : Author
Elizabeth Ferrara
  • Function : Author
Luca Foffano
  • Function : Author
Joseph Gelfand
Andrea Giuliani
  • Function : Author
Sean Griffin
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Sylvain Guiriec
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  • PersonId : 864501
Margarita Hernanz
  • Function : Author
Andrew Inglis
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Carolyn Kierans
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Joachim Kopp
  • Function : Author
John Krizmanic
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Amy Lien
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Tim Linden
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Jan Lommler
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Eileen Meyer
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Manuel Meyer
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Alexander Moiseev
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Uwe Oberlack
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Nepomuk Otte
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Maria Petropoulou
Martin Pohl
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Troy Porter
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Bindu Rani
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Marc Ribo
Pablo Saz Parkinson
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Chris Shrader
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Jacob Smith
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Antonio Stamerra
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Inga Stumke
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Hiro Tajima
  • Function : Author
Yasuyuki Tanaka
  • Function : Author
Lih-Sin The
  • Function : Author
Lucas Uhm
  • Function : Author
Zorawar Wadiasingh
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David Williams
Luca Zampieri
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Bing Zhang
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Stephan Zimmer
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Abstract

The All-sky Medium Energy Gamma-ray Observatory (AMEGO) is a probe class mission concept that will provide essential contributions to multimessenger astrophysics in the late 2020s and beyond. AMEGO combines high sensitivity in the 200 keV to 10 GeV energy range with a wide field of view, good spectral resolution, and polarization sensitivity. Therefore, AMEGO is key in the study of multimessenger astrophysical objects that have unique signatures in the gamma-ray regime, such as neutron star mergers, supernovae, and flaring active galactic nuclei. The order-of-magnitude improvement compared to previous MeV missions also enables discoveries of a wide range of phenomena whose energy output peaks in the relatively unexplored medium-energy gamma-ray band.

Dates and versions

in2p3-02194041 , version 1 (25-07-2019)

Identifiers

Cite

Julie Mcenery, Juan Abel Barrio, Ivan Agudo, Marco Ajello, José-Manuel Álvarez, et al.. All-sky Medium Energy Gamma-ray Observatory: Exploring the Extreme Multimessenger Universe. 2019. ⟨in2p3-02194041⟩
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