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Atmospheric Response for MeV γ Rays Observed with Balloon-borne Detectors

The atmospheric response for MeV γ rays (∼0.1–10 MeV) can be characterized in terms of two observed components. The first component is due to photons that reach the detector without scattering. The second component is due to photons that reach the detector after scattering one or more times. While t...

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Uloženo v:
Hlavní autoři: Christopher M. Karwin, Carolyn Kierans, Albert Y. Shih, Israel Martinez Castellanos, Alex Lowell, Thomas Siegert, Jarred Roberts, Savitri Gallego, Adrien Laviron, Andreas Zoglauer, John A. Tomsick, Steven E. Boggs, for the COSI Collaboration
Médium: Artigo
Jazyk:Inglês
Vydáno: IOP Publishing 2024-01-01
Edice:The Astrophysical Journal
Témata:
Gamma-rays
High altitude balloons
Atmospheric effects
High energy astrophysics
On-line přístup:https://doi.org/10.3847/1538-4357/ad6758
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