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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Veröffentlicht in:	The Astrophysical journal 2024-10, Vol.974 (1), p.146
Hauptverfasser:	Karwin, Christopher M., Kierans, Carolyn, Shih, Albert Y., Martinez Castellanos, Israel, Lowell, Alex, Siegert, Thomas, Roberts, Jarred, Gallego, Savitri, Laviron, Adrien, Zoglauer, Andreas, Tomsick, John A., Boggs, Steven E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Airborne observation Atmosphere Atmospheric effects Balloons Gamma-rays High altitude balloons High energy astrophysics Photons Point sources Scattering
Online-Zugang:	Volltext
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