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The Double-Sided Silicon Strip Detector Tracker onboard the ComPair Balloon Flight

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arxiv 2407.18737 v1 pith:NYB3IVWI submitted 2024-07-26 astro-ph.IM

classification astro-ph.IM
keywords trackercompairdetectorenergyballoonsiliconamegocalorimeter
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The ComPair balloon instrument is a prototype of the All-sky Medium Energy Gamma-ray Observatory (AMEGO) mission concept. AMEGO aims to bridge the spectral gap in sensitivity that currently exists from $\sim$100 keV to $\sim$100 MeV by being sensitive to both Compton and pair-production events. This is made possible through the use of four subsystems working together to reconstruct events: a double-sided silicon strip detector (DSSD) Tracker, a virtual Frisch grid cadmium zinc telluride (CZT) Low Energy Calorimeter, a ceasium iodide (CsI) High Energy Calorimeter, and an anti-coincidence detector (ACD) to reject charged particle backgrounds. Composed of 10 layers of DSSDs, ComPair's Tracker is designed to measure the position of photons that Compton scatter in the silicon, as well as reconstruct the tracks of electrons and positrons from pair-production as they propagate through the detector. By using these positions, as well as the absorbed energies in the Tracker and 2 Calorimeters, the energy and direction of the incident photon can be determined. This proceeding will present the development, testing, and calibration of the ComPair DSSD Tracker and early results from its balloon flight in August 2023.

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  1. Background Measurements and Simulations of the ComPair Balloon Flight

    astro-ph.IM 2025-06 conditional novelty 6.0 of 10

    ComPair's first balloon flight measured the gamma-ray background at 40 km and matched Monte Carlo simulations, validating the detector's charged-particle rejection and event reconstruction.

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