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Maximum Likelihood Compton Polarimetry with the Compton Spectrometer and Imager
Alexander W. Lowell, Steven E. Boggs, Jeng-Lun Chiu +11
Astrophysical polarization measurements in the soft gamma-ray band are becoming more feasible as detectors with high position and energy resolution are deployed. Previous work has…
A Combined Compton and Coded-aperture Telescope for Medium-energy Gamma-ray Astrophysics
Michelle Galloway, Andreas Zoglauer, Steven E. Boggs +1
A future mission in medium-energy gamma-ray astrophysics would allow for many scientific advancements, e.g. a possible explanation for the excess positron emission from the Galacti…
Benchmarking COSI's detector effects engine
Clio C. Sleator, Steven E. Boggs, Jeng-Lun Chiu +11
The Compton Spectrometer and Imager (COSI) is a balloon-borne gamma-ray (0.2-5 MeV) telescope with inherent sensitivity to polarization. COSI's main goal is to study astrophysical…
The 2016 Super Pressure Balloon flight of the Compton Spectrometer and Imager
Carolyn A. Kierans, Steven E. Boggs, Jeng-Lun Chiu +11
The Compton Spectrometer and Imager (COSI) is a balloon-borne, soft-gamma ray imager, spectrometer, and polarimeter with sensitivity from 0.2 to 5 MeV. Utilizing a compact Compton…