Search Results - "Lowell, Alexander W"
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Benchmarking simulations of the Compton Spectrometer and Imager with calibrations
Published in Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment (01-12-2019)“…The Compton Spectrometer and Imager (COSI) is a balloon-borne γ-ray (0.2-5 MeV) telescope designed to study astrophysical sources. COSI employs a compact…”
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Polarimetric Analysis of the Long Duration Gamma-Ray Burst GRB 160530A With the Balloon Borne Compton Spectrometer and Imager
Published in The Astrophysical journal (20-10-2017)“…A long duration gamma-ray burst, GRB 160530A, was detected by the Compton Spectrometer and Imager (COSI) during the 2016 COSI Super Pressure Balloon campaign…”
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Benchmarking simulations of the Compton Spectrometer and Imager with calibrations
Published 08-11-2019“…Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Volume 946, 2019, 162643, ISSN…”
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Maximum Likelihood Compton Polarimetry with the Compton Spectrometer and Imager
Published 15-09-2017“…Astrophysical polarization measurements in the soft gamma-ray band are becoming more feasible as detectors with high position and energy resolution are…”
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Polarimetric Analysis of the Long Duration Gamma Ray Burst GRB 160530A With the Balloon Borne Compton Spectrometer and Imager
Published 15-09-2017“…A long duration gamma-ray burst, GRB 160530A, was detected by the Compton Spectrometer and Imager (COSI) during the 2016 COSI Super Pressure Balloon campaign…”
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Positron clouds within thunderstorms
Published 14-05-2015“…J. Plasma Phys. 81 (2015) 475810405 We report the observation of two isolated clouds of positrons inside an active thunderstorm. These observations were made…”
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XMM-Newton Finds That SAX J1750.8-2900 May Harbor the Hottest, Most Luminous Known Neutron Star
Published 14-02-2012“…We have performed the first sensitive X-ray observation of the low-mass X-ray binary SAX J1750.8-2900 in quiescence with XMM-Newton. The spectrum was fit to…”
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