142 citations · 400 across the 12 of their papers we have counts for
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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…
Galactic Sources Detected in the NuSTAR Serendipitous Survey
John A. Tomsick, George B. Lansbury, Farid Rahoui +13
The Nuclear Spectroscopic Telescope Array (NuSTAR) provides an improvement in sensitivity at energies above 10 keV by two orders of magnitude over non-focusing satellites, making i…
The NuSTAR Hard X-ray Survey of the Norma Arm Region
Francesca M. Fornasini, John A. Tomsick, JaeSub Hong +32
We present a catalog of hard X-ray sources in a square-degree region surveyed by NuSTAR in the direction of the Norma spiral arm. This survey has a total exposure time of 1.7 Ms, a…
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…