Paper
13 September 2007 The Lunar Occultation Observer (LOCO) mission concept
Author Affiliations +
Abstract
The hard X-ray sky has tremendous potential for future discoveries and is one of the last electromagnetic regimes without a sensitive all-sky survey. A new approach to such a survey is to utilize the Moon as an occulting disk. The Lunar Occultation Observer (LOCO) mission concept, based on this Lunar Occultation Technique (LOT) and incorporating advanced inorganic scintillators as a detection medium, represents a sensitive and cost effective option for NASA's Beyond Einstein Black Hole Finder Probe or a future Explorer-class mission. We present the motivating factors for the LOT, outline developmental details and simulation results, as well as give preliminary estimates for source detection sensitivity.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Richard S. Miller "The Lunar Occultation Observer (LOCO) mission concept", Proc. SPIE 6686, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XV, 66860D (13 September 2007); https://doi.org/10.1117/12.735766
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KEYWORDS
Space operations

Hard x-rays

X-rays

Spectroscopy

Scintillators

Sensors

Monte Carlo methods

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