OSIRIS – The Scientific Camera System Onboard Rosetta

By H. Keller, C. Barbieri, P. Lamy, H. Rickman, R. Rodrigo, K. Wenzel, H. Sierks, M. A’Hearn, F. Angrilli, M. Angulo and 59 more. 2007

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Insolation, erosion, and morphology of comet 67P/Churyumov-Gerasimenko (2015, methodology): “The scientific optical camera system OSIRIS comprises the Narrow Angle Camera (NAC) and the Wide Angle Camera (WAC; Keller et al. 2007).”
EVOLUTION OF THE DUST SIZE DISTRIBUTION OF COMET 67P/CHURYUMOV–GERASIMENKO FROM 2.2 au TO PERIHELION (2016, methodology): “Detections of dust particles by the GIADA instrument (Colangeli et al. 2007; Della Corte et al. 2014) and by the OSIRIS Narrow Angle Camera (NAC, Keller et al. 2007) in the coma of 67P have already allowed us to measure the dust size distribution over eight mass bins, from 10−10 to 10−2 kg when the…”
Redistribution of particles across the nucleus of comet 67P/Churyumov-Gerasimenko (2015, background): “The OSIRIS observations suggest that these ideas are of considerable importance.”
Shape model, reference system definition, and cartographic mapping standards for comet 67P/Churyumov-Gerasimenko Stereo-photogrammetric analysis of Rosetta/OSIRIS image data (2015, methodology): “Within the first month of the comet-characterization phase, the Optical, Spectroscopic and Infrared Remote Imaging System (OSIRIS) camera system (Keller et al. 2007) acquired several hundred images of the illuminated surface of 67P (mainly on the northern hemisphere) using the Narrow Angle Camera…”