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The SOFIA Observatory at the Start of Routine Science Operations : Mission capabilities and performance

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arxiv 1405.7390 v1 pith:X3XCUDRQ submitted 2014-05-28 astro-ph.IM

The SOFIA Observatory at the Start of Routine Science Operations : Mission capabilities and performance

classification astro-ph.IM
keywords observatoryperformanceevaluationimagepointingsofiawelladditional
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Stratospheric Observatory for Infrared Astronomy (SOFIA) has recently concluded a set of engineering flights for Observatory performance evaluation. These in-flight opportunities are viewed as a first comprehensive assessment of the Observatory's performance and are used to guide future development activities, as well as to identify additional Observatory upgrades. Pointing stability was evaluated, including the image motion due to rigid-body and flexible-body telescope modes as well as possible aero-optical image motion. We report on recent improvements in pointing stability by using an active mass damper system installed on the telescope. Measurements and characterization of the shear layer and cavity seeing, as well as image quality evaluation as a function of wavelength have also been performed. Additional tests targeted basic Observatory capabilities and requirements, including pointing accuracy, chopper evaluation and imager sensitivity. This paper reports on the data collected during these flights and presents current SOFIA Observatory performance and characterization.

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