KEYWORDS: Sensors, Metrology, Large Synoptic Survey Telescope, Cameras, Distortion, Temperature metrology, Data acquisition, Active optics, Kinematics, Actuators
Meeting the science goals for the Large Synoptic Survey Telescope (LSST) translates into a demanding set of
imaging performance requirements for the optical system over a wide (3.5°) field of view. In turn, meeting those
imaging requirements necessitates maintaining precise control of the focal plane surface (10 μm P-V) over the
entire field of view (640 mm diameter) at the operating temperature (T ~ -100°C) and over the operational
elevation angle range. We briefly describe the heirarchical design approach for the LSST Camera focal plane and
the baseline design for assembling the flat focal plane at room temperature. Preliminary results of gravity load
and thermal distortion calculations are provided, and early metrological verification of candidate materials under
cold thermal conditions are presented. A detailed, generalized method for stitching together sparse metrology
data originating from differential, non-contact metrological data acquisition spanning multiple (non-continuous)
sensor surfaces making up the focal plane, is described and demonstrated. Finally, we describe some in situ
alignment verification alternatives, some of which may be integrated into the camera's focal plane.
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