Abstract
ABSTRACTThe Fan Mountain Near-Infrared Camera (FanCam) provides the University of Virginia’s 31 inch telescope with a near-infrared observing capability that is relatively unique among small-aperture telescopes. FanCam features an 8.7′ × 8.7′ field of view on a 1024 × 1024 Teledyne Imaging Sensors HAWAII-1 detector array. The instrument mounts at the f/15.5 focus of the 31 inch telescope. Its seeing-limited optical design, optimized for the JHK atmospheric bands, includes a field stop at the telescope focus, a doublet collimator, two eight-position filterwheels straddling a Lyot stop, and a doublet reimager. Four fold mirrors wrap the optical path onto a compact optical bench. The plate scale leads to a slightly oversampled point spread function for the typical seeing of 1.5″. The entire optical train is encased in a cryogenic dewar cooled by a closed-loop cooling system. This paper describes the optical, mechanical, cryogenic, and electronic design of the camera as well as some early results that illustrate the camera’s capabilities.
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