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24 September 2012 On-sky operations and performance of LMIRcam at the Large Binocular Telescope
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The L/M-band (3−5 μm) InfraRed Camera (LMIRcam) sits at the combined focal plane of the Large Binocular Telescope Interferometer (LBTI), ultimately imaging the coherently combined focus of the LBT’s two 8.4-meter mirrors. LMIRcam achieved first light at the LBT in May 2011 using a single AO-enabled 8.4-meter aperture. With the delivery of LBT’s final adaptive secondary mirror in Fall of 2011, dual-aperture AO-corrected interferometric fringes were realized in April 2012. We report on the performance of these configurations and characterize the noise performance of LMIRcam’s HAWAII-2RG 5.3-μm cutoff array paired with Cornell FORCAST readout electronics. In addition, we describe recent science highlights and discuss future improvements to the LMIRcam hardware.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J. M. Leisenring, M. F. Skrutskie, P. M. Hinz, A. Skemer, V. Bailey, J. Eisner, P. Garnavich, W. F. Hoffmann, T. Jones, M. Kenworthy, P. Kuzmenko, M. Meyer, M. Nelson, T. J. Rodigas, J. C. Wilson, and V. Vaitheeswaran "On-sky operations and performance of LMIRcam at the Large Binocular Telescope", Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 84464F (24 September 2012);


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