6 August 2014 Acquiring multiple stars with the LINC-NIRVANA Pathfinder
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The LINC-NIRVANA Pathfinder1 (LN-PF), a ground-layer adaptive optics (AO) system recently commissioned at the Large Binocular Telescope (LBT), is one of 4 sensors that provide AO corrected images to the full LINC-NIRVANA instrument. With first light having taken place on November 17, 2013,2, 3 the core goals for the LN-PF have been accomplished. In this report, we look forward to one of the LN-PF extended goals. In particular, we review the acquisition mechanism required to place each of several star probes on its corresponding star in the target asterism. For emerging AO systems in general, co-addition of light from multiple stars stands as one of several methods being pursued to boost sky coverage. With 12 probes patrolling a large field of view (an annulus 6-arcminutes in diameter), the LN-PF will provide a valuable testbed to verify this method.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Albert R. Conrad, Albert R. Conrad, Carmelo Arcidiacono, Carmelo Arcidiacono, Harald Baumeister, Harald Baumeister, Maria Bergomi, Maria Bergomi, Thomas Bertram, Thomas Bertram, Jürgen Berwein, Jürgen Berwein, Florian Briegel, Florian Briegel, Jacopo Farinato, Jacopo Farinato, Tom Herbst, Tom Herbst, Ralph Hofferbert, Ralph Hofferbert, Frank Kittmann, Frank Kittmann, Martin Kürster, Martin Kürster, Derek Kopon, Derek Kopon, Luca Marafatto, Luca Marafatto, Mark Norris, Mark Norris, Roberto Ragazzoni, Roberto Ragazzoni, Valentina Viotto, Valentina Viotto, } "Acquiring multiple stars with the LINC-NIRVANA Pathfinder", Proc. SPIE 9149, Observatory Operations: Strategies, Processes, and Systems V, 91491O (6 August 2014); doi: 10.1117/12.2055648; https://doi.org/10.1117/12.2055648


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