Laboratory Results and Status Update for Pathfinder at LBT, The LINC-NIRVANA NGS Ground- Layer AO Subsystem
Derek Kopon, Al Conrad, Thomas Bertram, Tom Herbst, Martin K\"urster,, J\"urgen Berwein, Roberto Ragazzoni, Jacopo Farinato, Valentina Viotto, Maria, Bergomi, Ralf-Rainer Rohloff, Harald Baumeister, Fulvio De Bonis, Ralph, Hofferbert, Alessandro Brunelli, Carmelo Arcidiacono

TL;DR
This paper reports on the testing and status update of the Pathfinder subsystem, a ground-layer adaptive optics system for the LINC-NIRVANA instrument at LBT, highlighting its design, assembly, and initial alignment results.
Contribution
It provides the first on-sky testing results and system alignment details of the Pathfinder, a key subsystem for the complex LINC-NIRVANA AO system.
Findings
Successful assembly and optical alignment of the Pathfinder system.
Initial system tests demonstrate proper star enlarger and system alignment.
Plans for on-sky closed-loop tests scheduled for late Fall.
Abstract
The full LINC-NIRVANA instrument will be one of the most complex ground-based astronomical systems ever built. It will consist of multiple subsystems, including two multi-conjugate ground layer AO systems (MCAO) that drive the LBT adaptive secondaries, two mid-high layer AO systems with their own Xynetics 349 actuator DM's , a fringe tracker, a beam combiner, and the NIR science camera. In order to mitigate risk, we take a modular approach to instrument testing and commissioning by decoupling these subsystems individually. The first subsystem tested on-sky will be one of the ground-layer AO systems, part of a test-bed known as the Pathfinder. The Pathfinder consists of a 12-star pyramid wavefront sensor (PWFS) that drives one of the LBT's adaptive secondaries, a support structure known as "The Foot," and the infrared test camera (IRTC), which is used for acquisition and alignment. The…
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Taxonomy
TopicsAdaptive optics and wavefront sensing · Optical Systems and Laser Technology · Stellar, planetary, and galactic studies
