4 August 2016 Development and construction of MAROON-X
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We report on the development and construction of a new fiber-fed, red-optical, high-precision radial-velocity spectrograph for one of the twin 6.5m Magellan Telescopes in Chile. MAROON-X will be optimized to find and characterize rocky planets around nearby M dwarfs with an intrinsic per measurement noise floor below 1ms-1. The instrument is based on a commercial echelle spectrograph customized for high stability and throughput. A microlens array based pupil slicer and double scrambler, as well as a rubidium-referenced etalon comb calibrator will turn this spectrograph into a high-precision radial-velocity machine. MAROON-X will undergo extensive lab tests in the second half of 2016.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andreas Seifahrt, Andreas Seifahrt, Jacob L. Bean, Jacob L. Bean, Julian Stürmer, Julian Stürmer, Luke Gers, Luke Gers, Deon S. Grobler, Deon S. Grobler, Tony Reed, Tony Reed, Damien J. Jones, Damien J. Jones, "Development and construction of MAROON-X", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 990818 (4 August 2016); doi: 10.1117/12.2232069; https://doi.org/10.1117/12.2232069

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