Abstract
NIRPS (Near Infra-Red Planet Searcher) is an AO-assisted and fiber-fed spectrograph for high precision radial velocity measurements that will operate in the YJH-bands. While using an AO system in such instrument is generally considered to feed a single-mode fiber, NIRPS is following a different path by using a small multi-mode fiber (more specifically called "few-mode fiber"). This choice offers an excellent trade-off by allowing to design a compact cryogenic spectrograph, while maintaining a high coupling efficiency under bad seeing conditions and for faint stars. The main drawback resides in a much more important modal-noise, a problem that has to be tackled for allowing 1m/s precision radial velocity measurements. We study the impact of using an AO system to couple light into few-mode fibers. We focus on two aspects: the coupling efficiency into few-mode fibers and the question of modal noise and scrambling. We show First that NIRPS can reach coupling 50% up to magnitude I=12, and offer a gain of 1-2 magnitudes over a single-mode solution. We finally show that the best strategy to mitigate modal noise with the AO system is among the simplest: a continuous tip-tilt scanning of the fiber core.
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Blind, N., Conod, U., & Wildi, F. (2017). Few-mode fibers and AO-assisted high resolution spectroscopy: Coupling efficiency and modal noise mitigation. In Adaptive Optics for Extremely Large Telescopes, 2017 AO4ELT5 (Vol. 2017-June). Instituto de Astrofisica de Canarias. https://doi.org/10.26698/ao4elt5.0094
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