Modal Noise Mitigation through Fiber Agitation for Fiber-fed Radial Velocity Spectrographs
Ryan R. Petersburg, Tyler M. McCracken, Dominic Eggerman, Colby A., Jurgenson, David Sawyer, Andrew E. Szymkowiak, and Debra A. Fischer

TL;DR
This paper investigates fiber agitation techniques to reduce modal noise in high-precision spectrographs, finding that quasi-chaotic motion of high-amplitude agitators effectively suppresses noise and improves radial velocity measurements.
Contribution
It explores and optimizes fiber agitation parameters, introducing a new agitation method that significantly reduces modal noise and RV errors in spectrographs.
Findings
Quasi-chaotic agitation best suppresses modal noise.
New agitator design reduces RV error to below 3.2 cm/s.
Optimized agitation improves high-precision spectroscopic measurements.
Abstract
Optical fiber modal noise is a limiting factor for high precision spectroscopy signal-to-noise in the near-infrared and visible. Unabated, especially when using highly coherent light sources for wavelength calibration, modal noise can induce radial velocity (RV) errors that hinder the discovery of low-mass (and potentially Earth-like) planets. Previous research in this field has found sufficient modal noise mitigation through the use of an integrating sphere, but this requires extremely bright light sources, a luxury not necessarily afforded by the next generation of high-resolution optical spectrographs. Otherwise, mechanical agitation, which "mixes" the fiber's modal patterns and allows the noise to be averaged over minutes-long exposures, provides some noise reduction but the exact mechanism behind improvement in signal-to-noise and RV drift has not been fully explored or optimized…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
