Ultra-Stable Environment Control for the NEID Spectrometer: Design and Performance Demonstration
Paul Robertson, Tyler Anderson, Gudmundur Stefansson, Frederick R., Hearty, Andrew Monson, Suvrath Mahadevan, Scott Blakeslee, Chad Bender, Joe, P. Ninan, David Conran, Eric Levi, Emily Lubar, Amanda Cole, Adam Dykhouse,, Shubham Kanodia, Colin Nitroy, Joseph Smolsky

TL;DR
This paper details the design and performance of an ultra-stable environment control system for the NEID spectrometer, achieving sub-milliKelvin temperature stability crucial for precise stellar radial velocity measurements in exoplanet research.
Contribution
It introduces an improved, open-source environment control system for NEID, demonstrating stability surpassing previous systems like HPF for high-precision spectrometry.
Findings
Achieved RMS temperature stability better than 0.4 mK over 30 days.
Maintained vacuum pressures below 10^-6 Torr.
System exceeds performance of previous similar systems.
Abstract
Two key areas of emphasis in contemporary experimental exoplanet science are the detailed characterization of transiting terrestrial planets, and the search for Earth analog planets to be targeted by future imaging missions. Both of these pursuits are dependent on an order-of-magnitude improvement in the measurement of stellar radial velocities (RV), setting a requirement on single-measurement instrumental uncertainty of order 10 cm/s. Achieving such extraordinary precision on a high-resolution spectrometer requires thermo-mechanically stabilizing the instrument to unprecedented levels. Here, we describe the Environment Control System (ECS) of the NEID Spectrometer, which will be commissioned on the 3.5 m WIYN Telescope at Kitt Peak National Observatory in 2019, and has a performance specification of on-sky RV precision < 50 cm/s. Because NEID's optical table and mounts are made from…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Spectroscopy and Laser Applications · Astronomy and Astrophysical Research
