Paper
9 August 2016 Ultra-stable temperature and pressure control for the Habitable-zone Planet Finder spectrograph
Gudmundur K. Stefánsson, Frederick R. Hearty, Paul M. Robertson, Eric I. Levi, Suvrath Mahadevan, Tyler B. Anderson, Andrew J. Monson, Chad F. Bender, Samuel P. Halverson, Yiting Li, Lawrence W. Ramsey, Arpita Roy, Christian Schwab, Ryan C. Terrien, Matthew J. Nelson, Basil Blank
Author Affiliations +
Abstract
We present recent long-term stability test results of the cryogenic Environmental Control System (ECS) for the Habitable zone Planet Finder (HPF), a near infrared ultra-stable spectrograph operating at 180 Kelvin. Exquisite temperature and pressure stability is required for high precision radial velocity (< 1m=s) instruments, as temperature and pressure variations can easily induce instrumental drifts of several tens-to-hundreds of meters per second. Here we present the results from long-term stability tests performed at the 180K operating temperature of HPF, demonstrating that the HPF ECS is stable at the 0:6mK level over 15-days, and <10-7 Torr over months.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gudmundur K. Stefánsson, Frederick R. Hearty, Paul M. Robertson, Eric I. Levi, Suvrath Mahadevan, Tyler B. Anderson, Andrew J. Monson, Chad F. Bender, Samuel P. Halverson, Yiting Li, Lawrence W. Ramsey, Arpita Roy, Christian Schwab, Ryan C. Terrien, Matthew J. Nelson, and Basil Blank "Ultra-stable temperature and pressure control for the Habitable-zone Planet Finder spectrograph", Proc. SPIE 9908, Ground-based and Airborne Instrumentation for Astronomy VI, 990871 (9 August 2016); https://doi.org/10.1117/12.2233443
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Cited by 4 scholarly publications.
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KEYWORDS
Spectrographs

Control systems

Sensors

Planets

Near infrared

Doppler effect

Exoplanets

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