Paper
11 September 2015 Fluoride fiber thermal emission study for SPIRou @ CFHT
Yoan Micheau, Marc Bouyé, Jérôme Parisot, Driss Kouach
Author Affiliations +
Abstract
SPIRou is a near-IR (0.98-2.35μm), echelle spectropolarimeter / high precision velocimeter being designed as a nextgeneration instrument for the 3.6m Canada-France-Hawaii Telescope on Mauna Kea, Hawaii, with the main goal of detecting Earth-like planets around low mass stars and magnetic fields of forming stars. The SPIRou science fibers, which connect the polarimeter unit to the cryogenic spectrograph unit (35 meter apart), emit an undesirable thermal flux into the spectrograph, due to their intrinsic absorption. This may degrade the signal to noise ratio and then the sensitivity of the instrument for the reddest wavelengths. For verifying the calculation model used to predict the thermal emission from the SPIRou science fibers, a test bench is set-up at LESIA (Observatory of Paris). In this paper, the experimental approach to measure the thermal emission from a 30 meter long fluoride fiber @3μm is described. Experimental results are then compared to those predicted by the theoretical model.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yoan Micheau, Marc Bouyé, Jérôme Parisot, and Driss Kouach "Fluoride fiber thermal emission study for SPIRou @ CFHT", Proc. SPIE 9605, Techniques and Instrumentation for Detection of Exoplanets VII, 96051Q (11 September 2015); https://doi.org/10.1117/12.2185188
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Sensors

Thermal modeling

Fiber science

Cryogenics

Black bodies

Infrared detectors

Optical filters

Back to Top