Published July 13, 2018 | Version Published
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The infrared Doppler (IRD) instrument for the Subaru telescope: instrument description and commissioning results

Abstract

The Infrared Doppler (IRD) instrument is a fiber-fed high-resolution NIR spectrometer for the Subaru telescope covering the Y,J,H-bands simultaneously with a maximum spectral resolution of 70,000. The main purpose of IRD is a search for Earth-mass planets around nearby M-dwarfs by precise radial velocity measurements, as well as a spectroscopic characterization of exoplanet atmospheres. We report the current status of the instrument, which is undergoing commissioning at the Subaru Telescope, and the first light observation successfully done in August 2017. The general description of the instrument will be given including spectrometer optics, fiber injection system, cryogenic system, scrambler, and laser frequency comb. A large strategic survey mainly focused on late-type M-dwarfs is planned to start from 2019.

Additional Information

© 2018 Society of Photo-optical Instrumentation Engineers (SPIE).

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Identifiers

Eprint ID
92170
Resolver ID
CaltechAUTHORS:20190109-111934554

Dates

Created
2019-01-09
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Updated
2021-11-16
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Series Name
Proceedings of SPIE
Series Volume or Issue Number
10702