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Near-infrared calibration systems for precise radial-velocity measurements

Published

Author(s)

Stephen L. Redman, Florian Kerber, Gillian Nave, Suvrath Mahadevan, Lawrence W. Ramsey, Jonathan Smoker, H-U Kaufl, Pedro Figueira

Abstract

We present work done to prepare two new near-infrared calibration sources for use on high-precision astrophysical spectrographs. Uranium-neon is an atomic calibration source, commercially available as a hollow-cathode lamp, with over 10 000 known emission lines between 0.85 and 4 ìm. Four gas cells — containing acetylene, H13CN, 12CO, and 13CO, respectively — are available as National Institute of Standards and Technology (nist)Standard Reference Materials (SRMs), and provide narrow absorption lines between 1.5 and 1.65 ìm. These calibration sources may prove useful for wavelength-calibrating the future near-infrared high-precision radialvelocity spectrometers, including the Calar Alto high-Resolution search for M dwarfs with Exo-earths with a Near-infrared Echelle Spectrograph (CARMENES)1 and the Habitable-Zone Planet Finder (HPF).2
Proceedings Title
Proceedings of SPIE
Volume
8446
Conference Dates
July 1-6, 2012
Conference Location
Amsterdam, NL
Conference Title
SPIE Astronomical Telescopes and Instrumentation

Keywords

near infrared, calibration, radial velocities, atomic spectra, molecular spectra, exoplanets

Citation

Redman, S. , Kerber, F. , Nave, G. , Mahadevan, S. , Ramsey, L. , Smoker, J. , Kaufl, H. and Figueira, P. (2012), Near-infrared calibration systems for precise radial-velocity measurements, Proceedings of SPIE, Amsterdam, NL, [online], https://doi.org/10.1117/12.925585 (Accessed May 21, 2024)

Issues

If you have any questions about this publication or are having problems accessing it, please contact reflib@nist.gov.

Created September 24, 2012, Updated July 18, 2023