The Measured Impact of Chromatic Atmospheric Effects on Barycentric Corrections: Results from the EXtreme PREcision Spectrograph
Abstract
One source of error in high-precision radial velocity measurements of exoplanet host stars is chromatic change in Earth’s atmospheric transmission during observations. Mitigation of this error requires that the photon-weighted barycentric correction be applied as a function of wavelength across the stellar spectrum. We have designed a system for chromatic photon-weighted barycentric corrections with the EXtreme PREcision Spectrograph and present results from the first year of operations, based on radial velocity measurements of more than 103 high-resolution stellar spectra. For observation times longer than 250 s, we find that if the chromatic component of the barycentric corrections is ignored, a range of radial velocity errors up to 1 m s-1 can be incurred with cross-correlation, depending on the nightly atmospheric conditions. For this distribution of errors, the standard deviation is 8.4 cm s-1 for G-type stars, 8.5 cm s-1 for K-type stars, and 2.1 cm s-1 for M-type stars. This error is reduced to well-below the instrumental and photon-noise limited floor by frequent flux sampling of the observed star with a low-resolution exposure meter spectrograph.
- Publication:
-
The Astronomical Journal
- Pub Date:
- July 2019
- DOI:
- 10.3847/1538-3881/ab24c3
- arXiv:
- arXiv:1906.01653
- Bibcode:
- 2019AJ....158...40B
- Keywords:
-
- atmospheric effects;
- instrumentation: spectrographs;
- techniques: radial velocities;
- Astrophysics - Earth and Planetary Astrophysics;
- Astrophysics - Instrumentation and Methods for Astrophysics
- E-Print:
- 11 pages, 7 figures, accepted to AJ