English

The eShel Spectrograph: A Radial-velocity Tool at the Wise Observatory

Instrumentation and Methods for Astrophysics 2017-05-03 v1 Solar and Stellar Astrophysics

Abstract

The eShel, an off-the-shelf, fiber-fed echelle spectrograph (R10,000R \approx 10,000), was installed on the 1m telescope at the Wise observatory in Israel. We report the installation of the multi-order spectrograph, and describe our pipeline to extract stellar radial velocity from the obtained spectra. We also introduce a new algorithm---UNICOR, to remove radial-velocity systematics that can appear in some of the observed orders. We show that the system performance is close to the photon-noise limit for exposures with more than 10710^7 counts, with a precision that can get better than 200 m/s for F--K stars, for which the eShel spectral response is optimal. This makes the eShel at Wise a useful tool for studying spectroscopic binaries brighter than mV=11m_V=11. We demonstrate this capability with orbital solutions of two binaries from projects being performed at Wise.

Keywords

Cite

@article{arxiv.1703.09937,
  title  = {The eShel Spectrograph: A Radial-velocity Tool at the Wise Observatory},
  author = {Michael Engel and Sahar Shahaf and Tsevi Mazeh},
  journal= {arXiv preprint arXiv:1703.09937},
  year   = {2017}
}

Comments

30 pages, 12 figures. Accepted for publication in PASP