Stellar Astrophysics with a Dispersed Fourier Transform Spectrograph. I. Instrument Description and Orbits of Single-lined Spectroscopic Binaries

TL;DR

This paper introduces the second-generation Dispersed Fourier Transform Spectrograph (dFTS2), detailing its design improvements, deployment on a telescope, and its application in precisely measuring stellar binary orbits.

Contribution

The paper presents the design, deployment, and application of dFTS2, a high-resolution spectrograph, achieving 0.1% accuracy in binary star orbit measurements, an improvement over previous methods.

Findings

Successful deployment of dFTS2 on the Bok Telescope.

Achieved high-precision radial velocity measurements.

Determined orbits for single-lined spectroscopic binaries.

Abstract

We have designed and constructed a second-generation version of the Dispersed Fourier Transform Spectrograph, or dFTS. This instrument combines a spectral interferometer with a dispersive spectrograph to provide high-accuracy, high-resolution optical spectra of stellar targets. The new version, dFTS2, is based upon the design of our prototype, with several modifications to improve the system throughput and performance. We deployed dFTS2 to the Steward Observatory 2.3-meter Bok Telescope from June 2007 to June 2008, and undertook an observing program on spectroscopic binary stars, with the goal of constraining the velocity amplitude K of the binary orbits with 0.1% accuracy, a significant improvement over most of the orbits reported in the literature. We present results for radial velocity reference stars and orbit solutions for single-lined spectroscopic binaries.