BACHES - a compact \'echelle spectrograph for radial velocity surveys with small telescopes

TL;DR

The paper evaluates BACHES, a compact echelle spectrograph, demonstrating its effectiveness for radial velocity surveys of binary stars using small, remote telescopes, enabling new research opportunities.

Contribution

It introduces and tests a new compact spectrograph, BACHES, showing its suitability for autonomous radial velocity measurements on small telescopes.

Findings

Capable of observing 10 mag targets with SNR of 20 in 30 minutes

Suitable for remote, autonomous operation with small telescopes

Provides a cost-effective solution for binary star radial velocity surveys

Abstract

We evaluate a pre-production BACHES \'{e}chelle spectrograph in terms of its usefulness for radial velocity surveys of binary stars with small telescopes in a remote and autonomous. We use the Solaris-4 observatory located in Casleo, Argentina, that is part of a global network of autonomous observatories as the test-bed for the instrument. The setup is designed in such a way that spectroscopy and photometry can be carried out using the same telescope without the need to mechanically modify the imaging train. We observe single spectroscopic standard stars as well as binary stars up to 9.75 mag. We present results of mechanical tests of the instruments and spectroscopic observations carried out between Nov 26th and Dec 8th 2013. We conclude that BACHES is a very compact and capable spectrograph well suited for remote and autonomous operation. Coupled to a 0.5-m telescope it is capable of obtaining spectra of 10 mag targets with a SNR of 20 for 30-minute exposures. This is a very good result considering the price and size of the instrument. It brings new possibilities to the scientific community and opens a whole new range of research opportunities available to new and existing observatories.