Share Email Print

Proceedings Paper

BESO: a high-resolution spectrograph for the Hexapod-Telescope
Author(s): Ingo Steiner; Walter Seifert; Otmar Stahl; Roland Lemke; Rolf Chini; Immo Appenzeller
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

BESO (Bochum Echelle Spectrograph for OCA) is a high-resolution echelle spectrograph which is built by the Ruhr-Universitaet, Bochum and the Landessternwarte Heidelberg. It will be operated with the 1.5m Hexapod-Telescope at the Observatorio Cerro Armazones (OCA), Chile - the new observatory of the Ruhr-Universitaet and the Universidad Catolica del Norte in Antofagasta. The site at 2800m altitude is located 30 km east of Paranal and provides superb observing conditions. BESO is fiber-coupled to the Hexapod-Telescope, covers a spectral range of 370 to 840nm with a resolution of 48,000. Instrument controls are embedded in the ALMA Common Software environment. The spectrograph is part of a monitoring project that studies the variability of young stars and AGN.

Paper Details

Date Published: 30 June 2006
PDF: 6 pages
Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62692W (30 June 2006); doi: 10.1117/12.671120
Show Author Affiliations
Ingo Steiner, Astronomisches Institut der Ruhr-Univ. Bochum (Germany)
Walter Seifert, ZAH Landessternwarte Heidelberg (Germany)
Otmar Stahl, ZAH Landessternwarte Heidelberg (Germany)
Roland Lemke, Astronomisches Institut der Ruhr-Univ. Bochum (Germany)
Rolf Chini, Astronomisches Institut der Ruhr-Univ. Bochum (Germany)
Immo Appenzeller, ZAH Landessternwarte Heidelberg (Germany)

Published in SPIE Proceedings Vol. 6269:
Ground-based and Airborne Instrumentation for Astronomy
Ian S. McLean; Masanori Iye, Editor(s)

© SPIE. Terms of Use
Back to Top