Implementation of interference filters in the UV-Visual Echelle Spectrograph (UVES)
- Author(s)
- S Hubrig, Gerardo Avila, A. Kaufer, S. D'Odorico, H. Dekker, R. Schmutzer, M. Marchesi, Burkhard Wolff, Nicole Nesvacil
- Abstract
The purpose of the recent installation of eight interference filters in UVES is to isolate certain echelle orders to allow the use of a maximal slit length of 30". The typical decker height of the spectrograph slit for science operations is usually of the order of 10-12". The central wavelength of each filter was chosen to permit observations of the most important emission lines in extended objects. We discuss the performance of these filters and show the first science images obtained with the test run.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- European Southern Observatory (Germany), European Southern Observatory (Chile)
- DOI
- https://doi.org/10.1117/12.670712
- Publication date
- 2006
- Austrian Fields of Science 2012
- 1030 Physics, Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/38d1d7ac-e87b-4c76-927d-07be5653a53a