Calibration concepts for the MUSE integral field
โ Scribed by Andreas Kelz; Svend M. Bauer; Martin M. Roth
- Publisher
- Elsevier Science
- Year
- 2006
- Tongue
- English
- Weight
- 272 KB
- Volume
- 50
- Category
- Article
- ISSN
- 1387-6473
No coin nor oath required. For personal study only.
โฆ Synopsis
The phase-A design study of the Calibration Unit (CU) for the Multi-Unit Spectroscopic Explorer (MUSE) is presented. MUSE is an integral-field spectrograph for the 2nd generation of VLT instruments and offers a relative wide integral-field, adaptive-optics assisted spatial resolution, and a wavelength coverage between 465 and 930 nm. MUSE is a project of seven European institutes and is led by the Centre de Recherche Atronomique de Lyon (CRAL). Amongst other work-packages, the Astrophysical Institute Potsdam (AIP) is responsible for the Calibration Unit. The paper describes the calibration requirements, including issues related to spectral, image quality, and geometrical calibration. The opto-mechanical layout of the calibration unit is presented and the use of focal plane masks to evaluate image distortions and PSF degradations is explained.
๐ SIMILAR VOLUMES
An integral field spectrograph following the TPF coronagraph can provide the required spectral resolving power R 70 with spatial resolution at the telescope diffraction limit, and covering the coronagraphic dark hole. This allows spectra to be obtained of all planets around the star simultaneously,
A recent formulation of a multiphase-field model is presented. The approach is employed to numerically simulate phase transitions in multiphase systems and to describe the evolution of the microstructure during solidification processes in alloy systems. A new method for modelling solute diffusion in