10 July 2008 Results of X-shooter data reduction software on laboratory frames
Author Affiliations +
Abstract
We present the current state of the Data Reduction Software (DRS) being developed at APC, Paris Observatory, Amsterdam University and ESO for the X-shooter echelle spectrograph. X-shooter is the first VLT second generation instrument, which will have its first light during the fall of the current year and will be available to the astronomical community starting April 2009. The DRS will be fully integrated in the ESO VLT data flow environment and it will use the ESO Common Pipeline Library. X-shooter data have two main characteristics, on the one hand the exceptionally wide band (0.3 - 2.4 micron) covered in a single exposure, and on the other hand the spectral format with highly curved orders and tilted lines. After a brief description of the reduction process, the main results obtained up to now on simulated and laboratory data are reported. In particular the precision of wavelength calibration and sky subtraction are discussed.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. Goldoni, F. Royer, M. Horrobin, P. François, L. Guglielmi, R. Haigron, J. Vernet, A. Modigliani, P. Bristow, "Results of X-shooter data reduction software on laboratory frames", Proc. SPIE 7014, Ground-based and Airborne Instrumentation for Astronomy II, 70145T (10 July 2008); doi: 10.1117/12.787844; https://doi.org/10.1117/12.787844
PROCEEDINGS
11 PAGES


SHARE
RELATED CONTENT

Calibration and modeling support for instruments at ESO
Proceedings of SPIE (July 09 2008)
The JWST/NIRSpec instrument performance simulator software
Proceedings of SPIE (August 04 2010)
Remote sensing experiment implementation: lessons learned
Proceedings of SPIE (October 14 2004)
Advanced 2D spectroscopic predicted data
Proceedings of SPIE (July 09 2008)
Data reduction software of the X-shooter spectrograph
Proceedings of SPIE (June 30 2006)
X-shooter physical model
Proceedings of SPIE (July 11 2008)

Back to Top