Alternative data reduction procedures for UVES: Wavelength calibration and spectrum addition
Journal article, 2009

This paper addresses alternative procedures to the ESO supplied pipeline procedures for the reduction of UVES spectra of two quasar spectra to determine the value of the fundamental constant μ=Mp/Me at early times in the universe. The procedures utilize intermediate product images and spectra produced by the pipeline with alternative wavelength calibration and spectrum addition methods. Spectroscopic studies that require extreme wavelength precision need customized wavelength calibration procedures beyond that usually supplied by the standard data reduction pipelines. An example of such studies is the measurement of the values of the fundamental constants at early times in the universe. This article describes a wavelength calibration procedure for the UV–visual Echelle spectrometer on the very large telescope, however, it can be extended to other spectrometers as well. The procedure described here provides relative wavelength precision of better than 3×10-7 for the long-slit Thorium–Argon calibration lamp exposures. The gain in precision over the pipeline wavelength calibration is almost entirely due to a more exclusive selection of Th/Ar calibration lines.

techniques: spectroscopic

Author

Rodger I. Thompson

University of Arizona

Jill Bechtold

University of Arizona

John H Black

Chalmers, Department of Radio and Space Science, Radio Astronomy and Astrophysics

Carlos Martins

Universidade do Porto

New Astronomy

1384-1076 (ISSN) 1384-1092 (eISSN)

Vol. 14 4 379-390

Subject Categories

Physical Sciences

Astronomy, Astrophysics and Cosmology

DOI

10.1016/j.newast.2008.11.001

More information

Latest update

3/29/2018