Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/148928

Title

Wavelength calibration of the VLT-UVES spectrograph

Author(s)

Whitmore, Jonathan B.;  Murphy, Michael T.;  Griest, Kim

Abstract

We attempt to measure possible miscalibration of the wavelength scale of the VLT-UVES spectrograph. We take spectra of QSO HE0515-4414 through the UVES iodine cell which contains thousands of well-calibrated iodine lines and compare these lines to the wavelength scale from the standard thorium-argon pipeline calibration. Analyzing three exposures of this z = 1.71 QSO, we find two distinct types of calibration shifts needed to correct the Th/Ar wavelength scale. First, there is an overall average velocity shift of between 100 m s–1 and 500 m s–1 depending upon the exposure. Second, within a given exposure, we find intra-order velocity distortions of 100 m s–1 up to more than 200 m s–1. These calibration errors are similar to, but smaller than, those found earlier in the Keck HIRES spectrometer. We discuss the possible origins of these two types of miscalibration. We also explore the implications of these calibration errors on the systematic error in measurements of ${\Delta \alpha \over \alpha }$, the change in the fine-structure constant derived from measurement of the relative redshifts of absorption lines in QSO absorption systems. The overall average, exposure-dependent shifts should be less relevant for fine-structure work, but the intra-order shifts have the potential to affect these results. Using either our measured calibration offsets or a Gaussian model with sigma of around 90 m s–1, Monte Carlo mock experiments find errors in ${\Delta \alpha \over \alpha }$ of between 1 × 10–6 N –1/2 sys and 3 × 10–6 N –1/2 sys, where N sys is the number of systems used and the range is due to dependence on how many metallic absorption lines in each system are compared.

Publication type

Journal article

Research centre

Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing

Source

Astrophysical Journal, Vol. 723, no. 1 (Nov 2010), pp. 89-99

Publication year

2010

FOR Code(s)

0201 Astronomical and Space Sciences

Keyword(s)

Absorption lines;  Atomic data;  Cosmological parameters;  Instrumentation;  Quasars;  Spectrographs;  Spectroscopic;  Techniques

Publisher

Institute of Physics Publishing

ISSN

0004-637X

Publisher URL

http://dx.doi.org/10.1088/0004-637X/723/1/89

Copyright

Copyright © 2010 The American Astronomical Society. All rights reserved. The American Astronomical Society does not allow institutions to archive either the accepted manuscript or the published version of the article. However, you can find an earlier version of the full text here: http://arxiv.org/abs/1004.3325.

Peer reviewed