Wavelength calibration of the VLT-UVES spectrograph

Abstract

We attempt to measure possible miscalibration of the wavelength scale of the VLT-UVES spectrograph. We take spectra ofQSOHE0515-4414 through theUVESiodine cellwhich 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 ms -1 and 500 ms-1 depending upon the exposure. Second, within a given exposure, we find intra-order velocity distortions of 100ms -1 up to more than 200 ms-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 Δα/α, 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 ms-1, Monte Carlo mock experiments find errors in Δα α of between 1×10-6N-1/2sys and 3×10-6N-1/2sys, where Nsys is the number of systems used and the range is due to dependence on how many metallic absorption lines in each system are compared. © 2010. The American Astronomical Society.