Relative Flux Calibration of Keck HIRES Echelle Spectra

Abstract

We describe a new method to calibrate the relative flux levels in spectra from the HIRES echelle spectrograph on the Keck-I telescope. Standard data reduction techniques that transfer the instrument response between HIRES integrations leave errors in the flux of 5 - 10%, because the effective response varies. The flux errors are most severe near the ends of each spectral order, where there can be discontinuous jumps. The source of these errors is uncertain, but may include changes in the vignetting connected to the optical alignment. Our new flux calibration method uses a calibrated reference spectrum of each target to calibrate individual HIRES integrations. We determine the instrument response independently for each integration, and hence we avoid the need to transfer the instrument response between HIRES integrations. The procedure can be applied to any HIRES spectrum, or any other spectrum. While the accuracy of the method depends upon many factors, we have been able to flux calibrate a HIRES spectrum to 1% over scales of 200 A that include order joins. We illustrate the method with spectra of Q1243+3047 towards which we have measured the deuterium to hydrogen abundance ratio.

arXiv comment24 pages, 17 figures, submitted to PASP

References in corpus (5)

• The Deuterium Abundance Towards Q1009+2956
• The Deuterium to Hydrogen Abundance Ratio Towards a Fourth QSO: HS0105+1619
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• Performance characteristics of the new Keck Observatory echelle spectrograph and imager
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