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Improved Data Reduction Techniques for the ESO CES Plus Reticon Spectra
Published online by Cambridge University Press: 19 July 2016
Abstract
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We developed routines for intensity, equivalent width, and radial velocity measurements on CES plus reticon spectra obtained with the ESO 1.4m telescope. In order to achieve the optimal recovery of the signal, the noise has to be minimized by removing any parasitical effect. Special care has been devoted to the correction for remanence effects in the reticon dark counts. Typical results are presented and discussed.
- Type
- VI. Chemical Composition of Stars
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- Copyright © Kluwer 1988
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