The INES system
Open Access
- 15 January 2000
- journal article
- Published by EDP Sciences in Astronomy and Astrophysics Supplement Series
- Vol. 141 (2) , 331-341
- https://doi.org/10.1051/aas:2000316
Abstract
In this paper we document the results of the study which led to the ripple correction and absolute calibration algorithms applied to the high resolution spectra processed with the software for the Final Archive of the Project. In this analysis, based on a very large number of spectra, we find that both the K and α parameters (not only the former as previously believed) vary with order number. This fact, together with the finding that the central peaks of the blaze function vary also as a function of the THDA temperature (for the SWP camera) and of the date of observations (for the LWP and LWR cameras), makes the ripple correction algorithm more complex than previously considered but, at the same time, considerably more reliable. As for the high resolution absolute calibration, the method followed is similar to the one implemented in . The internal accuracy of the high resolution calibration is about 4%. We note that the ripple correction and absolute calibration algorithms here described apply also to data processed and distributed with the system.Keywords
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