A. Cassatella et al., The INES system - II. Ripple correction and absolute calibration for IUE high resolution spectra, ASTR AST SS, 141(2), 2000, pp. 331-341
In this paper we document the results of the study which led to the ripple
correction and absolute calibration algorithms applied to the high resoluti
on spectra processed with the NEWSIPS software for the Final archive of the
IUE Project. In this analysis, based on a very large number of spectral we
find that both the It and alpha parameters (not only the former as previou
sly 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 compl
ex than previously considered but, at the same time, considerably more reli
able. As for the high resolution absolute calibration, the method followed
is similar to the one implemented in IUESIPS. 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 IUE data
processed and distributed with the INES system.