Bibcode
Doerr, H.-P.; Vitas, N.; Fabbian, D.
Bibliographical reference
Astronomy and Astrophysics, Volume 590, id.A118, 9 pp.
Advertised on:
5
2016
Journal
Citations
21
Refereed citations
20
Description
Context. The high-fidelity solar spectral atlas prepared by Delbouille
et al. (Liège atlas, 1973) and the atlas by
Neckel
(Hamburg atlas, 1999, Sol. Phys., 184, 421) are widely
recognised as the most important collection of reference spectra of the
Sun at disc centre in the visible wavelength range. The two datasets
serve as fundamental resources for many researchers, in particular for
chemical abundance analyses. But despite their similar published
specifications (spectral resolution and noise level), the shapes of the
spectral lines in the two atlases differ significantly and
systematically. Aims: Knowledge of any instrumental degradations
is imperative to fully exploit the information content of spectroscopic
data. We seek to investigate the magnitude of these differences and
explain the possible sources. We provide the wavelength-dependent
correction parameters that need to be taken into account when the
spectra are to be compared with synthetic data, for instance.
Methods: A parametrically degraded version of the Hamburg spectrum was
fitted to the Liège spectrum. The parameters of the model
(wavelength shift, broadening, intensity scaling, and intensity offset)
represent the different characteristics of the respective instruments,
observational strategies, and data processing. Results: The
wavelength scales of the Liège and Hamburg atlases differ on
average by 0.5 mÅ with a standard deviation of ± 2
mÅ, except for a peculiar region around 5500 Å. The
continuum levels are offset by up to 18% below 5000 Å, but remain
stably at a 0.8% difference towards the red. We find no evidence for
spectral stray light in the Liège spectrum. Its resolving power
is almost independent of wavelength but limited to about 216 000, which
is between two to six times lower than specified. When accounting for
the degradations determined in this work, the spectra of the two atlases
agree to within a few parts in 103.
The fit parameters displayed in Fig. 2 and derived data are only
available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/590/A118