| Issue |
Astron. Astrophys. Suppl. Ser.
Volume 128, Number 2, March I 1998
|
|
|---|---|---|
| Page(s) | 409 - 416 | |
| DOI | https://doi.org/10.1051/aas:1998151 | |
| Published online | 15 March 1998 | |
Wavelength calibration at moderately high resolution*
Royal Observatory of Belgium, Ringlaan 3, B–1180 Brussel, Belgium
Corresponding author: Send offprint request to: J.-P. De Cuyper, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
24
January
1997
Accepted:
11
July
1997
Abstract
Th–Ar lamps are commonly used as wavelength calibration units at
moderately high spectral resolutions because
of the richness of the Th spectrum in the visual. The inclusion of blended
lines whose position is assumed to coincide with the laboratory wavelength of
the principal component is shown to result in a calibration precision
significantly worse than the intrinsic random noise limit. In order to
avoid this degradation of the calibration,
we present resolution–dependent Th–Ar wavelengths
in the region 277 to
for use at pixel–scales between
and
.
Key words: methods: data analysis; techniques: spectroscopic
Full Tables 5 and 6 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract. html
© European Southern Observatory (ESO), 1998
