The UCSD/Keck Damped Lya Abundance Database: High Resolution Spectra
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This web site disseminates our ESI and HIRES spectra to the general
community. A full summary of what is released here, the quality of
the data, the DLA included, etc. are all given in Prochaska et al. (2007),
ApJS, in press.
Notes on the spectra:
Format: All of the spectra are written as
1d FITS files with a separate file for
flux and error array.
Wavelengths: The wavelength information is written to
each header. All of the wavelength solutions are 'log-linear', which
means each pixel has identical size in km/s (not Ang). This is
the best match to the properties of these instruments (i.e. roughly constant
resolution).
lambda_i = 10^(CRVAL1 + (CDELT1 * (i - CRPIX1) ) )
The HIRES data (pre CCD upgrade)
The ESI data (pre 2003)
e-mail: xavier@ucolick.org
last modified 11/08/06