- ... database
- Based on data gathered at the European Southern
Observatory (ESO) using the Ultraviolet and Visual Echelle
Spectrograph (UVES) installed at the Very Large Telescope (VLT), Unit-2
(Kueyen), on Cerro Paranal, Chile.
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- ...
distribution
- Note that the SDSS N(H I) distribution itself
may be biased, however it is currently the best available
representation of the DLA population.
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