This website is the author produced HTML version of
S. J. Curran, J. K. Webb, M. T. Murphy, R. Bandiera, E. Corbelli
and V. V. Flambaum, 2002, "A Catalogue of Damped Lyman Alpha
Absorption Systems and Radio Flux Densities of the Background Quasars"
(Publications
of the Astronomical Society of Australia 19, 455-474). By having this
catalogue on-line it is my hope that it can be continually updated so
that it retains its usefulness to the astronomical community. In order
to concentrate on the actual list of objects, the reader is referred
to the paper (linked above) for full details (such as scientific
motivation, etc). To use this catalogue, however, it is
necessary to note the following:
Column 1 This is the name, as obtained from NED, of the background quasar, illuminating the
damped Lyman alpha absorber (DLA). Note that those in red
are not part of the original published list (see the note in column 6).
Columns 2 & 3 The J2000 coordinates. Unfortunately, some of these may
be erroneous (see Sect. 2.1 of the
paper). Therefore, before observing these objects, it is strongly
recommended that the coordinates are checked, for example on the Digitized
Sky, APM and COSMOS Surveys (the coordinates in green have already been checked). I would be very grateful if you
could
notify me of any such errors (and any new DLAs) and I shall update
this list accordingly.
Column 4 The redshift of the
background quasar.
Column 5 The redshift of the DLA. As per Section 3 of the paper, this field links to any other absorption features of interest, e.g. the 21 cm hyperfine transition of neutral atomic hydrogen in the DLA.
Column 6 The base 10 logarithm of the column density of the DLA
in cm-2. The superscript denotes the reference to the
DLA, as given in the published paper, and each of these is a
hyper-link to the ADS abstract. In the case of new DLAs no superscripts are allocated but the
reference can still be reached via this column. Also not published in
the original paper are inferred
DLAs. Although, not yet observed in the Lyman alpha line, each
is believed, from other (e.g. metal or 21 cm) absorption lines, to
possess the column density of neutral atomic hydrogen (N HI>1020
cm-2 ) characteristic of a DLA. Since we were not
initially interested in these sources for our work, the catalogue at
this stage by no means constitutes an exhaustive list of these (note
also, in some cases the original references have yet to be
published). Column 7 The
visual magnitude, obtained either from the original reference (previous
column), the Véron catalogue of Quasars and Active
Galactic Nuclei (10th Ed.) or the NASA/IPAC
Extragalactic Database (NED).
``Radio flux densities'' These are the radio flux densities of the background
quasars in Janskys for 0.4, 1.4, 2.7, 5.0 and "higher" (frequency given in
parenthesis) GHz. ``X'' denotes no measured radio flux at the survey's detection limit (0.25 Jy for the Texas Survey at 365 MHz over -35.5o≤ δ &le 71.5o). As in column 5, the superscripts denote the references to the radio properties and link to the ADS abstract or
straight to the (CDS) catalogue (the CDS version of this catalogue
can be accessed here).
Finally, note that ``*'' denotes
a candidate DLA which has yet to be confirmed using higher resolution spectroscopy
(``**'' designates that this absorber has subsequently been found not to
be damped.)