A&A 458, 341-348 (2006)
DOI: 10.1051/0004-6361:20054545
An optical search for low surface brightness galaxies in the Arecibo HI Strip Survey
C. Trachternach, D. J. Bomans, L. Haberzettl and R.-J. DettmarAstronomisches Institut, Ruhr-Universität Bochum, Universitätstraße 150, 44780 Bochum, Germany
e-mail: trachter@astro.rub.de
(Received 18 November 2005 / Accepted 18 July 2006 )
Abstract
Aims.
In order to estimate the contribution of low surface brightness (LSB) galaxies
to the local (
) galaxy number density, we performed an optical search for LSB candidates in a 15.5 deg2 part of the
region covered by the 65 deg2 blind Arecibo HI Strip Survey (AHISS).
Methods.
Object
detection and galaxy profile fitting were done with analytical
algorithms. The detection efficiency and the selection effects were
evaluated using large samples of artificial galaxies.
Results.
Our final
catalogue is diameter-limited and contains 306 galaxies with diameters
at the limiting surface brightness of
. Of these 306 galaxies, 148 were
not catalogued previously. Our results indicate that low surface
brightness galaxies contribute at
least to 30% to the local galaxy number density.
Conclusions.
Without additional
distance information, choosing the limiting diameter and the surface
brightness at which the diameter is measured is crucial.
Depending on these choices, diameter-limited optical catalogues are either
biased against LSB galaxies, or contaminated with cosmologically dimmed high
surface brightness galaxies, which
affects the implied surface brightness distribution. The comparison to
the AHISS showed that although optical surveys detect more galaxies per
deg2 than HI surveys, their drawback is the need
for spectroscopic follow up observations to derive distances. Blind HI
surveys have no diameter limits, but tend to miss gas-poor galaxies and all
galaxies which lie outside their redshift limits.
HI and optical surveys thus provide complementary information and
sample different parts of the LSB galaxy population.
Key words: galaxies: general -- galaxies: fundamental parameters -- galaxies: statistics
© ESO 2006

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