... galaxies[*]
The full catalog tables (Tables 2 and 3) 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/cgi-bin/qcat?J/A+A/445/765
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
... webpages[*]
http://www.sdss.org/dr1/dm/flatFiles/fpC.html
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
... band[*]
For the selection from the photometric database we used the g band in order to make the parameters comparable to those used for selecting the FGC. In the following diagrams, however, we refer to the r band. This filter is mostly used in the other studies involving the CI (Nakamura et al. 2003; Shimasaku et al. 2001; Shen et al. 2003) because its quantum efficiency is the highest of all SDSS bands (Stoughton et al. 2002). In addition it includes the red light of the bulge which is important to separate galaxies with bulges from bulgeless galaxies.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
... data[*]
Note, however, that our catalog contains all edge-on disk galaxies that we identified with our selection criteria, including mixed-morphology and bulge-dominated galaxies. The galaxy type can be found in Tables 2 and 3 as explained earlier.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
Copyright ESO 2005