Spectroscopy of white dwarf candidates from the ESO Imaging Survey (EIS-WIDE)*
Institut für Theoretische Physik und Astrophysik, Universität Kiel, 24098 Kiel, Germany e-mail: email@example.com
Corresponding author: D. Koester, firstname.lastname@example.org
Accepted: 6 September 2001
In the ESO Imaging Survey of a 1.27 square degree field in the direction of the south galactic pole ("patch B" ) 32 point sources were identified as white dwarf candidates in the vs. two-color diagram by the EIS team and published as a candidate catalog. One of these was a previously known quasar. We have obtained low resolution spectra of 30 of the remaining sources. Of these only 6 are DA white dwarfs, one is a DQ white dwarf, one a DC. 11 candidates are quasars with redshifts between 1.4 and 3.3. The remaining sources are stars with narrow Balmer lines, in most cases probably field horizontal branch stars.
Key words: stars: white dwarfs / quasars: general
© ESO, 2001