  We use the GALEX (Galaxy Evolution Explorer) Medium Imaging Survey (MIS) and
All-Sky Imaging Survey (AIS) data available in the first internal release,
matched to the SDSS catalogs in the overlapping regions, to classify objects by
comparing the multi-band photometry to model colors. We show an example of the
advantage of such broad wavelength coverage (GALEX far-UV and near-UV, SDSS
ugriz) in classifying objects and augmenting the existing samples and catalogs.
  From the MIS [AIS] sample over an area of 75 [92] square degrees, we select a
total of 1736 [222] QSO candidates at redshift less than 2, significantly
extending the number of fainter candidates, and moderately increasing the
number of bright objects in the SDSS list of spectroscopically confirmed QSO.
  Numerous hot stellar objects are also revealed by the UV colors, as expected.
