AAS 197, January 2001
Session 116. Virtual Observatory: Data, Services, Tools and Software
Display, Thursday, January 11, 2001, 9:30-4:00pm, Exhibit Hall

## [116.07] Color-Space Outliers in DPOSS: Quasars and Peculiar Objects

S.G. Djorgovski, R.R. Gal, A. Mahabal, R. Brunner, S.M. Castro (Caltech), S.C. Odewahn (Caltech/ASU), R.R. de Carvalho (ON Brasil), DPOSS Team

The processing of DPOSS, a digital version of the POSS-II sky atlas, is now nearly complete. The resulting Palomar--Norris Sky Catalog (PNSC) is expected to contain > 5 \times 107 galaxies and > 109 stars, including large numbers of quasars and other unresolved sources. For objects morphologically classified as stellar (i.e., PSF-like), colors and magnitudes provide the only additional source of discriminating information. We investigate the distribution of objects in the parameter space of (g-r) and (r-i) colors as a function of magnitude. Normal stars form a well-defined (temperature) sequence in this parameter space, and we explore the nature of the objects which deviate significantly from this stellar locus. The causes of the deviations include: non-thermal or peculiar spectra, interagalactic absorption (for high-z quasars), presence of strong emission lines in one or more of the bandpasses, or strong variability (because the plates are taken at widely separated epochs). In addition to minor contamination by misclassified compact galaxies, we find the following: (1) Quasars at z > 4; to date, ~100 of these objects have been found, and used for a variety of follow-up studies. They are made publicly available immediately after discovery, through {\tt http://astro.caltech.edu/~george/z4.qsos}. (2) Type-2 quasars in the redshift interval z ~0.31 - 0.38. (3) Other quasars, starburst and emission-line galaxies, and emission-line stars. (4) Objects with highly peculiar spectra, some or all of which may be rare subtypes of BAL QSOs. (5) Highly variable stars and optical transients, some of which may be GRB orphan afterglows''. To date, systematic searches have been made only for (1) and (2); other types of objects were found serendipitously. However, we plan to explore systematically all of the statistically significant outliers in this parameter space. This illustrates the potential of large digital sky surveys for discovery of rare types of objects, both known (e.g., high-z quasars) and as yet unknown.