The Digitized First Byurakan Survey as an Efficient Tool for Future Large Multiwavelength Surveys

Details The Digitized First Byurakan Survey as an Efficient Tool for Future Large Multiwavelength Surveys The Digitized First Byurakan Survey as an Efficient Tool for Future Large Multiwavelength Surveys

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iauss...1e..26m&link_type=abstract

IAU XXVI GA abstract book, SPS1

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The future large multiwavelength surveys will provide numerous new objects and sources in various wavelength domains from gamma to radio. However, they will need a basis for a comparison and hence, new discoveries. Digitized Sky Surveys give excellent astrometric, photometric and morphological information on any object up to 21-23 magnitudes. However, an understanding on the nature of objects is absent. Together with the DSS1 and DSS2, the Digitized First Byurakan Survey (DFBS) will serve as a unique spectroscopic database for studies in a large area (17,000 sq. deg.) at high galactic latitudes: approximate classification of any object (20,000,000 objects are present), identification of gamma, X-ray, IR and radio sources, selection of a sample of objects for definite studies. Two groups of projects will be especially productive: search for new interesting objects of definite types by low-dispersion template spectra, and optical identifications of new non-optical sources. A joint usage of the direct images and spectra will give larger possibilities for various studies and more efficient use of the future surveys.

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