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The Digitized First Byurakan Survey - DFBS

Published online by Cambridge University Press:  23 September 2016

A. M. Mickaelian
Affiliation:
Byurakan Astrophysical Observatory, Byurakan 378433, Aragatzotn province, Armenia
L. A. Sargsyan
Affiliation:
Byurakan Astrophysical Observatory, Byurakan 378433, Aragatzotn province, Armenia
L. K. Erastova
Affiliation:
Byurakan Astrophysical Observatory, Byurakan 378433, Aragatzotn province, Armenia
S. K. Balayan
Affiliation:
Byurakan Astrophysical Observatory, Byurakan 378433, Aragatzotn province, Armenia
K. S. Gigoyan
Affiliation:
Byurakan Astrophysical Observatory, Byurakan 378433, Aragatzotn province, Armenia
L. R. Hovhannisyan
Affiliation:
Byurakan Astrophysical Observatory, Byurakan 378433, Aragatzotn province, Armenia
R. Nesci
Affiliation:
Dipartimento di Fisica, Universita di Roma “La Sapienza”, P.le Aldo Moro 2, I-00185, Roma, Italia
S. Gaudenzi
Affiliation:
Dipartimento di Fisica, Universita di Roma “La Sapienza”, P.le Aldo Moro 2, I-00185, Roma, Italia
E. Massaro
Affiliation:
Dipartimento di Fisica, Universita di Roma “La Sapienza”, P.le Aldo Moro 2, I-00185, Roma, Italia
C. Rossi
Affiliation:
Dipartimento di Fisica, Universita di Roma “La Sapienza”, P.le Aldo Moro 2, I-00185, Roma, Italia
S. Sclavi
Affiliation:
Dipartimento di Fisica, Universita di Roma “La Sapienza”, P.le Aldo Moro 2, I-00185, Roma, Italia
D. Trevese
Affiliation:
Dipartimento di Fisica, Universita di Roma “La Sapienza”, P.le Aldo Moro 2, I-00185, Roma, Italia
D. Weedman
Affiliation:
Department of Astronomy, Cornell University, Ithaca, NY 14853, U.S.A.
J. Houck
Affiliation:
Department of Astronomy, Cornell University, Ithaca, NY 14853, U.S.A.
D. Barry
Affiliation:
Department of Astronomy, Cornell University, Ithaca, NY 14853, U.S.A.
B. Brandl
Affiliation:
Department of Astronomy, Cornell University, Ithaca, NY 14853, U.S.A.

Abstract

The First Byurakan Survey (FBS) is the largest spectral survey in the Northern sky. One can select objects by color, broad absorption and emission lines, and SED; classify and investigate them. The digitization of the FBS is aimed at making a DFBS database available for the astronomical community. Besides scanning, we are creating plate solutions, extraction software, wavelength and flux calibration, templates for different types of objects, numerical classification, a catalog of objects, a database of spectra, a user interface and a DFBS web page. New research projects based on the DFBS are possible, including a search for new QSOs and other AGN, a continuation of the second part of FBS, and identifications of radio, IR and X-ray sources. The DFBS database will be available at the end of 2004.

Type
Session IV: Galaxy Evolution and Clusters of Galaxies
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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