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The Digitized First Byurakan Survey - DFBS

Published online by Cambridge University Press:  23 September 2016

A. M. Mickaelian ,
L. A. Sargsyan ,
L. K. Erastova ,
S. K. Balayan ,
K. S. Gigoyan ,
L. R. Hovhannisyan ,
R. Nesci ,
S. Gaudenzi ,
E. Massaro  and
C. Rossi
...Show all authors
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

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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
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 230 - 238
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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