The VLBA Imaging and Polarimetry Survey at 5 GHz
Author(s) -
J. F. Helmboldt,
G. B. Taylor,
S. E. Tremblay,
C. D. Fassnacht,
R. C. Walker,
S. T. Myers,
Loránt O. Sjouwerman,
T. J. Pearson,
A. C. S. Readhead,
L. Weintraub,
N. Gehrels,
Roger W. Romani,
S. E. Healey,
P. F. Michelson,
R. D. Blandford,
G. Cotter
Publication year - 2007
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/511005
Subject(s) - physics , astrophysics , very long baseline interferometry , polarimetry , flux (metallurgy) , position angle , sky , faraday effect , luminosity , very long baseline array , astronomy , jet (fluid) , active galactic nucleus , optics , galaxy , magnetic field , materials science , quantum mechanics , scattering , metallurgy , thermodynamics
We present the first results of the VLBA Imaging and Polarimetry Survey(VIPS), a 5 GHz VLBI survey of 1,127 sources with flat radio spectra. Throughautomated data reduction and imaging routines, we have produced publiclyavailable I, Q, and U images and have detected polarized flux density from 37%of the sources. We have also developed an algorithm to use each source's Iimage to automatically classify it as a point-like source, a core-jet, acompact symmetric object (CSO) candidate, or a complex source. The mean ratioof the polarized to total 5 GHz flux density for VIPS sources with detectedpolarized flux density ranges from 1% to 20% with a median value of about 5%.We have also found significant evidence that the directions of the jets incore-jet systems tend to be perpendicular to the electric vector positionangles (EVPAs). The data is consistent with a scenario in which ~24% of thepolarized core-jets have EVPAs that are anti-aligned with the directions oftheir jet components and which have a substantial amount of Faraday rotation.In addition to these initial results, plans for future follow-up observationsare discussed
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