CaltechAUTHORS
  A Caltech Library Service

The VLBA Imaging and Polarimetry Survey at 5 GHz

Helmboldt, J. F. and Taylor, G. B. and Tremblay, S. and Fassnacht, C. D. and Walker, R. C. and Myers, S. T. and Sjouwerman, L. O. and Pearson, T. J. and Readhead, A. C. S. and Weintraub, L. and Gehrels, N. and Romani, R. W. and Healey, S. and Michelson, P. F. and Blandford, R. D. and Cotter, G. (2007) The VLBA Imaging and Polarimetry Survey at 5 GHz. Astrophysical Journal, 658 (1). pp. 203-216. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20190604-105507986

[img] PDF - Published Version
See Usage Policy.

2360Kb
[img] PDF - Accepted Version
See Usage Policy.

1364Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190604-105507986

Abstract

We present the first results of the VLBA Imaging and Polarimetry Survey (VIPS), a 5 GHz VLBI survey of 1127 sources with flat radio spectra. Through automated data reduction and imaging routines, we have produced publicly available 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 I image to automatically classify it as a pointlike source, a core jet, a compact symmetric object (CSO) candidate, or a complex source. Using data from the Sloan Digital Sky Survey (SDSS), we have found no significant trend between optical flux and 5 GHz flux density for any of the source categories. Using the velocity width of the Hβ emission line and the monochromatic luminosity at 5100 Å to estimate the central black hole mass, M_(BH), we have found a weak trend between M_(BH) and 5 GHz luminosity density for objects with SDSS spectra. The mean ratio of the polarized to total 5 GHz flux density for VIPS sources with detected polarized 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 in core-jet systems tend to be perpendicular to the electric vector position angles (EVPAs). The data are consistent with a scenario in which ~24% of the polarized core jets have EVPAs that are antialigned with the directions of their jet components and that have a substantial amount of Faraday rotation. In addition to these initial results, plans for future follow-up observations are discussed.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1086/511005DOIArticle
https://arxiv.org/abs/astro-ph/0611459arXivDiscussion Paper
ORCID:
AuthorORCID
Taylor, G. B.0000-0001-6495-7731
Fassnacht, C. D.0000-0002-4030-5461
Pearson, T. J.0000-0001-5213-6231
Readhead, A. C. S.0000-0001-9152-961X
Romani, R. W.0000-0001-6711-3286
Blandford, R. D.0000-0002-1854-5506
Additional Information:© 2007 The American Astronomical Society. Received 2006 October 17; accepted 2006 November 14. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc. Information regarding SCHED can be found at http://www.aoc.nrao.edu/_cwalker/sched/sched/sched.html. The Web site for the 5GHzVLA/VLBA Polarization Calibration database is http://www.vla.nrao.edu/astro/calib/polar/. The authors would like to thank the University of New Mexico and Stanford University for the purchase of Mk 5 disks for the VLBA, which was instrumental in achieving a larger data rate, making this survey possible. Funding for the Sloan Digital Sky Survey (SDSS) and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web site is http://www.sdss.org/. The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, the Astrophysical Institute Potsdam, the University of Basel, the University of Cambridge, Case Western Reserve University, the University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), the Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, the University of Pittsburgh, the University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington.
Group:TAPIR
Funders:
Funding AgencyGrant Number
Alfred P. Sloan FoundationUNSPECIFIED
Participating InstitutionsUNSPECIFIED
NSFUNSPECIFIED
Department of Energy (DOE)UNSPECIFIED
NASAUNSPECIFIED
Japanese MonbukagakushoUNSPECIFIED
Max Planck SocietyUNSPECIFIED
Higher Education Funding Council for EnglandUNSPECIFIED
Subject Keywords:catalogs — galaxies: active — galaxies: jets — galaxies: nuclei — radio continuum: galaxies — surveys — techniques: image processing
Issue or Number:1
Record Number:CaltechAUTHORS:20190604-105507986
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190604-105507986
Official Citation:J. F. Helmboldt et al 2007 ApJ 658 203
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96108
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:04 Jun 2019 18:05
Last Modified:09 Apr 2020 17:33

Repository Staff Only: item control page