VLA search for 5GHz radio transients Virtual Observatory Resource

Authors
  1. Ofek E.O.
  2. Frail D.A.
  3. Breslauer B.
  4. Kulkarni S.R.
  5. Chandra P.
  6. Gal-Yam A.,Kasliwal M.M.
  7. Gehrels N.
  8. Published by
    CDS
Abstract

We present the results of a 5GHz survey with the Very Large Array (VLA) and the expanded VLA, designed to search for short-lived (<~1day) transients and to characterize the variability of radio sources at milli-Jansky levels. A total sky area of 2.66deg^2^, spread over 141 fields at low Galactic latitudes (b~6-8{deg}), was observed 16 times with a cadence that was chosen to sample timescales of days, months, and years. Most of the data were reduced, analyzed, and searched for transients in near real-time. Interesting candidates were followed up using visible light telescopes (typical delays of 1-2hr) and the X-ray Telescope on board the Swift satellite. The final processing of the data revealed a single possible transient with a peak flux density of f_{nu}_~2.4mJy. Furthermore, we use the data to measure the source variability on timescales of days to years, and we present the variability structure function of 5GHz sources.

Keywords
  1. radio-continuum-emission
  2. radio-sources
Bibliographic source Bibcode
2011ApJ...740...65O
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/740/65
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/740/65
Document Object Identifer DOI
doi:10.26093/cds/vizier.17400065

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History

2013-03-04T09:37:18Z
Resource record created
2013-03-04T09:37:18Z
Created
2018-02-12T08:45:34Z
Updated

Contact

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