2018MNRAS.475.1736V -
Mon. Not. R. Astron. Soc., 475, 1736-1755 (2018/April-1)
Radio polarization properties of quasars and active galaxies at high redshifts.
VERNSTROM T., GAENSLER B.M., VACCA V., FARNES J.S., HAVERKORN M. and O'SULLIVAN S.P.
Abstract (from CDS):
We present the largest ever sample of radio polarization properties for z > 4 sources, with 14 sources having significant polarization detections. Using wide-band data from the Karl G. Jansky Very Large Array, we obtained the rest-frame total intensity and polarization properties of 37 radio sources, nine of which have spectroscopic redshifts in the range 1 <= z <= 1.4, with the other 28 having spectroscopic redshifts in the range 3.5 <= z <= 6.21. Fits are performed for the Stokes I and fractional polarization spectra, and Faraday rotation measures are derived using rotation measure synthesis and QU fitting. Using archival data of 476 polarized sources, we compare high-redshift (z > 3) source properties to a 15 GHz rest-frame luminosity matched sample of low-redshift (z < 3) sources to investigate if the polarization properties of radio sources at high redshifts are intrinsically different than those at low redshift. We find a mean of the rotation measure absolute values, corrected for Galactic rotation, of 50 ± 22 rad m–2 for z > 3 sources and 57 ± 4 rad m–2 for z < 3. Although there is some indication of lower intrinsic rotation measures at high-z possibly due to higher depolarization from the high-density environments, using several statistical tests we detect no significant difference between low- and high-redshift sources. Larger samples are necessary to determine any true physical difference.
Abstract Copyright:
© 2017 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s):
methods: statistical - galaxies: high-redshift - galaxies: magnetic fields - radio continuum: galaxies
Simbad objects:
42
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