The Dominion Radio Astrophysical Observatory Deep Field polarization study has been matched with the Spitzer Wide-Area Infrared Extragalactic Survey of the European Large Area Infrared Space Observatory Survey North 1 field. We have used Very Large Array observations with a total intensity rms of 87μJy beam−1 to match SWIRE counterparts to the radio sources. Infrared color analysis of our radio sample shows that the majority of polarized sources are elliptical galaxies with an embedded active galactic nucleus. Using available redshift catalogs, we found 429 radio sources of which 69 are polarized with redshifts in the range of 0.04 <z< 3.2. We find no correlation between redshift and percentage polarization for our sample. However, fo...
We present stacking polarized intensity as a means to study the polarization of sources that are too...
We use the integrated polarized radio emission at 1.4 GHz (P1.4 GHz) from a large sample of active g...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...
We present the largest ever sample of radio polarization properties for z > 4 sources, with 14 sourc...
A sample of 129 unresolved radio sources with ultrahigh linear polarization (> 30 per cent) has been...
This research was supported by the Undergraduate Research Opportunities Program (UROP)
We present polarization properties at 1.4 GHz of two separate extragalactic source populations: pass...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
We describe a recent full-polarization radio continuum survey, performed using the Westerbork Synthe...
Context. In the context of structure formation and galaxy evolution, the contribution of magnetic fi...
This thesis reports the K-band polarizations of a representative sample of nine radio galaxies: seve...
We present the results of K-band imaging polarimetry of seven 3CR radio galaxies at redshifts (z) be...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...
Radio emission in the form of giant radio relics is observed at the periphery of galaxy clusters. Th...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...
We present stacking polarized intensity as a means to study the polarization of sources that are too...
We use the integrated polarized radio emission at 1.4 GHz (P1.4 GHz) from a large sample of active g...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...
We present the largest ever sample of radio polarization properties for z > 4 sources, with 14 sourc...
A sample of 129 unresolved radio sources with ultrahigh linear polarization (> 30 per cent) has been...
This research was supported by the Undergraduate Research Opportunities Program (UROP)
We present polarization properties at 1.4 GHz of two separate extragalactic source populations: pass...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
We describe a recent full-polarization radio continuum survey, performed using the Westerbork Synthe...
Context. In the context of structure formation and galaxy evolution, the contribution of magnetic fi...
This thesis reports the K-band polarizations of a representative sample of nine radio galaxies: seve...
We present the results of K-band imaging polarimetry of seven 3CR radio galaxies at redshifts (z) be...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...
Radio emission in the form of giant radio relics is observed at the periphery of galaxy clusters. Th...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...
We present stacking polarized intensity as a means to study the polarization of sources that are too...
We use the integrated polarized radio emission at 1.4 GHz (P1.4 GHz) from a large sample of active g...
Context. The characteristics of the polarised radio sky are a key ingredient in constraining evoluti...