We will discuss about wideband and multiband VLBI observations taken with linear-polarization feeds (the simplest hardware polarimetry for wide bands), and how these observations can be calibrated and fringe-fitted with special software, in order to produce full-polarization images with a high fidelity. We will show results from real observations, taken with the VGOS array, and discuss about future applicability of these algorithms in future VLBI arrays
We present the first results of the VLBA Imaging and Polarimetry Survey (VIPS), a 5 GHz VLBI survey ...
We present full polarization Very Long Baseline Array (VLBA) observations at 5 and 15 GHz of 24 comp...
The goals of this thesis were to study the observational radio-polarimetric properties of gravitatio...
We report the development of a semi-automatic pipeline for the calibration of 86 GHz full-polarizati...
The calibration and analysis of polarization observations in very long baseline interferometry (VLBI...
We report the development of a semi-automatic pipeline for the calibration of 86GHz full-polarizatio...
The Atacama Large mm-submm Array (ALMA) is, by far, the most sensitive mm/submm telescope in the Wor...
We present the first results of the VLBA Imaging and Polarimetry Survey (VIPS), a 5 GHz VLBI survey ...
We have obtained total and polarized intensity images of 15 AGNs with the VLBA at 7 mm at 17 epochs ...
Heterodyne receivers register the sky signal on either a circular polarization basis (where it is sp...
Heterodyne receivers register the sky signal on either a circular polarization basis (where it is sp...
VGOS antennas observe in dual linear polarization mode. To obtain the maximum signal-to-noise ratio,...
We present MeqSilhouette v2.0 (MeqSv2), a fully polarimetric, time-and frequency-resolved synthetic ...
High-frequency VLBI is demonstrating its power with recent achievements such as imaging the shadow o...
We present a detailed description of the special procedures for calibration and quality assurance of...
We present the first results of the VLBA Imaging and Polarimetry Survey (VIPS), a 5 GHz VLBI survey ...
We present full polarization Very Long Baseline Array (VLBA) observations at 5 and 15 GHz of 24 comp...
The goals of this thesis were to study the observational radio-polarimetric properties of gravitatio...
We report the development of a semi-automatic pipeline for the calibration of 86 GHz full-polarizati...
The calibration and analysis of polarization observations in very long baseline interferometry (VLBI...
We report the development of a semi-automatic pipeline for the calibration of 86GHz full-polarizatio...
The Atacama Large mm-submm Array (ALMA) is, by far, the most sensitive mm/submm telescope in the Wor...
We present the first results of the VLBA Imaging and Polarimetry Survey (VIPS), a 5 GHz VLBI survey ...
We have obtained total and polarized intensity images of 15 AGNs with the VLBA at 7 mm at 17 epochs ...
Heterodyne receivers register the sky signal on either a circular polarization basis (where it is sp...
Heterodyne receivers register the sky signal on either a circular polarization basis (where it is sp...
VGOS antennas observe in dual linear polarization mode. To obtain the maximum signal-to-noise ratio,...
We present MeqSilhouette v2.0 (MeqSv2), a fully polarimetric, time-and frequency-resolved synthetic ...
High-frequency VLBI is demonstrating its power with recent achievements such as imaging the shadow o...
We present a detailed description of the special procedures for calibration and quality assurance of...
We present the first results of the VLBA Imaging and Polarimetry Survey (VIPS), a 5 GHz VLBI survey ...
We present full polarization Very Long Baseline Array (VLBA) observations at 5 and 15 GHz of 24 comp...
The goals of this thesis were to study the observational radio-polarimetric properties of gravitatio...
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