International audienceWe have analyzed 1+2+4+6 cm VLBA polarization data for the TeV BL Lac object Mrk 501 obtained at three epochs separated by 3--4 weeks in 1998 March--April. These observations show no significant total-intensity or polarization variability over the interval covered by the observations, supporting previous claims that variability in the parsec-scale structure of this source (e.g., motions in its VLBI jet) is modest. The B field structure is complex, and shows a sheath-like structure. The rotation-measure distribution shows evidence for variations across the jet, suggesting the presence of a helical B field associated with the VLBI jet
To determine the location of the intra-day variable (IDV) emission region within the jet of the BL L...
A comparison between low-frequency space very long baseline interferometry (VLBI) and high-frequency...
We present four high dynamic range, dual-circular polarization, Very Long Baseline Array (VLBA) obse...
International audienceWe have analyzed 1+2+4+6 cm VLBA polarization data for the TeV BL Lac object M...
This thesis presents the results of a series of polarization VLBI experiments on the wellknown varia...
We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the ...
We have obtained total and polarized intensity images of 15 AGNs with the VLBA at 7 mm at 17 epochs,...
Aims. We present an extensive study of the BL Lac object Mrk 501 based on a data set collected durin...
We report preliminary results of a 3-year multifrequency polarization campaign of 15 ...
Previous very long baseline interferometry (VLBI) observations of the nearby (z = 0.0337) active gal...
and Cronin 2004, showed systematic Faraday rotation gradients across the parsec-scale jets of severa...
Context. This is the third paper in a series devoted to the analysis of the multiwavelength data fro...
Polarization-sensitive lambda= 6 cm global VLBI images of BL Lac for data taken at three epochs are ...
Context. High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal too...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
To determine the location of the intra-day variable (IDV) emission region within the jet of the BL L...
A comparison between low-frequency space very long baseline interferometry (VLBI) and high-frequency...
We present four high dynamic range, dual-circular polarization, Very Long Baseline Array (VLBA) obse...
International audienceWe have analyzed 1+2+4+6 cm VLBA polarization data for the TeV BL Lac object M...
This thesis presents the results of a series of polarization VLBI experiments on the wellknown varia...
We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the ...
We have obtained total and polarized intensity images of 15 AGNs with the VLBA at 7 mm at 17 epochs,...
Aims. We present an extensive study of the BL Lac object Mrk 501 based on a data set collected durin...
We report preliminary results of a 3-year multifrequency polarization campaign of 15 ...
Previous very long baseline interferometry (VLBI) observations of the nearby (z = 0.0337) active gal...
and Cronin 2004, showed systematic Faraday rotation gradients across the parsec-scale jets of severa...
Context. This is the third paper in a series devoted to the analysis of the multiwavelength data fro...
Polarization-sensitive lambda= 6 cm global VLBI images of BL Lac for data taken at three epochs are ...
Context. High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal too...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
To determine the location of the intra-day variable (IDV) emission region within the jet of the BL L...
A comparison between low-frequency space very long baseline interferometry (VLBI) and high-frequency...
We present four high dynamic range, dual-circular polarization, Very Long Baseline Array (VLBA) obse...