BL Lacertae objects are an extreme subclass of AGNs showing rapid and large-amplitude variability, high and variable polarization, and core-dominated radio emissions. If a strong beaming effect is the cause of the extreme observation properties, one would expect that these properties would be correlated with each other. Based on the relativistic beaming model, relationships between the polarization and the magnitude variation in brightness, as well as the core-dominance parameter are derived and used statistically to compare with the observational data of a BL Lacertae object sample. The statistical results are consistent with these correlations, which suggests that the polarization, the variation, and the core-dominance parameter are possi...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
In this paper, based on the polarization-Doppler factor result (Fan et al. 1997, paper I), relations...
In the present work, using the data base of the University of Michigan Radio Astronomy Observatory (...
Based on the beaming model, a relation between the observed polarization and the Doppler factor was ...
Context. We investigate the optical polarization properties of high-energy BL Lac objects using data...
We have used the optical polarization properties of BL Lacertae objects to gain insights into the ra...
We present and discuss polarimetric observations of 182 targets drawn from an optically selected sam...
BL Lacertae objects are the most extreme members of a class of objects known as Active Galactic Nucl...
We present the results of a systematic observational campaign designed to search for microvariabilit...
We present results from a long-term program to quantify the range of behavior of the cm-wavelength t...
International audienceBlazars are a class of jet-dominated active galactic nuclei with a typical dou...
Photometric observations of AGNs are important to construct light curves and to study variability be...
This thesis presents the results of a series of polarization VLBI experiments on the wellknown varia...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
In this paper, based on the polarization-Doppler factor result (Fan et al. 1997, paper I), relations...
In the present work, using the data base of the University of Michigan Radio Astronomy Observatory (...
Based on the beaming model, a relation between the observed polarization and the Doppler factor was ...
Context. We investigate the optical polarization properties of high-energy BL Lac objects using data...
We have used the optical polarization properties of BL Lacertae objects to gain insights into the ra...
We present and discuss polarimetric observations of 182 targets drawn from an optically selected sam...
BL Lacertae objects are the most extreme members of a class of objects known as Active Galactic Nucl...
We present the results of a systematic observational campaign designed to search for microvariabilit...
We present results from a long-term program to quantify the range of behavior of the cm-wavelength t...
International audienceBlazars are a class of jet-dominated active galactic nuclei with a typical dou...
Photometric observations of AGNs are important to construct light curves and to study variability be...
This thesis presents the results of a series of polarization VLBI experiments on the wellknown varia...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...