Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]The authors present measurements of the polarization and flux of a sample of 28 blazars (21 BL Lacs and 7 OVV quasars) at optical and near-infrared wavelengths, with repeated observations for some objects. As in earlier work, the authors find that the level of polarization in the infrared are generally equal to, or lower than, those in the optical, although for some objects with low levels of polarization (P < 10 per cent), the polarization in the infrared can exceed that in the optical. Large wavelength dependences of polarization, in which the polarization increases with decreasing wav...
The results of intensive multiwavelength observations of a sample of 19 blazars reveal a distinct co...
Polarization variability is one of the most ubiquitous characteristic of blazars. Near infrared (NIR...
Context. Blazars are astrophysical sources whose emission is dominated by non-thermal processes, i.e...
Original article can be found at: http://www.adsabs.harvard.edu/ Copyright European Southern Observa...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA]A pola...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
Incl. reprint in wallet at backSIGLEAvailable from British Library Document Supply Centre- DSC:D6825...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical...
A sample of blazars has been studied with infrared photometry and polarimetry in the J,H & K waveba...
Original article can be found at: http://www.nature.com/nature/ Copyright Nature Publishing Group. D...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
This thesis presents a study of some of the optical and infrared properties of blazars. A review of...
Context. Blazars are astrophysical sources whose emission is dominated by non-thermal processes, i.e...
The results of intensive multiwavelength observations of a sample of 19 blazars reveal a distinct co...
Polarization variability is one of the most ubiquitous characteristic of blazars. Near infrared (NIR...
Context. Blazars are astrophysical sources whose emission is dominated by non-thermal processes, i.e...
Original article can be found at: http://www.adsabs.harvard.edu/ Copyright European Southern Observa...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA]A pola...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
Incl. reprint in wallet at backSIGLEAvailable from British Library Document Supply Centre- DSC:D6825...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical...
A sample of blazars has been studied with infrared photometry and polarimetry in the J,H & K waveba...
Original article can be found at: http://www.nature.com/nature/ Copyright Nature Publishing Group. D...
Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society ...
This thesis presents a study of some of the optical and infrared properties of blazars. A review of...
Context. Blazars are astrophysical sources whose emission is dominated by non-thermal processes, i.e...
The results of intensive multiwavelength observations of a sample of 19 blazars reveal a distinct co...
Polarization variability is one of the most ubiquitous characteristic of blazars. Near infrared (NIR...
Context. Blazars are astrophysical sources whose emission is dominated by non-thermal processes, i.e...