We used data from the University of Michigan Radio Astronomy Observatory (UMRAO) at three different bands (4.8 GHz, 8 GHz, and 14.5 GHz) to calculate the radio spectral index and the averaged polarization in a sample of 92 flat spectrum radio quasars (FSRQs). We analyzed the relationship between the polarization and other physical parameters for these objects. The results show that: 1) the polarization and its variability at high radio frequencies are higher than those at lower frequencies, 2) the degree of linear polarization is correlated with the radio spectral index, suggesting that the synchrotron mechanism is responsible for the radio emission, 3) the polarization is correlated with the core-dominance parameter for those objects for w...
•Radio galaxies are a subset of all galaxies that emit high amounts of radio waves into space. •The ...
International audienceA small subset of optically selected radio-quiet quasars showing weak or no em...
Context. Rapid variations in optical flux are seen in many quasars and all blazars. The amount of va...
We used data from the University of Michigan Radio Astronomy Observatory (UMRAO) at three different ...
In the present work, using the data base of the University of Michigan Radio Astronomy Observatory (...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Aims. We performed observations with the Effelsberg 100-m radio telescope to measure flux ...
The “bright” High Frequency Peakers (HFPs) sample is a mixture of blazars and intrinsically small an...
Accepted for publication in the Astrophysical Journal. A significant fraction of flat-spectrum, rad...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
We present polarization properties at 1.4 GHz of two separate extragalactic source populations: pass...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
Aims.The “bright” High Frequency Peakers (HFPs) sample is a mixture of blazars and intrinsically sm...
We present polarization images of 9 radio-loud (RL) quasars from the VLA B-array at 6 GHz. These qua...
•Radio galaxies are a subset of all galaxies that emit high amounts of radio waves into space. •The ...
International audienceA small subset of optically selected radio-quiet quasars showing weak or no em...
Context. Rapid variations in optical flux are seen in many quasars and all blazars. The amount of va...
We used data from the University of Michigan Radio Astronomy Observatory (UMRAO) at three different ...
In the present work, using the data base of the University of Michigan Radio Astronomy Observatory (...
International audienceWe present a polarization variability analysis of a sample of 26 γ-ray blazars...
Aims. We performed observations with the Effelsberg 100-m radio telescope to measure flux ...
The “bright” High Frequency Peakers (HFPs) sample is a mixture of blazars and intrinsically small an...
Accepted for publication in the Astrophysical Journal. A significant fraction of flat-spectrum, rad...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
We present the results of two multiwavelength campaigns - in October of 2005 and March of 2006 - dur...
We present polarization properties at 1.4 GHz of two separate extragalactic source populations: pass...
We investigate the statistical properties of the polarized emission of extragalactic radio sources a...
Aims.The “bright” High Frequency Peakers (HFPs) sample is a mixture of blazars and intrinsically sm...
We present polarization images of 9 radio-loud (RL) quasars from the VLA B-array at 6 GHz. These qua...
•Radio galaxies are a subset of all galaxies that emit high amounts of radio waves into space. •The ...
International audienceA small subset of optically selected radio-quiet quasars showing weak or no em...
Context. Rapid variations in optical flux are seen in many quasars and all blazars. The amount of va...