Add to ORKGThe OVRO 40 m Telescope monitoring program carries out twice-weekly measurements of the 15 GHz flux density of nearly 1600 blazars and other AGN, including all those associated with northern (declination > −20°) Fermi Large Area Telescope (LAT) detections and a preselected sample ideal for statistical studies. We present some results from the program and describe the statistical method we have developed to assess the intrinsic radio variability of the sources in our sample. We also present a method for assessing the significance of correlations between radio and gamma-ray light curves
Blazars are known to show periods of quiescence followed by outbursts visible throughout the electro...
In order to determine the location of the gamma-ray emission site in blazars, we investigate the tim...
We collect the second Large Area Telescope AGN catalog (2LAC) and Monitor of Jets in AGN with VLBA E...
The OVRO 40 m Telescope monitoring program carries out twice-weekly measurements of the 15 GHz flux ...
Variability is an important and defining characteristic of AGN, that along with their broadband spec...
The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented ...
Since mid-2007, we have been monitoring similar to 1200 sources at 15 GHz with the 40 M Telescope ...
Since late 2007, we have been monitoring a large sample of known and likely gamma-ray–loud blazars a...
We have continued our monitoring program of ~1200 sources with the Owens Valley Radio Observatory 4...
Since mid-2007 we have carried out a dedicated long-term monitoring programme at 15 GHz using the Ow...
A large sample of blazar from the Candidate Gamma Ray Blazar Survey (CGRaBS) has been observed with ...
The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented ...
We have carried out a multifrequency analysis of the radio variability of blazars, exploiting the da...
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future b...
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future b...
Blazars are known to show periods of quiescence followed by outbursts visible throughout the electro...
In order to determine the location of the gamma-ray emission site in blazars, we investigate the tim...
We collect the second Large Area Telescope AGN catalog (2LAC) and Monitor of Jets in AGN with VLBA E...
The OVRO 40 m Telescope monitoring program carries out twice-weekly measurements of the 15 GHz flux ...
Variability is an important and defining characteristic of AGN, that along with their broadband spec...
The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented ...
Since mid-2007, we have been monitoring similar to 1200 sources at 15 GHz with the 40 M Telescope ...
Since late 2007, we have been monitoring a large sample of known and likely gamma-ray–loud blazars a...
We have continued our monitoring program of ~1200 sources with the Owens Valley Radio Observatory 4...
Since mid-2007 we have carried out a dedicated long-term monitoring programme at 15 GHz using the Ow...
A large sample of blazar from the Candidate Gamma Ray Blazar Survey (CGRaBS) has been observed with ...
The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented ...
We have carried out a multifrequency analysis of the radio variability of blazars, exploiting the da...
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future b...
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future b...
Blazars are known to show periods of quiescence followed by outbursts visible throughout the electro...
In order to determine the location of the gamma-ray emission site in blazars, we investigate the tim...
We collect the second Large Area Telescope AGN catalog (2LAC) and Monitor of Jets in AGN with VLBA E...