We investigate the relationship between the 5 GHz interstellar scintillation (ISS) and the 15 GHz intrinsic variability of the compact, radio-selected active galactic nuclei (AGN) common to the Microarcsecond Scintillation-Induced Variability (MASIV) Survey and the Owens Valley Radio Observatory blazar flux density monitoring program. As part of this investigation, we also re-examine the reported intrinsic nature of the February 1990 VLA observations of the blazar S5 0716+714. We are also examining the presence of IDV/ISS in the Owens Valley 15 GHz flux density monitoring data. We find a significant relationship between the Owens Valley 15 GHz modulation index and the MASIV modulation index. We also discuss the implications of these finding...
From 1979--1996 the Green Bank Interferometer was used by the Naval Research Laboratory to monitor t...
The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optic...
The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optic...
We investigate the relationship between the 5 GHz interstellar scintillation (ISS) and the 15 GHz in...
We investigate the relationship between the 5 GHz interstellar scintillation (ISS) and the 15 GHz in...
We investigate the relationship between 5 GHz interstellar scintillation (ISS) and 15 GHz intrinsic ...
We investigate the relationship between 5 GHz interstellar scintillation (ISS) and 15 GHz intrinsic...
We have conducted the first systematic search for interday variability in a large sample of extragal...
The Micro-arcsecond Scintillation-Induced Variability (MASIV) Survey and its follow-up observations ...
A large fraction of compact, extragalactic radio sources exhibit rapid variability at centimetre wav...
Intraday variability (IDV) of the radio emission from active galactic nuclei is now known to be pred...
This thesis presents several observational studies based on radio variability and interstellar scin...
We present the first results of an ongoing intra-day variability (IDV) flux density monitoring progr...
We have conducted the first systematic search for interday variability in a large sample of extragal...
Intraday variability (IDV) of the radio emission from active galactic nuclei is now known to be pred...
From 1979--1996 the Green Bank Interferometer was used by the Naval Research Laboratory to monitor t...
The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optic...
The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optic...
We investigate the relationship between the 5 GHz interstellar scintillation (ISS) and the 15 GHz in...
We investigate the relationship between the 5 GHz interstellar scintillation (ISS) and the 15 GHz in...
We investigate the relationship between 5 GHz interstellar scintillation (ISS) and 15 GHz intrinsic ...
We investigate the relationship between 5 GHz interstellar scintillation (ISS) and 15 GHz intrinsic...
We have conducted the first systematic search for interday variability in a large sample of extragal...
The Micro-arcsecond Scintillation-Induced Variability (MASIV) Survey and its follow-up observations ...
A large fraction of compact, extragalactic radio sources exhibit rapid variability at centimetre wav...
Intraday variability (IDV) of the radio emission from active galactic nuclei is now known to be pred...
This thesis presents several observational studies based on radio variability and interstellar scin...
We present the first results of an ongoing intra-day variability (IDV) flux density monitoring progr...
We have conducted the first systematic search for interday variability in a large sample of extragal...
Intraday variability (IDV) of the radio emission from active galactic nuclei is now known to be pred...
From 1979--1996 the Green Bank Interferometer was used by the Naval Research Laboratory to monitor t...
The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optic...
The discovery of the first quasar 3C 273 led directly to the discovery of their variability at optic...