Add to ORKGThe quasar PKS 0405-385 exhibits episode's of unusually strong hourly variability at 8.6, 4.8, 2.4 and 1.4 GHz. These variations, seen first in June 1996, ceased after several weeks, but reappeared in November 1998 and were monitored closely at the. ATCA. We argue that our data are in agreement with interstellar scintillation of a source component which is a few micro-arcseconds in size. This claim is further supported by our recent finding of the time delay in the variability pattern measured between the ATCA and the VLA
We present the results from a study of the timing properties and the energy spectrum of the radio-qu...
We examine the long-term evolution of the intra-hour variable quasar, J1819+3845, whose ...
The University of Tasmania Ceduna radio telescope has been used to investigate rapid variability in ...
The quasar PKS 0405-385 exhibits episode's of unusually strong hourly variability at 8.6, 4.8, 2.4 a...
PKS 1257-326 is one of three quasars known to show unusually large and rapid, intra-hour intensity v...
We report measurements of time delays of up to 8 minutes in the centimeter-wavelength variability pa...
Rapid radio intraday variability (IDV) has been discovered in the southern quasar PKS 1257-326. Flux...
Interstellar scintillation (ISS) has been established as the cause of the random variations seen at ...
Rapid radio intra-day variability (IDV) has been discovered in the southern quasar PKS 1257−326. Flu...
We report measurements of time delays of up to 8 minutes in the centimeter wavelength variability pa...
We have measured annual cycles in the time scales of the rapid, intra-day variability of the total a...
Aims. The quasar 1156+295 (4C +29.45) is one of the targets in the Urumqi monitoring program which a...
We have observed profound variability in the radio flux density of the quasar PKS 0405-385 on timesc...
We present the results from a study of the timing properties and the energy spectrum of the radio-qu...
We examine the long-term evolution of the intra-hour variable quasar, J1819+3845, whose ...
The University of Tasmania Ceduna radio telescope has been used to investigate rapid variability in ...
The quasar PKS 0405-385 exhibits episode's of unusually strong hourly variability at 8.6, 4.8, 2.4 a...
PKS 1257-326 is one of three quasars known to show unusually large and rapid, intra-hour intensity v...
We report measurements of time delays of up to 8 minutes in the centimeter-wavelength variability pa...
Rapid radio intraday variability (IDV) has been discovered in the southern quasar PKS 1257-326. Flux...
Interstellar scintillation (ISS) has been established as the cause of the random variations seen at ...
Rapid radio intra-day variability (IDV) has been discovered in the southern quasar PKS 1257−326. Flu...
We report measurements of time delays of up to 8 minutes in the centimeter wavelength variability pa...
We have measured annual cycles in the time scales of the rapid, intra-day variability of the total a...
Aims. The quasar 1156+295 (4C +29.45) is one of the targets in the Urumqi monitoring program which a...
We have observed profound variability in the radio flux density of the quasar PKS 0405-385 on timesc...
We present the results from a study of the timing properties and the energy spectrum of the radio-qu...
We examine the long-term evolution of the intra-hour variable quasar, J1819+3845, whose ...
The University of Tasmania Ceduna radio telescope has been used to investigate rapid variability in ...