PKS 1257-326 is one of three quasars known to show unusually large and rapid, intra-hour intensity variations, as a result of scintillation in the turbulent Galactic interstellar medium. We have measured time delays in the variability pattern arrival times at the VLA and the ATCA, as well as an annual cycle in the time-scale of variability for this source. Results of the two-station time delay observations are presented here. Implications for the, scintillation of this source axe discussed in the light of these results, together with results from two years of monitoring with the ATCA
The liberation of gravitational energy as matter falls onto a supermassive black hole at the centre ...
We have measured annual cycles in the time scales of the rapid, intra-day variability of the total a...
We have used the University of Tasmania's 30-m radio telescope at Ceduna in South Australia to regul...
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...
The quasar PKS 0405-385 exhibits episode's of unusually strong hourly variability at 8.6, 4.8, 2.4 a...
Rapid radio intraday variability (IDV) has been discovered in the southern quasar PKS 1257-326. Flux...
We report measurements of time delays of up to 8 minutes in the centimeter wavelength variability pa...
Rapid radio intra-day variability (IDV) has been discovered in the southern quasar PKS 1257−326. Flu...
Interstellar scintillation (ISS) has been established as the cause of the random variations seen at ...
The line of sight towards the compact, radio loud quasar PKS 1257-326 passesthrough a patch of scatt...
Rapid radio intraday variability (IDV) has been discovered in the southern quasar PKS 1257326. Fluxd...
International audienceObservations of the millisecond pulsar B1937+214 made at Nan\c cay over 6 year...
The University of Tasmania Ceduna radio telescope has been used to investigate rapid variability in ...
The liberation of gravitational energy as matter falls onto a supermassive black hole at the centre ...
We have measured annual cycles in the time scales of the rapid, intra-day variability of the total a...
We have used the University of Tasmania's 30-m radio telescope at Ceduna in South Australia to regul...
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...
The quasar PKS 0405-385 exhibits episode's of unusually strong hourly variability at 8.6, 4.8, 2.4 a...
Rapid radio intraday variability (IDV) has been discovered in the southern quasar PKS 1257-326. Flux...
We report measurements of time delays of up to 8 minutes in the centimeter wavelength variability pa...
Rapid radio intra-day variability (IDV) has been discovered in the southern quasar PKS 1257−326. Flu...
Interstellar scintillation (ISS) has been established as the cause of the random variations seen at ...
The line of sight towards the compact, radio loud quasar PKS 1257-326 passesthrough a patch of scatt...
Rapid radio intraday variability (IDV) has been discovered in the southern quasar PKS 1257326. Fluxd...
International audienceObservations of the millisecond pulsar B1937+214 made at Nan\c cay over 6 year...
The University of Tasmania Ceduna radio telescope has been used to investigate rapid variability in ...
The liberation of gravitational energy as matter falls onto a supermassive black hole at the centre ...
We have measured annual cycles in the time scales of the rapid, intra-day variability of the total a...
We have used the University of Tasmania's 30-m radio telescope at Ceduna in South Australia to regul...