activity
20032008
most citedThe Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey II: The First Four Epochs

132 citations · 193 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph2008132 cited

The Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey II: The First Four Epochs

J. E. J. Lovell, B. J. Rickett, J-P. Macquart +8

We report on the variability of 443 flat spectrum, compact radio sources monitored using the VLA for 3 days in 4 epochs at ~ 4 month intervals at 5 GHz as part of the Micro-Arcseco…

astro-ph200761 cited

The Origin of Radio Scintillation In the Local Interstellar Medium

Jeffrey L. Linsky, Barney J. Rickett, Seth Redfield

We study three quasar radio sources (B1257-326, B1519-273, and J1819+385) that show large amplitude intraday and annual scintillation variability produced by the Earth's motion rel…

astro-ph2007

MASIV:The Microarcsecond Scintillation-Induced Variability Survey

J. E. J. Lovell, D. L. Jauncey, C. Senkbeil +8

We are undertaking a large-scale 5 GHz VLA survey of the northern sky to search for rapid intra-day variability (IDV). Over four observing epochs we found that 56% of the sources s…

astro-ph2006

International Colloquium "Scattering and Scintillation in Radio Astronomy" was held on June 19-23, 2006 in Pushchino, Moscow region, Russia

V. I. Shishov, W. A. Coles, B. J. Rickett +52

Topics of the Colloquium: a) Interplanetary scintillation b) Interstellar scintillation c) Modeling and physical origin of the interplanetary and the interstellar plasma turbulence…

astro-ph2005

Interstellar Scintillation Observations of 146 Extragalactic Radio Sources

B. Rickett, T. J. W. Lazio, F. D. Ghigo

From 1979--1996 the Green Bank Interferometer was used by the Naval Research Laboratory to monitor the flux density from 146 compact radio sources at frequencies near 2 and 8 GHz.…

astro-ph2005

Long-term Scintillation Observations of Five Pulsars at 1540 MHz

N. Wang, R. N. Manchester, S. Johnston +4

From 2001 January to 2002 June, we monitored PSRs B0329+54, B0823+26, B1929+10, B2020+28 and B2021+51 using the Nanshan 25-m radio telescope of Urumqi Observatory to study their di…