549 citations · 5.8k across the 130 of their papers we have counts for
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15 GHz Monitoring of Gamma-ray Blazars with the OVRO 40 Meter Telescope in Support of Fermi
J. L. Richards, W. Max-Moerbeck, V. Pavlidou +11
We present results from the first two years of our fast-cadence 15 GHz gamma-ray blazar monitoring program, part of the F-GAMMA radio monitoring project. Our sample includes the 11…
High resolution AMI Large Array imaging of spinning dust sources: spatially correlated 8 micron emission and evidence of a stellar wind in L675
Anna M. M. Scaife, David A. Green, Guy G. Pooley +15
We present 25 arcsecond resolution radio images of five Lynds Dark Nebulae (L675, L944, L1103, L1111 & L1246) at 16 GHz made with the Arcminute Microkelvin Imager (AMI) Large Array…
VSA Observations of the Anomalous Microwave Emission in the Perseus Region
Christopher T. Tibbs, Robert A. Watson, Clive Dickinson +13
The dust feature G159.6--18.5 in the Perseus region has previously been observed with the COSMOSOMAS experiment \citep{Watson:05} on angular scales of 1, and wa…
AMI observations of Lynds Dark Nebulae: further evidence for anomalous cm-wave emission
Anna M. M. Scaife, Natasha Hurley-Walker, David A. Green +13
Observations at 14.2 to 17.9 GHz made with the AMI Small Array towards fourteen Lynds Dark Nebulae with a resolution of 2' are reported. These sources are selected from the SCUBA o…
9C continued: a radio-source survey at 15 GHz
E. M. Waldram, G. G. Pooley, M. L. Davies +2
In our first paper we described three regions of the 9C survey of radio sources with the Ryle telescope at 15.2 GHz, constituting a total area of 520 deg^2 to a completeness limit…
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: II - Flux-density variability
Thomas M. O. Franzen, Matthew L. Davies, Rod D. Davies +22
Using the Arcminute Microkelvin Imager (AMI) at 16 GHz and the Very Small Array (VSA) at 33 GHz to make follow-up observations of sources in the New Extragalactic WMAP Point Source…