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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…
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…
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…
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: I - Spectral properties
Matthew L. Davies, Thomas M. O. Franzen, Rod D. Davies +22
We present follow-up observations of 97 point sources from the Wilkinson Microwave Anisotropy Probe (WMAP) 3-year data, contained within the New Extragalactic WMAP Point Source (NE…
G64.5+0.9, a new shell supernova remnant with unusual central emission
AMI Consortium, :, Natasha Hurley-Walker +15
We present observations between 1.4 and 18 GHz confirming that G64.5+0.9 is new Galactic shell supernova remnant, using the Very Large Array and the Arcminute Microkelvin Imager. T…
AMI observations of northern supernova remnants at 14-18 GHz
Natasha Hurley-Walker, A. M. M. Scaife, D. A. Green +12
We present observations between 14.2 and 17.9 GHz of 12 reported supernova remnants (SNRs) made with the Arcminute Microkelvin Imager Small Array (AMI SA). In conjunction with data…