256 citations · 2.6k across the 84 of their papers we have counts for
7 papers · 2 filters
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…
The relationship between star formation rate and radio synchrotron luminosity at 0 < z < 2
Timothy Garn, David A. Green, Julia M. Riley +1
We probe the relationship between star formation rate (SFR) and radio synchrotron luminosity in galaxies at 0 < z < 2 within the northern Spitzer Wide-area Infrared Extragalactic s…
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…
X-ray Spectral Variations in the Youngest Galactic Supernova Remnant G1.9+0.3
S. P. Reynolds, K. J. Borkowski, D. A. Green +3
The discovery of the youngest Galactic supernova remnant (SNR) G1.9+0.3 has allowed a look at a stage of SNR evolution never before observed. We analyze the 50 ks Chandra observati…
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…
The nature of the ASCA/INTEGRAL source AX J183039-1002: a new Compton-thick AGN?
L. Bassani, R. Landi, R. Campana +6
We report on the identification of the X/soft gamma-ray source AX J183039-1002 detected with ASCA and INTEGRAL/IBIS. The source, which has an observed 20-100 keV flux of about 8.6…