SPITZER-IRAC Identification of HERSCHEL-ATLAS SPIRE Sources
\apj 756 (2012) 28-28
Star formation in high-redshift quasars: excess [O II] emission in the radio-loud population
ArXiv e-prints (2012)
Future Science Prospects for AMI
ArXiv 1208.1966 (2012)
Abstract:
The Arcminute Microkelvin Imager (AMI) is a telescope specifically designed for high sensitivity measurements of low-surface-brightness features at cm-wavelength and has unique, important capabilities. It consists of two interferometer arrays operating over 13.5-18 GHz that image structures on scales of 0.5-10 arcmin with very low systematics. The Small Array (AMI-SA; ten 3.7-m antennas) couples very well to Sunyaev-Zel'dovich features from galaxy clusters and to many Galactic features. The Large Array (AMI-LA; eight 13-m antennas) has a collecting area ten times that of the AMI-SA and longer baselines, crucially allowing the removal of the effects of confusing radio point sources from regions of low surface-brightness, extended emission. Moreover AMI provides fast, deep object surveying and allows monitoring of large numbers of objects. In this White Paper we review the new science - both Galactic and extragalactic - already achieved with AMI and outline the prospects for much more.Cosmological measurements with forthcoming radio continuum surveys
\mnras 424 (2012) 801-819-801-819
Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z \lt 0.5
ArXiv e-prints (2012)