Dust-correlated cm wavelength continuum emission from translucent clouds ζ Oph and LDN 1780
Monthly Notices of the Royal Astronomical Society (2011)
The Cosmic Background Imager 2
Monthly Notices of the Royal Astronomical Society (2011)
A 43-GHz VLA survey in the ELAIS N2 area
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 408:2 (2010) 657-668
The C-Band All-Sky Survey: Instrument design, status, and first-look data
Proceedings of SPIE - The International Society for Optical Engineering 7741 (2010)
Abstract:
The C-Band All-Sky Survey (C-BASS) aims to produce sensitive, all-sky maps of diffuse Galactic emission at 5 GHz in total intensity and linear polarization. These maps will be used (with other surveys) to separate the several astrophysical components contributing to microwave emission, and in particular will allow an accurate map of synchrotron emission to be produced for the subtraction of foregrounds from measurements of the polarized Cosmic Microwave Background. We describe the design of the analog instrument, the optics of our 6.1 m dish at the Owens Valley Radio Observatory, the status of observations, and first-look data. © 2010 SPIE.The C-Band All-Sky Survey: Instrument design, status, and first-look data
ArXiv 1008.4082 (2010)