Peter A. R. Ade

TL;DR: In this paper, the authors discuss the potential of a next generation space-borne Cosmic Microwave Background (CMB) experiment for studies of extragalactic sources, which has particular bearing on the definition of the future space project, CORE, that has been submitted in response to ESA's call for a Medium-size mission opportunity as the successor of the Planck satellite.

TL;DR: In 2012, the South Pole Telescope (SPT) will begin a 625 deg2 survey to measure the polarization anisotropy of the cosmic microwave background (CMB).

TL;DR: In this paper, the authors presented Cygnus X in a new multi-wavelength perspective based on an unbiased BLAST survey at 250, 350, and 500 micron, combined with rich datasets for this well-studied region.

TL;DR: The design of the receiver and its performance when installed on the APEX telescope is described and the instrument has a higher instantaneous sensitivity and covers a larger field-of-view than earlier generations of Sunyaev-Zel'dovich instruments.

TL;DR: In this paper, the sky opacity at 200 μm at the French-Italian station, Concordia, at Dome C, Antarctica was measured with a tipper and compared with satellite measurements from the Infrared Atmospheric Sounding Interferometer (IASI) on Metop-A, with balloon humidity sondes and with results obtained by a ground-based microwave radiometer (HAMSTRAD).