Peter A. R. Ade

TL;DR: In this article, the authors have placed 860 GHz sky brightness monitors at all three sites and present a comparative study of the measured sub-millimeter brightness due to atmospheric thermal emission.

TL;DR: The BICEP2 and the Keck Array are part of a program of experiments at the South Pole whose main goal is to achieve the sensitivity and systematic control necessary for measurements of the tensor-to-scalar ratio at σ(r) ~ 0:01 as discussed by the authors.

TL;DR: The Exoplanet Characterisation Observatory (EChO) as mentioned in this paper is the first dedicated mission to investigate the physics and chemistry of exoplanetary atmospheres and has been selected by the European Space Agency to be assessed as one of four M3 mission candidates.

TL;DR: The Arcminute Cosmology Bolometer Array Receiver (ACBAR) as discussed by the authors is a multifrequency millimeter-wave receiver designed for observations of the Cosmic Microwave Background (CMB) and the Sunyaev-Zel'dovich effect in clusters of galaxies.

TL;DR: Chiang et al. as mentioned in this paper extended the two-year result with additional data from the third season and relaxed detector-selection criteria, and presented a more comprehensive estimation of band-power window functions, improved likelihood estimation methods and a new technique for deprojecting monopole temperature-to-polarization leakage.