Until recently, only about 10% of the total intracluster gas volume had been studied with high
accuracy, leaving a vast region essentially unexplored. This is now changing and a wide …

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2
and Keck Array have observed the same approximately 400 deg 2 patch of sky centered on …

We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

Superconducting detector arrays have become the standard technology for the current
generation of millimeter-wave and submm-wave astronomical instruments on individual …

An all sky map of the apparent temperature and optical depth of thermal dust emission is
constructed using the Planck-HFI (350μm to 2 mm) andIRAS (100μm) data. The optical …

We present the Planck Sky Model (PSM), a parametric model for generating all-sky, few
arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in …

Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub-
) millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution …

Taking advantage of the all-sky coverage and broadfrequency range of the Planck satellite,
we study the Sunyaev-Zeldovich (SZ) and pressure profiles of 62 nearby massive clusters …

Measurements in the infrared wavelength domain allow direct assessment of the physical
state and energy balance of cool matter in space, enabling the detailed study of the …

We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based
surveys, with known spectroscopic redshifts and observed with the Herschel Space …