2.5k citations · 8.4k across the 72 of their papers we have counts for
72 papers
The Keck Array: a pulse tube cooled CMB polarimeter
C. D. Sheehy, P. A. R. Ade, R. W. Aikin +41
The Keck Array is a cosmic microwave background (CMB) polarimeter that will begin observing from the South Pole in late 2010. The initial deployment will consist of three telescope…
Planck early results: first assessment of the High Frequency Instrument in-flight performance
Planck HFI Core Team, P. A. R. Ade, N. Aghanim +163
The Planck High Frequency Instrument (HFI) is designed to measure the temperature and polarization anisotropies of the Cosmic Microwave Background and galactic foregrounds in six w…
The QUaD Galactic Plane Survey II: A Compact Source Catalog
T. Culverhouse, P. Ade, J. Bock +28
We present a catalog of compact sources derived from the QUaD Galactic Plane Survey. The survey covers ~800 square degrees of the inner galaxy (|b|<4 degrees) in Stokes I, Q and U…
Antenna-coupled TES Bolometer Arrays for BICEP2/Keck and SPIDER
A. Orlando, R. W Aikin, M. Amiri +28
BICEP2/Keck and SPIDER are cosmic microwave background (CMB) polarimeters targeting the B-mode polarization induced by primordial gravitational waves from inflation. They will be u…
Measuring Planck beams with planets
K. M. Huffenberger, B. P. Crill, A. E. Lange +2
Accurate measurement of the cosmic microwave background (CMB) anisotropy requires precise knowledge of the instrument beam. We explore how well the Planck beams will be determined…
Planck pre-launch status: High Frequency Instrument polarization calibration
C. Rosset, M. Tristram, N. Ponthieu +34
The High Frequency Instrument of Planck will map the entire sky in the millimeter and sub-millimeter domain from 100 to 857 GHz with unprecedented sensitivity to polarization ($ΔP/…