most citedACTPol: A polarization-sensitive receiver for the Atacama Cosmology Telescope

200 citations · 624 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.IM201129 cited

Design and performance of the Spider instrument

M. C. Runyan, P. A. R. Ade, M. Amiri +40

Here we describe the design and performance of the Spider instrument. Spider is a balloon-borne cosmic microwave background polarization imager that will map part of the sky at 90,…

astro-ph.CO2011165 cited

Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements

Blake D. Sherwin, Joanna Dunkley, Sudeep Das +35

For the first time, measurements of the cosmic microwave background radiation (CMB) alone favor cosmologies with dark energy over models without dark energy at a 3.2-sigma l…

astro-ph.IM20112 cited

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…

astro-ph.IM201016 cited

The Atacama B-Mode Search: CMB Polarimetry with Transition-Edge-Sensor Bolometers

T. Essinger-Hileman, J. W. Appel, J. A. Beall +15

The Atacama B-mode Search (ABS) experiment is a 145 GHz polarimeter designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB) at large angular scales. Th…

astro-ph.CO201094 cited

The Atacama Cosmology Telescope: Extragalactic Sources at 148 GHz in the 2008 Survey

T. A. Marriage, J. B. Juin, Y. -T. Lin +66

We report on extragalactic sources detected in a 455 square-degree map of the southern sky made with data at a frequency of 148 GHz from the Atacama Cosmology Telescope 2008 observ…

astro-ph.IM2010200 cited

ACTPol: A polarization-sensitive receiver for the Atacama Cosmology Telescope

M. D. Niemack, P. A. R. Ade, J. Aguirre +39

The six-meter Atacama Cosmology Telescope (ACT) in Chile was built to measure the cosmic microwave background (CMB) at arcminute angular scales. We are building a new polarization…