activity
20102015
most citedPlanck Early Results. II. The thermal performance of Planck

143 citations · 440 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2015★ 25 cited

Peculiar Velocity Constraints from Five-Band SZ Effect Measurements Towards RX J1347.5-1145 with MUSIC and Bolocam from the CSO

Jack Sayers, Michael Zemcov, Jason Glenn +25

We present Sunyaev-Zel'dovich (SZ) effect measurements from wide-field images towards the galaxy cluster RX J1347.5-1145 obtained from the Caltech Submillimeter Observatory with th…

astro-ph.IM2015★ 90 cited

Antenna-coupled TES bolometers used in BICEP2, Keck array, and SPIDER

P. A. R. Ade, R. W. Aikin, M. Amiri +64

We have developed antenna-coupled transition-edge sensor (TES) bolometers for a wide range of cosmic microwave background (CMB) polarimetry experiments, including BICEP2, Keck Arra…

astro-ph.IM2013★ 8 cited

In-flight calibration and verification of the Planck-LFI instrument

Anna Gregorio, Francesco Cuttaia, Aniello Mennella +40

In this paper we discuss the Planck-LFI in-flight calibration campaign. After a brief overview of the ground test campaigns, we describe in detail the calibration and performance v…

astro-ph.IM2012★ 40 cited

Status of MUSIC, the MUltiwavelength Sub/millimeter Inductance Camera

Sunil R. Golwala, Clint Bockstiegel, Spencer Brugger +21

We present the status of MUSIC, the MUltiwavelength Sub/millimeter Inductance Camera, a new instrument for the Caltech Submillimeter Observatory. MUSIC is designed to have a 14', d…

astro-ph.IM2012★ 18 cited

Antenna-coupled TES bolometers for the Keck Array, Spider, and Polar-1

R. O'Brient, P. A. R. Ade, Z. Ahmed +50

Between the BICEP2 and Keck Array experiments, we have deployed over 1500 dual polarized antenna coupled bolometers to map the Cosmic Microwave Background's polarization. We have b…

astro-ph.IM2012★ 17 cited

Optimization and sensitivity of the Keck Array

S. Kernasovskiy, P. A. R. Ade, R. W. Aikin +41

The Keck Array (SPUD) began observing the cosmic microwave background's polarization in the winter of 2011 at the South Pole. The Keck Array follows the success of the predecessor…