papers

Publications (14)

astro-ph.CO2014

BICEP2 II: Experiment and Three-Year Data Set

BICEP2 Collaboration, P. A. R Ade, R. W. Aikin +49

We report on the design and performance of the BICEP2 instrument and on its three-year data set. BICEP2 was designed to measure the polarization of the cosmic microwave background…

astro-ph.GA2010

Herschel-SPIRE spectroscopy of G29.96-0.02: fitting the full SED

J. M. Kirk, E. Polehampton, L. D. Anderson +42

We use the SPIRE Fourier-Transform Spectrometer (FTS) on-board the ESA Herschel Space Telescope to analyse the submillimetre spectrum of the Ultra-compact HII region G29.96-0.02. S…

astro-ph.CO2013

SPIDER: Probing the Early Universe with a Suborbital Polarimeter

A. A. Fraisse, P. A. R. Ade, M. Amiri +43

We evaluate the ability of SPIDER, a balloon-borne polarimeter, to detect a divergence-free polarization pattern ("B-modes") in the Cosmic Microwave Background (CMB). In the inflat…

astro-ph.IM2015

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.CO2011

Spider Optimization II: Optical, Magnetic and Foreground Effects

D. T. O'Dea, P. A. R. Ade, M. Amiri +43

Spider is a balloon-borne instrument designed to map the polarization of the cosmic microwave background (CMB) with degree-scale resolution over a large fraction of the sky. Spider…

astro-ph.EP2010

The Herschel-SPIRE submillimetre spectrum of Mars

B. M. Swinyard, P. Hartogh, S. Sidher +44

We have obtained the first continuous disk averaged spectrum of Mars from 450 to 1550 Ghz using the Herschel-SPIRE Fourier Transform Spectrometer. The spectrum was obtained at a co…

astro-ph.GA2010

Herschel-SPIRE observations of the Polaris flare : structure of the diffuse interstellar medium at the sub-parsec scale

M. -A. Miville-Deschênes, P. G. Martin, A. Abergel +42

We present a power spectrum analysis of the Herschel-SPIRE observations of the Polaris flare, a high Galactic latitude cirrus cloud midway between the diffuse and molecular phases.…

astro-ph.GA2010

The physical properties of the dust in the RCW 120 HII region as seen by Herschel

L. D. Anderson, A. Zavagno, J. A. Rodon +41

Context. RCW 120 is a well-studied, nearby Galactic HII region with ongoing star formation in its surroundings. Previous work has shown that it displays a bubble morphology at mid-…

astro-ph.GA2010

Physical properties of the Sh2-104 HII region as seen by Herschel

J. A. Rodón, A. Zavagno, J. -P. Baluteau +46

Context: Sh2-104 is a Galactic H ii region with a bubble morphology, detected at optical and radio wavelengths. It is considered the first observational confirmation of the collect…

astro-ph.GA2010

Herschel-SPIRE spectroscopy of the DR21 molecular cloud core

Glenn J. White, A. Abergel, L. Spencer +47

We present far-infrared spectra and maps of the DR21 molecular cloud core between 196 and 671 microns, using the Herschel-SPIRE spectrometer. Nineteen molecular lines originating f…

astro-ph.IM2012

BICEP2 and Keck Array operational overview and status of observations

R. W. Ogburn, P. A. R. Ade, R. W. Aikin +50

The BICEP2 and Keck Array experiments are designed to measure the polarization of the cosmic microwave background (CMB) on angular scales of 2-4 degrees (l=50-100). This is the reg…

astro-ph.IM2012

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

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…

astro-ph.GA2010

First detection of the Methylidyne cation (CH+) fundamental rotational line with the Herschel/SPIRE FTS

D. A. Naylor, E. Dartois, E. Habart +41

Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Methods. SPIRE FTS sparse sampled maps of the Orion bar & compact HII regions G29.96-0…