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19942024
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 24.5k across the 122 of their papers we have counts for

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19 papers · 1 filter

astro-ph2006★ 38 cited

An upper limit to polarized submillimetre emission in Arp 220

Michael Seiffert, Colin Borys, Douglas Scott +1

We report the results of pointed observations of the prototypical ultra-luminous infrared galaxy (ULIRG) Arp 220 at 850 microns using the polarimeter on the SCUBA instrument on the…

astro-ph2006★ 29 cited

ARCADE: Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission

A. Kogut, D. Fixsen, S. Fixsen +8

The Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission (ARCADE) is a balloon-borne instrument designed to measure the temperature of the cosmic microwave backgro…

astro-ph2005★ 130 cited

CMB component separation by parameter estimation

H. K. Eriksen, C. Dickinson, C. R. Lawrence +9

We propose a solution to the CMB component separation problem based on standard parameter estimation techniques. We assume a parametric spectral model for each signal component, an…

astro-ph2005

Probing Dark Energy via Weak Gravitational Lensing with the SuperNova Acceleration Probe (SNAP)

SNAP Collaboration

SNAP is a candidate for the Joint Dark Energy Mission (JDEM) that seeks to place constraints on the dark energy using two distinct methods. The first, Type Ia SN, is discussed in a…

astro-ph2005★ 14 cited

Angular power spectrum of the FastICA CMB component from BEAST data

S. Donzelli, D. Maino, M. Bersanelli +9

We present the angular power spectrum of the CMB component extracted with FastICA from the Background Emission Anisotropy Scanning Telescope (BEAST) data. BEAST is a 2.2 meter off-…

astro-ph2004★ 14 cited

Galactic foreground contribution to the BEAST CMB Anisotropy Maps

Jorge Mejía, Marco Bersanelli, Carlo Burigana +17

We report limits on the Galactic foreground emission contribution to the Background Emission Anisotropy Scanning Telescope (BEAST) Ka- and Q-band CMB anisotropy maps. We estimate t…