activity
19942011
most citedCosmological constraints from Archeops

203 citations · 1.1k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.IM2011★ 190 cited

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…

astro-ph2006★ 30 cited

Archeops In-flight Performance, Data Processing and Map Making

J. F. Macias-Perez, G. Lagache, B. Maffei +69

Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave B…

astro-ph2005★ 61 cited

Temperature and polarization angular power spectra of Galactic dust radiation at 353 GHz as measured by Archeops

N. Ponthieu, J. F. Macías-Pérez, M. Tristram +47

We present the first measurement of temperature and polarization angular power spectra of the diffuse emission of Galactic dust at 353 GHz as seen by Archeops on 20% of the sky. Th…

astro-ph2004★ 56 cited

The CMB temperature power spectrum from an improved analysis of the Archeops data

M. Tristram, G. Patanchon, J. F. Macias-Perez +47

We present improved results on the measurement of the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops…

astro-ph2003★ 100 cited

First Detection of Polarization of the Submillimetre Diffuse Galactic Dust Emission by Archeops

A. Benoit, P. Ade, A. Amblard +65

We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--bor…

astro-ph2002★ 203 cited

Cosmological constraints from Archeops

A. Benoit, P. Ade, A. Amblard +65

We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum ha…