Reconstruction of HI power spectra with radio-interferometers to study dark energy (2008)
Ansari, R., Goff, J. -M. Le, Magneville, Ch., Moniez, M., Palanque-Delabrouille, N., Rich, J., ...
Among the tools available for the study of the dark energy driving the expansion of the Universe, Baryon Acoustic Oscillations (BAO) and their effects on the matter power spectrum are particularly...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
Cosmological constraints from Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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 has small bins in l...
Cosmological constraints from Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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 has small bins in l...
Cosmological constraints from Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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 has small bins in l...
Archeops In-flight Performance, Data Processing and Map Making (2006)
Macias-Perez, J. F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
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 Background (CMB)...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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--borne instrument was...
The CMB temperature power spectrum from an improved analysis of the Archeops data (2004)
Tristram, M., Patanchon, G., Macias-Perez, J. F., Ade, P., Amblard, A., Ansari, R., ...
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 flight. This...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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--borne instrument was...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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--borne instrument was...
Cosmological constraints from Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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 has small bins in l...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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--borne instrument was...
Cosmological constraints from Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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 has small bins in l...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2002)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
Cosmological constraints from Archeops (2002)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
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 has small bins in l...