32 citations · 32 across the 1 of their papers we have counts for
6 papers
Inverse temperature dependence of the dust submillimeter spectral index
X. Dupac, J. -P. Bernard, N. Boudet +5
We present here a compilation of PRONAOS-based results concerning the temperature dependence of the dust submillimeter spectral index, including data from Galactic cirrus, star-for…
The XMM-Newton Project
J. G. Bartlett, N. Aghanim, M. Arnaud +16
The abundance of high-redshift galaxy clusters depends sensitively on the matter density $\OmM$ and, to a lesser extent, on the cosmological constant . Measurements of this abun…
Analysis of ProNaOS submillimeter maps in the M42 Orion Nebula - Temperature - spectral index inverse correlation in several regions
Xavier Dupac, M. Giard, J. -P. Bernard +5
We have mapped with the French submillimeter balloon-borne telescope ProNaOS the thermal emission of the dust in the M42 Orion Nebula. The map obtained is 50' by 40' with an angula…
All sky mapping of the Cosmic Microwave Background at 8' angular resolution with a 0.1 K bolometer: simulations
M. Giard, E. Hivon, C. Nguyen +4
We present simulations of observations with the 143 GHz channel of the Planck High Frequency Instrument (HFI). These simulations are performed over the entire sky, using the true a…
A Sunyaev-Zel'dovich map of the massive core in the luminous X-ray cluster RXJ1347-1145
E. Pointecouteau, M. Giard, A. Benoit +5
We have mapped the Sunyaev-Zel'dovich decrement (hereafter SZ) in the direction of the most luminous X-ray cluster known to date, RXJ1347-1145, at z=0.451. This has been achieved w…
Determination of the hot intracluster gas temperature from submillimeter measurements
E. Pointecouteau, M. Giard, D. Barret
Measurements of the Sunyaev-Zeldovich (hereafter SZ) distorsion of the cosmic microwave background can give interesting physical informations on clusters of galaxies, provided that…