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Archeops: A High Resolution, Large Sky Coverage Balloon Experiment for Mapping CMB Anisotropies
A. Benoit, P. Ade, A. Amblard +3
Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (8 arcminutes) over a large frac…
How accurately can the SZ effect measure peculiar cluster velocities and bulk flows?
N. Aghanim, K. M. Górski, J. -L. Puget
The Sunyaev-Zel'dovich effect is a powerful tool for cosmology that can be used to measure the radial peculiar velocities of galaxy clusters, and thus to test, and constrain, theor…
FIRBACK: III. Catalog, Source counts, and cosmological implications of the 170 micron ISO Deep survey
Herve Dole, Richard Gispert, Guilaine Lagache +17
The FIRBACK (Far Infrared BACKground) survey is one of the deepest imaging surveys carried out at 170 microns with ISOPHOT onboard ISO, and is aimed at the study of the structure o…
ISOCAM observations of the rho Ophiuchi cloud: Luminosity and mass functions of the pre-main sequence embedded cluster
S. Bontemps, P. Andre, A. A. Kaas +19
We present the results of the first extensive mid-infrared (IR) imaging survey of the rho Ophiuchi embedded cluster, performed with the ISOCAM camera on board the ISO satellite. Th…
Far-Infrared Source Counts and the Diffuse Infrared Background
Jean-Loup Puget, Guilaine Lagache
The cosmic far-infrared background is now well measured from 140 micron to 1 mm. Uncertainties remain at 100 micron (and even more at 60 micron). These are dominated by limitations…