The study of the Cosmic Microwave Background (CMB) is a rapidly maturing field. In remarkable advances in the past two years, experiments have begun to probe the detailed structure of the CMB angular spectrum thereby providing insight into the contents of the universe. We briefly review the BOOMERanG and DASI results with an emphasis on what the data tell us with only minimal cosmological assumptions. After a short discussion about a grand future for CMB physics, key features of the MAP satellite, now in orbit, are described. We also discuss how we anticipate MAP will advance the field beyond what we know now
International audienceThe Cosmic Microwave Background (CMB) is one of the pillars on which the Big B...
Over the past decades, precision measurements of the Cosmic Microwave Background (CMB) have led to r...
We measure the cosmic microwave background (CMB) power spectrum on angular scales l~30-200 from the ...
Observations of the Cosmic Microwave Background (CMB) are discussed, with particular emphasis on cur...
We review recent strides in understanding the universe through measurements of anisotropies in the c...
The first quarter of the 20th century witnessed a rebirth of cosmology, study of our Universe, as a ...
Experimental study of the anisotropy in the cosmic microwave background (CMB) is gathering momentum....
Almost 50 years of research on the Cosmic Microwave Background (CMB) have produced a revolution in o...
The Cosmic Microwave Background (CMB) consists of photons that were last created about 2 months afte...
The advent of high signal-to-noise cosmic microwave background (CMB) anisotropy experiments has allo...
AbstractObservations of the cosmic microwave background (CMB) anisotropies in temperature and polari...
International audienceThe 2.725 K cosmic microwave background has played a key role in the developme...
Observations of the cosmic microwave background represent a remarkable source of information for mod...
To appear in the proceedings of "Where Cosmology and Fundamental Physics Meet", 23-26 June, 2003, Ma...
The details of the CMB power spectrum are being revealed through the combined efforts of the world's...
International audienceThe Cosmic Microwave Background (CMB) is one of the pillars on which the Big B...
Over the past decades, precision measurements of the Cosmic Microwave Background (CMB) have led to r...
We measure the cosmic microwave background (CMB) power spectrum on angular scales l~30-200 from the ...
Observations of the Cosmic Microwave Background (CMB) are discussed, with particular emphasis on cur...
We review recent strides in understanding the universe through measurements of anisotropies in the c...
The first quarter of the 20th century witnessed a rebirth of cosmology, study of our Universe, as a ...
Experimental study of the anisotropy in the cosmic microwave background (CMB) is gathering momentum....
Almost 50 years of research on the Cosmic Microwave Background (CMB) have produced a revolution in o...
The Cosmic Microwave Background (CMB) consists of photons that were last created about 2 months afte...
The advent of high signal-to-noise cosmic microwave background (CMB) anisotropy experiments has allo...
AbstractObservations of the cosmic microwave background (CMB) anisotropies in temperature and polari...
International audienceThe 2.725 K cosmic microwave background has played a key role in the developme...
Observations of the cosmic microwave background represent a remarkable source of information for mod...
To appear in the proceedings of "Where Cosmology and Fundamental Physics Meet", 23-26 June, 2003, Ma...
The details of the CMB power spectrum are being revealed through the combined efforts of the world's...
International audienceThe Cosmic Microwave Background (CMB) is one of the pillars on which the Big B...
Over the past decades, precision measurements of the Cosmic Microwave Background (CMB) have led to r...
We measure the cosmic microwave background (CMB) power spectrum on angular scales l~30-200 from the ...