Archeops: Difference between revisions

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== Results ==
[[Image:Archeops last flight map.jpg|thumb|300px|right|Archeops CMB map]]
Archeops has linked, for the first time and before [[WMAP]], the large angular scales (previously measured by [[Cosmic Background Explorer|COBE]]) to the first acoustic peak region.<ref>{{cite journal | first=A. | last=Benoit | coauthors=et al. | year=2003 | title=The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops | journal=A&A | volume=399 | pages=L19 | arxiv=astro-ph/0210305 |bibcode = 2003A&A...399L..19B |doi = 10.1051/0004-6361:20021850 }}</ref><ref>{{cite journal | first=M. | last=Tristram | coauthors=et al. | year=2005 | title=The CMB temperature power spectrum from an improved analysis of the Archeops data | journal=A&A | volume=436 | pages=785 | arxiv=astro-ph/0411633 |bibcode = 2005A&A...436..785T |doi = 10.1051/0004-6361:20042416 }}</ref>
 
From its results, inflation motivated cosmologies have been reinforced with a flat Universe (total energy density Ω<sub>tot</sub> = 1 within 3 %).