The cosmic microwave background anisotropy power spectrum measured by Archeops

Author:

Benoît A.,Ade P.,Amblard A.,Ansari R.,Aubourg É.,Bargot S.,Bartlett J. G.,J.–Ph. Bernard ,Bhatia R. S.,Blanchard A.,Bock J. J.,Boscaleri A.,Bouchet F. R.,Bourrachot A.,Camus P.,Couchot F.,de Bernardis P.,Delabrouille J.,F.–X. Désert ,Doré O.,Douspis M.,Dumoulin L.,Dupac X.,Filliatre P.,Fosalba P.,Ganga K.,Gannaway F.,Gautier B.,Giard M.,Giraud–Héraud Y.,Gispert R.,Guglielmi L.,J.–Ch. Hamilton ,Hanany S.,Henrot–Versillé S.,Kaplan J.,Lagache G.,J.–M. Lamarre ,Lange A. E.,Macías–Pérez J. F.,Madet K.,Maffei B.,Magneville Ch.,Marrone D. P.,Masi S.,Mayet F.,Murphy A.,Naraghi F.,Nati F.,Patanchon G.,Perrin G.,Piat M.,Ponthieu N.,Prunet S.,J.–L. Puget ,Renault C.,Rosset C.,Santos D.,Starobinsky A.,Strukov I.,Sudiwala R. V.,Teyssier R.,Tristram M.,Tucker C.,J.–C. Vanel ,Vibert D.,Wakui E.,Yvon D.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference29 articles.

1. Archeops: a high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies

2. Cosmological constraints from Archeops

3. Benoît, A., Ade, P., Amblard, A., et al. 2003b, in preparation

4. Benoît, A., Ade, P., Amblard, A., et al. 2003c, in preparation

5. Benoît, A., Ade, P., Amblard, A., et al. 2003d, in preparation

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