The cosmic microwave background anisotropy power spectrum measured by Archeops

• Main Authors: Benoit, A., Ade, Peter A. R., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., Bartlett, J. G., Bernard, J. -Ph., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., de Bernardis, P., Delabrouille, J., D?sert, F. -X., Dor?, O., Douspis, M., Dumoulin, L., Dupac, X., Filliatre, P., Fosalba, P., Ganga, K., Gannaway, Frederick Charles, Gautier, B., Giard, M., Giraud-Heraud, Y., Gispert, R., Guglielmi, L., Hamilton, J. -Ch., Hanany, S., Henrot-Versille, S., Kaplan, J., Lagache, G., Lamarre, J. -M., Lange, A. E., Macias-Perez, J. F., Madet, K., Maffei, Bruno, Magneville, Ch., Marrone, D. P., Masi, S., Mayet, F., Murphy, A., Naraghi, F., Nati, F., Patanchon, G.
• Format: Article in Journal/Newspaper
• Language: unknown
• Published: EDP Sciences 2003
• Subjects: QB Astronomy; Arctic; Esrange
• Online Access: https://orca.cardiff.ac.uk/id/eprint/43001/; https://doi.org/10.1051/0004-6361:20021850

We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range $\ell=15{-}350$. Archeops was conceived as a precursor of the Planck HFI instrument by using the same optical design and the same tech...