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Archeops in-flight performance, data processing, and map making

Authors :
Macías-Pérez, J. F.
Lagache, G.
Maffei, B.
Ganga, K.
Bourrachot, A.
Ade, P.
Amblard, A.
Ansari, R.
Aubourg, E.
Aumont, J.
Bargot, S.
Bartlett, J.
Benoît, A.
Bernard, J.-Ph.
Bhatia, R.
Blanchard, A.
Bock, J. J.
Boscaleri, A.
Bouchet, F. R.
Camus, P.
Cardoso, J.-F.
Couchot, F.
de Bernardis, P.
Delabrouille, J.
Désert, F.-X.
Doré, O.
Douspis, M.
Dumoulin, L.
Dupac, X.
Filliatre, Ph.
Fosalba, P.
Gannaway, F.
Gautier, B.
Giard, M.
Giraud-Héraud, Y.
Gispert, R.
Guglielmi, L.
Hamilton, J.-Ch.
Hanany, S.
Henrot-Versillé, S.
Hristov, V.
Kaplan, J.
Lamarre, J.-M.
Lange, A. E.
Madet, K.
Magneville, Ch.
Marrone, D. P.
Masi, S.
Mayet, F.
Murphy, J. A.
Naraghi, F.
Nati, F.
Patanchon, G.
Perdereau, O.
Perrin, G.
Plaszczynski, S.
Piat, M.
Ponthieu, N.
Prunet, S.
Puget, J.-L.
Renault, C.
Rosset, C.
Santos, D.
Starobinsky, A.
Strukov, I.
Sudiwala, R. V.
Teyssier, R.
Tristram, M.
Tucker, C.
Vanel, J.-Ch.
Vibert, D.
Wakui, E.
Yvon, D.
Macías-Pérez, J. F.
Lagache, G.
Maffei, B.
Ganga, K.
Bourrachot, A.
Ade, P.
Amblard, A.
Ansari, R.
Aubourg, E.
Aumont, J.
Bargot, S.
Bartlett, J.
Benoît, A.
Bernard, J.-Ph.
Bhatia, R.
Blanchard, A.
Bock, J. J.
Boscaleri, A.
Bouchet, F. R.
Camus, P.
Cardoso, J.-F.
Couchot, F.
de Bernardis, P.
Delabrouille, J.
Désert, F.-X.
Doré, O.
Douspis, M.
Dumoulin, L.
Dupac, X.
Filliatre, Ph.
Fosalba, P.
Gannaway, F.
Gautier, B.
Giard, M.
Giraud-Héraud, Y.
Gispert, R.
Guglielmi, L.
Hamilton, J.-Ch.
Hanany, S.
Henrot-Versillé, S.
Hristov, V.
Kaplan, J.
Lamarre, J.-M.
Lange, A. E.
Madet, K.
Magneville, Ch.
Marrone, D. P.
Masi, S.
Mayet, F.
Murphy, J. A.
Naraghi, F.
Nati, F.
Patanchon, G.
Perdereau, O.
Perrin, G.
Plaszczynski, S.
Piat, M.
Ponthieu, N.
Prunet, S.
Puget, J.-L.
Renault, C.
Rosset, C.
Santos, D.
Starobinsky, A.
Strukov, I.
Sudiwala, R. V.
Teyssier, R.
Tristram, M.
Tucker, C.
Vanel, J.-Ch.
Vibert, D.
Wakui, E.
Yvon, D.
Source :
Astronomy and Astrophysics; June 2007, Vol. 467 Issue: 3 p1313-1344, 32p
Publication Year :
2007

Abstract

Aims.Archeops is a balloon-borne experiment inspired by the Planck satellite and its high frequency instrument (HFI). It is designed to measure the cosmic microwave background (CMB) temperature anisotropies at high angular resolution (~12 arcmin) over a large fraction of the sky (around 30%) at 143, 217, 353, and 545 GHz. The Archeops 353 GHz channel consists of three pairs of polarized sensitive bolometers designed to detect the polarized diffuse emission of Galactic dust.

Details

Language :
English
ISSN :
00046361 and 14320746
Volume :
467
Issue :
3
Database :
Supplemental Index
Journal :
Astronomy and Astrophysics
Publication Type :
Periodical
Accession number :
ejs53169633
Full Text :
https://doi.org/10.1051/0004-6361:20065258
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