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

A. Benot; P. Ade; A. Amblard; R. Ansari; E. Aubourg; J. Bartlett; J. P. Bernard; R. S. Bhatia; A. Blanchard; J. J. Bock; A. Boscaleri; F. R. Bouchet; A. Bourrachot; P. Camus; F. Couchot; P. De Bernardis; J. Delabrouille; F. X. Désert; O. Doré; M. Douspis; L. Dumoulin; X. Dupac; P. Filliatre; K. Ganga; F. Gannaway; B. Gautier; M. Giard; Y. Giraud-Héraud; R. Gispert; L. Guglielmi; J. C. Hamilton; S. Hanany; S. Henrot-Versillé; V. V. Hristov; J. Kaplan; G. Lagache; J. M. Lamarre; A. E. Lange; K. Madet; B. Maffei; D. Marrone; S. Masi; J. A. Murphy; F. Naraghi; F. Nati; G. Perrin; M. Piat; J. L. Puget; D. Santos; R. V. Sudiwala; J. C. Vanel; D. Vibert; E. Wakui; D. Yvon

doi:10.1016/S0927-6505(01)00141-4

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

A. Benot, P. Ade, A. Amblard, R. Ansari, E. Aubourg, J. Bartlett, J. P. Bernard, R. S. Bhatia, A. Blanchard, J. J. Bock, A. Boscaleri, F. R. Bouchet, A. Bourrachot, P. Camus, F. Couchot, P. De Bernardis, J. Delabrouille, F. X. Désert, O. Doré, M. DouspisL. Dumoulin, X. Dupac, P. Filliatre, K. Ganga, F. Gannaway, B. Gautier, M. Giard, Y. Giraud-Héraud, R. Gispert, L. Guglielmi, J. C. Hamilton, S. Hanany, S. Henrot-Versillé, V. V. Hristov, J. Kaplan, G. Lagache, J. M. Lamarre, A. E. Lange, K. Madet, B. Maffei, D. Marrone, S. Masi, J. A. Murphy, F. Naraghi, F. Nati, G. Perrin, M. Piat, J. L. Puget, D. Santos, R. V. Sudiwala, J. C. Vanel, D. Vibert, E. Wakui, D. Yvon

Physics and Astronomy (Twin Cities)

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Abstract

Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (∼8′) over a large fraction (∼25%) of the sky in the millimetre domain. Based on Planck high frequency instrument technology, cooled bolometers (0.1 K) scan the sky in total power mode with large circles at constant elevation. During the course of a 24-h Arctic-night balloon flight, Archeops will observe a complete annulus on the sky in four frequency bands centered at 143, 217, 353 and 545 GHz with an expected sensitivity to CMB fluctuations of ∼100 μK for each of the 90 thousand 20′ average pixels. We describe the instrument and its performance obtained during a test flight from Trapani (Sicily) to Spain in July 1999.

Original language	English (US)
Pages (from-to)	101-124
Number of pages	24
Journal	Astroparticle Physics
Volume	17
Issue number	2
DOIs	https://doi.org/10.1016/S0927-6505(01)00141-4
State	Published - 2002

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Benot, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bartlett, J., Bernard, J. P., Bhatia, R. S., Blanchard, A., Bock, J. J., Boscaleri, A., Bouchet, F. R., Bourrachot, A., Camus, P., Couchot, F., De Bernardis, P., Delabrouille, J., Désert, F. X., Doré, O., ... Yvon, D. (2002). Archeops: A high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies. Astroparticle Physics, 17(2), 101-124. https://doi.org/10.1016/S0927-6505(01)00141-4

Benot, A, Ade, P, Amblard, A, Ansari, R, Aubourg, E, Bartlett, J, Bernard, JP, Bhatia, RS, Blanchard, A, Bock, JJ, Boscaleri, A, Bouchet, FR, Bourrachot, A, Camus, P, Couchot, F, De Bernardis, P, Delabrouille, J, Désert, FX, Doré, O, Douspis, M, Dumoulin, L, Dupac, X, Filliatre, P, Ganga, K, Gannaway, F, Gautier, B, Giard, M, Giraud-Héraud, Y, Gispert, R, Guglielmi, L, Hamilton, JC, Hanany, S, Henrot-Versillé, S, Hristov, VV, Kaplan, J, Lagache, G, Lamarre, JM, Lange, AE, Madet, K, Maffei, B, Marrone, D, Masi, S, Murphy, JA, Naraghi, F, Nati, F, Perrin, G, Piat, M, Puget, JL, Santos, D, Sudiwala, RV, Vanel, JC, Vibert, D, Wakui, E & Yvon, D 2002, 'Archeops: A high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies', Astroparticle Physics, vol. 17, no. 2, pp. 101-124. https://doi.org/10.1016/S0927-6505(01)00141-4

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title = "Archeops: A high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies",

abstract = "Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (∼8′) over a large fraction (∼25%) of the sky in the millimetre domain. Based on Planck high frequency instrument technology, cooled bolometers (0.1 K) scan the sky in total power mode with large circles at constant elevation. During the course of a 24-h Arctic-night balloon flight, Archeops will observe a complete annulus on the sky in four frequency bands centered at 143, 217, 353 and 545 GHz with an expected sensitivity to CMB fluctuations of ∼100 μK for each of the 90 thousand 20′ average pixels. We describe the instrument and its performance obtained during a test flight from Trapani (Sicily) to Spain in July 1999.",

author = "A. Benot and P. Ade and A. Amblard and R. Ansari and E. Aubourg and J. Bartlett and Bernard, {J. P.} and Bhatia, {R. S.} and A. Blanchard and Bock, {J. J.} and A. Boscaleri and Bouchet, {F. R.} and A. Bourrachot and P. Camus and F. Couchot and {De Bernardis}, P. and J. Delabrouille and D{\'e}sert, {F. X.} and O. Dor{\'e} and M. Douspis and L. Dumoulin and X. Dupac and P. Filliatre and K. Ganga and F. Gannaway and B. Gautier and M. Giard and Y. Giraud-H{\'e}raud and R. Gispert and L. Guglielmi and Hamilton, {J. C.} and S. Hanany and S. Henrot-Versill{\'e} and Hristov, {V. V.} and J. Kaplan and G. Lagache and Lamarre, {J. M.} and Lange, {A. E.} and K. Madet and B. Maffei and D. Marrone and S. Masi and Murphy, {J. A.} and F. Naraghi and F. Nati and G. Perrin and M. Piat and Puget, {J. L.} and D. Santos and Sudiwala, {R. V.} and Vanel, {J. C.} and D. Vibert and E. Wakui and D. Yvon",

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doi = "10.1016/S0927-6505(01)00141-4",

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TY - JOUR

T1 - Archeops

T2 - A high resolution, large sky coverage balloon experiment for mapping cosmic microwave background anisotropies

AU - Benot, A.

AU - Ade, P.

AU - Amblard, A.

AU - Ansari, R.

AU - Aubourg, E.

AU - Bartlett, J.

AU - Bernard, J. P.

AU - Bhatia, R. S.

AU - Blanchard, A.

AU - Bock, J. J.

AU - Boscaleri, A.

AU - Bouchet, F. R.

AU - Bourrachot, A.

AU - Camus, P.

AU - Couchot, F.

AU - De Bernardis, P.

AU - Delabrouille, J.

AU - Désert, F. X.

AU - Doré, O.

AU - Douspis, M.

AU - Dumoulin, L.

AU - Dupac, X.

AU - Filliatre, P.

AU - Ganga, K.

AU - Gannaway, F.

AU - Gautier, B.

AU - Giard, M.

AU - Giraud-Héraud, Y.

AU - Gispert, R.

AU - Guglielmi, L.

AU - Hamilton, J. C.

AU - Hanany, S.

AU - Henrot-Versillé, S.

AU - Hristov, V. V.

AU - Kaplan, J.

AU - Lagache, G.

AU - Lamarre, J. M.

AU - Lange, A. E.

AU - Madet, K.

AU - Maffei, B.

AU - Marrone, D.

AU - Masi, S.

AU - Murphy, J. A.

AU - Naraghi, F.

AU - Nati, F.

AU - Perrin, G.

AU - Piat, M.

AU - Puget, J. L.

AU - Santos, D.

AU - Sudiwala, R. V.

AU - Vanel, J. C.

AU - Vibert, D.

AU - Wakui, E.

AU - Yvon, D.

PY - 2002

Y1 - 2002

N2 - Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (∼8′) over a large fraction (∼25%) of the sky in the millimetre domain. Based on Planck high frequency instrument technology, cooled bolometers (0.1 K) scan the sky in total power mode with large circles at constant elevation. During the course of a 24-h Arctic-night balloon flight, Archeops will observe a complete annulus on the sky in four frequency bands centered at 143, 217, 353 and 545 GHz with an expected sensitivity to CMB fluctuations of ∼100 μK for each of the 90 thousand 20′ average pixels. We describe the instrument and its performance obtained during a test flight from Trapani (Sicily) to Spain in July 1999.

AB - Archeops is a balloon-borne instrument dedicated to measuring cosmic microwave background (CMB) temperature anisotropies at high angular resolution (∼8′) over a large fraction (∼25%) of the sky in the millimetre domain. Based on Planck high frequency instrument technology, cooled bolometers (0.1 K) scan the sky in total power mode with large circles at constant elevation. During the course of a 24-h Arctic-night balloon flight, Archeops will observe a complete annulus on the sky in four frequency bands centered at 143, 217, 353 and 545 GHz with an expected sensitivity to CMB fluctuations of ∼100 μK for each of the 90 thousand 20′ average pixels. We describe the instrument and its performance obtained during a test flight from Trapani (Sicily) to Spain in July 1999.

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U2 - 10.1016/S0927-6505(01)00141-4

DO - 10.1016/S0927-6505(01)00141-4

M3 - Article

AN - SCOPUS:0036228502

SN - 0927-6505

VL - 17

SP - 101

EP - 124

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 2

ER -

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

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