Cosmological constraints from archeops

A. Benoît; P. Ade; A. Amblard; R. Ansari; E. Aubourg; S. Bargot; J. G. Bartlett; J. Ph 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; P. Fosalba; K. Ganga; F. Gannaway; B. Gautier; M. Giard; Y. Giraud-Héraud; R. Gispert; L. Guglielmi; J. Ch Hamilton; S. Hanany; S. Henrot-Versillé; J. Kaplan; G. Lagache; J. M. Lamarre; A. E. Lange; J. F. Macías-Pérez; K. Madet; B. Maffei; Ch Magneville; D. P. Marrone; S. Masi; F. Mayet; A. Murphy; F. Naraghi; F. Nati; G. Patanchon; G. Perrin; M. Piat; N. Ponthieu; S. Prunet; J. L. Puget; C. Renault; C. Rosset; D. Santos; A. Starobinsky; I. Strukov; R. V. Sudiwala; R. Teyssier; M. Tristram; C. Tucker; J. C. Vanel; D. Vibert; E. Wakui; D. Yvon

doi:10.1051/0004-6361:20021722

Cosmological constraints from archeops

A. Benoît
, P. Ade
, A. Amblard
, R. Ansari
, E. Aubourg
, S. Bargot
, J. G. Bartlett
, J. Ph 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, P. Fosalba, K. Ganga, F. Gannaway, B. Gautier, M. Giard, Y. Giraud-Héraud, R. Gispert, L. Guglielmi, J. Ch Hamilton, S. Hanany, S. Henrot-Versillé, J. Kaplan, G. Lagache, J. M. Lamarre, A. E. Lange, J. F. Macías-Pérez, K. Madet, B. Maffei, Ch Magneville, D. P. Marrone, S. Masi, F. Mayet, A. Murphy, F. Naraghi, F. Nati, G. Patanchon, G. Perrin, M. Piat, N. Ponthieu, S. Prunet, J. L. Puget, C. Renault, C. Rosset, D. Santos, A. Starobinsky, I. Strukov, R. V. Sudiwala, R. Teyssier, M. Tristram, C. Tucker, J. C. Vanel, D. Vibert, E. Wakui, D. Yvon

Institut NÉEL
Physics Department
Cardiff University
Physique Corpusculaire et Cosmologie
Collège de France
Federation de Recherche APC
Laboratoire de Probabilités et Modèles Aléatoires
Laboratoire de l'Accélérateur Linéaire
Institut Pierre Simon Laplace, CNRS and CEA
Institut d'Astrophysique Spatiale
IRAP/CNRS
California Institute of Technology
Science Division
Ev-K2-CNR Committee
Institut d’Astrophysique de Paris
Gruppo di Cosmologia Sperimentale
Dipartimento di Fisica
Université Grenoble Alpes
University of Oxford
Université Paris-Sud
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
California Institute of Technology
University of Minnesota
Sorbonne Univ.
Department of Experimental Physics
Maynooth University
Landau Institute for Theoretical Physics, Russian Academy of Sciences
Space Research Institute (IKI)
Université Paris-Diderot

Résultats de recherche: Contribution à un journal › Lettre › Revue par des pairs

203 Citations (Scopus)

Résumé

We analyze the cosmological constraints that Archeops (Benoît et al. 2003) places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in ℓ and large ℓ coverage down to COBE scales, Archeops provides a precise determination of the first acoustic peak in terms of position at multipole l_peak = 220 ± 6, height and width. An analysis of Archeops data in combination with other CMB datasets constraints the baryon content of the Universe, Ω_bh² = 0.022_-0.004^+0.003, compatible with Big-Bang nucleosynthesis and with a similar accuracy. Using cosmological priors obtained from recent non-CMB data leads to yet tighter constraints on the total density, e.g. Ω_tot = 1.00_-0.02^+0.03 using the HST determination of the Hubble constant. An excellent absolute calibration consistency is found between Archeops and other CMB experiments, as well as with the previously quoted best fit model. The spectral index n is measured to be 1.04_-0.12^+0.10 when the optical depth to reionization, τ, is allowed to vary as a free parameter, and 0.96_-0.04^+0.03 when τ is fixed to zero, both in good agreement with inflation.

langue originale	Anglais
Pages (de - à)	L25-L30
journal	Astronomy and Astrophysics
Volume	399
Numéro de publication	3
Les DOIs	https://doi.org/10.1051/0004-6361:20021722
état	Publié - 1 janv. 2003
Modification externe	Oui

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10.1051/0004-6361:20021722

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Benoît, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., Bartlett, J. G., 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., ... Yvon, D. (2003). Cosmological constraints from archeops. Astronomy and Astrophysics, 399(3), L25-L30. https://doi.org/10.1051/0004-6361:20021722

@article{59ba280ced2c4a939e43eed3835e1a7e,

title = "Cosmological constraints from archeops",

abstract = "We analyze the cosmological constraints that Archeops (Beno{\^i}t et al. 2003) places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in ℓ and large ℓ coverage down to COBE scales, Archeops provides a precise determination of the first acoustic peak in terms of position at multipole lpeak = 220 ± 6, height and width. An analysis of Archeops data in combination with other CMB datasets constraints the baryon content of the Universe, Ωbh2 = 0.022-0.004+0.003, compatible with Big-Bang nucleosynthesis and with a similar accuracy. Using cosmological priors obtained from recent non-CMB data leads to yet tighter constraints on the total density, e.g. Ωtot = 1.00-0.02+0.03 using the HST determination of the Hubble constant. An excellent absolute calibration consistency is found between Archeops and other CMB experiments, as well as with the previously quoted best fit model. The spectral index n is measured to be 1.04-0.12+0.10 when the optical depth to reionization, τ, is allowed to vary as a free parameter, and 0.96-0.04+0.03 when τ is fixed to zero, both in good agreement with inflation.",

keywords = "Cosmic microwave background, Cosmological parameters, Early Universe, Large-scale structure of the Universe",

author = "A. Beno{\^i}t and P. Ade and A. Amblard and R. Ansari and E. Aubourg and S. Bargot and Bartlett, \{J. G.\} and Bernard, \{J. Ph\} 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 P. Fosalba 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. Ch\} and S. Hanany and S. Henrot-Versill{\'e} and J. Kaplan and G. Lagache and Lamarre, \{J. M.\} and Lange, \{A. E.\} and Mac{\'i}as-P{\'e}rez, \{J. F.\} and K. Madet and B. Maffei and Ch Magneville and Marrone, \{D. P.\} and S. Masi and F. Mayet and A. Murphy and F. Naraghi and F. Nati and G. Patanchon and G. Perrin and M. Piat and N. Ponthieu and S. Prunet and Puget, \{J. L.\} and C. Renault and C. Rosset and D. Santos and A. Starobinsky and I. Strukov and Sudiwala, \{R. V.\} and R. Teyssier and M. Tristram and C. Tucker and Vanel, \{J. C.\} and D. Vibert and E. Wakui and D. Yvon",

year = "2003",

month = jan,

day = "1",

doi = "10.1051/0004-6361:20021722",

language = "English",

volume = "399",

pages = "L25--L30",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "3",

}

Benoît, A, Ade, P, Amblard, A, Ansari, R, Aubourg, E, Bargot, S, Bartlett, JG, 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, Fosalba, P, Ganga, K, Gannaway, F, Gautier, B, Giard, M, Giraud-Héraud, Y, Gispert, R, Guglielmi, L, Hamilton, JC, Hanany, S, Henrot-Versillé, S, Kaplan, J, Lagache, G, Lamarre, JM, Lange, AE, Macías-Pérez, JF, Madet, K, Maffei, B, Magneville, C, Marrone, DP, Masi, S, Mayet, F, Murphy, A, Naraghi, F, Nati, F, Patanchon, G, Perrin, G, Piat, M, Ponthieu, N, Prunet, S, Puget, JL, Renault, C, Rosset, C, Santos, D, Starobinsky, A, Strukov, I, Sudiwala, RV, Teyssier, R, Tristram, M, Tucker, C, Vanel, JC, Vibert, D, Wakui, E & Yvon, D 2003, 'Cosmological constraints from archeops', Astronomy and Astrophysics, VOL. 399, Numéro 3, p. L25-L30. https://doi.org/10.1051/0004-6361:20021722

TY - JOUR

T1 - Cosmological constraints from archeops

AU - Benoît, A.

AU - Ade, P.

AU - Amblard, A.

AU - Ansari, R.

AU - Aubourg, E.

AU - Bargot, S.

AU - Bartlett, J. G.

AU - Bernard, J. Ph

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 - Fosalba, 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. Ch

AU - Hanany, S.

AU - Henrot-Versillé, S.

AU - Kaplan, J.

AU - Lagache, G.

AU - Lamarre, J. M.

AU - Lange, A. E.

AU - Macías-Pérez, J. F.

AU - Madet, K.

AU - Maffei, B.

AU - Magneville, Ch

AU - Marrone, D. P.

AU - Masi, S.

AU - Mayet, F.

AU - Murphy, A.

AU - Naraghi, F.

AU - Nati, F.

AU - Patanchon, G.

AU - Perrin, G.

AU - Piat, M.

AU - Ponthieu, N.

AU - Prunet, S.

AU - Puget, J. L.

AU - Renault, C.

AU - Rosset, C.

AU - Santos, D.

AU - Starobinsky, A.

AU - Strukov, I.

AU - Sudiwala, R. V.

AU - Teyssier, R.

AU - Tristram, M.

AU - Tucker, C.

AU - Vanel, J. C.

AU - Vibert, D.

AU - Wakui, E.

AU - Yvon, D.

PY - 2003/1/1

Y1 - 2003/1/1

N2 - We analyze the cosmological constraints that Archeops (Benoît et al. 2003) places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in ℓ and large ℓ coverage down to COBE scales, Archeops provides a precise determination of the first acoustic peak in terms of position at multipole lpeak = 220 ± 6, height and width. An analysis of Archeops data in combination with other CMB datasets constraints the baryon content of the Universe, Ωbh2 = 0.022-0.004+0.003, compatible with Big-Bang nucleosynthesis and with a similar accuracy. Using cosmological priors obtained from recent non-CMB data leads to yet tighter constraints on the total density, e.g. Ωtot = 1.00-0.02+0.03 using the HST determination of the Hubble constant. An excellent absolute calibration consistency is found between Archeops and other CMB experiments, as well as with the previously quoted best fit model. The spectral index n is measured to be 1.04-0.12+0.10 when the optical depth to reionization, τ, is allowed to vary as a free parameter, and 0.96-0.04+0.03 when τ is fixed to zero, both in good agreement with inflation.

AB - We analyze the cosmological constraints that Archeops (Benoît et al. 2003) places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in ℓ and large ℓ coverage down to COBE scales, Archeops provides a precise determination of the first acoustic peak in terms of position at multipole lpeak = 220 ± 6, height and width. An analysis of Archeops data in combination with other CMB datasets constraints the baryon content of the Universe, Ωbh2 = 0.022-0.004+0.003, compatible with Big-Bang nucleosynthesis and with a similar accuracy. Using cosmological priors obtained from recent non-CMB data leads to yet tighter constraints on the total density, e.g. Ωtot = 1.00-0.02+0.03 using the HST determination of the Hubble constant. An excellent absolute calibration consistency is found between Archeops and other CMB experiments, as well as with the previously quoted best fit model. The spectral index n is measured to be 1.04-0.12+0.10 when the optical depth to reionization, τ, is allowed to vary as a free parameter, and 0.96-0.04+0.03 when τ is fixed to zero, both in good agreement with inflation.

KW - Cosmic microwave background

KW - Cosmological parameters

KW - Early Universe

KW - Large-scale structure of the Universe

UR - https://www.scopus.com/pages/publications/0037337397

U2 - 10.1051/0004-6361:20021722

DO - 10.1051/0004-6361:20021722

M3 - Letter

AN - SCOPUS:0037337397

SN - 0004-6361

VL - 399

SP - L25-L30

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 3

ER -

Cosmological constraints from archeops

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