The cosmic microwave background anisotropy power spectrum measured by Archeops
6 pages, 4 figures, see also http://www.archeops.org 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...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2003
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Online Access: | https://hal.science/hal-00009160 https://hal.science/hal-00009160/document https://hal.science/hal-00009160/file/aaej161.pdf https://doi.org/10.1051/0004-6361:20021850 |
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Open Polar |
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Institut national des sciences de l'Univers: HAL-INSU |
op_collection_id |
ftinsu |
language |
English |
topic |
cosmic microwave background cosmology: observations submillimeter [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
spellingShingle |
cosmic microwave background cosmology: observations submillimeter [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Benoit, Alain Ade, P. 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. Desert, F. -X. Dore, O. Douspis, M. Dumoulin, L. Dupac, X. Filliatre, P. Fosalba, P. Ganga, K. Gannaway, F. Gautier, B. Giard, M. Giraud-Heraud, Y. Gispert, R. Guglielmi, L. Hamilton, J. -Ch. Hanany, S. Henrot-Versille, S. Kaplan, J. Lagache, Guilaine Lamarre, J. -M. Lange, A. E. Macias-Perez, 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. Puget, J. -L. Renault, C. Rosset, C. Santos, D. Starobinsky, A. Strukov, I. Sudiwala, R. V. Teyssier, R. Tristram, M. Tucker, C. Vanel, J. -C. Vibert, D. Wakui, E. Yvon, D. The cosmic microwave background anisotropy power spectrum measured by Archeops |
topic_facet |
cosmic microwave background cosmology: observations submillimeter [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
description |
6 pages, 4 figures, see also http://www.archeops.org 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 technology for the detectors and their cooling. Archeops is a balloon-borne instrument consisting of a 1.5 m aperture diameter telescope and an array of 21 photometers maintained at ~100 mK that are operating in 4 frequency bands centered at 143, 217, 353 and 545 GHz. The data were taken during the Arctic night of February 7, 2002 after the instrument was launched by CNES from Esrange base (Sweden). The entire data cover ~ 30% of the sky.This first analysis was obtained with a small subset of the dataset using the most sensitive photometer in each CMB band (143 and 217 GHz) and 12.6% of the sky at galactic latitudes above 30 degrees where the foreground contamination is measured to be negligible. The large sky coverage and medium resolution (better than 15 arcminutes) provide for the first time a high signal-to-noise ratio determination of the power spectrum over angular scales that include both the first acoustic peak and scales probed by COBE/DMR. With a binning of $\Delta \ell$=7 to 25 the error bars are dominated by sample variance for $\ell$ below 200. A companion paper details the cosmological implications. |
author2 |
Centre de Recherches sur les Très Basses Températures (CRTBT) Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS) Cardiff University Physique Corpusculaire et Cosmologie - Collège de France (PCC) Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de l'Accélérateur Linéaire (LAL) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA) Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Institut d'astrophysique spatiale (IAS) Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) California Institute of Technology (CALTECH) Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) Istituto di Ricerca sulle Onde Elettromagnetiche “Nello Carrara” (IROE) National Research Council of Italy Institut d'Astrophysique de Paris (IAP) Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Università degli Studi di Roma "La Sapienza" = Sapienza University Rome (UNIROMA) Laboratoire d'Astrophysique de Grenoble (LAOG) Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM) Centre d'étude spatiale des rayonnements (CESR) Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS) Infrared Processing and Analysis Center (IPAC) Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA) École normale supérieure - Paris (ENS-PSL) Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP) Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS) School of Physics and Astronomy Minneapolis University of Minnesota Twin Cities (UMN) University of Minnesota System-University of Minnesota System Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) National University of Ireland Maynooth (Maynooth University) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) L.D. Landau Institute for Theoretical Physics of RAS Russian Academy of Sciences Moscow (RAS) Space Research Institute of the Russian Academy of Sciences (IKI) |
format |
Article in Journal/Newspaper |
author |
Benoit, Alain Ade, P. 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. Desert, F. -X. Dore, O. Douspis, M. Dumoulin, L. Dupac, X. Filliatre, P. Fosalba, P. Ganga, K. Gannaway, F. Gautier, B. Giard, M. Giraud-Heraud, Y. Gispert, R. Guglielmi, L. Hamilton, J. -Ch. Hanany, S. Henrot-Versille, S. Kaplan, J. Lagache, Guilaine Lamarre, J. -M. Lange, A. E. Macias-Perez, 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. Puget, J. -L. Renault, C. Rosset, C. Santos, D. Starobinsky, A. Strukov, I. Sudiwala, R. V. Teyssier, R. Tristram, M. Tucker, C. Vanel, J. -C. Vibert, D. Wakui, E. Yvon, D. |
author_facet |
Benoit, Alain Ade, P. 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. Desert, F. -X. Dore, O. Douspis, M. Dumoulin, L. Dupac, X. Filliatre, P. Fosalba, P. Ganga, K. Gannaway, F. Gautier, B. Giard, M. Giraud-Heraud, Y. Gispert, R. Guglielmi, L. Hamilton, J. -Ch. Hanany, S. Henrot-Versille, S. Kaplan, J. Lagache, Guilaine Lamarre, J. -M. Lange, A. E. Macias-Perez, 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. Puget, J. -L. Renault, C. Rosset, C. Santos, D. Starobinsky, A. Strukov, I. Sudiwala, R. V. Teyssier, R. Tristram, M. Tucker, C. Vanel, J. -C. Vibert, D. Wakui, E. Yvon, D. |
author_sort |
Benoit, Alain |
title |
The cosmic microwave background anisotropy power spectrum measured by Archeops |
title_short |
The cosmic microwave background anisotropy power spectrum measured by Archeops |
title_full |
The cosmic microwave background anisotropy power spectrum measured by Archeops |
title_fullStr |
The cosmic microwave background anisotropy power spectrum measured by Archeops |
title_full_unstemmed |
The cosmic microwave background anisotropy power spectrum measured by Archeops |
title_sort |
cosmic microwave background anisotropy power spectrum measured by archeops |
publisher |
HAL CCSD |
publishDate |
2003 |
url |
https://hal.science/hal-00009160 https://hal.science/hal-00009160/document https://hal.science/hal-00009160/file/aaej161.pdf https://doi.org/10.1051/0004-6361:20021850 |
long_lat |
ENVELOPE(21.117,21.117,67.883,67.883) |
geographic |
Arctic Esrange |
geographic_facet |
Arctic Esrange |
genre |
Arctic |
genre_facet |
Arctic |
op_source |
ISSN: 0004-6361 EISSN: 1432-0756 Astronomy and Astrophysics - A&A https://hal.science/hal-00009160 Astronomy and Astrophysics - A&A, 2003, 399, pp.L19-L23. ⟨10.1051/0004-6361:20021850⟩ http://www.aanda.org |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/0210305 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20021850 hal-00009160 https://hal.science/hal-00009160 https://hal.science/hal-00009160/document https://hal.science/hal-00009160/file/aaej161.pdf ARXIV: astro-ph/0210305 doi:10.1051/0004-6361:20021850 |
op_rights |
info:eu-repo/semantics/OpenAccess |
op_doi |
https://doi.org/10.1051/0004-6361:20021850 |
_version_ |
1796305867484692480 |
spelling |
ftinsu:oai:HAL:hal-00009160v1 2024-04-14T08:08:26+00:00 The cosmic microwave background anisotropy power spectrum measured by Archeops Benoit, Alain Ade, P. 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. Desert, F. -X. Dore, O. Douspis, M. Dumoulin, L. Dupac, X. Filliatre, P. Fosalba, P. Ganga, K. Gannaway, F. Gautier, B. Giard, M. Giraud-Heraud, Y. Gispert, R. Guglielmi, L. Hamilton, J. -Ch. Hanany, S. Henrot-Versille, S. Kaplan, J. Lagache, Guilaine Lamarre, J. -M. Lange, A. E. Macias-Perez, 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. Puget, J. -L. Renault, C. Rosset, C. Santos, D. Starobinsky, A. Strukov, I. Sudiwala, R. V. Teyssier, R. Tristram, M. Tucker, C. Vanel, J. -C. Vibert, D. Wakui, E. Yvon, D. Centre de Recherches sur les Très Basses Températures (CRTBT) Université Joseph Fourier - Grenoble 1 (UJF)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS) Cardiff University Physique Corpusculaire et Cosmologie - Collège de France (PCC) Collège de France (CdF (institution))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Laboratoire de l'Accélérateur Linéaire (LAL) Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS) Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (DAPNIA) Commissariat à l'énergie atomique et aux énergies alternatives (CEA) Institut d'astrophysique spatiale (IAS) Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) California Institute of Technology (CALTECH) Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées (LATT) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) Jet Propulsion Laboratory (JPL) NASA-California Institute of Technology (CALTECH) Istituto di Ricerca sulle Onde Elettromagnetiche “Nello Carrara” (IROE) National Research Council of Italy Institut d'Astrophysique de Paris (IAP) Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Università degli Studi di Roma "La Sapienza" = Sapienza University Rome (UNIROMA) Laboratoire d'Astrophysique de Grenoble (LAOG) Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM) Centre d'étude spatiale des rayonnements (CESR) Laboratoire de Physique Subatomique et de Cosmologie (LPSC) Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut National Polytechnique de Grenoble (INPG)-Centre National de la Recherche Scientifique (CNRS) Infrared Processing and Analysis Center (IPAC) Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA) École normale supérieure - Paris (ENS-PSL) Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université de Cergy Pontoise (UCP) Université Paris-Seine-Université Paris-Seine-Centre National de la Recherche Scientifique (CNRS) School of Physics and Astronomy Minneapolis University of Minnesota Twin Cities (UMN) University of Minnesota System-University of Minnesota System Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES) National University of Ireland Maynooth (Maynooth University) Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) L.D. Landau Institute for Theoretical Physics of RAS Russian Academy of Sciences Moscow (RAS) Space Research Institute of the Russian Academy of Sciences (IKI) 2003 https://hal.science/hal-00009160 https://hal.science/hal-00009160/document https://hal.science/hal-00009160/file/aaej161.pdf https://doi.org/10.1051/0004-6361:20021850 en eng HAL CCSD EDP Sciences info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/0210305 info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361:20021850 hal-00009160 https://hal.science/hal-00009160 https://hal.science/hal-00009160/document https://hal.science/hal-00009160/file/aaej161.pdf ARXIV: astro-ph/0210305 doi:10.1051/0004-6361:20021850 info:eu-repo/semantics/OpenAccess ISSN: 0004-6361 EISSN: 1432-0756 Astronomy and Astrophysics - A&A https://hal.science/hal-00009160 Astronomy and Astrophysics - A&A, 2003, 399, pp.L19-L23. ⟨10.1051/0004-6361:20021850⟩ http://www.aanda.org cosmic microwave background cosmology: observations submillimeter [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/article Journal articles 2003 ftinsu https://doi.org/10.1051/0004-6361:20021850 2024-03-21T17:16:00Z 6 pages, 4 figures, see also http://www.archeops.org 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 technology for the detectors and their cooling. Archeops is a balloon-borne instrument consisting of a 1.5 m aperture diameter telescope and an array of 21 photometers maintained at ~100 mK that are operating in 4 frequency bands centered at 143, 217, 353 and 545 GHz. The data were taken during the Arctic night of February 7, 2002 after the instrument was launched by CNES from Esrange base (Sweden). The entire data cover ~ 30% of the sky.This first analysis was obtained with a small subset of the dataset using the most sensitive photometer in each CMB band (143 and 217 GHz) and 12.6% of the sky at galactic latitudes above 30 degrees where the foreground contamination is measured to be negligible. The large sky coverage and medium resolution (better than 15 arcminutes) provide for the first time a high signal-to-noise ratio determination of the power spectrum over angular scales that include both the first acoustic peak and scales probed by COBE/DMR. With a binning of $\Delta \ell$=7 to 25 the error bars are dominated by sample variance for $\ell$ below 200. A companion paper details the cosmological implications. Article in Journal/Newspaper Arctic Institut national des sciences de l'Univers: HAL-INSU Arctic Esrange ENVELOPE(21.117,21.117,67.883,67.883) |