Planck pre-launch status: The Planck mission

被引：279

作者：

Tauber, J. A. ^{[1
]}

Mandolesi, N. ^{[44
]}

Puget, J. -L. ^{[52
]}

Banos, T. ^{[82
]}

Bersanelli, M. ^{[32
]}

Bouchet, F. R. ^{[50
,51
]}

Butler, R. C. ^{[44
]}

Charra, J. ^{[52
]}

Crone, G. ^{[36
]}

Dodsworth, J. ^{[37
]}

Efstathiou, G. ^{[90
]}

Gispert, R. ^{[52
]}

Guyot, G. ^{[52
]}

Gregorio, A. ^{[93
]}

Juillet, J. J. ^{[82
]}

Lamarre, J. -M. ^{[66
]}

Laureijs, R. J. ^{[1
]}

Lawrence, C. R. ^{[61
]}

Norgaard-Nielsen, H. U. ^{[35
]}

Passvogel, T. ^{[36
]}

Reix, J. M. ^{[82
]}

Texier, D. ^{[38
]}

Vibert, L. ^{[52
]}

Zacchei, A. ^{[45
]}

Ade, P. A. R. ^{[7
]}

Aghanim, N. ^{[52
]}

Aja, B. ^{[18
]}

Alippi, E. ^{[84
]}

Aloy, L. ^{[36
]}

Armand, P. ^{[82
]}

Arnaud, M. ^{[8
]}

Arondel, A. ^{[52
]}

Arreola-Villanueva, A. ^{[61
]}

Artal, E. ^{[18
]}

Artina, E. ^{[84
]}

Arts, A. ^{[36
]}

Ashdown, M. ^{[89
]}

Aumont, J. ^{[10
]}

Azzaro, M. ^{[39
]}

Bacchetta, A. ^{[83
]}

Baccigalupi, C. ^{[6
]}

Baker, M. ^{[36
]}

Balasini, M. ^{[84
]}

Balbi, A. ^{[33
]}

Banday, A. J. ^{[13
,67
]}

Barbier, G. ^{[64
]}

Barreiro, R. B. ^{[58
]}

Bartelmann, M. ^{[67
,95
]}

Battaglia, P. ^{[84
]}

Battaner, E. ^{[91
]}

机构：

[1] ESTEC, European Space Agcy, Div Astrophys, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands

[2] ESRIN, Agenzia Spaziale Italiana, Sci Data Ctr, Frascati, Italy

[3] Agenzia Spaziale Italiana, Rome, Italy

[4] Astrium GmbH, Friedrichshafen, Germany

[5] Univ Denis Diderot Paris 7, CNRS, UMR7164, Paris, France

[6] SISSA ISAS, Astrophys Sect, Trieste, Italy

[7] Cardiff Univ, Dept Phys & Astron, Cardiff, Wales

[8] IrfU SAp, CEA Saclay, Gif Sur Yvette, France

[9] IrfU SPP, CEA Saclay, Gif Sur Yvette, France

[10] Ctr Etud Spatiale Rayonnements, UMR 5187, Toulouse, France

[11] Univ Oslo, Ctr Math Applicat, Oslo, Norway

[12] Ctr Spatial Liege, Angleur, Belgium

[13] CNRS Univ Toulouse, CESR, Toulouse, France

[14] Univ Toronto, CITA, Toronto, ON, Canada

[15] Ctr Spatial Toulouse, CNES, Toulouse, France

[16] CNR ISTI, Area Ric, Pisa, Italy

[17] Univ Oviedo, Dept Fis, E-33007 Oviedo, Spain

[18] Univ Cantabria, Dept Ingn Comunicac, E-39005 Santander, Spain

[19] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V5Z 1M9, Canada

[20] Univ So Calif, Dept Phys & Astron, Los Angeles, CA USA

[21] Univ Helsinki, Dept Phys, Helsinki, Finland

[22] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[23] Purdue Univ, Dept Phys, W Lafayette, IN 47907 USA

[24] Standford Univ, Dept Phys, Stanford, CA USA

[25] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[26] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

[27] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[28] Univ Illinois, Dept Phys, Urbana, IL 61801 USA

[29] Univ Oxford, Dept Phys, Oxford, England

[30] Univ Calif Berkeley, Dept Phys & Astron, Berkeley, CA 94720 USA

[31] Univ Padua, Dipartimento Fis G Galilei, Padua, Italy

[32] Univ Milan, Dipartimento Fis, Milan, Italy

[33] Univ Roma Tor Vergata, Dipartimento Fis, I-00173 Rome, Italy

[34] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy

[35] DTU Space, Natl Space Inst, Copenhagen, Denmark

[36] Estec, European Space Agcy, Herschel Planck Project, NL-2201 AZ Noordwijk, Netherlands

[37] ESOC, European Space Agcy, Herschel Planck Project, Darmstadt, Germany

[38] Planck Sci Off ESAC, European Space Agcy, Madrid, Spain

[39] Univ Granada, Granada, Spain

[40] Haverford Coll, Dept Astron, Haverford, PA 19041 USA

[41] Aalto Univ, Univ Helsinki, Helsinki Inst Phys, Helsinki, Finland

[42] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London, England

[43] INAF Arcetri Astrophys Observ, Florence, Italy

[44] INAF Ist Astrofis Spaziale & Fis Cosm, Bologna, Italy

[45] INAF Osservatorio Astronom Trieste, Trieste, Italy

[46] INAF, Osservatorio Astrofis Catania, Catania, Italy

[47] INAF IASF Milano, Milan, Italy

[48] INAF Osservatorio Astronom Padova, Padua, Italy

[49] CALTECH, Ctr Infrared Proc & Anal, Pasadena, CA 91125 USA

[50] Univ Paris 06, CNRS, Inst Astrophys Paris, Paris, France

来源：

ASTRONOMY & ASTROPHYSICS | 2010年 / 520卷

关键词：

cosmic microwave background; space vehicles: instruments; instrumentation: detectors; instrumentation: polarimeters; submillimeter: general; radio continuum: general; POLARIZATION; ANISOTROPY; SPACE; PERFORMANCE; CALIBRATION; DESIGN;

D O I：

10.1051/0004-6361/200912983

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The European Space Agency's Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity (Delta T/T similar to 2 x 10(-6)) and angular resolution (similar to 5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30-350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis.

引用

页数：22

共 44 条

[1] Planck pre-launch status: The optical architecture of the HFI [J].

Ade, P. A. R. ;

Savini, G. ;

Sudiwala, R. ;

Tucker, C. ;

Catalano, A. ;

Church, S. ;

Colgan, R. ;

Desert, F. X. ;

Gleeson, E. ;

Jones, W. C. ;

Lamarre, J. -M. ;

Lange, A. ;

Longval, Y. ;

Maffei, B. ;

Murphy, J. A. ;

Noviello, F. ;

Pajot, F. ;

Puget, J. -L. ;

Ristorcelli, I. ;

Woodcraft, A. ;

Yurchenko, V. .

ASTRONOMY & ASTROPHYSICS, 2010, 520

[2]

[Anonymous], ESA PUBL

[3] Measurement of the Crab nebula polarization at 90 GHz as a calibrator for CMB experiments [J].

Aumont, J. ;

Conversi, L. ;

Thum, C. ;

Wiesemeyer, H. ;

Falgarone, E. ;

Macias-Perez, J. F. ;

Piacentini, F. ;

Pointecouteau, E. ;

Ponthieu, N. ;

Puget, J. L. ;

Rosset, C. ;

Tauber, J. A. ;

Tristram, M. .

ASTRONOMY & ASTROPHYSICS, 2010, 514

[4]

Benoit A, 1997, ESA SP PUBL, V400, P497

[5] Planck pre-launch status: Design and description of the Low Frequency Instrument [J].

Bersanelli, M. ;

Mandolesi, N. ;

Butler, R. C. ;

Mennella, A. ;

Villa, F. ;

Aja, B. ;

Artal, E. ;

Artina, E. ;

Baccigalupi, C. ;

Balasini, M. ;

Baldan, G. ;

Banday, A. ;

Bastia, P. ;

Battaglia, P. ;

Bernardino, T. ;

Blackhurst, E. ;

Boschini, L. ;

Burigana, C. ;

Cafagna, G. ;

Cappellini, B. ;

Cavaliere, F. ;

Colombo, F. ;

Crone, G. ;

Cuttaia, F. ;

D'Arcangelo, O. ;

Danese, L. ;

Davies, R. D. ;

Davis, R. J. ;

De Angelis, L. ;

De Gasperis, G. C. ;

De La Fuente, L. ;

De Rosa, A. ;

De Zotti, G. ;

Falvella, M. C. ;

Ferrari, F. ;

Ferretti, R. ;

Figini, L. ;

Fogliani, S. ;

Franceschet, C. ;

Franceschi, E. ;

Gaier, T. ;

Garavaglia, S. ;

Gomez, F. ;

Gorski, K. ;

Gregorio, A. ;

Guzzi, P. ;

Herreros, J. M. ;

Hildebrandt, S. R. ;

Hoyland, R. ;

Hughes, N. .

ASTRONOMY & ASTROPHYSICS, 2010, 520

[6] Sub-degree CMB anisotropy from space .2. In-flight calibration [J].

Bersanelli, M ;

Muciaccia, PF ;

Natoli, P ;

Vittorio, N ;

Mandolesi, N .

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 121 (02) :393-404

[7]

BERSANELLI M, 1996, ESA D SCI, V96, P3

[8] Sorption coolers using a continuous cycle to produce 20 K for the Planck flight mission [J].

Bhandari, P ;

Prina, M ;

Bowman, RC ;

Paine, C ;

Pearson, D ;

Nash, A .

CRYOGENICS, 2004, 44 (6-8) :395-401

[9] THE COBE MISSION - ITS DESIGN AND PERFORMANCE 2 YEARS AFTER LAUNCH [J].

BOGGESS, NW ;

MATHER, JC ;

WEISS, R ;

BENNETT, CL ;

CHENG, ES ;

DWEK, E ;

GULKIS, S ;

HAUSER, MG ;

JANSSEN, MA ;

KELSALL, T ;

MEYER, SS ;

MOSELEY, SH ;

MURDOCK, TL ;

SHAFER, RA ;

SILVERBERG, RF ;

SMOOT, GF ;

WILKINSON, DT ;

WRIGHT, EL .

ASTROPHYSICAL JOURNAL, 1992, 397 (02) :420-429

[10]

BRADSHAW TW, 1997, ESA, P465

← 1 2 3 4 5 →