Planck 2013 results. III. LFI systematic uncertainties

被引：47

作者：

Aghanim, N. ^{[60
]}

Armitage-Caplan, C. ^{[93
]}

Arnaud, M. ^{[74
]}

Ashdown, M. ^{[6
,71
]}

Atrio-Barandela, F. ^{[17
]}

Aumont, J. ^{[60
]}

Baccigalupi, C. ^{[87
]}

Banday, A. J. ^{[8
,96
]}

Barreiro, R. B. ^{[67
]}

Battaner, E. ^{[97
]}

Benabed, K. ^{[61
,95
]}

Benoit, A. ^{[35
,45
,58
,69
]}

Benoit-Levy, A. ^{[25
,61
,95
]}

Bernard, J. -P. ^{[8
,96
]}

Bersanelli, M. ^{[35
,50
]}

Bielewicz, P. ^{[8
,87
,96
]}

Bobin, J. ^{[74
]}

Bock, J. J. ^{[9
,69
]}

Bonaldi, A. ^{[70
]}

Bonavera, L. ^{[67
]}

Bond, J. R. ^{[7
]}

Borrill, J. ^{[12
,90
]}

Bouchet, F. R. ^{[61
,95
]}

Bridges, M. ^{[6
,64
,71
]}

Bucher, M. ^{[1
]}

Burigana, C. ^{[33
,49
]}

Butler, R. C. ^{[49
]}

Cardoso, J. -F. ^{[1
,61
,75
,76
]}

Catalano, A. ^{[73
,77
]}

Chamballu, A. ^{[14
,60
,74
]}

Chiang, L. -Y ^{[63
]}

Cristensen, P. R. ^{[38
,84
]}

Church, S. ^{[92
]}

Olombi, S. C. ^{[61
,95
]}

Colombo, L. P. L. ^{[24
,69
]}

Crill, B. P. ^{[69
,85
]}

Cruz, M. ^{[19
]}

Curto, A. ^{[6
,67
]}

Cuttaia, F. ^{[49
]}

Danese, L. ^{[87
]}

Davies, R. D. ^{[70
]}

Davis, R. J. ^{[70
]}

de Bernardis, P. ^{[34
]}

de Rose, A. ^{[49
]}

de Zotti, G. ^{[45
,87
]}

Delabrouillei, J. ^{[1
]}

Dick, J. ^{[87
]}

Dickinson, C. ^{[70
]}

Diego, J. M. ^{[67
]}

Dole, H. ^{[59
,60
]}

机构：

[1] Univ Paris Diderot, Sorbonne Paris Cite, CNRS, IN2P3,CEA Irfu,Observ Paris,APC, F-75205 Paris 13, France

[2] Aalto Univ Metsahovi Radio Observ, Kylmala 02540, Finland

[3] African Inst Math Sci, ZA-7701 Rondebosch Cape Town, South Africa

[4] Aeenzia Spaziale Italiana, Sci Data Ctr, I-00133 Rome, Italy

[5] Agenzia Spaziale ilaliana, I-00198 Rome, Italy

[6] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England

[7] Univ Toronto, CITA, Toronto, ON M5S 3H8, Canada

[8] CNRS, IRAP, F-4 Toulouse 4, France

[9] CALTECH, Pasadena, CA 91125 USA

[10] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Cambridge CB3 0WA, England

[11] CEFCA, Teruel 44001, Spain

[12] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA 94720 USA

[13] CSIC, E-28006 Madrid, Spain

[14] CEA Saclay, DSM Irfu SPP, F-91191 Gif Sur Yvette, France

[15] Tech Univ Denmark, Natl Space Inst, DTU Space, DK-2800 Lyngby, Denmark

[16] Univ Geneva, Dept Phys Theor, CH-1211 Geneva 4, Switzerland

[17] Univ Salamanca, Fac Ciencias, Dept Fis Fundamental, E-37008 Salamanca, Spain

[18] Univ Oviedo, Dept Fis, Oviedo 33007, Spain

[19] Univ Cantabria, Dept Matemat Estadist & Computac, E-39005 Santander, Spain

[20] Univ Toronto, Dept Astron & Astrophys, Toronto, ON, Canada

[21] Radboud Univ Nijmegen, IMAPP, Dept Astrophys, NL-6500 GL Nijmegen, Netherlands

[22] Univ Calif Berkeley, Dept Elect Engn & Comp Sci, Berkeley, CA 94720 USA

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

[24] Univ So Calif, Dana & David Dornsife Coll Letter Arts & Sci, Dept Phys & Astron, Los Angeles, CA 90089 USA

[25] UCL, Dept Phys & Astron, London WC1E 6BT, England

[26] Florida State Univ, Dept Phys, Tallahassee, FL USA

[27] Univ Helsinki, Dept Phys, FIN-00014 Helsinki, Finland

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

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

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

[31] Univ Illinois, Dept Phys, Urbana, IL USA

[32] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy

[33] Univ Ferrara, Dipartimento Fis & Sci Terra, I-44122 Ferrara, Italy

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

[35] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy

[36] Univ Trieste, Dipartmento Fis, I-34127 Trieste, Italy

[37] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy

[38] Niels Bohr Inst, Discovery Ctr, DK-2100 Copenhagen, Denmark

[39] Univ La Laguna, Dpto Astrofis, E-38206 Tenerife, Spain

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

[41] European Space Agcy, Estec, NL-2201 AZ Noordwijk, Netherlands

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

[43] Aalto Univ, Univ Helsinki, Helsinki Inst Phys, FIN-00014 Helsinki, Finland

[44] Osserv Astrofis Catania, INAF, I-95123 Catania, Italy

[45] Osserv Astron Padova, INAF, I-35122 Padua, Italy

[46] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy

[47] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy

[48] Ist Radioastron, INAF, I-40129 Bologna, Italy

[49] IASF Bologna, INAF, I-40129 Bologna, Italy

[50] IASF Bologna, INAF, I-40129 Milan, Italy

来源：

ASTRONOMY & ASTROPHYSICS | 2014年 / 571卷

关键词：

cosmic background radiation; cosmology: observations; methods: data analysis;

D O I：

10.1051/0004-6361/201321574

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of the Planck cosmological results. We give an overview of the main effects and of the tools and methods applied to assess residuals in maps and power spectra. We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-up and imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave background fluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipole range l < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reduce the level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibration uncertainties.

引用

页数：23

共 50 条

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Church, S.
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[28] Planck 2013 results. II. Low Frequency Instrument data processing
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Battaner, E.
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Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bobin, J.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bridges, M.
Bucher, M.
Burigana, C.
Butler, R. C.
Cappellini, B.
Cardoso, J. -F.
Catalano, A.
Chamballu, A.
Chen, X.
Chiang, L. -Y
Christensen, P. R.
Church, S.
Colombi, S.
Colombo, L. P. L.
Crill, B. P.
Cruz, M.
Curto, A.
Cattaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J. M.
ASTRONOMY & ASTROPHYSICS, 2014, 571
[29] Planck 2013 results. VI. High Frequency Instrument data processing
Ade, P. A. R.
Aghanim, N.
Armitage-Caplan, C.
Arnaud, M.
Ashdown, M.
Atrio-Barandela, F.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bobin, J.
Bock, J. J.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Boulanger, F.
Bowyer, J. W.
Bridges, M.
Bucher, M.
Burigana, C.
Cardoso, J. -F.
Catalano, A.
Chamballu, A.
Chary, R. -R.
Chen, X.
Chiang, H. C.
Chiang, L. -Y
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Combet, C.
Couchot, F.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
de Rose, A.
ASTRONOMY & ASTROPHYSICS, 2014, 571
[30] Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
Ade, P. A. R.
Aghanim, N.
Armitage-Caplan, C.
Arnaud, M.
Ashdown, M.
Atrio-Barandelals, E.
Aumont, J.
Baccigalupi, C.
Banday, A. J.
Barreiro, R. B.
Bartlett, J. G.
Bartolo, N.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J. -P.
Bersanelli, M.
Bielewicz, P.
Bobin, J.
Bock, J. J.
Bonaldi, A.
Bonavera, L.
Bond, J. R.
Borrill, J.
Bouchet, F. R.
Bridges, M.
Bucher, M.
Burigana, C.
Butler, R. C.
Cardoso, J. -F.
Catalano, A.
Challinor, A.
Chamballu, A.
Chiang, H. C.
Chiang, L. -Y.
Christensen, P. R.
Church, S.
Clements, D. L.
Colombi, S.
Colombo, L. P. L.
Couchot, E.
Coulais, A.
Crill, B. P.
Curto, A.
Cuttaia, E.
Danese, L.
Davies, R. D.
Davis, R. J.
de Bernardis, P.
ASTRONOMY & ASTROPHYSICS, 2014, 571

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