Planck 2015 results VII. High Frequency Instrument data processing: Time-ordered information and beams

被引：84

作者：

Adam, R. ^{[72
]}

Ade, P. A. R. ^{[84
]}

Aghanim, N. ^{[56
]}

Arnaud, M. ^{[70
]}

Ashdown, M. ^{[5
,66
]}

Aumont, J. ^{[56
]}

Baccigalupi, C. ^{[83
]}

Banday, A. J. ^{[9
,92
]}

Barreiro, R. B. ^{[61
]}

Bartolo, N. ^{[28
,62
]}

Battaner, E. ^{[93
,94
]}

Benabed, K. ^{[57
,91
]}

Benoit, A. ^{[54
]}

Benoit-Levy, A. ^{[22
,57
,91
]}

Bernard, J. -P. ^{[9
,92
]}

Bersanelli, M. ^{[31
,46
]}

Bertincourt, B. ^{[56
]}

Bielewicz, P. ^{[9
,80
,83
]}

Bock, J. J. ^{[11
,63
]}

Bonavera, L. ^{[61
]}

Bond, J. R. ^{[8
]}

Borrill, J. ^{[13
,87
]}

Bouchet, F. R. ^{[57
,86
]}

Boulanger, F. ^{[56
]}

Bucher, M. ^{[1
]}

Burigana, C. ^{[29
,45
,47
]}

Calabrese, E. ^{[89
]}

Cardoso, J. -F. ^{[1
,57
,71
]}

Catalano, A. ^{[68
,72
]}

Challinor, A. ^{[12
,59
,66
]}

Chamballu, A. ^{[14
,56
,70
]}

Chary, R. -R. ^{[53
]}

Chiang, H. C. ^{[6
,25
]}

Christensen, P. R. ^{[33
,81
]}

Clements, D. L. ^{[52
]}

Colombi, S. ^{[57
,91
]}

Colombo, L. P. L. ^{[21
,63
]}

Combet, C. ^{[72
]}

Couchot, F. ^{[67
]}

Coulais, A. ^{[68
]}

Crill, B. P. ^{[11
,63
]}

Curto, A. ^{[5
,61
,66
]}

Cuttaia, F. ^{[45
]}

Danese, L. ^{[83
]}

Davies, R. D. ^{[64
]}

Davis, R. J. ^{[64
]}

de Bernardis, P. ^{[30
]}

de Rosa, A. ^{[45
]}

de Zotti, G. ^{[42
,83
]}

Delabrouille, J. ^{[1
]}

机构：

[1] Univ Paris Diderot, APC, CNRS IN2P3, CEA Lrfu,Observ Paris,Sorbonne Paris Cite, 10 Rue Alice Domon & Leonie, F-75205 Paris 13, France

[2] African Inst Math Sci, 6-8 Melrose Rd, ZA-7945 Cape Town, South Africa

[3] Agenzia Spaziale Italiana, Sci Data Ctr, Via Politecn Snc, I-00133 Rome, Italy

[4] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France

[5] Univ Cambridge, Astrophys Grp, Cavendish Lab, JJ Thomson Ave, Cambridge CB3 0HE, England

[6] Univ KwaZulu Natal, Sch Math Stat & Comp Sci, Astrophys & Cosmol Res Unit, Westville Campus,Private Bag X54001, ZA-4000 Durban, South Africa

[7] ALMA Santiago Cent Off, Atacama Large Millimeter Submillimeter Array, Alonso Cordova 3107,Vitacura,763 0355 Casilla, Santiago, Chile

[8] Univ Toronto, CITA, 60 St George St, Toronto, ON M5S 3H8, Canada

[9] IRAP, CNRS, 9 Ave Colonel Roche,BP 44346, F-31028 Toulouse 4, France

[10] Trinity Coll Dublin, CRANN, Dublin, Ireland

[11] CALTECH, Pasadena, CA 91125 USA

[12] Univ Cambridge, DAMTP, Ctr Theoret Cosmol, Wilberforce Rd, Cambridge CB3 0WA, England

[13] Lawrence Berkeley Natl Lab, Computat Cosmol Ctr, Berkeley, CA USA

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

[15] Tech Univ Denmark, Natl Space Inst, DTU Space, Elektrovej 327, DK-2800 Lyngby, Denmark

[16] Univ Geneva, Dept Phys Theor, 24 Quai E Ansermet, CH-1211 Geneva 4, Switzerland

[17] Univ Oviedo, Dept Fis, Avda Calvo Sotelo S-N, Oviedo, Spain

[18] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON, Canada

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

[20] Univ British Columbia, Dept Phys & Astron, 6224 Agr Rd, Vancouver, BC V6T 1Z4, Canada

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

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

[23] Florida State Univ, Dept Phys, Keen Phys Bldg,77 Chieftan Way, Tallahassee, FL 32306 USA

[24] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00100, Finland

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

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

[27] Univ Illinois, Dept Phys, 1110 West Green St, Urbana, IL 61801 USA

[28] Univ Padua, Dipartimento Fis & Astron G Galilei, Via Marzolo 8, I-35131 Padua, Italy

[29] Univ Ferrara, Dipartimento Fis & Sci Terra, Via Saragat 1, I-44122 Ferrara, Italy

[30] Univ Roma La Sapienza, Dipartimento Fis, Ple A Moro 2, I-00185 Rome, Italy

[31] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20122 Milan, Italy

[32] Univ Roma Tor Vergata, Dipartimento Matemat, Via Ric Sci 1, Rome, Italy

[33] Niels Bohr Inst, Discovery Ctr, 17 Blegdamsvej, Copenhagen, Denmark

[34] European Southern Observ, ESO Vitacura, Alonso Cordova 3107,19001 Casilla, Santiago, Chile

[35] European Space Agcy, ESAC, Planck Sci Off, Camino Bajo Castillo S-N, Madrid 28692, Spain

[36] European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands

[37] Univ E Campus, Fac Ingn, Via Isimbardi 10, I-22060 Novedrate, CO, Italy

[38] Ist Nazl Fis Nucl, Gran Sasso Sci Inst, Viale F Crispi 7, I-67100 Laquila, Italy

[39] HGSFP, Philosophenweg 16, D-69120 Heidelberg, Germany

[40] Heidelberg Univ, Dept Theoret Phys, Philosophenweg 16, D-69120 Heidelberg, Germany

[41] Univ Helsinki, Dept Theoret Phys, Gustaf Hallstromin Katu 2, Helsinki 00100, Finland

[42] INAF Osservatorio Astron Padova, Vicolo Osservatorio 5, I-35141 Padua, Italy

[43] INAF Osservatorio Astron Roma, Via Frascati 33, I-0036 Rome, Italy

[44] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34131 Trieste, Italy

[45] INAF IASF Bologna, Via Gobetti 101, I-40147 Bologna, Italy

[46] INAF IASF Milano, Via E Bassini 15, I-20133 Milan, Italy

[47] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy

[48] Univ Roma Sapienza, Sez Roma 1, Ist Nazl Fis Nucl, Piazzale Aldo Moro 2, I-00185 Rome, Italy

[49] Univ Roma Tor Vergata, Sez Roma 2, Ist Nazl Fis Nucl, Via Ric Sci 1, Rome, Italy

[50] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble, France

来源：

ASTRONOMY & ASTROPHYSICS | 2016年 / 594卷

关键词：

methods: data analysis; cosmic background radiation; instrumentation: detectors; PRE-LAUNCH STATUS;

D O I：

10.1051/0004-6361/201525844

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Planck High Frequency Instrument (HFI) has observed the full sky at six frequencies (100, 143, 217, 353, 545, and 857 GHz) in intensity and at four frequencies in linear polarization (100, 143, 217, and 353 GHz). In order to obtain sky maps, the time-ordered information (TOI) containing the detector and pointing samples must be processed and the angular response must be assessed. The full mission TOI is included in the Planck 2015 release. This paper describes the HFI TOI and beam processing for the 2015 release. HFI calibration and map making are described in a companion paper. The main pipeline has been modified since the last release (2013 nominal mission in intensity only), by including a correction for the nonlinearity of the warm readout and by improving the model of the bolometer time response. The beam processing is an essential tool that derives the angular response used in all the Planck science papers and we report an improvement in the effective beam window function uncertainty of more than a factor of 10 relative to the 2013 release. Noise correlations introduced by pipeline filtering function are assessed using dedicated simulations. Angular cross-power spectra using data sets that are decorrelated in time are immune to the main systematic effects.

引用

页数：30

共 12 条

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