Planck early results. VI. The High Frequency Instrument data processing

P.A.R. Ade; N. Aghanim; R. Ansari; M. Arnaud; M. Ashdown; J. Aumont; A.J. Banday; M. Bartelmann; J.G. Bartlett; E. Battaner; K. Benabed; A. Benoit; J.-P. Bernard; M. Bersanelli; J.J. Bock; J.R. Bond; J. Borrill; F.R. Bouchet; F. Boulanger; T. Bradshaw; M. Bucher; J.-F. Cardoso; G. Castex; A. Catalano; A. Challinor; A. Chamballu; R.-R. Chary; X. Chen; C. Chiang; S. Church; D.L. Clements; J.-M. Colley; S. Colombi; F. Couchot; A. Coulais; C. Cressiot; B.P. Crill; M. Crook; P. de Bernardis; J. Delabrouille; J.-M. Delouis; F.-X. Désert; K. Dolag; H. Dole; O. Doré; M. Douspis; J. Dunkley; G. Efstathiou; C. Filliard; O. Forni; P. Fosalba; K. Ganga; M. Giard; D. Girard; Y. Giraud-Héraud; R. Gispert; K.M. Górski; S. Gratton; M. Griffin; G. Guyot; J. Haissinski; D. Harrison; G. Helou; S. Henrot-Versillé; C. Hernández-Monteagudo; S.R. Hildebrandt; R. Hills; E. Hivon; M. Hobson; W.A. Holmes; K.M. Huffenberger; A.H. Jaffe; W.C. Jones; J. Kaplan; R. Kneissl; L. Knox; M. Kunz; Guilaine Lagache; J.-M. Lamarre; A.E. Lange; A. Lasenby; A. Lavabre; C.R. Lawrence; M. Le Jeune; C. Leroy; J. Lesgourgues; A. Lewis; J.F. Macías-Pérez; C.J. Mactavish; B. Maffei; N. Mandolesi; R. Mann; F. Marleau; D.J. Marshall; S. Masi; T. Matsumura; I. Mcauley; P. Mcgehee; J.-B. Melin; C. Mercier; Subhabrata Mitra; M.-A. Miville-Deschênes; A. Moneti; L. Montier; D. Mortlock; A. Murphy; F. Nati; C.B. Netterfield; H.U. Nørgaard-Nielsen; C. North; F. Noviello; D. Novikov; S. Osborne; F. Pajot; G. Patanchon; T. Peacocke; T.J. Pearson; O. Perdereau; L. Perotto; F. Piacentini; M. Piat; Stéphane Plaszczynski; E. Pointecouteau; N. Ponthieu; G. Prézeau; S. Prunet; J.-L. Puget; W.T. Reach; M. Remazeilles; C. Renault; A. Riazuelo; I. Ristorcelli; G. Rocha; C. Rosset; G. Roudier; M. Rowan-Robinson; B. Rusholme; R. Saha; D. Santos; G. Savini; B.M. Schaefer; P. Shellard; L. Spencer; Jean-Luc Starck; V. Stolyarov; Radek Stompor; R. Sudiwala; R. Sunyaev; D. Sutton; J.-F. Sygnet; J.A. Tauber; C. Thum; J.-P. Torre; F. Touze; M. Tristram; F. van Leeuwen; L. Vibert; D. Vibert; B.D. Wandelt; S.D.M. White; Helmut Wiesemeyer; A. Woodcraft; V. Yurchenko; D. Yvon; A. Zacchei

doi:10.1051/0004-6361/201116462

Journal articles

Planck early results. VI. The High Frequency Instrument data processing

P.A.R. Ade N. Aghanim ¹ R. Ansari ² M. Arnaud ³ M. Ashdown J. Aumont ¹ A.J. Banday ⁴ M. Bartelmann J.G. Bartlett ⁵ E. Battaner K. Benabed ⁶ A. Benoit ⁷ J.-P. Bernard ⁴ M. Bersanelli J.J. Bock J.R. Bond J. Borrill F.R. Bouchet ⁶ F. Boulanger ¹ T. Bradshaw M. Bucher ⁸ J.-F. Cardoso ^{8, 6, 9} G. Castex ⁸ A. Catalano ^{8, 10} A. Challinor A. Chamballu R.-R. Chary X. Chen C. Chiang S. Church D.L. Clements J.-M. Colley ⁸ S. Colombi ⁶ F. Couchot ² A. Coulais ¹⁰ C. Cressiot ⁸ B.P. Crill M. Crook P. de Bernardis J. Delabrouille ¹¹ J.-M. Delouis ⁶ F.-X. Désert ¹² K. Dolag H. Dole ¹ O. Doré M. Douspis ¹ J. Dunkley G. Efstathiou C. Filliard ² O. Forni ⁴ P. Fosalba K. Ganga ⁸ M. Giard ⁴ D. Girard ¹³ Y. Giraud-Héraud ⁵ R. Gispert ¹ K.M. Górski S. Gratton M. Griffin G. Guyot ¹⁴ J. Haissinski ² D. Harrison G. Helou S. Henrot-Versillé ² C. Hernández-Monteagudo S.R. Hildebrandt ¹³ R. Hills E. Hivon ⁶ M. Hobson W.A. Holmes K.M. Huffenberger A.H. Jaffe W.C. Jones J. Kaplan ⁸ R. Kneissl L. Knox M. Kunz ¹ Guilaine Lagache ¹ J.-M. Lamarre ¹⁰ A.E. Lange A. Lasenby A. Lavabre ² C.R. Lawrence M. Le Jeune ⁸ C. Leroy ^{1, 4} J. Lesgourgues ⁶ A. Lewis J.F. Macías-Pérez ¹³ C.J. Mactavish B. Maffei N. Mandolesi R. Mann F. Marleau D.J. Marshall ⁴ S. Masi T. Matsumura I. Mcauley P. Mcgehee J.-B. Melin ¹⁵ C. Mercier ¹ Subhabrata Mitra M.-A. Miville-Deschênes ¹ A. Moneti ⁶ L. Montier ⁴ D. Mortlock A. Murphy F. Nati C.B. Netterfield H.U. Nørgaard-Nielsen C. North F. Noviello ¹ D. Novikov S. Osborne F. Pajot ¹ G. Patanchon ⁸ T. Peacocke T.J. Pearson O. Perdereau ² L. Perotto ¹³ F. Piacentini M. Piat ⁸ Stéphane Plaszczynski ² E. Pointecouteau ⁴ N. Ponthieu ¹ G. Prézeau S. Prunet ⁶ J.-L. Puget ¹ W.T. Reach M. Remazeilles ⁸ C. Renault ¹³ A. Riazuelo ⁶ I. Ristorcelli ⁴ G. Rocha C. Rosset ⁸ G. Roudier ⁸ M. Rowan-Robinson B. Rusholme R. Saha D. Santos ¹³ G. Savini B.M. Schaefer P. Shellard L. Spencer Jean-Luc Starck ^{3, 15} V. Stolyarov Radek Stompor ¹¹ R. Sudiwala R. Sunyaev D. Sutton J.-F. Sygnet ⁶ J.A. Tauber C. Thum ¹⁶ J.-P. Torre ¹ F. Touze ² M. Tristram ² F. van Leeuwen L. Vibert ¹ D. Vibert ¹⁷ B.D. Wandelt ⁶ S.D.M. White Helmut Wiesemeyer A. Woodcraft V. Yurchenko D. Yvon ¹⁵ A. Zacchei

1 IAS - Institut d'astrophysique spatiale

2 LAL - Laboratoire de l'Accélérateur Linéaire

3 DAP - Département d'Astrophysique (ex SAP)

4 IRAP - Institut de recherche en astrophysique et planétologie

5 APC - Cosmologie

APC (UMR_7164) - AstroParticule et Cosmologie

6 IAP - Institut d'Astrophysique de Paris

7 HELFA [2007-2015] - Hélium : du fondamental aux applications [2007-2015]

NEEL [2007-2015] - Institut Néel [2007-2015]

8 APC (UMR_7164) - AstroParticule et Cosmologie

9 LTCI - Laboratoire Traitement et Communication de l'Information

10 LERMA - Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique

11 APC-Gravitation - APC - Gravitation

APC (UMR_7164) - AstroParticule et Cosmologie, AEI - Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )

12 IPAG [2011-2015] - Institut de Planétologie et d'Astrophysique de Grenoble [2011-2015]

13 LPSC - Laboratoire de Physique Subatomique et de Cosmologie

14 INSU - CNRS - Institut national des sciences de l'Univers

15 DPP - Département de Physique des Particules (ex SPP)

16 IRAM - Institut de RadioAstronomie Millimétrique

17 LAM - Laboratoire d'Astrophysique de Marseille

Abstract : We describe the processing of the 334 billion raw data samples from the High Frequency Instrument (hereafter HFI) which we performed to produce six temperature maps from the first 295 days of Planck-HFI survey data. These maps provide an accurate rendition of the sky emission at 100, 143, 217, 353, 545 and 857GHz with an angular resolution ranging from 9.9 to 4.4 arcmin. The white noise level is around 1.5 microK.degree or less in the 3 main CMB channels (100-217GHz). The photometric accuracy is better than 2% at frequencies lower or equal to 353GHz, and around 7% at the two highest frequencies. The maps created by the HFI Data Processing Centre reach our goals in terms of sensitivity, resolution, and photometric accuracy. They are already sufficiently accurate and well-characterised to allow scientific analyses which are presented in an accompanying series of early papers. At this stage, HFI data appears to be of high quality and we expect that with further refinements of the data processing we should be able to achieve, or exceed, the science goals of the project.

Document type :

Journal articles

Domain :

Physics [physics] / Astrophysics [astro-ph] / Instrumentation and Methods for Astrophysic [astro-ph.IM]

Sciences of the Universe [physics] / Astrophysics [astro-ph] / Instrumentation and Methods for Astrophysic [astro-ph.IM]

Complete list of metadatas

http://hal.in2p3.fr/in2p3-00556506
Contributor : Emmanuelle Vernay <>
Submitted on : Monday, January 17, 2011 - 9:22:04 AM
Last modification on : Saturday, September 19, 2020 - 3:09:28 AM

Planck early results. VI. The High Frequency Instrument data processing

Links full text

Identifiers

Collections

Citation

Export

Metrics

1431

Planck early results. VI. The High Frequency Instrument data processing

Links full text

Identifiers

Collections

Citation

Export

Share

Metrics

1431