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. Benoît; 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; G. Lagache; J. M. Lamarre; A. E. Lange; A. Lasenby; A. Lavabre; C. R. Lawrence; M. Le Jeune; C. Leroy; J. Lesgourgues; 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; S. Mitra

doi:10.1051/0004-6361/201116462

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. Benoît, J. P. Bernard, M. Bersanelli, J. J. Bock, J. R. Bond, J. Borrill, F. R. Bouchet, F. Boulanger, T. BradshawM. 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, G. Lagache, J. M. Lamarre, A. E. Lange, A. Lasenby, A. Lavabre, C. R. Lawrence, M. Le Jeune, C. Leroy, J. Lesgourgues, 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, S. Mitra

Research output: Contribution to journal › Article › Research › peer-review

24 Citations (Scopus)

Abstract

We describe the processing of the 336 billion raw data samples from the High Frequency Instrument (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 857 GHz with an angular resolution ranging from 9.9 to 4.4′. The white noise level is around 1.5 μK degree or less in the 3 main CMB channels (100-217 GHz). The photometric accuracy is better than 2% at frequencies between 100 and 353 GHz 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 Planck project. © ESO, 2011.

Original language	English
Article number	A6
Journal	Astronomy and Astrophysics
Volume	536
DOIs	https://doi.org/10.1051/0004-6361/201116462
Publication status	Published - 12 Dec 2011

Keywords

Cosmic background radiation
Cosmology
data analysis
Methods
observations
Surveys

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10.1051/0004-6361/201116462

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Ade, P. A. R., Aghanim, N., Ansari, R., Arnaud, M., Ashdown, M., Aumont, J., Banday, A. J., Bartelmann, M., Bartlett, J. G., Battaner, E., Benabed, K., Benoît, A., Bernard, J. P., Bersanelli, M., Bock, J. J., Bond, J. R., Borrill, J., Bouchet, F. R., Boulanger, F., ... Mitra, S. (2011). Planck early results. VI. The High Frequency Instrument data processing. Astronomy and Astrophysics, 536, [A6]. https://doi.org/10.1051/0004-6361/201116462

Ade, P. A.R. ; Aghanim, N. ; Ansari, R. ; Arnaud, M. ; Ashdown, M. ; Aumont, J. ; Banday, A. J. ; Bartelmann, M. ; Bartlett, J. G. ; Battaner, E. ; Benabed, K. ; Benoît, A. ; Bernard, J. P. ; Bersanelli, M. ; Bock, J. J. ; Bond, J. R. ; Borrill, J. ; Bouchet, F. R. ; Boulanger, F. ; Bradshaw, T. ; Bucher, M. ; Cardoso, J. F. ; Castex, G. ; Catalano, A. ; Challinor, A. ; Chamballu, A. ; Chary, R. R. ; Chen, X. ; Chiang, C. ; Church, S. ; Clements, D. L. ; Colley, J. M. ; Colombi, S. ; Couchot, F. ; Coulais, A. ; Cressiot, C. ; Crill, B. P. ; Crook, M. ; De Bernardis, P. ; Delabrouille, J. ; Delouis, J. M. ; Désert, F. X. ; Dolag, K. ; Dole, H. ; Doré, O. ; Douspis, M. ; Dunkley, J. ; Efstathiou, G. ; Filliard, C. ; Forni, O. ; Fosalba, P. ; Ganga, K. ; Giard, M. ; Girard, D. ; Giraud-Héraud, Y. ; Gispert, R. ; Górski, K. M. ; Gratton, S. ; Griffin, M. ; Guyot, G. ; Haissinski, J. ; Harrison, D. ; Helou, G. ; Henrot-Versillé, S. ; Hernández-Monteagudo, C. ; Hildebrandt, S. R. ; Hills, R. ; Hivon, E. ; Hobson, M. ; Holmes, W. A. ; Huffenberger, K. M. ; Jaffe, A. H. ; Jones, W. C. ; Kaplan, J. ; Kneissl, R. ; Knox, L. ; Kunz, M. ; Lagache, G. ; Lamarre, J. M. ; Lange, A. E. ; Lasenby, A. ; Lavabre, A. ; Lawrence, C. R. ; Le Jeune, M. ; Leroy, C. ; Lesgourgues, J. ; MacÍas-Pérez, J. F. ; MacTavish, C. J. ; Maffei, B. ; Mandolesi, N. ; Mann, R. ; Marleau, F. ; Marshall, D. J. ; Masi, S. ; Matsumura, T. ; McAuley, I. ; McGehee, P. ; Melin, J. B. ; Mercier, C. ; Mitra, S. / Planck early results. VI. The High Frequency Instrument data processing. In: Astronomy and Astrophysics. 2011 ; Vol. 536.

@article{ad907bb55c78478188b3bbbd51f79e4c,

title = "Planck early results. VI. The High Frequency Instrument data processing",

abstract = "We describe the processing of the 336 billion raw data samples from the High Frequency Instrument (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 857 GHz with an angular resolution ranging from 9.9 to 4.4′. The white noise level is around 1.5 μK degree or less in the 3 main CMB channels (100-217 GHz). The photometric accuracy is better than 2% at frequencies between 100 and 353 GHz 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 Planck project. {\textcopyright} ESO, 2011.",

keywords = "Cosmic background radiation, Cosmology, data analysis, Methods, observations, Surveys",

author = "Ade, {P. A.R.} and N. Aghanim and R. Ansari and M. Arnaud and M. Ashdown and J. Aumont and Banday, {A. J.} and M. Bartelmann and Bartlett, {J. G.} and E. Battaner and K. Benabed and A. Beno{\^i}t and Bernard, {J. P.} and M. Bersanelli and Bock, {J. J.} and Bond, {J. R.} and J. Borrill and Bouchet, {F. R.} and F. Boulanger and T. Bradshaw and M. Bucher and Cardoso, {J. F.} and G. Castex and A. Catalano and A. Challinor and A. Chamballu and Chary, {R. R.} and X. Chen and C. Chiang and S. Church and Clements, {D. L.} and Colley, {J. M.} and S. Colombi and F. Couchot and A. Coulais and C. Cressiot and Crill, {B. P.} and M. Crook and {De Bernardis}, P. and J. Delabrouille and Delouis, {J. M.} and D{\'e}sert, {F. X.} and K. Dolag and H. Dole and O. Dor{\'e} and M. Douspis and J. Dunkley and G. Efstathiou and C. Filliard and O. Forni and P. Fosalba and K. Ganga and M. Giard and D. Girard and Y. Giraud-H{\'e}raud and R. Gispert and G{\'o}rski, {K. M.} and S. Gratton and M. Griffin and G. Guyot and J. Haissinski and D. Harrison and G. Helou and S. Henrot-Versill{\'e} and C. Hern{\'a}ndez-Monteagudo and Hildebrandt, {S. R.} and R. Hills and E. Hivon and M. Hobson and Holmes, {W. A.} and Huffenberger, {K. M.} and Jaffe, {A. H.} and Jones, {W. C.} and J. Kaplan and R. Kneissl and L. Knox and M. Kunz and G. Lagache and Lamarre, {J. M.} and Lange, {A. E.} and A. Lasenby and A. Lavabre and Lawrence, {C. R.} and {Le Jeune}, M. and C. Leroy and J. Lesgourgues and Mac{\'I}as-P{\'e}rez, {J. F.} and MacTavish, {C. J.} and B. Maffei and N. Mandolesi and R. Mann and F. Marleau and Marshall, {D. J.} and S. Masi and T. Matsumura and I. McAuley and P. McGehee and Melin, {J. B.} and C. Mercier and S. Mitra",

year = "2011",

month = dec,

day = "12",

doi = "10.1051/0004-6361/201116462",

language = "English",

volume = "536",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

}

Ade, PAR, Aghanim, N, Ansari, R, Arnaud, M, Ashdown, M, Aumont, J, Banday, AJ, Bartelmann, M, Bartlett, JG, Battaner, E, Benabed, K, Benoît, A, Bernard, JP, Bersanelli, M, Bock, JJ, Bond, JR, Borrill, J, Bouchet, FR, Boulanger, F, Bradshaw, T, Bucher, M, Cardoso, JF, Castex, G, Catalano, A, Challinor, A, Chamballu, A, Chary, RR, Chen, X, Chiang, C, Church, S, Clements, DL, Colley, JM, Colombi, S, Couchot, F, Coulais, A, Cressiot, C, Crill, BP, Crook, M, De Bernardis, P, Delabrouille, J, Delouis, JM, Désert, FX, Dolag, K, Dole, H, Doré, O, Douspis, M, Dunkley, J, Efstathiou, G, Filliard, C, Forni, O, Fosalba, P, Ganga, K, Giard, M, Girard, D, Giraud-Héraud, Y, Gispert, R, Górski, KM, Gratton, S, Griffin, M, Guyot, G, Haissinski, J, Harrison, D, Helou, G, Henrot-Versillé, S, Hernández-Monteagudo, C, Hildebrandt, SR, Hills, R, Hivon, E, Hobson, M, Holmes, WA, Huffenberger, KM, Jaffe, AH, Jones, WC, Kaplan, J, Kneissl, R, Knox, L, Kunz, M, Lagache, G, Lamarre, JM, Lange, AE, Lasenby, A, Lavabre, A, Lawrence, CR, Le Jeune, M, Leroy, C, Lesgourgues, J, MacÍas-Pérez, JF, MacTavish, CJ, Maffei, B, Mandolesi, N, Mann, R, Marleau, F, Marshall, DJ, Masi, S, Matsumura, T, McAuley, I, McGehee, P, Melin, JB, Mercier, C & Mitra, S 2011, 'Planck early results. VI. The High Frequency Instrument data processing', Astronomy and Astrophysics, vol. 536, A6. https://doi.org/10.1051/0004-6361/201116462

Planck early results. VI. The High Frequency Instrument data processing. / Ade, P. A.R.; Aghanim, N.; Ansari, R.; Arnaud, M.; Ashdown, M.; Aumont, J.; Banday, A. J.; Bartelmann, M.; Bartlett, J. G.; Battaner, E.; Benabed, K.; Benoît, A.; Bernard, J. P.; Bersanelli, M.; Bock, J. J.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bradshaw, T.; Bucher, M.; Cardoso, J. F.; Castex, G.; Catalano, A.; Challinor, A.; Chamballu, A.; Chary, R. R.; Chen, X.; Chiang, C.; Church, S.; Clements, D. L.; Colley, J. M.; Colombi, S.; Couchot, F.; Coulais, A.; Cressiot, C.; Crill, B. P.; Crook, M.; De Bernardis, P.; Delabrouille, J.; Delouis, J. M.; Désert, F. X.; Dolag, K.; Dole, H.; Doré, O.; Douspis, M.; Dunkley, J.; Efstathiou, G.; Filliard, C.; Forni, O.; Fosalba, P.; Ganga, K.; Giard, M.; Girard, D.; Giraud-Héraud, Y.; Gispert, R.; Górski, K. M.; Gratton, S.; Griffin, M.; Guyot, G.; Haissinski, J.; Harrison, D.; Helou, G.; Henrot-Versillé, S.; Hernández-Monteagudo, C.; Hildebrandt, S. R.; Hills, R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Huffenberger, K. M.; Jaffe, A. H.; Jones, W. C.; Kaplan, J.; Kneissl, R.; Knox, L.; Kunz, M.; Lagache, G.; Lamarre, J. M.; Lange, A. E.; Lasenby, A.; Lavabre, A.; Lawrence, C. R.; Le Jeune, M.; Leroy, C.; Lesgourgues, J.; MacÍas-Pérez, J. F.; MacTavish, C. J.; Maffei, B.; Mandolesi, N.; Mann, R.; Marleau, F.; Marshall, D. J.; Masi, S.; Matsumura, T.; McAuley, I.; McGehee, P.; Melin, J. B.; Mercier, C.; Mitra, S.

In: Astronomy and Astrophysics, Vol. 536, A6, 12.12.2011.

Research output: Contribution to journal › Article › Research › peer-review

TY - JOUR

T1 - Planck early results. VI. The High Frequency Instrument data processing

AU - Ade, P. A.R.

AU - Aghanim, N.

AU - Ansari, R.

AU - Arnaud, M.

AU - Ashdown, M.

AU - Aumont, J.

AU - Banday, A. J.

AU - Bartelmann, M.

AU - Bartlett, J. G.

AU - Battaner, E.

AU - Benabed, K.

AU - Benoît, A.

AU - Bernard, J. P.

AU - Bersanelli, M.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Boulanger, F.

AU - Bradshaw, T.

AU - Bucher, M.

AU - Cardoso, J. F.

AU - Castex, G.

AU - Catalano, A.

AU - Challinor, A.

AU - Chamballu, A.

AU - Chary, R. R.

AU - Chen, X.

AU - Chiang, C.

AU - Church, S.

AU - Clements, D. L.

AU - Colley, J. M.

AU - Colombi, S.

AU - Couchot, F.

AU - Coulais, A.

AU - Cressiot, C.

AU - Crill, B. P.

AU - Crook, M.

AU - De Bernardis, P.

AU - Delabrouille, J.

AU - Delouis, J. M.

AU - Désert, F. X.

AU - Dolag, K.

AU - Dole, H.

AU - Doré, O.

AU - Douspis, M.

AU - Dunkley, J.

AU - Efstathiou, G.

AU - Filliard, C.

AU - Forni, O.

AU - Fosalba, P.

AU - Ganga, K.

AU - Giard, M.

AU - Girard, D.

AU - Giraud-Héraud, Y.

AU - Gispert, R.

AU - Górski, K. M.

AU - Gratton, S.

AU - Griffin, M.

AU - Guyot, G.

AU - Haissinski, J.

AU - Harrison, D.

AU - Helou, G.

AU - Henrot-Versillé, S.

AU - Hernández-Monteagudo, C.

AU - Hildebrandt, S. R.

AU - Hills, R.

AU - Hivon, E.

AU - Hobson, M.

AU - Holmes, W. A.

AU - Huffenberger, K. M.

AU - Jaffe, A. H.

AU - Jones, W. C.

AU - Kaplan, J.

AU - Kneissl, R.

AU - Knox, L.

AU - Kunz, M.

AU - Lagache, G.

AU - Lamarre, J. M.

AU - Lange, A. E.

AU - Lasenby, A.

AU - Lavabre, A.

AU - Lawrence, C. R.

AU - Le Jeune, M.

AU - Leroy, C.

AU - Lesgourgues, J.

AU - MacÍas-Pérez, J. F.

AU - MacTavish, C. J.

AU - Maffei, B.

AU - Mandolesi, N.

AU - Mann, R.

AU - Marleau, F.

AU - Marshall, D. J.

AU - Masi, S.

AU - Matsumura, T.

AU - McAuley, I.

AU - McGehee, P.

AU - Melin, J. B.

AU - Mercier, C.

AU - Mitra, S.

PY - 2011/12/12

Y1 - 2011/12/12

N2 - We describe the processing of the 336 billion raw data samples from the High Frequency Instrument (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 857 GHz with an angular resolution ranging from 9.9 to 4.4′. The white noise level is around 1.5 μK degree or less in the 3 main CMB channels (100-217 GHz). The photometric accuracy is better than 2% at frequencies between 100 and 353 GHz 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 Planck project. © ESO, 2011.

AB - We describe the processing of the 336 billion raw data samples from the High Frequency Instrument (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 857 GHz with an angular resolution ranging from 9.9 to 4.4′. The white noise level is around 1.5 μK degree or less in the 3 main CMB channels (100-217 GHz). The photometric accuracy is better than 2% at frequencies between 100 and 353 GHz 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 Planck project. © ESO, 2011.

KW - Cosmic background radiation

KW - Cosmology

KW - data analysis

KW - Methods

KW - observations

KW - Surveys

U2 - 10.1051/0004-6361/201116462

DO - 10.1051/0004-6361/201116462

M3 - Article

VL - 536

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

M1 - A6

ER -

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

Abstract

Keywords

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