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

[No Value] Planck HFI Core Team; 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; 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; S. 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; J.-L. Starck; V. Stolyarov; R. 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; L. A. Wade; B. D. Wandelt; S. D. M. White; H. Wiesemeyer; A. Woodcraft; V. Yurchenko; D. Yvon; A. Zacchei

doi:10.1051/0004-6361/201116462

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

[No Value] Planck HFI Core Team, 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. BoulangerT. 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, 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, S. 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, J.-L. Starck, V. Stolyarov, R. 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, L. A. Wade, B. D. Wandelt, S. D. M. White, H. Wiesemeyer, A. Woodcraft, V. Yurchenko, D. Yvon, A. Zacchei

School of Physics and Astronomy

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

Abstract / Description of output

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. Corresponding author: F. R. Bouchet, e-mail: [email protected]

Original language	English
Article number	A6
Number of pages	47
Journal	Astronomy & Astrophysics
Volume	536
DOIs	https://doi.org/10.1051/0004-6361/201116462
Publication status	Published - 1 Dec 2011

Access to Document

10.1051/0004-6361/201116462

http://adsabs.harvard.edu/abs/2011A%26A...536A...6P

Cite this

Planck HFI Core Team, N. V., 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., ... Zacchei, A. (2011). Planck early results. VI. The High Frequency Instrument data processing. Astronomy & Astrophysics, 536, Article A6. https://doi.org/10.1051/0004-6361/201116462

@article{ed706c4305f8497da48c41ed72edd3d5,

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. Corresponding author: F. R. Bouchet, e-mail: [email protected]",

author = "{Planck HFI Core Team}, {[No Value]} and 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 J.-P. Bernard 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 J.-F. Cardoso and G. Castex and A. Catalano and A. Challinor and A. Chamballu and R.-R. Chary and X. Chen and C. Chiang and S. Church and Clements, {D. L.} and J.-M. Colley 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 J.-M. Delouis and F.-X. D{\'e}sert 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 J.-M. Lamarre 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 J.-B. Melin and C. Mercier and S. Mitra and M.-A. Miville-Desch{\^e}nes and A. Moneti and L. Montier and D. Mortlock and A. Murphy and F. Nati and Netterfield, {C. B.} and N{\o}rgaard-Nielsen, {H. U.} and C. North and F. Noviello and D. Novikov and S. Osborne and F. Pajot and G. Patanchon and T. Peacocke and Pearson, {T. J.} and O. Perdereau and L. Perotto and F. Piacentini and M. Piat and S. Plaszczynski and E. Pointecouteau and N. Ponthieu and G. Pr{\'e}zeau and S. Prunet and J.-L. Puget and Reach, {W. T.} and M. Remazeilles and C. Renault and A. Riazuelo and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and M. Rowan-Robinson and B. Rusholme and R. Saha and D. Santos and G. Savini and Schaefer, {B. M.} and P. Shellard and L. Spencer and J.-L. Starck and V. Stolyarov and R. Stompor and R. Sudiwala and R. Sunyaev and D. Sutton and J.-F. Sygnet and Tauber, {J. A.} and C. Thum and J.-P. Torre and F. Touze and M. Tristram and {van Leeuwen}, F. and L. Vibert and D. Vibert and Wade, {L. A.} and Wandelt, {B. D.} and White, {S. D. M.} and H. Wiesemeyer and A. Woodcraft and V. Yurchenko and D. Yvon and A. Zacchei",

year = "2011",

month = dec,

day = "1",

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

language = "English",

volume = "536",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Planck HFI Core Team, NV, 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, J-P, Bersanelli, M, Bock, JJ, Bond, JR, Borrill, J, Bouchet, FR, 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, DL, Colley, J-M, Colombi, S, Couchot, F, Coulais, A, Cressiot, C, Crill, BP, 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, 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, J-M, 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, J-B, Mercier, C, Mitra, S, Miville-Deschênes, M-A, Moneti, A, Montier, L, Mortlock, D, Murphy, A, Nati, F, Netterfield, CB, Nørgaard-Nielsen, HU, North, C, Noviello, F, Novikov, D, Osborne, S, Pajot, F, Patanchon, G, Peacocke, T, Pearson, TJ, Perdereau, O, Perotto, L, Piacentini, F, Piat, M, Plaszczynski, S, Pointecouteau, E, Ponthieu, N, Prézeau, G, Prunet, S, Puget, J-L, Reach, WT, Remazeilles, M, Renault, C, Riazuelo, A, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan-Robinson, M, Rusholme, B, Saha, R, Santos, D, Savini, G, Schaefer, BM, Shellard, P, Spencer, L, Starck, J-L, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Sutton, D, Sygnet, J-F, Tauber, JA, Thum, C, Torre, J-P, Touze, F, Tristram, M, van Leeuwen, F, Vibert, L, Vibert, D, Wade, LA, Wandelt, BD, White, SDM, Wiesemeyer, H, Woodcraft, A, Yurchenko, V, Yvon, D & Zacchei, A 2011, 'Planck early results. VI. The High Frequency Instrument data processing', Astronomy & Astrophysics, vol. 536, A6. https://doi.org/10.1051/0004-6361/201116462

TY - JOUR

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

AU - Planck HFI Core Team, [No Value]

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.

AU - Miville-Deschênes, M.-A.

AU - Moneti, A.

AU - Montier, L.

AU - Mortlock, D.

AU - Murphy, A.

AU - Nati, F.

AU - Netterfield, C. B.

AU - Nørgaard-Nielsen, H. U.

AU - North, C.

AU - Noviello, F.

AU - Novikov, D.

AU - Osborne, S.

AU - Pajot, F.

AU - Patanchon, G.

AU - Peacocke, T.

AU - Pearson, T. J.

AU - Perdereau, O.

AU - Perotto, L.

AU - Piacentini, F.

AU - Piat, M.

AU - Plaszczynski, S.

AU - Pointecouteau, E.

AU - Ponthieu, N.

AU - Prézeau, G.

AU - Prunet, S.

AU - Puget, J.-L.

AU - Reach, W. T.

AU - Remazeilles, M.

AU - Renault, C.

AU - Riazuelo, A.

AU - Ristorcelli, I.

AU - Rocha, G.

AU - Rosset, C.

AU - Roudier, G.

AU - Rowan-Robinson, M.

AU - Rusholme, B.

AU - Saha, R.

AU - Santos, D.

AU - Savini, G.

AU - Schaefer, B. M.

AU - Shellard, P.

AU - Spencer, L.

AU - Starck, J.-L.

AU - Stolyarov, V.

AU - Stompor, R.

AU - Sudiwala, R.

AU - Sunyaev, R.

AU - Sutton, D.

AU - Sygnet, J.-F.

AU - Tauber, J. A.

AU - Thum, C.

AU - Torre, J.-P.

AU - Touze, F.

AU - Tristram, M.

AU - van Leeuwen, F.

AU - Vibert, L.

AU - Vibert, D.

AU - Wade, L. A.

AU - Wandelt, B. D.

AU - White, S. D. M.

AU - Wiesemeyer, H.

AU - Woodcraft, A.

AU - Yurchenko, V.

AU - Yvon, D.

AU - Zacchei, A.

PY - 2011/12/1

Y1 - 2011/12/1

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. Corresponding author: F. R. Bouchet, e-mail: [email protected]

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. Corresponding author: F. R. Bouchet, e-mail: [email protected]

UR - http://www.scopus.com/inward/record.url?scp=82955187932&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201116462

DO - 10.1051/0004-6361/201116462

M3 - Article

SN - 0004-6361

VL - 536

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A6

ER -

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

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