Planck early results: V. The Low Frequency Instrument data processing

A. Zacchei; D. Maino; C. Baccigalupi; M. Bersanelli; A. Bonaldi; L. Bonavera; C. Burigana; R.C. Butler; F. Cuttaia; G. de Zotti; J. Dick; M. Frailis; S. Galeotta; J. González-Nuevo; K.M. Górski; A. Gregorio; E. Keihänen; R. Keskitalo; J. Knoche; H. Kurki-Suonio; C.R. Lawrence; S. Leach; J.P. Leahy; M. López-Caniego; N. Mandolesi; M. Maris; F. Matthai; P.R. Meinhold; A. Mennella; G. Morgante; N. Morisset; P. Natoli; F. Pasian; F. Perrotta; G. Polenta; T. Poutanen; M. Reinecke; S. Ricciardi; R. Rohlfs; M. Sandri; A. -S. Suur-Uski; J.A. Tauber; D. Tavagnacco; L. Terenzi; M. Tomasi; J. Valiviita; F. Villa; A. Zonca; A.J. Banday; R.B. Barreiro; J.G. Bartlett; N. Bartolo; L. Bedini; K. Bennett; P. Binko; J. Borrill; F.R. Bouchet; M. Bremer; P. Cabella; B. Cappellini; X. Chen; L. Colombo; M. Cruz; A. Curto; L. Danese; R.D. Davies; R.J. Davis; G. de Gasperis; A. de Rosa; G. de Troia; C. Dickinson; J.M. Diego; S. Donzelli; U. Dörl; G. Efstathiou; T.A. En\sslin; H.K. Eriksen; M.C. Falvella; F. Finelli; E. Franceschi; T.C. Gaier; F. Gasparo; R.T. Génova-Santos; G. Giardino; F. Gómez; A. Gruppuso; F.K. Hansen; R. Hell; D. Herranz; W. Hovest; J. Jewell; M. Juvela; T.S. Kisner; L. Knox; A. Lähteenmäki; J. -M. Lamarre; R. Leonardi; J. León-Tavares; P.B. Lilje; P.M. Lubin; G. Maggio; D. Marinucci; E. Martínez-González; M. Massardi; S. Matarrese; M.T. Meharga; A. Melchiorri; M. Migliaccio; S. Mitra; A. Moss; H.U. N\orgaard-Nielsen; L. Pagano; R. Paladini; D. Paoletti; B. Partridge; D. Pearson; V. Pettorino; D. Pietrobon; G. Prézeau; P. Procopio; J. -L. Puget; C. Quercellini; J.P. Rachen; R. Rebolo; G. Robbers; G. Rocha; J.A. Rubi\no-Martín; E. Salerno; M. Savelainen; D. Scott; M.D. Seiffert; J.I. Silk; G.F. Smoot; J. Sternberg; F. Stivoli; R. Stompor; G. Tofani; J. Tuovinen; M. Türler; G. Umana; P. Vielva; N. Vittorio; C. Vuerli; L.A. Wade; R. Watson; S.D.M. White; A. Wilkinson

Planck early results: V. The Low Frequency Instrument data processing

A. Zacchei, D. Maino, C. Baccigalupi, M. Bersanelli, A. Bonaldi, L. Bonavera, C. Burigana, R.C. Butler, F. Cuttaia, G. de Zotti, J. Dick, M. Frailis, S. Galeotta, J. González-Nuevo, K.M. Górski, A. Gregorio, E. Keihänen, R. Keskitalo, J. Knoche, H. Kurki-SuonioC.R. Lawrence, S. Leach, J.P. Leahy, M. López-Caniego, N. Mandolesi, M. Maris, F. Matthai, P.R. Meinhold, A. Mennella, G. Morgante, N. Morisset, P. Natoli, F. Pasian, F. Perrotta, G. Polenta, T. Poutanen, M. Reinecke, S. Ricciardi, R. Rohlfs, M. Sandri, A. -S. Suur-Uski, J.A. Tauber, D. Tavagnacco, L. Terenzi, M. Tomasi, J. Valiviita, F. Villa, A. Zonca, A.J. Banday, R.B. Barreiro, J.G. Bartlett, N. Bartolo, L. Bedini, K. Bennett, P. Binko, J. Borrill, F.R. Bouchet, M. Bremer, P. Cabella, B. Cappellini, X. Chen, L. Colombo, M. Cruz, A. Curto, L. Danese, R.D. Davies, R.J. Davis, G. de Gasperis, A. de Rosa, G. de Troia, C. Dickinson, J.M. Diego, S. Donzelli, U. Dörl, G. Efstathiou, T.A. En\sslin, H.K. Eriksen, M.C. Falvella, F. Finelli, E. Franceschi, T.C. Gaier, F. Gasparo, R.T. Génova-Santos, G. Giardino, F. Gómez, A. Gruppuso, F.K. Hansen, R. Hell, D. Herranz, W. Hovest, J. Jewell, M. Juvela, T.S. Kisner, L. Knox, A. Lähteenmäki, J. -M. Lamarre, R. Leonardi, J. León-Tavares, P.B. Lilje, P.M. Lubin, G. Maggio, D. Marinucci, E. Martínez-González, M. Massardi, S. Matarrese, M.T. Meharga, A. Melchiorri, M. Migliaccio, S. Mitra, A. Moss, H.U. N\orgaard-Nielsen, L. Pagano, R. Paladini, D. Paoletti, B. Partridge, D. Pearson, V. Pettorino, D. Pietrobon, G. Prézeau, P. Procopio, J. -L. Puget, C. Quercellini, J.P. Rachen, R. Rebolo, G. Robbers, G. Rocha, J.A. Rubi\no-Martín, E. Salerno, M. Savelainen, D. Scott, M.D. Seiffert, J.I. Silk, G.F. Smoot, J. Sternberg, F. Stivoli, R. Stompor, G. Tofani, J. Tuovinen, M. Türler, G. Umana, P. Vielva, N. Vittorio, C. Vuerli, L.A. Wade, R. Watson, S.D.M. White, A. Wilkinson

University of Helsinki

Tutkimustuotos: Lehtiartikkeli › Article › Scientific › vertaisarvioitu

83 Sitaatiot (Scopus)

Abstrakti

We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discuss the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps. Data are continuously calibrated using the modulation of the temperature of the cosmic microwave background radiation induced by the motion of the spacecraft. Noise properties are estimated from TOD from which the sky signal has been removed using a generalized least square map-making algorithm. Measured 1/f noise knee-frequencies range from ~100 mHz at 30 GHz to a few tens of mHz at 70GHz. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices required to compute statistical uncertainties on LFI and Planck products are also produced. Main beams are estimated down to the ≈−10dB level using Jupiter transits, which are also used for geometrical calibration of the focal plane.

Alkuperäiskieli	Englanti
Artikkeli	A5
Sivumäärä	19
Julkaisu	Astronomy and Astrophysics
Vuosikerta	536
Tila	Julkaistu - 2011
OKM-julkaisutyyppi	A1 Alkuperäisartikkeli tieteellisessä aikakauslehdessä

Muut tiedostot ja linkit

http://arxiv.org/abs/1101.2040

Metsähovin radiotutkimusasema
Tammi, J. (Manager)
Sähkötekniikan korkeakoulu
Laitteistot/tilat: Facility

Siteeraa tätä

Zacchei, A., Maino, D., Baccigalupi, C., Bersanelli, M., Bonaldi, A., Bonavera, L., Burigana, C., Butler, R. C., Cuttaia, F., de Zotti, G., Dick, J., Frailis, M., Galeotta, S., González-Nuevo, J., Górski, K. M., Gregorio, A., Keihänen, E., Keskitalo, R., Knoche, J., ... Wilkinson, A. (2011). Planck early results: V. The Low Frequency Instrument data processing. Astronomy and Astrophysics, 536, Artikkeli A5.

@article{14e400ce724f48ba91c63ea3ed44fc9d,

title = "Planck early results: V. The Low Frequency Instrument data processing",

abstract = "We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discuss the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps. Data are continuously calibrated using the modulation of the temperature of the cosmic microwave background radiation induced by the motion of the spacecraft. Noise properties are estimated from TOD from which the sky signal has been removed using a generalized least square map-making algorithm. Measured 1/f noise knee-frequencies range from ~100 mHz at 30 GHz to a few tens of mHz at 70GHz. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices required to compute statistical uncertainties on LFI and Planck products are also produced. Main beams are estimated down to the ≈−10dB level using Jupiter transits, which are also used for geometrical calibration of the focal plane.",

keywords = "methods: data analysis, cosmic background radiation, cosmology: observations, surveys",

author = "A. Zacchei and D. Maino and C. Baccigalupi and M. Bersanelli and A. Bonaldi and L. Bonavera and C. Burigana and R.C. Butler and F. Cuttaia and {de Zotti}, G. and J. Dick and M. Frailis and S. Galeotta and J. Gonz{\'a}lez-Nuevo and K.M. G{\'o}rski and A. Gregorio and E. Keih{\"a}nen and R. Keskitalo and J. Knoche and H. Kurki-Suonio and C.R. Lawrence and S. Leach and J.P. Leahy and M. L{\'o}pez-Caniego and N. Mandolesi and M. Maris and F. Matthai and P.R. Meinhold and A. Mennella and G. Morgante and N. Morisset and P. Natoli and F. Pasian and F. Perrotta and G. Polenta and T. Poutanen and M. Reinecke and S. Ricciardi and R. Rohlfs and M. Sandri and Suur-Uski, {A. -S.} and J.A. Tauber and D. Tavagnacco and L. Terenzi and M. Tomasi and J. Valiviita and F. Villa and A. Zonca and A.J. Banday and R.B. Barreiro and J.G. Bartlett and N. Bartolo and L. Bedini and K. Bennett and P. Binko and J. Borrill and F.R. Bouchet and M. Bremer and P. Cabella and B. Cappellini and X. Chen and L. Colombo and M. Cruz and A. Curto and L. Danese and R.D. Davies and R.J. Davis and {de Gasperis}, G. and {de Rosa}, A. and {de Troia}, G. and C. Dickinson and J.M. Diego and S. Donzelli and U. D{\"o}rl and G. Efstathiou and T.A. En\sslin and H.K. Eriksen and M.C. Falvella and F. Finelli and E. Franceschi and T.C. Gaier and F. Gasparo and R.T. G{\'e}nova-Santos and G. Giardino and F. G{\'o}mez and A. Gruppuso and F.K. Hansen and R. Hell and D. Herranz and W. Hovest and J. Jewell and M. Juvela and T.S. Kisner and L. Knox and A. L{\"a}hteenm{\"a}ki and Lamarre, {J. -M.} and R. Leonardi and J. Le{\'o}n-Tavares and P.B. Lilje and P.M. Lubin and G. Maggio and D. Marinucci and E. Mart{\'i}nez-Gonz{\'a}lez and M. Massardi and S. Matarrese and M.T. Meharga and A. Melchiorri and M. Migliaccio and S. Mitra and A. Moss and H.U. N\orgaard-Nielsen and L. Pagano and R. Paladini and D. Paoletti and B. Partridge and D. Pearson and V. Pettorino and D. Pietrobon and G. Pr{\'e}zeau and P. Procopio and Puget, {J. -L.} and C. Quercellini and J.P. Rachen and R. Rebolo and G. Robbers and G. Rocha and J.A. Rubi\no-Mart{\'i}n and E. Salerno and M. Savelainen and D. Scott and M.D. Seiffert and J.I. Silk and G.F. Smoot and J. Sternberg and F. Stivoli and R. Stompor and G. Tofani and J. Tuovinen and M. T{\"u}rler and G. Umana and P. Vielva and N. Vittorio and C. Vuerli and L.A. Wade and R. Watson and S.D.M. White and A. Wilkinson",

year = "2011",

language = "English",

volume = "536",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Zacchei, A, Maino, D, Baccigalupi, C, Bersanelli, M, Bonaldi, A, Bonavera, L, Burigana, C, Butler, RC, Cuttaia, F, de Zotti, G, Dick, J, Frailis, M, Galeotta, S, González-Nuevo, J, Górski, KM, Gregorio, A, Keihänen, E, Keskitalo, R, Knoche, J, Kurki-Suonio, H, Lawrence, CR, Leach, S, Leahy, JP, López-Caniego, M, Mandolesi, N, Maris, M, Matthai, F, Meinhold, PR, Mennella, A, Morgante, G, Morisset, N, Natoli, P, Pasian, F, Perrotta, F, Polenta, G, Poutanen, T, Reinecke, M, Ricciardi, S, Rohlfs, R, Sandri, M, Suur-Uski, A-S, Tauber, JA, Tavagnacco, D, Terenzi, L, Tomasi, M, Valiviita, J, Villa, F, Zonca, A, Banday, AJ, Barreiro, RB, Bartlett, JG, Bartolo, N, Bedini, L, Bennett, K, Binko, P, Borrill, J, Bouchet, FR, Bremer, M, Cabella, P, Cappellini, B, Chen, X, Colombo, L, Cruz, M, Curto, A, Danese, L, Davies, RD, Davis, RJ, de Gasperis, G, de Rosa, A, de Troia, G, Dickinson, C, Diego, JM, Donzelli, S, Dörl, U, Efstathiou, G, En\sslin, TA, Eriksen, HK, Falvella, MC, Finelli, F, Franceschi, E, Gaier, TC, Gasparo, F, Génova-Santos, RT, Giardino, G, Gómez, F, Gruppuso, A, Hansen, FK, Hell, R, Herranz, D, Hovest, W, Jewell, J, Juvela, M, Kisner, TS, Knox, L, Lähteenmäki, A, Lamarre, J-M, Leonardi, R, León-Tavares, J, Lilje, PB, Lubin, PM, Maggio, G, Marinucci, D, Martínez-González, E, Massardi, M, Matarrese, S, Meharga, MT, Melchiorri, A, Migliaccio, M, Mitra, S, Moss, A, N\orgaard-Nielsen, HU, Pagano, L, Paladini, R, Paoletti, D, Partridge, B, Pearson, D, Pettorino, V, Pietrobon, D, Prézeau, G, Procopio, P, Puget, J-L, Quercellini, C, Rachen, JP, Rebolo, R, Robbers, G, Rocha, G, Rubi\no-Martín, JA, Salerno, E, Savelainen, M, Scott, D, Seiffert, MD, Silk, JI, Smoot, GF, Sternberg, J, Stivoli, F, Stompor, R, Tofani, G, Tuovinen, J, Türler, M, Umana, G, Vielva, P, Vittorio, N, Vuerli, C, Wade, LA, Watson, R, White, SDM & Wilkinson, A 2011, 'Planck early results: V. The Low Frequency Instrument data processing', Astronomy and Astrophysics, Vuosikerta 536, A5.

TY - JOUR

T1 - Planck early results

T2 - V. The Low Frequency Instrument data processing

AU - Zacchei, A.

AU - Maino, D.

AU - Baccigalupi, C.

AU - Bersanelli, M.

AU - Bonaldi, A.

AU - Bonavera, L.

AU - Burigana, C.

AU - Butler, R.C.

AU - Cuttaia, F.

AU - de Zotti, G.

AU - Dick, J.

AU - Frailis, M.

AU - Galeotta, S.

AU - González-Nuevo, J.

AU - Górski, K.M.

AU - Gregorio, A.

AU - Keihänen, E.

AU - Keskitalo, R.

AU - Knoche, J.

AU - Kurki-Suonio, H.

AU - Lawrence, C.R.

AU - Leach, S.

AU - Leahy, J.P.

AU - López-Caniego, M.

AU - Mandolesi, N.

AU - Maris, M.

AU - Matthai, F.

AU - Meinhold, P.R.

AU - Mennella, A.

AU - Morgante, G.

AU - Morisset, N.

AU - Natoli, P.

AU - Pasian, F.

AU - Perrotta, F.

AU - Polenta, G.

AU - Poutanen, T.

AU - Reinecke, M.

AU - Ricciardi, S.

AU - Rohlfs, R.

AU - Sandri, M.

AU - Suur-Uski, A. -S.

AU - Tauber, J.A.

AU - Tavagnacco, D.

AU - Terenzi, L.

AU - Tomasi, M.

AU - Valiviita, J.

AU - Villa, F.

AU - Zonca, A.

AU - Banday, A.J.

AU - Barreiro, R.B.

AU - Bartlett, J.G.

AU - Bartolo, N.

AU - Bedini, L.

AU - Bennett, K.

AU - Binko, P.

AU - Borrill, J.

AU - Bouchet, F.R.

AU - Bremer, M.

AU - Cabella, P.

AU - Cappellini, B.

AU - Chen, X.

AU - Colombo, L.

AU - Cruz, M.

AU - Curto, A.

AU - Danese, L.

AU - Davies, R.D.

AU - Davis, R.J.

AU - de Gasperis, G.

AU - de Rosa, A.

AU - de Troia, G.

AU - Dickinson, C.

AU - Diego, J.M.

AU - Donzelli, S.

AU - Dörl, U.

AU - Efstathiou, G.

AU - En\sslin, T.A.

AU - Eriksen, H.K.

AU - Falvella, M.C.

AU - Finelli, F.

AU - Franceschi, E.

AU - Gaier, T.C.

AU - Gasparo, F.

AU - Génova-Santos, R.T.

AU - Giardino, G.

AU - Gómez, F.

AU - Gruppuso, A.

AU - Hansen, F.K.

AU - Hell, R.

AU - Herranz, D.

AU - Hovest, W.

AU - Jewell, J.

AU - Juvela, M.

AU - Kisner, T.S.

AU - Knox, L.

AU - Lähteenmäki, A.

AU - Lamarre, J. -M.

AU - Leonardi, R.

AU - León-Tavares, J.

AU - Lilje, P.B.

AU - Lubin, P.M.

AU - Maggio, G.

AU - Marinucci, D.

AU - Martínez-González, E.

AU - Massardi, M.

AU - Matarrese, S.

AU - Meharga, M.T.

AU - Melchiorri, A.

AU - Migliaccio, M.

AU - Mitra, S.

AU - Moss, A.

AU - N\orgaard-Nielsen, H.U.

AU - Pagano, L.

AU - Paladini, R.

AU - Paoletti, D.

AU - Partridge, B.

AU - Pearson, D.

AU - Pettorino, V.

AU - Pietrobon, D.

AU - Prézeau, G.

AU - Procopio, P.

AU - Puget, J. -L.

AU - Quercellini, C.

AU - Rachen, J.P.

AU - Rebolo, R.

AU - Robbers, G.

AU - Rocha, G.

AU - Rubi\no-Martín, J.A.

AU - Salerno, E.

AU - Savelainen, M.

AU - Scott, D.

AU - Seiffert, M.D.

AU - Silk, J.I.

AU - Smoot, G.F.

AU - Sternberg, J.

AU - Stivoli, F.

AU - Stompor, R.

AU - Tofani, G.

AU - Tuovinen, J.

AU - Türler, M.

AU - Umana, G.

AU - Vielva, P.

AU - Vittorio, N.

AU - Vuerli, C.

AU - Wade, L.A.

AU - Watson, R.

AU - White, S.D.M.

AU - Wilkinson, A.

PY - 2011

Y1 - 2011

N2 - We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discuss the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps. Data are continuously calibrated using the modulation of the temperature of the cosmic microwave background radiation induced by the motion of the spacecraft. Noise properties are estimated from TOD from which the sky signal has been removed using a generalized least square map-making algorithm. Measured 1/f noise knee-frequencies range from ~100 mHz at 30 GHz to a few tens of mHz at 70GHz. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices required to compute statistical uncertainties on LFI and Planck products are also produced. Main beams are estimated down to the ≈−10dB level using Jupiter transits, which are also used for geometrical calibration of the focal plane.

AB - We describe the processing of data from the Low Frequency Instrument (LFI) used in production of the Planck Early Release Compact Source Catalogue (ERCSC). In particular, we discuss the steps involved in reducing the data from telemetry packets to cleaned, calibrated, time-ordered data (TOD) and frequency maps. Data are continuously calibrated using the modulation of the temperature of the cosmic microwave background radiation induced by the motion of the spacecraft. Noise properties are estimated from TOD from which the sky signal has been removed using a generalized least square map-making algorithm. Measured 1/f noise knee-frequencies range from ~100 mHz at 30 GHz to a few tens of mHz at 70GHz. A destriping code (Madam) is employed to combine radiometric data and pointing information into sky maps, minimizing the variance of correlated noise. Noise covariance matrices required to compute statistical uncertainties on LFI and Planck products are also produced. Main beams are estimated down to the ≈−10dB level using Jupiter transits, which are also used for geometrical calibration of the focal plane.

KW - methods: data analysis

KW - cosmic background radiation

KW - cosmology: observations

KW - surveys

UR - http://arxiv.org/abs/1101.2040

M3 - Article

SN - 0004-6361

VL - 536

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A5

ER -

Planck early results: V. The Low Frequency Instrument data processing

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