Planck 2013 results. III. LFI systematic uncertainties

N. Aghanim; C. Armitage-Caplan; M. Arnaud; M. Ashdown; F. Atrio-Barandela; J. Aumont; C. Baccigalupi; A. J. Banday; R. B. Barreiro; E. Battaner; K. Benabed; A. Benoît; A. Benoit-Lévy; J. -P. Bernard; M. Bersanelli; P. Bielewicz; J. Bobin; Jacob Bock; A. Bonaldi; L. Bonavera; J. R. Bond; J. Borrill; F. R. Bouchet; M. Bridges; M. Bucher; C. Burigana; Robb Butler; J. -F. Cardoso; A. Catalano; A. Chamballu; Lung-Yih Chiang; P. R. Christensen; S. Church; S. Colombi; L. P. L. Colombo; B. P. Crill; M. Cruz; A. Curto; F. Cuttaia; L. Danese; R. D. Davies; Rebecca Davis; P. de Bernardis; A. de Rosa; G. de Zotti; J. Delabrouille; J. Dick; C. Dickinson; J. M. Diego; H. Dole; S. Donzelli; O. Doré; M. Douspis; X. Dupac; G. Efstathiou; T. A. Enßlin; H. K. Eriksen; F. Finelli; O. Forni; M. Frailis; E. Franceschi; T. C. Gaier; S. Galeotta; K. Ganga; M. Giard; Y. Giraud-Héraud; E. Gjerløw; J. González-Nuevo; K. M. Górski; S. Gratton; A. Gregorio; A. Gruppuso; F. K. Hansen; D. Hanson; D. Harrison; S. Henrot-Versillé; C. Hernández-Monteagudo; D. Herranz; Steen Hildebrandt; E. Hivon; M. Hobson; W. A. Holmes; Allan Hornstrup; W. Hovest; K. M. Huffenberger; T. R. Jaffe; A. H. Jaffe; J. Jewell; W. C. Jones; M. Juvela; P. Kangaslahti; E. Keihänen; R. Keskitalo; K. Kiiveri; T. S. Kisner; J. Knoche; L. Knox; M. Kunz; H. Kurki-Suonio; G. Lagache; A. Lähteenmäki; J. -M. Lamarre; A. Lasenby; R. J. Laureijs; C. R. Lawrence; J. P. Leahy; R. Leonardi; J. Lesgourgues; M. Liguori; P. B. Lilje; V. Lindholm; Michael Linden-Vørnle; M. López-Caniego; P. M. Lubin; J. F. Macías-Pérez; D. Maino; N. Mandolesi; M. Maris; D. J. Marshall; P. G. Martin; E. Martínez-González; S. Masi; S. Matarrese; F. Matthai; P. Mazzotta; P. R. Meinhold; A. Melchiorri; L. Mendes; A. Mennella; M. Migliaccio; S. Mitra; A. Moneti; L. Montier; G. Morgante; D. Mortlock; A. Moss; D. Munshi; P. Naselsky; P. Natoli; C. B. Netterfield; Hans Ulrik Nørgaard-Nielsen; D. Novikov; Igor Dmitrievich Novikov; I. J. O'Dwyer; S. Osborne; F. Paci; L. Pagano; R. Paladini; D. Paoletti; B. Partridge; F. Pasian; G. Patanchon; D. Pearson; M. Peel; O. Perdereau; L. Perotto; F. Perrotta; E. Pierpaoli; D. Pietrobon; S. Plaszczynski; P. Platania; E. Pointecouteau; G. Polenta; N. Ponthieu; L. Popa; T. Poutanen; G. W. Pratt; G. Prézeau; S. Prunet; J. -L. Puget; J. P. Rachen; R. Rebolo; M. Reinecke; M. Remazeilles; S. Ricciardi; T. Riller; G. Rocha; C. Rosset; M. Rossetti; G. Roudier; J. A. Rubiño-Martín; B. Rusholme; M. Sandri; D. Santos; D. Scott; M. D. Seiffert; E. P. S. Shellard; L. D. Spencer; J. -L. Starck; V. Stolyarov; R. Stompor; F. Sureau; D. Sutton; A. -S. Suur-Uski; J. -F. Sygnet; J. A. Tauber; D. Tavagnacco; L. Terenzi; L. Toffolatti; M. Tomasi; M. Tristram; M. Tucci; J. Tuovinen; M. Türler; G. Umana; L. Valenziano; J. Valiviita; B. Van Tent; J. Varis; P. Vielva; Frank Villa; N. Vittorio; L. A. Wade; B. D. Wandelt; R. Watson; A. Wilkinson; D. Yvon; A. Zacchei; A. Zonca

doi:10.1051/0004-6361/201321574

Planck 2013 results. III. LFI systematic uncertainties

N. Aghanim, C. Armitage-Caplan, M. Arnaud, M. Ashdown, F. Atrio-Barandela, J. Aumont, C. Baccigalupi, A. J. Banday, R. B. Barreiro, E. Battaner, K. Benabed, A. Benoît, A. Benoit-Lévy, J. -P. Bernard, M. Bersanelli, P. Bielewicz, J. Bobin, Jacob Bock, A. Bonaldi, L. BonaveraJ. R. Bond, J. Borrill, F. R. Bouchet, M. Bridges, M. Bucher, C. Burigana, Robb Butler, J. -F. Cardoso, A. Catalano, A. Chamballu, Lung-Yih Chiang, P. R. Christensen, S. Church, S. Colombi, L. P. L. Colombo, B. P. Crill, M. Cruz, A. Curto, F. Cuttaia, L. Danese, R. D. Davies, Rebecca Davis, P. de Bernardis, A. de Rosa, G. de Zotti, J. Delabrouille, J. Dick, C. Dickinson, J. M. Diego, H. Dole, S. Donzelli, O. Doré, M. Douspis, X. Dupac, G. Efstathiou, T. A. Enßlin, H. K. Eriksen, F. Finelli, O. Forni, M. Frailis, E. Franceschi, T. C. Gaier, S. Galeotta, K. Ganga, M. Giard, Y. Giraud-Héraud, E. Gjerløw, J. González-Nuevo, K. M. Górski, S. Gratton, A. Gregorio, A. Gruppuso, F. K. Hansen, D. Hanson, D. Harrison, S. Henrot-Versillé, C. Hernández-Monteagudo, D. Herranz, Steen Hildebrandt, E. Hivon, M. Hobson, W. A. Holmes, Allan Hornstrup, W. Hovest, K. M. Huffenberger, T. R. Jaffe, A. H. Jaffe, J. Jewell, W. C. Jones, M. Juvela, P. Kangaslahti, E. Keihänen, R. Keskitalo, K. Kiiveri, T. S. Kisner, J. Knoche, L. Knox, M. Kunz, H. Kurki-Suonio, G. Lagache, A. Lähteenmäki, J. -M. Lamarre, A. Lasenby, R. J. Laureijs, C. R. Lawrence, J. P. Leahy, R. Leonardi, J. Lesgourgues, M. Liguori, P. B. Lilje, V. Lindholm, Michael Linden-Vørnle, M. López-Caniego, P. M. Lubin, J. F. Macías-Pérez, D. Maino, N. Mandolesi, M. Maris, D. J. Marshall, P. G. Martin, E. Martínez-González, S. Masi, S. Matarrese, F. Matthai, P. Mazzotta, P. R. Meinhold, A. Melchiorri, L. Mendes, A. Mennella, M. Migliaccio, S. Mitra, A. Moneti, L. Montier, G. Morgante, D. Mortlock, A. Moss, D. Munshi, P. Naselsky, P. Natoli, C. B. Netterfield, Hans Ulrik Nørgaard-Nielsen, D. Novikov, Igor Dmitrievich Novikov, I. J. O'Dwyer, S. Osborne, F. Paci, L. Pagano, R. Paladini, D. Paoletti, B. Partridge, F. Pasian, G. Patanchon, D. Pearson, M. Peel, O. Perdereau, L. Perotto, F. Perrotta, E. Pierpaoli, D. Pietrobon, S. Plaszczynski, P. Platania, E. Pointecouteau, G. Polenta, N. Ponthieu, L. Popa, T. Poutanen, G. W. Pratt, G. Prézeau, S. Prunet, J. -L. Puget, J. P. Rachen, R. Rebolo, M. Reinecke, M. Remazeilles, S. Ricciardi, T. Riller, G. Rocha, C. Rosset, M. Rossetti, G. Roudier, J. A. Rubiño-Martín, B. Rusholme, M. Sandri, D. Santos, D. Scott, M. D. Seiffert, E. P. S. Shellard, L. D. Spencer, J. -L. Starck, V. Stolyarov, R. Stompor, F. Sureau, D. Sutton, A. -S. Suur-Uski, J. -F. Sygnet, J. A. Tauber, D. Tavagnacco, L. Terenzi, L. Toffolatti, M. Tomasi, M. Tristram, M. Tucci, J. Tuovinen, M. Türler, G. Umana, L. Valenziano, J. Valiviita, B. Van Tent, J. Varis, P. Vielva, Frank Villa, N. Vittorio, L. A. Wade, B. D. Wandelt, R. Watson, A. Wilkinson, D. Yvon, A. Zacchei, A. Zonca

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Abstract

We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the firstrelease of the Planck cosmological results.We give an overview of the main effects and of the tools and methods applied to assess residuals in mapsand power spectra.We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-upand imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave backgroundfluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipolerange ∫ < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reducethe level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibrationuncertainties.

Original language	English
Article number	A3
Journal	Astronomy and Astrophysics
Volume	571
Number of pages	23
ISSN	0004-6361
DOIs	https://doi.org/10.1051/0004-6361/201321574
Publication status	Published - 2013

Keywords

Cosmic background radiation
Cosmology: observations
Methods: data analysis

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10.1051/0004-6361/201321574

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Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. .-P., Bersanelli, M., Bielewicz, P., Bobin, J., Bock, J., Bonaldi, A., ... Zonca, A. (2013). Planck 2013 results. III. LFI systematic uncertainties. Astronomy and Astrophysics, 571, Article A3. https://doi.org/10.1051/0004-6361/201321574

@article{4013cf45777944c590a2e7e1f89bcae5,

title = "Planck 2013 results. III. LFI systematic uncertainties",

abstract = "We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the firstrelease of the Planck cosmological results.We give an overview of the main effects and of the tools and methods applied to assess residuals in mapsand power spectra.We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-upand imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave backgroundfluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipolerange ∫ < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reducethe level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibrationuncertainties.",

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

author = "N. Aghanim and C. Armitage-Caplan and M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and Banday, {A. J.} and Barreiro, {R. B.} and E. Battaner and K. Benabed and A. Beno{\^i}t and A. Benoit-L{\'e}vy and Bernard, {J. -P.} and M. Bersanelli and P. Bielewicz and J. Bobin and Jacob Bock and A. Bonaldi and L. Bonavera and Bond, {J. R.} and J. Borrill and Bouchet, {F. R.} and M. Bridges and M. Bucher and C. Burigana and Robb Butler and Cardoso, {J. -F.} and A. Catalano and A. Chamballu and Lung-Yih Chiang and Christensen, {P. R.} and S. Church and S. Colombi and Colombo, {L. P. L.} and Crill, {B. P.} and M. Cruz and A. Curto and F. Cuttaia and L. Danese and Davies, {R. D.} and Rebecca Davis and {de Bernardis}, P. and {de Rosa}, A. and {de Zotti}, G. and J. Delabrouille and J. Dick and C. Dickinson and Diego, {J. M.} and H. Dole and S. Donzelli and O. Dor{\'e} and M. Douspis and X. Dupac and G. Efstathiou and En{\ss}lin, {T. A.} and Eriksen, {H. K.} and F. Finelli and O. Forni and M. Frailis and E. Franceschi and Gaier, {T. C.} and S. Galeotta and K. Ganga and M. Giard and Y. Giraud-H{\'e}raud and E. Gjerl{\o}w and J. Gonz{\'a}lez-Nuevo and G{\'o}rski, {K. M.} and S. Gratton and A. Gregorio and A. Gruppuso and Hansen, {F. K.} and D. Hanson and D. Harrison and S. Henrot-Versill{\'e} and C. Hern{\'a}ndez-Monteagudo and D. Herranz and Steen Hildebrandt and E. Hivon and M. Hobson and Holmes, {W. A.} and Allan Hornstrup and W. Hovest and Huffenberger, {K. M.} and Jaffe, {T. R.} and Jaffe, {A. H.} and J. Jewell and Jones, {W. C.} and M. Juvela and P. Kangaslahti and E. Keih{\"a}nen and R. Keskitalo and K. Kiiveri and Kisner, {T. S.} and J. Knoche and L. Knox and M. Kunz and H. Kurki-Suonio and G. Lagache and A. L{\"a}hteenm{\"a}ki and Lamarre, {J. -M.} and A. Lasenby and Laureijs, {R. J.} and Lawrence, {C. R.} and Leahy, {J. P.} and R. Leonardi and J. Lesgourgues and M. Liguori and Lilje, {P. B.} and V. Lindholm and Michael Linden-V{\o}rnle and M. L{\'o}pez-Caniego and Lubin, {P. M.} and Mac{\'i}as-P{\'e}rez, {J. F.} and D. Maino and N. Mandolesi and M. Maris and Marshall, {D. J.} and Martin, {P. G.} and E. Mart{\'i}nez-Gonz{\'a}lez and S. Masi and S. Matarrese and F. Matthai and P. Mazzotta and Meinhold, {P. R.} and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and A. Moneti and L. Montier and G. Morgante and D. Mortlock and A. Moss and D. Munshi and P. Naselsky and P. Natoli and Netterfield, {C. B.} and N{\o}rgaard-Nielsen, {Hans Ulrik} and D. Novikov and Novikov, {Igor Dmitrievich} and O'Dwyer, {I. J.} and S. Osborne and F. Paci and L. Pagano and R. Paladini and D. Paoletti and B. Partridge and F. Pasian and G. Patanchon and D. Pearson and M. Peel and O. Perdereau and L. Perotto and F. Perrotta and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and P. Platania and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and T. Poutanen and Pratt, {G. W.} and G. Pr{\'e}zeau and S. Prunet and Puget, {J. -L.} and Rachen, {J. P.} and R. Rebolo and M. Reinecke and M. Remazeilles and S. Ricciardi and T. Riller and G. Rocha and C. Rosset and M. Rossetti and G. Roudier and Rubi{\~n}o-Mart{\'i}n, {J. A.} and B. Rusholme and M. Sandri and D. Santos and D. Scott and Seiffert, {M. D.} and Shellard, {E. P. S.} and Spencer, {L. D.} and Starck, {J. -L.} and V. Stolyarov and R. Stompor and F. Sureau and D. Sutton and Suur-Uski, {A. -S.} and Sygnet, {J. -F.} and Tauber, {J. A.} and D. Tavagnacco and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and J. Tuovinen and M. T{\"u}rler and G. Umana and L. Valenziano and J. Valiviita and {Van Tent}, B. and J. Varis and P. Vielva and Frank Villa and N. Vittorio and Wade, {L. A.} and Wandelt, {B. D.} and R. Watson and A. Wilkinson and D. Yvon and A. Zacchei and A. Zonca",

year = "2013",

doi = "10.1051/0004-6361/201321574",

language = "English",

volume = "571",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Aghanim, N, Armitage-Caplan, C, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Battaner, E, Benabed, K, Benoît, A, Benoit-Lévy, A, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bobin, J, Bock, J, Bonaldi, A, Bonavera, L, Bond, JR, Borrill, J, Bouchet, FR, Bridges, M, Bucher, M, Burigana, C, Butler, R, Cardoso, J-F, Catalano, A, Chamballu, A, Chiang, L-Y, Christensen, PR, Church, S, Colombi, S, Colombo, LPL, Crill, BP, Cruz, M, Curto, A, Cuttaia, F, Danese, L, Davies, RD, Davis, R, de Bernardis, P, de Rosa, A, de Zotti, G, Delabrouille, J, Dick, J, Dickinson, C, Diego, JM, Dole, H, Donzelli, S, Doré, O, Douspis, M, Dupac, X, Efstathiou, G, Enßlin, TA, Eriksen, HK, Finelli, F, Forni, O, Frailis, M, Franceschi, E, Gaier, TC, Galeotta, S, Ganga, K, Giard, M, Giraud-Héraud, Y, Gjerløw, E, González-Nuevo, J, Górski, KM, Gratton, S, Gregorio, A, Gruppuso, A, Hansen, FK, Hanson, D, Harrison, D, Henrot-Versillé, S, Hernández-Monteagudo, C, Herranz, D, Hildebrandt, S, Hivon, E, Hobson, M, Holmes, WA, Hornstrup, A, Hovest, W, Huffenberger, KM, Jaffe, TR, Jaffe, AH, Jewell, J, Jones, WC, Juvela, M, Kangaslahti, P, Keihänen, E, Keskitalo, R, Kiiveri, K, Kisner, TS, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lagache, G, Lähteenmäki, A, Lamarre, J-M, Lasenby, A, Laureijs, RJ, Lawrence, CR, Leahy, JP, Leonardi, R, Lesgourgues, J, Liguori, M, Lilje, PB, Lindholm, V, Linden-Vørnle, M, López-Caniego, M, Lubin, PM, Macías-Pérez, JF, Maino, D, Mandolesi, N, Maris, M, Marshall, DJ, Martin, PG, Martínez-González, E, Masi, S, Matarrese, S, Matthai, F, Mazzotta, P, Meinhold, PR, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Mitra, S, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Moss, A, Munshi, D, Naselsky, P, Natoli, P, Netterfield, CB, Nørgaard-Nielsen, HU, Novikov, D, Novikov, ID, O'Dwyer, IJ, Osborne, S, Paci, F, Pagano, L, Paladini, R, Paoletti, D, Partridge, B, Pasian, F, Patanchon, G, Pearson, D, Peel, M, Perdereau, O, Perotto, L, Perrotta, F, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Platania, P, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, GW, Prézeau, G, Prunet, S, Puget, J-L, Rachen, JP, Rebolo, R, Reinecke, M, Remazeilles, M, Ricciardi, S, Riller, T, Rocha, G, Rosset, C, Rossetti, M, Roudier, G, Rubiño-Martín, JA, Rusholme, B, Sandri, M, Santos, D, Scott, D, Seiffert, MD, Shellard, EPS, Spencer, LD, Starck, J-L, Stolyarov, V, Stompor, R, Sureau, F, Sutton, D, Suur-Uski, A-S, Sygnet, J-F, Tauber, JA, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Tuovinen, J, Türler, M, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Varis, J, Vielva, P, Villa, F, Vittorio, N, Wade, LA, Wandelt, BD, Watson, R, Wilkinson, A, Yvon, D, Zacchei, A & Zonca, A 2013, 'Planck 2013 results. III. LFI systematic uncertainties', Astronomy and Astrophysics, vol. 571, A3. https://doi.org/10.1051/0004-6361/201321574

TY - JOUR

T1 - Planck 2013 results. III. LFI systematic uncertainties

AU - Aghanim, N.

AU - Armitage-Caplan, C.

AU - Arnaud, M.

AU - Ashdown, M.

AU - Atrio-Barandela, F.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Battaner, E.

AU - Benabed, K.

AU - Benoît, A.

AU - Benoit-Lévy, A.

AU - Bernard, J. -P.

AU - Bersanelli, M.

AU - Bielewicz, P.

AU - Bobin, J.

AU - Bock, Jacob

AU - Bonaldi, A.

AU - Bonavera, L.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Bridges, M.

AU - Bucher, M.

AU - Burigana, C.

AU - Butler, Robb

AU - Cardoso, J. -F.

AU - Catalano, A.

AU - Chamballu, A.

AU - Chiang, Lung-Yih

AU - Christensen, P. R.

AU - Church, S.

AU - Colombi, S.

AU - Colombo, L. P. L.

AU - Crill, B. P.

AU - Cruz, M.

AU - Curto, A.

AU - Cuttaia, F.

AU - Danese, L.

AU - Davies, R. D.

AU - Davis, Rebecca

AU - de Bernardis, P.

AU - de Rosa, A.

AU - de Zotti, G.

AU - Delabrouille, J.

AU - Dick, J.

AU - Dickinson, C.

AU - Diego, J. M.

AU - Dole, H.

AU - Donzelli, S.

AU - Doré, O.

AU - Douspis, M.

AU - Dupac, X.

AU - Efstathiou, G.

AU - Enßlin, T. A.

AU - Eriksen, H. K.

AU - Finelli, F.

AU - Forni, O.

AU - Frailis, M.

AU - Franceschi, E.

AU - Gaier, T. C.

AU - Galeotta, S.

AU - Ganga, K.

AU - Giard, M.

AU - Giraud-Héraud, Y.

AU - Gjerløw, E.

AU - González-Nuevo, J.

AU - Górski, K. M.

AU - Gratton, S.

AU - Gregorio, A.

AU - Gruppuso, A.

AU - Hansen, F. K.

AU - Hanson, D.

AU - Harrison, D.

AU - Henrot-Versillé, S.

AU - Hernández-Monteagudo, C.

AU - Herranz, D.

AU - Hildebrandt, Steen

AU - Hivon, E.

AU - Hobson, M.

AU - Holmes, W. A.

AU - Hornstrup, Allan

AU - Hovest, W.

AU - Huffenberger, K. M.

AU - Jaffe, T. R.

AU - Jaffe, A. H.

AU - Jewell, J.

AU - Jones, W. C.

AU - Juvela, M.

AU - Kangaslahti, P.

AU - Keihänen, E.

AU - Keskitalo, R.

AU - Kiiveri, K.

AU - Kisner, T. S.

AU - Knoche, J.

AU - Knox, L.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lagache, G.

AU - Lähteenmäki, A.

AU - Lamarre, J. -M.

AU - Lasenby, A.

AU - Laureijs, R. J.

AU - Lawrence, C. R.

AU - Leahy, J. P.

AU - Leonardi, R.

AU - Lesgourgues, J.

AU - Liguori, M.

AU - Lilje, P. B.

AU - Lindholm, V.

AU - Linden-Vørnle, Michael

AU - López-Caniego, M.

AU - Lubin, P. M.

AU - Macías-Pérez, J. F.

AU - Maino, D.

AU - Mandolesi, N.

AU - Maris, M.

AU - Marshall, D. J.

AU - Martin, P. G.

AU - Martínez-González, E.

AU - Masi, S.

AU - Matarrese, S.

AU - Matthai, F.

AU - Mazzotta, P.

AU - Meinhold, P. R.

AU - Melchiorri, A.

AU - Mendes, L.

AU - Mennella, A.

AU - Migliaccio, M.

AU - Mitra, S.

AU - Moneti, A.

AU - Montier, L.

AU - Morgante, G.

AU - Mortlock, D.

AU - Moss, A.

AU - Munshi, D.

AU - Naselsky, P.

AU - Natoli, P.

AU - Netterfield, C. B.

AU - Nørgaard-Nielsen, Hans Ulrik

AU - Novikov, D.

AU - Novikov, Igor Dmitrievich

AU - O'Dwyer, I. J.

AU - Osborne, S.

AU - Paci, F.

AU - Pagano, L.

AU - Paladini, R.

AU - Paoletti, D.

AU - Partridge, B.

AU - Pasian, F.

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PY - 2013

Y1 - 2013

N2 - We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the firstrelease of the Planck cosmological results.We give an overview of the main effects and of the tools and methods applied to assess residuals in mapsand power spectra.We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-upand imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave backgroundfluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipolerange ∫ < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reducethe level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibrationuncertainties.

AB - We present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the firstrelease of the Planck cosmological results.We give an overview of the main effects and of the tools and methods applied to assess residuals in mapsand power spectra.We also present an overall budget of known systematic effect uncertainties, which are dominated by sidelobe straylight pick-upand imperfect calibration. However, even these two effects are at least two orders of magnitude weaker than the cosmic microwave backgroundfluctuations as measured in terms of the angular temperature power spectrum. A residual signal above the noise level is present in the multipolerange ∫ < 20, most notably at 30GHz, and is probably caused by residual Galactic straylight contamination. Current analysis aims to further reducethe level of spurious signals in the data and to improve the systematic effects modelling, in particular with respect to straylight and calibrationuncertainties.

KW - Cosmic background radiation

KW - Cosmology: observations

KW - Methods: data analysis

U2 - 10.1051/0004-6361/201321574

DO - 10.1051/0004-6361/201321574

M3 - Journal article

SN - 0004-6361

VL - 571

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A3

ER -

Planck 2013 results. III. LFI systematic uncertainties

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