J. A. Tauber et al.: <strong>Planck</strong> pre-launch status: The optical systemFig. B.1. (Left) Measureddependenceofthereflectionloss(1− R) ofasampleof<strong>Planck</strong> reflector material as a function of frequency, when thesample is at room temperature (296 K, upper curve), and at ∼110 K (lower curve). The solid lines are fits to the expected root-square dependenceon frequency and (temperature-dependent) resistivity. (Right) Dependenceofthereflectionlossofthesamesampleasafunctionoftemperature,for two frequencies: 340 GHz (diamonds) and 141 GHz (triangles). The solid line is a theoretical calculation of the reflectivity of pure aluminium,including the abnormal skin effect, which sets in at a temperature below ∼60 K. The dots are measurements of a 0.3 mm thick sheet of purealuminium.afactorof∼2 atthehighestfrequencies.However,athighfrequenciesdust will be a large, possibly dominant, element of theeffective emissivity of the reflectors; an in-flight contaminationlevel of 5000 ppm (see Sect. 6.3) leads in a worst case (large,black particles) to an emissivity of order 0.5%.Some reflectors made from CFRP have been shown to haveadifferent reflectivity (∼10%) along and across the direction ofthe carbon fibres; the <strong>Planck</strong> samples however have been verifiedto have no orientation dependence (Parshin & Klooster 2008).ReferencesAmiri Parian, J., Gruen, A., & Cozzani, A. 2006a, in 6th InternationalConference on Space Optics, ESTEC, Noordwijk, 27−30 JuneAmiri Parian, J., Gruen, A., & Cozzani, A. 2006b, in 3rd IAG Symposiumon Geodesy for Geothechnical and Structural Engineering, Baden, Austria,22−24 MayAmiri Parian, J., Riti, J. B., & Cozzani, A. 2007a, in 6th InternationalSymposium on Environmental Testing for Space Programmes, ESTEC,Noordwijk, 12−14 JuneAmiri Parian, J., Gruen, A., & Cozzani, A. 2007b, J. Appl. Geodesy, 1, 137Aumont, J., Conversi, L., Thum, C., et al. 2010, A&A, 514, A70Bersanelli, M., Bouchet, F. R., Efstathiou, G., et al. 1996, Report on the Phase AStudy of COBRAS/SAMBA, ESA Report D/SCI(96)3Bersanelli, M., Mandolesi, N., Butler, C. R., et al. 2010, A&A, 520, A4Burigana, C., Natoli, P., Vittorio, N., Mandolesi, N, & Bersanelli, M. 2001a,Experim. Astron., 12, 87Burigana, C., Maino, D., Górski, K. M., et al. 2001b, A&A, 373, 345Burigana, C., Sandri, M., Villa, F., et al. 2004, A&A, 428, 311Burigana, C., Gruppuso, A., & Finelli, F. 2006, MNRAS, 371, 1570De Maagt, P., Martín Polegre, A., & Crone, G. 2000, ESA doc. PT-TN-05967,Iss. 2, Dec. 2000Dubruel, D., Cornut, M., Fargant, G., et al. 2000, ESA Conf. Proc., SP-444Fargant, G., Dubruel, D., Cornut, M., et al. 2000, SPIE Proc., 4013, 69Fischer, J., Klaassen, T., Hovenier, N., et al. 2005, Appl. Opt., 43, 3765Forma, G., Dubruel, D., Martí-Canales, J., et al. 2008, Proc. of AMTA AnnualSymposium, Boston MA, Nov. 16−21, 99Franco, G., Fosalba, P., & Tauber, J. 2003, A&A, 405, 349GRASP9 manual 2008, TICRA, http://www.ticra.com/Hamaker, J. P., & Leahy, J. P. 2004, A study of CMB differencing polarimetrywith particular reference to <strong>Planck</strong>, ESAReportSCI-A/2003.312/JTHill, R. S., Weiland, J. L., Odegard, N., et al. 2009, ApJS, 180, 246Huffenberger, K. M., Crill, B. P., Lange, A. E., Górski, K. M., & Lawrence, C. R.2010, A&A, 510, A58Lamarre, J.-M., Puget, J.-L., Ade, P. A. R., et al. 2010, A&A, 520, A9Leahy, J. P., Bersanelli, M., D’Arcangelo, O., et al. 2010, A&A, 520, A8Macías-Pérez, J.-F., Mayet, F., Aumont, J., & Désert, F.-X. 2010, ApJ, 711, 417Maffei, B., Noviello, F., Murphy, J. A., et al. 2010, A&A, 520, A12Mandolesi, N., & Smoot, G. F. 1993, Proposal for COBRAS – the CosmicBackground Radiation Anisotropy Satellite, submitted to ESA in 2003 in answerto the M3 call for mission ideasNaselsky, P. D., Verkhodanov, O. V., Christensen, P. R., & Chiang, L.-Y. 2007,Astr. Bull., 62, 285Nielsen, P. H. 1999, TICRA Report S-801-04Nielsen, P. H. 2008, TICRA Report S-1287-01Nielsen, P. H. 2009, Ticra report S-1487-05Nolta, M. R., Dunkley, J., Hill, R. S., et al. 2009, ApJS, 180, 296Pagana, E. 1993, COBRAS Antenna Subsystem <strong>Pre</strong>limnary Study, TechnicalNote F.P.M. Space srl Nr. 009/V93/PGMPaquay, M., Martí-Canales, J., Rolo, L., et al. 2008, Proc. of AMTA annual symposium,Boston MA, Nov. 16−21, 32Parshin, V., & van der Klooster, C. 2008, 30th ESA Antenna WorkshopPuget, J.-L. 1993, Proposal for SAMBA – the Satellite for Measurements ofBackground Anisotropies, submitted to ESA in 2003 in answer to the M3call for mission ideasRocha, G., Pagano, L., Górski, K. M., et al. 2010, A&A, 513, A23Roose, S., Houbrechts, Y., Mazzoli, A., et al. 2005, in Proceedings of the2nd SPIE symposium on Advanced Optical Manufacturing and TestingTechnologies, Xian, Proc. SPIE, 6150Roose, S., Houbrechts, Y., Mazzoli, A., et al. 2006, in Proceedings of theInternational Conference SPECKLE06: Speckles, from grains to flowers,Nimes, France, Proc. SPIE, 6341Rosset, C., Tristram, M., Ponthieu, N., et al. 2010, A&A, 520, A13Sandri, M., Villa, F., Bersanelli, M., et al. 2010, A&A, 520, A7Stute, T. 2005, paper 105516 in 28th ESA Antenna WorkshopTauber, J. A., De Chambure, D., Crone, G.,etal.2005,inProceedingsoftheXXVIIIth General Assembly of URSI, New Delhi, IndiaTauber, J. A., Mandolesi, N., Puget, J.-L., et al. 2010, A&A, 520, A1Villa, F., Bersanelli, M., Burigana, C., et al. 2001, AIP Proceedings of theWorkshop on Experimental Cosmology at millimeter wavelengths, Cervinia,Italy, 9−13 JulyYurchenko, V. B., & Lamarre, J.-M. 2005, JOSA A, 22, 28381 European Space Agency (ESA), Research and Scientific SupportDpt., Astrophysics Division, Keplerlaan 1, 2201AZ Noordwijk,The Netherlandse-mail: jtauber@rssd.esa.int2 Danish National Space Center, Juliane Mariesvej 28, 2100,Copenhagen, Denmark3 PhotoCore GmbH, Affolternstrasse 115, 8050 Zürich, Switzerland4 Thales Alenia Space, 100 Boulevard du Midi, BP 99, 06156 Cannesla Bocca, FrancePage 21 of 22
A&A 520, A2 (2010)5 Università degli Studi di Milano, via Celoria 16, 20133 Milano, Italy6 INAF-Istituto di Astrofisica SpazialeeFisicaCosmica,Bologna,viaGobetti 101, 40129 Bologna, Italy7 Blackett Laboratory, Imperial College, London SW7 2AZ, UK8 Niels Bohr Institute, Blegdamsvej 17,2100Copenhagen,Denmark9 European Space Agency, ESTEC, Keplerlaan 1, 2201 AZNoordwijk, The Netherlands10 Jet Propulsion Laboratory, California Institute of Technology, 4800Oak Grove Drive, Pasadena, CA 91109, USA11 IFP-CNR, Via Cozzi 53, Milano, Italy12 Cavendish Laboratory, Dpt. of Physics, University of Cambridge, J.J. Thomson Avenue, Cambridge CB3 0HE, UK13 LERMA, Observatoire de <strong>Paris</strong>, 61 Av. de l’Observatoire, 75014<strong>Paris</strong>, France14 Jodrell Bank Centre for Astrophysics, The University ofManchester, M13 9PL, UK15 <strong>Planck</strong> Science Office, European Space Agency, European SpaceAstronomy Centre, PO Box – Apdo. de correos 78, 28691Villanueva de la Cañada, Madrid, Spain16 NUI Maynooth, Dpt of Experimental Physics, Maynooth, Co.Kildare, Ireland17 Ticra, Laederstraede 34, 21201 Copenhagen, Denmark18 Institut d’Astrophysique Spatiale, CNRS (UMR8617), Université<strong>Paris</strong>-Sud 11, Batiment 121, 91405 Orsay, France19 CESR, Centre d’Étude Spatiale des Rayonnements, Université PaulSabatier and CNRS, 9 Av. du colonel Roche, BP44346, 31038Toulouse Cedex 4, France20 Laboratoire Astroparticule et Cosmologie (<strong>APC</strong>), Université <strong>Paris</strong><strong>Diderot</strong> – <strong>Paris</strong> 7 and CNRS, 10 rue A. Domon et L. Duquet, 75205<strong>Paris</strong> Cedex 13, France21 Optical Science Laboratory, Dpt of Physics and Astronomy, UCL,London, WC1E 6BT, UK22 Cardiff University, School of Physics and Astronomy, The Parade,Cardiff CF24 3AA, UK23 Laboratoire de l’Accélerateur Linéaire, Université <strong>Paris</strong> 11,Bâtiment 200, 91898 Orsay, France24 European Space Agency, Headquarters, 8–10 rue Mario Nikis,75015 <strong>Paris</strong>, FrancePage 22 of 22
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- Page 3 and 4: ABSTRACTThe European Space Agency
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M. Sandri et al.: Planck pre-launch
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unmodelled long-timescale thermally
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arrangement was also constrained by
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of frequencies and shown to have po
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C. Rosset et al.: Planck-HFI: polar