{"paper":{"title":"Planck 2015 results. III. LFI systematic uncertainties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Benoit-L\\'evy, A. Bonaldi, A. Catalano, A. Curto, A. De Rosa, A. Ducout, A. Gregorio, A. Gruppuso, A. H. Jaffe, A. Hornstrup, A. J. Banday, A. Mangilli, A. Mennella, A. Renzi, A.-S. Suur-Uski, A. Zacchei, A. Zonca, B. D. Wandelt, B. Maffei, B. Partridge, B. Rusholme, B. Van Tent, C. Baccigalupi, C. Burigana, C. Dickinson, C. Franceschet, C. Hern\\'andez-Monteagudo, C. R. Lawrence, C. Rosset, D. Herranz, D. L. Harrison, D. Maino, D. Mortlock, D. Munshi, D. Paoletti, D. Santos, D. Scott, D. Tavagnacco, D. Yvon, E. Battaner, E. Calabrese, E. Franceschi, E. Gjerl{\\o}w, E. Hivon, E. Keih\\\"aen, E. Mart\\'inez-Gonz\\'alez, E. Pointecouteau, F. Cuttaia, F. Elsner, F. Finelli, F. K. Hansen, F. Levrier, F. Nati, F. Noviello, F. Paci, F. Pajot, F. Pasian, F. Piacentini, F. Villa, G. de Zotti, G. Hurier, G. Lagache, G. Maggio, G. Morgante, G. Polenta, G. Rocha, G. Roudier, G. Umana, G. W. Pratt, H. K. Eriksen, H. Kurki-Suonio, I. K. Wehus, I. Ristorcelli, J. A. Murphy, J. A. Rubi\\~no-Mart\\'in, J. A. Tauber, J. Aumont, J. Borrill, J. Delabrouille, J. F. Mac\\'ias-P\\'erez, J.-F. Sygnet, J. Gonz\\'alez-Nuevo, J. Knoche, J.-L. Puget, J. M. Diego, J.-M. Lamarre, J.-P. Bernard, J. P. Leahy, J. P. Rachen, J. P. Zibin, J. R. Bond, J. Valiviita, K. Benabed, K. Ganga, K. Kiiveri, K. M. G\\'orski, K. M. Huffenberger, L. A. Wade, L. Bonavera, L. Danese, L. Montier, L. Pagano, L. P. L. Colombo, L. Terenzi, L. Toffolatti, L. Valenziano, M. Bersanelli, M. Cruz, M. Frailis, M. Giard, M. Hobson, M. Kunz, M. Lattanzi, M. Linden-V{\\o}rnle, M. L\\'opez-Caniego, M. Maris, M. Migliaccio, M. Reinecke, M. Remazeilles, M. Rossetti, M. Sandri, M. Savelainen, M. Tomasi, M. Tristram, M. Tucci, N. Bartolo, N. Krachmalnicoff, N. Mandolesi, O. Dor\\'e, O. Perdereau, P. Battaglia, P. Bielewicz, P. B. Lilje, P. De Bernardis, P. G. Martin, Planck Collaboration: P. A. R. Ade, P. M. Lubin, P. Natoli, P. R. Christensen, P. R. Meinhold, P. Vielva, R. B. Barreiro, R. C. Butler, R. D. Davies, R. J. Davis, R. Keskitalo, R. Leonardi, R. Stompor, R. Watson, S. Basak, S. Galeotta, S. Galli, S. Masi, S. Matarrese, S. Mitra, S. R. Hildebrandt, T. A. En{\\ss}lin, T. Ghosh, T. J. Pearson, T. R. Jaffe, T. S. Kisner, T. Vassallo, V. Lindholm, V. Pettorino, V. Stolyarov, W. Hovest, X. Dupac, Y. Giraud-H\\'eraud","submitted_at":"2015-07-31T12:24:48Z","abstract_excerpt":"We present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, showing the robustness and consistency of our data set, especially for polarization analysis. We use two complementary approaches: (i) simulations based on measured data and physical models of the known systematic effects; and (ii) analysis of difference maps containing the same sky signal (\"null-maps\"). The LFI temperature data are limited by instrumental noise. At large angular scales the systematic effects are b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1507.08853","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}