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Planck 2015 results. V. LFI calibration

We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchrono...

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Detalles Bibliográficos
Autores principales: Ade, P.A.R., Aghanim, N., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Bartolo, N., Battaglia, P., Battaner, E., Benabed, K., Benoit, A., Benoit-Levy, A., Bernard, J.P., Bersanelli, M., Bielewicz, P., Bock, J.J., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.F., Catalano, A., Chamballu, A., Christensen, P.R., Colombi, S., Colombo, L.P.L., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Dickinson, C., Diego, J.M., Dole, H., Donzelli, S., Dore, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Ensslin, T.A., Eriksen, H.K., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Frejsel, A., Galeotta, S., Galli, S., Ganga, K., Giard, M., Giraud-Heraud, Y., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D.L., Henrot-Versille, S., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Juvela, M., Keihanen, E., Keskitalo, R., Kisner, T.S., Knoche, J., Krachmalnicoff, N., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J.M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Leahy, J.P., Leonardi, R., Lesgourgues, J., Levrier, F., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Macias-Perez, J.F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Maris, M., Martin, P.G., Martinez-Gonzalez, E., Masi, S., Matarrese, S., McGehee, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Novikov, D., Novikov, I., Paci, F., Pagano, L., Pajot, F., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Pearson, T.J., Peel, M., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Pierpaoli, E., Pietrobon, D., Pointecouteau, E., Polenta, G., Pratt, G.W., Prezeau, G., Prunet, S., Puget, J.L., Rachen, J.P., Rebolo, R., Reinecke, M., Remazeilles, M., Renzi, A., Rocha, G., Romelli, E., Rosset, C., Rossetti, M., Roudier, G., Rubino-Martin, J.A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Scott, D., Seiffert, M.D., Shellard, E.P.S., Spencer, L.D., Stolyarov, V., Sutton, D., Suur-Uski, A.S., Sygnet, J.F., Tauber, J.A., Tavagnacco, D., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Tucci, M., Tuovinen, J., Turler, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vassallo, T., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Watson, R., Wehus, I.K., Wilkinson, A., Yvon, D., Zacchei, A., Zonca, A.
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1051/0004-6361/201526632
http://cds.cern.ch/record/2020648
_version_ 1780946851337338880
author Ade, P.A.R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartolo, N.
Battaglia, P.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bock, J.J.
Bonaldi, A.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Bucher, M.
Burigana, C.
Butler, R.C.
Calabrese, E.
Cardoso, J.F.
Catalano, A.
Chamballu, A.
Christensen, P.R.
Colombi, S.
Colombo, L.P.L.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J.M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T.A.
Eriksen, H.K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T.S.
Knoche, J.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J.M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Leahy, J.P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P.G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P.R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Norgaard-Nielsen, H.U.
Novikov, D.
Novikov, I.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Peel, M.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Pierpaoli, E.
Pietrobon, D.
Pointecouteau, E.
Polenta, G.
Pratt, G.W.
Prezeau, G.
Prunet, S.
Puget, J.L.
Rachen, J.P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Rocha, G.
Romelli, E.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J.A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M.D.
Shellard, E.P.S.
Spencer, L.D.
Stolyarov, V.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Watson, R.
Wehus, I.K.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
author_facet Ade, P.A.R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartolo, N.
Battaglia, P.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bock, J.J.
Bonaldi, A.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Bucher, M.
Burigana, C.
Butler, R.C.
Calabrese, E.
Cardoso, J.F.
Catalano, A.
Chamballu, A.
Christensen, P.R.
Colombi, S.
Colombo, L.P.L.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J.M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T.A.
Eriksen, H.K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Frejsel, A.
Galeotta, S.
Galli, S.
Ganga, K.
Giard, M.
Giraud-Heraud, Y.
Gjerlow, E.
Gonzalez-Nuevo, J.
Gorski, K.M.
Gratton, S.
Gregorio, A.
Gruppuso, A.
Hansen, F.K.
Hanson, D.
Harrison, D.L.
Henrot-Versille, S.
Herranz, D.
Hildebrandt, S.R.
Hivon, E.
Hobson, M.
Holmes, W.A.
Hornstrup, A.
Hovest, W.
Huffenberger, K.M.
Hurier, G.
Jaffe, A.H.
Jaffe, T.R.
Juvela, M.
Keihanen, E.
Keskitalo, R.
Kisner, T.S.
Knoche, J.
Krachmalnicoff, N.
Kunz, M.
Kurki-Suonio, H.
Lagache, G.
Lahteenmaki, A.
Lamarre, J.M.
Lasenby, A.
Lattanzi, M.
Lawrence, C.R.
Leahy, J.P.
Leonardi, R.
Lesgourgues, J.
Levrier, F.
Liguori, M.
Lilje, P.B.
Linden-Vornle, M.
Lopez-Caniego, M.
Lubin, P.M.
Macias-Perez, J.F.
Maggio, G.
Maino, D.
Mandolesi, N.
Mangilli, A.
Maris, M.
Martin, P.G.
Martinez-Gonzalez, E.
Masi, S.
Matarrese, S.
McGehee, P.
Meinhold, P.R.
Melchiorri, A.
Mendes, L.
Mennella, A.
Migliaccio, M.
Mitra, S.
Montier, L.
Morgante, G.
Mortlock, D.
Moss, A.
Munshi, D.
Murphy, J.A.
Naselsky, P.
Nati, F.
Natoli, P.
Netterfield, C.B.
Norgaard-Nielsen, H.U.
Novikov, D.
Novikov, I.
Paci, F.
Pagano, L.
Pajot, F.
Paoletti, D.
Partridge, B.
Pasian, F.
Patanchon, G.
Pearson, T.J.
Peel, M.
Perdereau, O.
Perotto, L.
Perrotta, F.
Pettorino, V.
Piacentini, F.
Pierpaoli, E.
Pietrobon, D.
Pointecouteau, E.
Polenta, G.
Pratt, G.W.
Prezeau, G.
Prunet, S.
Puget, J.L.
Rachen, J.P.
Rebolo, R.
Reinecke, M.
Remazeilles, M.
Renzi, A.
Rocha, G.
Romelli, E.
Rosset, C.
Rossetti, M.
Roudier, G.
Rubino-Martin, J.A.
Rusholme, B.
Sandri, M.
Santos, D.
Savelainen, M.
Scott, D.
Seiffert, M.D.
Shellard, E.P.S.
Spencer, L.D.
Stolyarov, V.
Sutton, D.
Suur-Uski, A.S.
Sygnet, J.F.
Tauber, J.A.
Tavagnacco, D.
Terenzi, L.
Toffolatti, L.
Tomasi, M.
Tristram, M.
Tucci, M.
Tuovinen, J.
Turler, M.
Umana, G.
Valenziano, L.
Valiviita, J.
Van Tent, B.
Vassallo, T.
Vielva, P.
Villa, F.
Wade, L.A.
Wandelt, B.D.
Watson, R.
Wehus, I.K.
Wilkinson, A.
Yvon, D.
Zacchei, A.
Zonca, A.
author_sort Ade, P.A.R.
collection CERN
description We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. Our 2015 LFI analysis provides an independent Solar dipole estimate in excellent agreement with that of HFI and within $1\sigma$ (0.3 % in amplitude) of the WMAP value. This 0.3 % shift in the peak-to-peak dipole temperature from WMAP and a global overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45 % (30 GHz), 0.64 % (44 GHz), and 0.82 % (70 GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is at the level of 0.20 % for the 70 GHz map, 0.26 % for the 44 GHz map, and 0.35 % for the 30 GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.
id cern-2020648
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
record_format invenio
spelling cern-20206482022-01-12T03:05:17Zdoi:10.1051/0004-6361/201526632http://cds.cern.ch/record/2020648engAde, P.A.R.Aghanim, N.Ashdown, M.Aumont, J.Baccigalupi, C.Banday, A.J.Barreiro, R.B.Bartolo, N.Battaglia, P.Battaner, E.Benabed, K.Benoit, A.Benoit-Levy, A.Bernard, J.P.Bersanelli, M.Bielewicz, P.Bock, J.J.Bonaldi, A.Bonavera, L.Bond, J.R.Borrill, J.Bouchet, F.R.Bucher, M.Burigana, C.Butler, R.C.Calabrese, E.Cardoso, J.F.Catalano, A.Chamballu, A.Christensen, P.R.Colombi, S.Colombo, L.P.L.Crill, B.P.Curto, A.Cuttaia, F.Danese, L.Davies, R.D.Davis, R.J.de Bernardis, P.de Rosa, A.de Zotti, G.Delabrouille, J.Dickinson, C.Diego, J.M.Dole, H.Donzelli, S.Dore, O.Douspis, M.Ducout, A.Dupac, X.Efstathiou, G.Elsner, F.Ensslin, T.A.Eriksen, H.K.Fergusson, J.Finelli, F.Forni, O.Frailis, M.Franceschi, E.Frejsel, A.Galeotta, S.Galli, S.Ganga, K.Giard, M.Giraud-Heraud, Y.Gjerlow, E.Gonzalez-Nuevo, J.Gorski, K.M.Gratton, S.Gregorio, A.Gruppuso, A.Hansen, F.K.Hanson, D.Harrison, D.L.Henrot-Versille, S.Herranz, D.Hildebrandt, S.R.Hivon, E.Hobson, M.Holmes, W.A.Hornstrup, A.Hovest, W.Huffenberger, K.M.Hurier, G.Jaffe, A.H.Jaffe, T.R.Juvela, M.Keihanen, E.Keskitalo, R.Kisner, T.S.Knoche, J.Krachmalnicoff, N.Kunz, M.Kurki-Suonio, H.Lagache, G.Lahteenmaki, A.Lamarre, J.M.Lasenby, A.Lattanzi, M.Lawrence, C.R.Leahy, J.P.Leonardi, R.Lesgourgues, J.Levrier, F.Liguori, M.Lilje, P.B.Linden-Vornle, M.Lopez-Caniego, M.Lubin, P.M.Macias-Perez, J.F.Maggio, G.Maino, D.Mandolesi, N.Mangilli, A.Maris, M.Martin, P.G.Martinez-Gonzalez, E.Masi, S.Matarrese, S.McGehee, P.Meinhold, P.R.Melchiorri, A.Mendes, L.Mennella, A.Migliaccio, M.Mitra, S.Montier, L.Morgante, G.Mortlock, D.Moss, A.Munshi, D.Murphy, J.A.Naselsky, P.Nati, F.Natoli, P.Netterfield, C.B.Norgaard-Nielsen, H.U.Novikov, D.Novikov, I.Paci, F.Pagano, L.Pajot, F.Paoletti, D.Partridge, B.Pasian, F.Patanchon, G.Pearson, T.J.Peel, M.Perdereau, O.Perotto, L.Perrotta, F.Pettorino, V.Piacentini, F.Pierpaoli, E.Pietrobon, D.Pointecouteau, E.Polenta, G.Pratt, G.W.Prezeau, G.Prunet, S.Puget, J.L.Rachen, J.P.Rebolo, R.Reinecke, M.Remazeilles, M.Renzi, A.Rocha, G.Romelli, E.Rosset, C.Rossetti, M.Roudier, G.Rubino-Martin, J.A.Rusholme, B.Sandri, M.Santos, D.Savelainen, M.Scott, D.Seiffert, M.D.Shellard, E.P.S.Spencer, L.D.Stolyarov, V.Sutton, D.Suur-Uski, A.S.Sygnet, J.F.Tauber, J.A.Tavagnacco, D.Terenzi, L.Toffolatti, L.Tomasi, M.Tristram, M.Tucci, M.Tuovinen, J.Turler, M.Umana, G.Valenziano, L.Valiviita, J.Van Tent, B.Vassallo, T.Vielva, P.Villa, F.Wade, L.A.Wandelt, B.D.Watson, R.Wehus, I.K.Wilkinson, A.Yvon, D.Zacchei, A.Zonca, A.Planck 2015 results. V. LFI calibrationAstrophysics and AstronomyWe present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering 4 years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the CMB dipole, exploiting both the orbital and solar components. Our 2015 LFI analysis provides an independent Solar dipole estimate in excellent agreement with that of HFI and within $1\sigma$ (0.3 % in amplitude) of the WMAP value. This 0.3 % shift in the peak-to-peak dipole temperature from WMAP and a global overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45 % (30 GHz), 0.64 % (44 GHz), and 0.82 % (70 GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is at the level of 0.20 % for the 70 GHz map, 0.26 % for the 44 GHz map, and 0.35 % for the 30 GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering four years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the cosmic microwave background dipole, but we now use the orbital component, rather than adopting the Wilkinson Microwave Anisotropy Probe (WMAP) solar dipole. This allows our 2015 LFI analysis to provide an independent Solar dipole estimate, which is in excellent agreement with that of HFI and within 1sigma (0.3% in amplitude) of the WMAP value. This 0.3% shift in the peak-to-peak dipole temperature from WMAP and a general overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45% (30GHz), 0.64% (44GHz), and 0.82% (70GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is now at the level of 0.20% for the 70GHz map, 0.26% for the 44GHz map, and 0.35% for the 30GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.We present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the Planck 2015 data release, covering four years of uninterrupted operations. As in the 2013 data release, our calibrator is provided by the spin-synchronous modulation of the cosmic microwave background dipole, but we now use the orbital component, rather than adopting the Wilkinson Microwave Anisotropy Probe (WMAP) solar dipole. This allows our 2015 LFI analysis to provide an independent Solar dipole estimate, which is in excellent agreement with that of HFI and within $1\sigma$ (0.3% in amplitude) of the WMAP value. This 0.3% shift in the peak-to-peak dipole temperature from WMAP and a global overhaul of the iterative calibration code increases the overall level of the LFI maps by 0.45% (30 GHz), 0.64% (44 GHz), and 0.82% (70 GHz) in temperature with respect to the 2013 Planck data release, thus reducing the discrepancy with the power spectrum measured by WMAP. We estimate that the LFI calibration uncertainty is now at the level of 0.20% for the 70 GHz map, 0.26% for the 44 GHz map, and 0.35% for the 30 GHz map. We provide a detailed description of the impact of all the changes implemented in the calibration since the previous data release.arXiv:1505.08022oai:cds.cern.ch:20206482015-05-29
spellingShingle Astrophysics and Astronomy
Ade, P.A.R.
Aghanim, N.
Ashdown, M.
Aumont, J.
Baccigalupi, C.
Banday, A.J.
Barreiro, R.B.
Bartolo, N.
Battaglia, P.
Battaner, E.
Benabed, K.
Benoit, A.
Benoit-Levy, A.
Bernard, J.P.
Bersanelli, M.
Bielewicz, P.
Bock, J.J.
Bonaldi, A.
Bonavera, L.
Bond, J.R.
Borrill, J.
Bouchet, F.R.
Bucher, M.
Burigana, C.
Butler, R.C.
Calabrese, E.
Cardoso, J.F.
Catalano, A.
Chamballu, A.
Christensen, P.R.
Colombi, S.
Colombo, L.P.L.
Crill, B.P.
Curto, A.
Cuttaia, F.
Danese, L.
Davies, R.D.
Davis, R.J.
de Bernardis, P.
de Rosa, A.
de Zotti, G.
Delabrouille, J.
Dickinson, C.
Diego, J.M.
Dole, H.
Donzelli, S.
Dore, O.
Douspis, M.
Ducout, A.
Dupac, X.
Efstathiou, G.
Elsner, F.
Ensslin, T.A.
Eriksen, H.K.
Fergusson, J.
Finelli, F.
Forni, O.
Frailis, M.
Franceschi, E.
Frejsel, A.
Galeotta, S.
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Planck 2015 results. V. LFI calibration
title Planck 2015 results. V. LFI calibration
title_full Planck 2015 results. V. LFI calibration
title_fullStr Planck 2015 results. V. LFI calibration
title_full_unstemmed Planck 2015 results. V. LFI calibration
title_short Planck 2015 results. V. LFI calibration
title_sort planck 2015 results. v. lfi calibration
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1051/0004-6361/201526632
http://cds.cern.ch/record/2020648
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