Planck pre-launch status: Low Frequency Instrument calibration and expected scientific performance
We present the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters characterise the instrument response and constitute our optimal pre-launch knowledge of the LFI scientific performance. T...
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Veröffentlicht in: | Astronomy and astrophysics (Berlin) 2010-09, Vol.520, p.A5 |
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creator | Mennella, A. Bersanelli, M. Butler, R. C. Cuttaia, F. D'Arcangelo, O. Davis, R. J. Frailis, M. Galeotta, S. Gregorio, A. Lawrence, C. R. Leonardi, R. Lowe, S. R. Mandolesi, N. Maris, M. Meinhold, P. Mendes, L. Morgante, G. Sandri, M. Stringhetti, L. Terenzi, L. Tomasi, M. Valenziano, L. Villa, F. Zacchei, A. Zonca, A. Balasini, M. Franceschet, C. Battaglia, P. Lapolla, P. M. Leutenegger, P. Miccolis, M. Pagan, L. Silvestri, R. Aja, B. Artal, E. Baldan, G. Bastia, P. Bernardino, T. Boschini, L. Cafagna, G. Cappellini, B. Cavaliere, F. Colombo, F. de La Fuente, L. Edgeley, J. Falvella, M. C. Ferrari, F. Fogliani, S. Franceschi, E. Gaier, T. Gomez, F. Herreros, J. M. Hildebrandt, S. Hoyland, R. Hughes, N. Jukkala, P. Kettle, D. Laaninen, M. Lawson, D. Leahy, P. Levin, S. Lilje, P. B. Maino, D. Malaspina, M. Manzato, P. Marti-Canales, J. Martinez-Gonzalez, E. Mediavilla, A. Pasian, F. Pascual, J. P. Pecora, M. Peres-Cuevas, L. Platania, P. Pospieszalsky, M. Poutanen, T. Rebolo, R. Roddis, N. Salmon, M. Seiffert, M. Simonetto, A. Sozzi, C. Tauber, J. Tuovinen, J. Varis, J. Wilkinson, A. Winder, F. |
description | We present the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters characterise the instrument response and constitute our optimal pre-launch knowledge of the LFI scientific performance. The LFI shows excellent 1/f stability and rejection of instrumental systematic effects; its measured noise performance shows that LFI is the most sensitive instrument of its kind. The calibration parameters will be updated during flight operations until the end of the mission. |
doi_str_mv | 10.1051/0004-6361/200912849 |
format | Article |
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C. ; Cuttaia, F. ; D'Arcangelo, O. ; Davis, R. J. ; Frailis, M. ; Galeotta, S. ; Gregorio, A. ; Lawrence, C. R. ; Leonardi, R. ; Lowe, S. R. ; Mandolesi, N. ; Maris, M. ; Meinhold, P. ; Mendes, L. ; Morgante, G. ; Sandri, M. ; Stringhetti, L. ; Terenzi, L. ; Tomasi, M. ; Valenziano, L. ; Villa, F. ; Zacchei, A. ; Zonca, A. ; Balasini, M. ; Franceschet, C. ; Battaglia, P. ; Lapolla, P. M. ; Leutenegger, P. ; Miccolis, M. ; Pagan, L. ; Silvestri, R. ; Aja, B. ; Artal, E. ; Baldan, G. ; Bastia, P. ; Bernardino, T. ; Boschini, L. ; Cafagna, G. ; Cappellini, B. ; Cavaliere, F. ; Colombo, F. ; de La Fuente, L. ; Edgeley, J. ; Falvella, M. C. ; Ferrari, F. ; Fogliani, S. ; Franceschi, E. ; Gaier, T. ; Gomez, F. ; Herreros, J. M. ; Hildebrandt, S. ; Hoyland, R. ; Hughes, N. ; Jukkala, P. ; Kettle, D. ; Laaninen, M. ; Lawson, D. ; Leahy, P. ; Levin, S. ; Lilje, P. 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M. ; Leutenegger, P. ; Miccolis, M. ; Pagan, L. ; Silvestri, R. ; Aja, B. ; Artal, E. ; Baldan, G. ; Bastia, P. ; Bernardino, T. ; Boschini, L. ; Cafagna, G. ; Cappellini, B. ; Cavaliere, F. ; Colombo, F. ; de La Fuente, L. ; Edgeley, J. ; Falvella, M. C. ; Ferrari, F. ; Fogliani, S. ; Franceschi, E. ; Gaier, T. ; Gomez, F. ; Herreros, J. M. ; Hildebrandt, S. ; Hoyland, R. ; Hughes, N. ; Jukkala, P. ; Kettle, D. ; Laaninen, M. ; Lawson, D. ; Leahy, P. ; Levin, S. ; Lilje, P. B. ; Maino, D. ; Malaspina, M. ; Manzato, P. ; Marti-Canales, J. ; Martinez-Gonzalez, E. ; Mediavilla, A. ; Pasian, F. ; Pascual, J. 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B.</creatorcontrib><creatorcontrib>Maino, D.</creatorcontrib><creatorcontrib>Malaspina, M.</creatorcontrib><creatorcontrib>Manzato, P.</creatorcontrib><creatorcontrib>Marti-Canales, J.</creatorcontrib><creatorcontrib>Martinez-Gonzalez, E.</creatorcontrib><creatorcontrib>Mediavilla, A.</creatorcontrib><creatorcontrib>Pasian, F.</creatorcontrib><creatorcontrib>Pascual, J. P.</creatorcontrib><creatorcontrib>Pecora, M.</creatorcontrib><creatorcontrib>Peres-Cuevas, L.</creatorcontrib><creatorcontrib>Platania, P.</creatorcontrib><creatorcontrib>Pospieszalsky, M.</creatorcontrib><creatorcontrib>Poutanen, T.</creatorcontrib><creatorcontrib>Rebolo, R.</creatorcontrib><creatorcontrib>Roddis, N.</creatorcontrib><creatorcontrib>Salmon, M.</creatorcontrib><creatorcontrib>Seiffert, M.</creatorcontrib><creatorcontrib>Simonetto, A.</creatorcontrib><creatorcontrib>Sozzi, C.</creatorcontrib><creatorcontrib>Tauber, J.</creatorcontrib><creatorcontrib>Tuovinen, J.</creatorcontrib><creatorcontrib>Varis, J.</creatorcontrib><creatorcontrib>Wilkinson, A.</creatorcontrib><creatorcontrib>Winder, F.</creatorcontrib><title>Planck pre-launch status: Low Frequency Instrument calibration and expected scientific performance</title><title>Astronomy and astrophysics (Berlin)</title><description>We present the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters characterise the instrument response and constitute our optimal pre-launch knowledge of the LFI scientific performance. The LFI shows excellent 1/f stability and rejection of instrumental systematic effects; its measured noise performance shows that LFI is the most sensitive instrument of its kind. The calibration parameters will be updated during flight operations until the end of the mission.</description><subject>cosmic microwave background</subject><subject>instrumentation: detectors</subject><subject>instrumentation: polarimeters</subject><subject>space vehicles: instruments</subject><subject>submillimeter: general</subject><subject>telescopes</subject><issn>0004-6361</issn><issn>1432-0746</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNo9kEtLAzEUhYMoWKu_wE12rsbmMZlk3Em1tlBQoSK4CZnMHYzOyySD7b93SqWry-Wec7jnQ-iakltKBJ0RQtIk4xmdMUJyylSan6AJTTlLiEyzUzQ5Ks7RRQhf48qo4hNUvNSmtd-495DUZmjtJw7RxCHc4XX3ixcefgZo7Q6v2hD90EAbsTW1K7yJrmuxaUsM2x5shBIH68a7q5zFPfiq882YDZforDJ1gKv_OUVvi8fNfJmsn59W8_t1YjnNY2IUFaDyquCgDOcst6I0XGUik7SUpDAsL0TBU6IYYZYraWilZJWnSpRgqeVTdHPI7X03Ph2iblywUI8FoRuCVhnhMhVKjkp-UFrfheCh0r13jfE7TYneA9V7XHqPSx-Bjq7k4HIhwvZoMf5bZ5JLoRV513O53iw_Xrl-4H_Vg3iX</recordid><startdate>20100901</startdate><enddate>20100901</enddate><creator>Mennella, A.</creator><creator>Bersanelli, M.</creator><creator>Butler, R. 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P.</creatorcontrib><creatorcontrib>Pecora, M.</creatorcontrib><creatorcontrib>Peres-Cuevas, L.</creatorcontrib><creatorcontrib>Platania, P.</creatorcontrib><creatorcontrib>Pospieszalsky, M.</creatorcontrib><creatorcontrib>Poutanen, T.</creatorcontrib><creatorcontrib>Rebolo, R.</creatorcontrib><creatorcontrib>Roddis, N.</creatorcontrib><creatorcontrib>Salmon, M.</creatorcontrib><creatorcontrib>Seiffert, M.</creatorcontrib><creatorcontrib>Simonetto, A.</creatorcontrib><creatorcontrib>Sozzi, C.</creatorcontrib><creatorcontrib>Tauber, J.</creatorcontrib><creatorcontrib>Tuovinen, J.</creatorcontrib><creatorcontrib>Varis, J.</creatorcontrib><creatorcontrib>Wilkinson, A.</creatorcontrib><creatorcontrib>Winder, F.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mennella, A.</au><au>Bersanelli, M.</au><au>Butler, R. C.</au><au>Cuttaia, F.</au><au>D'Arcangelo, O.</au><au>Davis, R. J.</au><au>Frailis, M.</au><au>Galeotta, S.</au><au>Gregorio, A.</au><au>Lawrence, C. R.</au><au>Leonardi, R.</au><au>Lowe, S. R.</au><au>Mandolesi, N.</au><au>Maris, M.</au><au>Meinhold, P.</au><au>Mendes, L.</au><au>Morgante, G.</au><au>Sandri, M.</au><au>Stringhetti, L.</au><au>Terenzi, L.</au><au>Tomasi, M.</au><au>Valenziano, L.</au><au>Villa, F.</au><au>Zacchei, A.</au><au>Zonca, A.</au><au>Balasini, M.</au><au>Franceschet, C.</au><au>Battaglia, P.</au><au>Lapolla, P. M.</au><au>Leutenegger, P.</au><au>Miccolis, M.</au><au>Pagan, L.</au><au>Silvestri, R.</au><au>Aja, B.</au><au>Artal, E.</au><au>Baldan, G.</au><au>Bastia, P.</au><au>Bernardino, T.</au><au>Boschini, L.</au><au>Cafagna, G.</au><au>Cappellini, B.</au><au>Cavaliere, F.</au><au>Colombo, F.</au><au>de La Fuente, L.</au><au>Edgeley, J.</au><au>Falvella, M. C.</au><au>Ferrari, F.</au><au>Fogliani, S.</au><au>Franceschi, E.</au><au>Gaier, T.</au><au>Gomez, F.</au><au>Herreros, J. M.</au><au>Hildebrandt, S.</au><au>Hoyland, R.</au><au>Hughes, N.</au><au>Jukkala, P.</au><au>Kettle, D.</au><au>Laaninen, M.</au><au>Lawson, D.</au><au>Leahy, P.</au><au>Levin, S.</au><au>Lilje, P. B.</au><au>Maino, D.</au><au>Malaspina, M.</au><au>Manzato, P.</au><au>Marti-Canales, J.</au><au>Martinez-Gonzalez, E.</au><au>Mediavilla, A.</au><au>Pasian, F.</au><au>Pascual, J. P.</au><au>Pecora, M.</au><au>Peres-Cuevas, L.</au><au>Platania, P.</au><au>Pospieszalsky, M.</au><au>Poutanen, T.</au><au>Rebolo, R.</au><au>Roddis, N.</au><au>Salmon, M.</au><au>Seiffert, M.</au><au>Simonetto, A.</au><au>Sozzi, C.</au><au>Tauber, J.</au><au>Tuovinen, J.</au><au>Varis, J.</au><au>Wilkinson, A.</au><au>Winder, F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Planck pre-launch status: Low Frequency Instrument calibration and expected scientific performance</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2010-09-01</date><risdate>2010</risdate><volume>520</volume><spage>A5</spage><pages>A5-</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><abstract>We present the calibration and scientific performance parameters of the Planck Low Frequency Instrument (LFI) measured during the ground cryogenic test campaign. These parameters characterise the instrument response and constitute our optimal pre-launch knowledge of the LFI scientific performance. The LFI shows excellent 1/f stability and rejection of instrumental systematic effects; its measured noise performance shows that LFI is the most sensitive instrument of its kind. The calibration parameters will be updated during flight operations until the end of the mission.</abstract><pub>EDP Sciences</pub><doi>10.1051/0004-6361/200912849</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-6361 |
ispartof | Astronomy and astrophysics (Berlin), 2010-09, Vol.520, p.A5 |
issn | 0004-6361 1432-0746 |
language | eng |
recordid | cdi_proquest_miscellaneous_860374587 |
source | Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; EZB-FREE-00999 freely available EZB journals |
subjects | cosmic microwave background instrumentation: detectors instrumentation: polarimeters space vehicles: instruments submillimeter: general telescopes |
title | Planck pre-launch status: Low Frequency Instrument calibration and expected scientific performance |
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