The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast
The measurement of the polarization of the Cosmic Microwave Background (CMB) radiation is one of the current frontiers in cosmology. In particular, the detection of the primordial divergence-free component of the polarization field, the B-mode, could reveal the presence of gravitational waves in the...
Published in: | Journal of Cosmology and Astroparticle Physics |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Article in Journal/Newspaper |
Language: | English |
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IOP Publishing Ltd
2021
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Online Access: | http://hdl.handle.net/11573/1566999 https://doi.org/10.1088/1475-7516/2021/08/008 |
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Sapienza Università di Roma: CINECA IRIS |
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CMBR experiment CMBR polarisation cosmological parameters from CMBR |
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CMBR experiment CMBR polarisation cosmological parameters from CMBR Addamo G. Ade P. A. R. Baccigalupi C. Baldini A. M. Battaglia P. M. Battistelli E. S. Bau A. De Bernardis P. Bersanelli M. Biasotti M. Boscaleri A. Caccianiga B. Caprioli S. Cavaliere F. Cei F. Cleary K. A. Columbro F. Coppi G. Coppolecchia A. Cuttaia F. D'Alessandro G. De Gasperis G. De Petris M. Fafone V. Farsian F. Ferrari Barusso L. Fontanelli F. Franceschet C. Gaier T. C. Galli L. Gatti F. Genova-Santos R. Gerbino M. Gervasi M. Ghigna T. Grosso D. Gruppuso A. Gualtieri R. Incardona F. Jones M. E. Kangaslahti P. Krachmalnicoff N. Lamagna L. Lattanzi M. Lopez-Caraballo C. H. Lumia M. Mainini R. Maino D. Mandelli S. Maris M. Masi S. Matarrese S. May A. Mele L. Mena P. Mennella A. Molina R. Molinari D. Morgante G. Natale U. Nati F. Natoli P. Pagano L. Paiella A. Panico F. Paonessa F. Paradiso S. Passerini A. Perez-De-Taoro M. Peverini O. A. Pezzotta F. Piacentini F. Piccirillo L. Pisano G. Polenta G. Poletti D. Presta G. Realini S. Reyes N. Rocchi A. Rubino-Martin J. A. Sandri M. Sartor S. Schillaci A. Signorelli G. Siri B. Soria M. Spinella F. Tapia V. Tartari A. Taylor A. C. Terenzi L. Tomasi M. Tommasi E. Tucker C. Vaccaro D. Vigano D. M. Villa F. Virone G. Vittorio N. Volpe A. Watkins R. E. J. Zacchei A. Zannoni M. The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast |
topic_facet |
CMBR experiment CMBR polarisation cosmological parameters from CMBR |
description |
The measurement of the polarization of the Cosmic Microwave Background (CMB) radiation is one of the current frontiers in cosmology. In particular, the detection of the primordial divergence-free component of the polarization field, the B-mode, could reveal the presence of gravitational waves in the early Universe. The detection of such a component is at the moment the most promising technique to probe the inflationary theory describing the very early evolution of the Universe. We present the updated performance forecast of the Large Scale Polarization Explorer (LSPE), a program dedicated to the measurement of the CMB polarization. LSPE is composed of two instruments: LSPE-Strip, a radiometer-based telescope on the ground in Tenerife-Teide observatory, and LSPE-SWIPE (Short-Wavelength Instrument for the Polarization Explorer) a bolometer-based instrument designed to fly on a winter arctic stratospheric long-duration balloon. The program is among the few dedicated to observation of the Northern Hemisphere, while most of the international effort is focused into ground-based observation in the Southern Hemisphere. Measurements are currently scheduled in Winter 2022/23 for LSPE-SWIPE, with a flight duration up to 15 days, and in Summer 2022 with two years observations for LSPE-Strip. We describe the main features of the two instruments, identifying the most critical aspects of the design, in terms of impact on the performance forecast. We estimate the expected sensitivity of each instrument and propagate their combined observing power to the sensitivity to cosmological parameters, including the effect of scanning strategy, component separation, residual foregrounds and partial sky coverage. We also set requirements on the control of the most critical systematic effects and describe techniques to mitigate their impact. LSPE will reach a sensitivity in tensor-to-scalar ratio of σ r < 0.01, set an upper limit r < 0.015 at 95% confidence level, and improve constraints on other cosmological parameters. |
author2 |
Addamo, G. Ade, P. A. R. Baccigalupi, C. Baldini, A. M. Battaglia, P. M. Battistelli, E. S. Bau, A. De Bernardis, P. Bersanelli, M. Biasotti, M. Boscaleri, A. Caccianiga, B. Caprioli, S. Cavaliere, F. Cei, F. Cleary, K. A. Columbro, F. Coppi, G. Coppolecchia, A. Cuttaia, F. D'Alessandro, G. De Gasperis, G. De Petris, M. Fafone, V. Farsian, F. Ferrari Barusso, L. Fontanelli, F. Franceschet, C. Gaier, T. C. Galli, L. Gatti, F. Genova-Santos, R. Gerbino, M. Gervasi, M. Ghigna, T. Grosso, D. Gruppuso, A. Gualtieri, R. Incardona, F. Jones, M. E. Kangaslahti, P. Krachmalnicoff, N. Lamagna, L. Lattanzi, M. Lopez-Caraballo, C. H. Lumia, M. Mainini, R. Maino, D. Mandelli, S. Maris, M. |
format |
Article in Journal/Newspaper |
author |
Addamo G. Ade P. A. R. Baccigalupi C. Baldini A. M. Battaglia P. M. Battistelli E. S. Bau A. De Bernardis P. Bersanelli M. Biasotti M. Boscaleri A. Caccianiga B. Caprioli S. Cavaliere F. Cei F. Cleary K. A. Columbro F. Coppi G. Coppolecchia A. Cuttaia F. D'Alessandro G. De Gasperis G. De Petris M. Fafone V. Farsian F. Ferrari Barusso L. Fontanelli F. Franceschet C. Gaier T. C. Galli L. Gatti F. Genova-Santos R. Gerbino M. Gervasi M. Ghigna T. Grosso D. Gruppuso A. Gualtieri R. Incardona F. Jones M. E. Kangaslahti P. Krachmalnicoff N. Lamagna L. Lattanzi M. Lopez-Caraballo C. H. Lumia M. Mainini R. Maino D. Mandelli S. Maris M. Masi S. Matarrese S. May A. Mele L. Mena P. Mennella A. Molina R. Molinari D. Morgante G. Natale U. Nati F. Natoli P. Pagano L. Paiella A. Panico F. Paonessa F. Paradiso S. Passerini A. Perez-De-Taoro M. Peverini O. A. Pezzotta F. Piacentini F. Piccirillo L. Pisano G. Polenta G. Poletti D. Presta G. Realini S. Reyes N. Rocchi A. Rubino-Martin J. A. Sandri M. Sartor S. Schillaci A. Signorelli G. Siri B. Soria M. Spinella F. Tapia V. Tartari A. Taylor A. C. Terenzi L. Tomasi M. Tommasi E. Tucker C. Vaccaro D. Vigano D. M. Villa F. Virone G. Vittorio N. Volpe A. Watkins R. E. J. Zacchei A. Zannoni M. |
author_facet |
Addamo G. Ade P. A. R. Baccigalupi C. Baldini A. M. Battaglia P. M. Battistelli E. S. Bau A. De Bernardis P. Bersanelli M. Biasotti M. Boscaleri A. Caccianiga B. Caprioli S. Cavaliere F. Cei F. Cleary K. A. Columbro F. Coppi G. Coppolecchia A. Cuttaia F. D'Alessandro G. De Gasperis G. De Petris M. Fafone V. Farsian F. Ferrari Barusso L. Fontanelli F. Franceschet C. Gaier T. C. Galli L. Gatti F. Genova-Santos R. Gerbino M. Gervasi M. Ghigna T. Grosso D. Gruppuso A. Gualtieri R. Incardona F. Jones M. E. Kangaslahti P. Krachmalnicoff N. Lamagna L. Lattanzi M. Lopez-Caraballo C. H. Lumia M. Mainini R. Maino D. Mandelli S. Maris M. Masi S. Matarrese S. May A. Mele L. Mena P. Mennella A. Molina R. Molinari D. Morgante G. Natale U. Nati F. Natoli P. Pagano L. Paiella A. Panico F. Paonessa F. Paradiso S. Passerini A. Perez-De-Taoro M. Peverini O. A. Pezzotta F. Piacentini F. Piccirillo L. Pisano G. Polenta G. Poletti D. Presta G. Realini S. Reyes N. Rocchi A. Rubino-Martin J. A. Sandri M. Sartor S. Schillaci A. Signorelli G. Siri B. Soria M. Spinella F. Tapia V. Tartari A. Taylor A. C. Terenzi L. Tomasi M. Tommasi E. Tucker C. Vaccaro D. Vigano D. M. Villa F. Virone G. Vittorio N. Volpe A. Watkins R. E. J. Zacchei A. Zannoni M. |
author_sort |
Addamo G. |
title |
The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast |
title_short |
The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast |
title_full |
The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast |
title_fullStr |
The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast |
title_full_unstemmed |
The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast |
title_sort |
large scale polarization explorer (lspe) for cmb measurements: performance forecast |
publisher |
IOP Publishing Ltd |
publishDate |
2021 |
url |
http://hdl.handle.net/11573/1566999 https://doi.org/10.1088/1475-7516/2021/08/008 |
geographic |
Arctic |
geographic_facet |
Arctic |
genre |
Arctic |
genre_facet |
Arctic |
op_relation |
info:eu-repo/semantics/altIdentifier/wos/WOS:000683047800008 volume:2021 issue:8 firstpage:008 journal:JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS http://hdl.handle.net/11573/1566999 doi:10.1088/1475-7516/2021/08/008 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85113175572 |
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info:eu-repo/semantics/closedAccess |
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https://doi.org/10.1088/1475-7516/2021/08/008 |
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Journal of Cosmology and Astroparticle Physics |
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2021 |
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ftunivromairis:oai:iris.uniroma1.it:11573/1566999 2024-04-14T08:08:28+00:00 The large scale polarization explorer (LSPE) for CMB measurements: Performance forecast Addamo G. Ade P. A. R. Baccigalupi C. Baldini A. M. Battaglia P. M. Battistelli E. S. Bau A. De Bernardis P. Bersanelli M. Biasotti M. Boscaleri A. Caccianiga B. Caprioli S. Cavaliere F. Cei F. Cleary K. A. Columbro F. Coppi G. Coppolecchia A. Cuttaia F. D'Alessandro G. De Gasperis G. De Petris M. Fafone V. Farsian F. Ferrari Barusso L. Fontanelli F. Franceschet C. Gaier T. C. Galli L. Gatti F. Genova-Santos R. Gerbino M. Gervasi M. Ghigna T. Grosso D. Gruppuso A. Gualtieri R. Incardona F. Jones M. E. Kangaslahti P. Krachmalnicoff N. Lamagna L. Lattanzi M. Lopez-Caraballo C. H. Lumia M. Mainini R. Maino D. Mandelli S. Maris M. Masi S. Matarrese S. May A. Mele L. Mena P. Mennella A. Molina R. Molinari D. Morgante G. Natale U. Nati F. Natoli P. Pagano L. Paiella A. Panico F. Paonessa F. Paradiso S. Passerini A. Perez-De-Taoro M. Peverini O. A. Pezzotta F. Piacentini F. Piccirillo L. Pisano G. Polenta G. Poletti D. Presta G. Realini S. Reyes N. Rocchi A. Rubino-Martin J. A. Sandri M. Sartor S. Schillaci A. Signorelli G. Siri B. Soria M. Spinella F. Tapia V. Tartari A. Taylor A. C. Terenzi L. Tomasi M. Tommasi E. Tucker C. Vaccaro D. Vigano D. M. Villa F. Virone G. Vittorio N. Volpe A. Watkins R. E. J. Zacchei A. Zannoni M. Addamo, G. Ade, P. A. R. Baccigalupi, C. Baldini, A. M. Battaglia, P. M. Battistelli, E. S. Bau, A. De Bernardis, P. Bersanelli, M. Biasotti, M. Boscaleri, A. Caccianiga, B. Caprioli, S. Cavaliere, F. Cei, F. Cleary, K. A. Columbro, F. Coppi, G. Coppolecchia, A. Cuttaia, F. D'Alessandro, G. De Gasperis, G. De Petris, M. Fafone, V. Farsian, F. Ferrari Barusso, L. Fontanelli, F. Franceschet, C. Gaier, T. C. Galli, L. Gatti, F. Genova-Santos, R. Gerbino, M. Gervasi, M. Ghigna, T. Grosso, D. Gruppuso, A. Gualtieri, R. Incardona, F. Jones, M. E. Kangaslahti, P. Krachmalnicoff, N. Lamagna, L. Lattanzi, M. Lopez-Caraballo, C. H. Lumia, M. Mainini, R. Maino, D. Mandelli, S. Maris, M. 2021 http://hdl.handle.net/11573/1566999 https://doi.org/10.1088/1475-7516/2021/08/008 eng eng IOP Publishing Ltd place:TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND info:eu-repo/semantics/altIdentifier/wos/WOS:000683047800008 volume:2021 issue:8 firstpage:008 journal:JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS http://hdl.handle.net/11573/1566999 doi:10.1088/1475-7516/2021/08/008 info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85113175572 info:eu-repo/semantics/closedAccess CMBR experiment CMBR polarisation cosmological parameters from CMBR info:eu-repo/semantics/article 2021 ftunivromairis https://doi.org/10.1088/1475-7516/2021/08/008 2024-03-21T19:30:47Z The measurement of the polarization of the Cosmic Microwave Background (CMB) radiation is one of the current frontiers in cosmology. In particular, the detection of the primordial divergence-free component of the polarization field, the B-mode, could reveal the presence of gravitational waves in the early Universe. The detection of such a component is at the moment the most promising technique to probe the inflationary theory describing the very early evolution of the Universe. We present the updated performance forecast of the Large Scale Polarization Explorer (LSPE), a program dedicated to the measurement of the CMB polarization. LSPE is composed of two instruments: LSPE-Strip, a radiometer-based telescope on the ground in Tenerife-Teide observatory, and LSPE-SWIPE (Short-Wavelength Instrument for the Polarization Explorer) a bolometer-based instrument designed to fly on a winter arctic stratospheric long-duration balloon. The program is among the few dedicated to observation of the Northern Hemisphere, while most of the international effort is focused into ground-based observation in the Southern Hemisphere. Measurements are currently scheduled in Winter 2022/23 for LSPE-SWIPE, with a flight duration up to 15 days, and in Summer 2022 with two years observations for LSPE-Strip. We describe the main features of the two instruments, identifying the most critical aspects of the design, in terms of impact on the performance forecast. We estimate the expected sensitivity of each instrument and propagate their combined observing power to the sensitivity to cosmological parameters, including the effect of scanning strategy, component separation, residual foregrounds and partial sky coverage. We also set requirements on the control of the most critical systematic effects and describe techniques to mitigate their impact. LSPE will reach a sensitivity in tensor-to-scalar ratio of σ r < 0.01, set an upper limit r < 0.015 at 95% confidence level, and improve constraints on other cosmological parameters. Article in Journal/Newspaper Arctic Sapienza Università di Roma: CINECA IRIS Arctic Journal of Cosmology and Astroparticle Physics 2021 08 008 |