Planck 2013 results. XVII. Gravitational lensing by large-scale structure
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ftunivhelsihelda:oai:helda.helsinki.fi:10138/233676 2024-01-07T09:46:42+01:00 Planck 2013 results. XVII. Gravitational lensing by large-scale structure Ade, P. A. R. Juvela, M. Keihanen, E. Kurki-Suonio, H. Poutanen, T. Suur-Uski, A. -S. Tuovinen, J. Valiviita, J. Planck Collaboration Department of Physics Helsinki Institute of Physics 2018-03-22T14:00:04Z 39 application/pdf http://hdl.handle.net/10138/233676 eng eng EDP sciences 10.1051/0004-6361/201321543 The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.soirees.esa.int/index.php?project=planck&pagess-Planck_Collaboration. Some of the results in this paper have been derived using the HEALPix package (Gorski et al. 2005). This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231, as well as of the IN2P3 Computer Center (http://cc.in2p3.fr) and the Planck-HFI data processing center infrastructures hosted at the Institut d'Astrophysique de Paris (France) and financially supported by CNES. We acknowledge support from the Science and Technology Facilities Council [grant number ST/I000976/1]. Ade , P A R , Juvela , M , Keihanen , E , Kurki-Suonio , H , Poutanen , T , Suur-Uski , A -S , Tuovinen , J , Valiviita , J & Planck Collaboration 2014 , ' Planck 2013 results. XVII. Gravitational lensing by large-scale structure ' , Astronomy & Astrophysics , vol. 571 , A17 . https://doi.org/10.1051/0004-6361/201321543 ORCID: /0000-0002-5809-4834/work/43222500 ORCID: /0000-0002-4618-3063/work/43223672 ORCID: /0000-0001-5029-2863/work/43227437 ORCID: /0000-0001-6225-3693/work/43229384 ORCID: /0000-0003-1804-7715/work/43224015 84908673670 adf90404-4835-48af-89e3-063159739fb3 http://hdl.handle.net/10138/233676 000345282600013 other openAccess info:eu-repo/semantics/openAccess gravitational lensing: weak methods: data analysis cosmic background radiation large-scale structure of Universe MICROWAVE BACKGROUND ANISOTROPIES SOUTH-POLE TELESCOPE PROBE WMAP OBSERVATIONS DIGITAL SKY SURVEY POWER SPECTRUM CROSS-CORRELATION GALAXY CLUSTERS NON-GAUSSIANITY DAMPING TAIL MAPS 115 Astronomy Space science Article publishedVersion 2018 ftunivhelsihelda 2023-12-14T00:06:21Z Peer reviewed Article in Journal/Newspaper South pole HELDA – University of Helsinki Open Repository South Pole Astronomy & Astrophysics 571 A17 |
institution |
Open Polar |
collection |
HELDA – University of Helsinki Open Repository |
op_collection_id |
ftunivhelsihelda |
language |
English |
topic |
gravitational lensing: weak methods: data analysis cosmic background radiation large-scale structure of Universe MICROWAVE BACKGROUND ANISOTROPIES SOUTH-POLE TELESCOPE PROBE WMAP OBSERVATIONS DIGITAL SKY SURVEY POWER SPECTRUM CROSS-CORRELATION GALAXY CLUSTERS NON-GAUSSIANITY DAMPING TAIL MAPS 115 Astronomy Space science |
spellingShingle |
gravitational lensing: weak methods: data analysis cosmic background radiation large-scale structure of Universe MICROWAVE BACKGROUND ANISOTROPIES SOUTH-POLE TELESCOPE PROBE WMAP OBSERVATIONS DIGITAL SKY SURVEY POWER SPECTRUM CROSS-CORRELATION GALAXY CLUSTERS NON-GAUSSIANITY DAMPING TAIL MAPS 115 Astronomy Space science Ade, P. A. R. Juvela, M. Keihanen, E. Kurki-Suonio, H. Poutanen, T. Suur-Uski, A. -S. Tuovinen, J. Valiviita, J. Planck Collaboration Planck 2013 results. XVII. Gravitational lensing by large-scale structure |
topic_facet |
gravitational lensing: weak methods: data analysis cosmic background radiation large-scale structure of Universe MICROWAVE BACKGROUND ANISOTROPIES SOUTH-POLE TELESCOPE PROBE WMAP OBSERVATIONS DIGITAL SKY SURVEY POWER SPECTRUM CROSS-CORRELATION GALAXY CLUSTERS NON-GAUSSIANITY DAMPING TAIL MAPS 115 Astronomy Space science |
description |
Peer reviewed |
author2 |
Department of Physics Helsinki Institute of Physics |
format |
Article in Journal/Newspaper |
author |
Ade, P. A. R. Juvela, M. Keihanen, E. Kurki-Suonio, H. Poutanen, T. Suur-Uski, A. -S. Tuovinen, J. Valiviita, J. Planck Collaboration |
author_facet |
Ade, P. A. R. Juvela, M. Keihanen, E. Kurki-Suonio, H. Poutanen, T. Suur-Uski, A. -S. Tuovinen, J. Valiviita, J. Planck Collaboration |
author_sort |
Ade, P. A. R. |
title |
Planck 2013 results. XVII. Gravitational lensing by large-scale structure |
title_short |
Planck 2013 results. XVII. Gravitational lensing by large-scale structure |
title_full |
Planck 2013 results. XVII. Gravitational lensing by large-scale structure |
title_fullStr |
Planck 2013 results. XVII. Gravitational lensing by large-scale structure |
title_full_unstemmed |
Planck 2013 results. XVII. Gravitational lensing by large-scale structure |
title_sort |
planck 2013 results. xvii. gravitational lensing by large-scale structure |
publisher |
EDP sciences |
publishDate |
2018 |
url |
http://hdl.handle.net/10138/233676 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
10.1051/0004-6361/201321543 The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.soirees.esa.int/index.php?project=planck&pagess-Planck_Collaboration. Some of the results in this paper have been derived using the HEALPix package (Gorski et al. 2005). This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the US Department of Energy under Contract No. DE-AC02-05CH11231, as well as of the IN2P3 Computer Center (http://cc.in2p3.fr) and the Planck-HFI data processing center infrastructures hosted at the Institut d'Astrophysique de Paris (France) and financially supported by CNES. We acknowledge support from the Science and Technology Facilities Council [grant number ST/I000976/1]. Ade , P A R , Juvela , M , Keihanen , E , Kurki-Suonio , H , Poutanen , T , Suur-Uski , A -S , Tuovinen , J , Valiviita , J & Planck Collaboration 2014 , ' Planck 2013 results. XVII. Gravitational lensing by large-scale structure ' , Astronomy & Astrophysics , vol. 571 , A17 . https://doi.org/10.1051/0004-6361/201321543 ORCID: /0000-0002-5809-4834/work/43222500 ORCID: /0000-0002-4618-3063/work/43223672 ORCID: /0000-0001-5029-2863/work/43227437 ORCID: /0000-0001-6225-3693/work/43229384 ORCID: /0000-0003-1804-7715/work/43224015 84908673670 adf90404-4835-48af-89e3-063159739fb3 http://hdl.handle.net/10138/233676 000345282600013 |
op_rights |
other openAccess info:eu-repo/semantics/openAccess |
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Astronomy & Astrophysics |
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571 |
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