| HAL : hal-00001299, version 1 |
| arXiv : astro-ph/0403363 |
| DOI : 10.1007/b100528 |
| Fiche détaillée | Récupérer au format |
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| Grenade : (2004) |
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| Source separation on astrophysical data sets from the WMAP satellite |
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| G. Patanchon1J. Delabrouille2J.-F. Cardoso3 |
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| (2004) |
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| This paper presents and discusses the application of blind source separation to astrophysical data obtained with the WMAP satellite. Blind separation permits to identify and isolate a component compatible with CMB emission, and to measure both its spatial power spectrum and its emission law. Both are found to be compatible with the present concordance cosmological model. This application demonstrates the usefulness of blind ICA for cosmological applications. |
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| 1 : | Département de Physique - Département de Physique |
| 2 : | PCC - Physique Corpusculaire et Cosmologie - Collège de France |
| 3 : | LTCI - Laboratoire Traitement et Communication de l'Information [Paris] |
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| Domaine | : | Physique/Astrophysique/Cosmologie et astrophysique extra-galactique Planète et Univers/Astrophysique |
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| cosmology – cosmic microwave background – data analysis |
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| Liste des fichiers attachés à ce document : | ||||||||||
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| hal-00001299, version 1 | |
| http://hal.archives-ouvertes.fr/hal-00001299 | |
| oai:hal.archives-ouvertes.fr:hal-00001299 | |
| Contributeur : Jacques Delabrouille | |
| Soumis le : Mardi 16 Mars 2004, 01:08:05 | |
| Dernière modification le : Mardi 5 Septembre 2006, 15:49:52 | |