dc.contributor.author | Lanz Oca, Luis Fernando | |
dc.contributor.author | Herranz Muñoz, Diego | |
dc.contributor.author | Sanz Estévez, José Luis | |
dc.contributor.author | González-Nuevo, J. | |
dc.contributor.author | López-Caniego Alcarria, Marcos | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2023-03-10T12:17:50Z | |
dc.date.available | 2023-03-10T12:17:50Z | |
dc.date.issued | 2010 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.issn | 1365-2966 | |
dc.identifier.other | ESP2004-07067-C03-01 | es_ES |
dc.identifier.uri | https://hdl.handle.net/10902/28128 | |
dc.description.abstract | In this work, we deal with the problem of simultaneous multifrequency detection of extragalactic point sources in maps of the cosmic microwave background. We developed a linear filtering technique that takes into account the spatial and the cross-power spectrum information at the same time. By using realistic simulations, we compared this technique with the monofrequency matched filter in terms of completeness, reliability, flux and spectral index accuracy. The multifrequency method outperforms the matched filter in all the studied cases in this work. | es_ES |
dc.description.sponsorship | The authors acknowledge partial financial support from the Spanish Ministry of Education (MEC) under project ESP2004-07067-C03-01 and the joint CNR-CSIC research projects 2006-IT-0037 and 2008IT0059. LFL acknowledges the Spanish CSIC for a JAE-Predoc fellowship and the hospitality of the Osservatorio Astronomico di Padova (INAF) during a research stay. Partial financial support for this research has been provided to JLS by the Spanish MEC and to JG-N by the Italian ASI (contracts Planck LFI Activity of Phase E2 and I/016/07/0 COFIS) and MUR. JG-N also acknowledges a researcher position grant at the SISSA (Trieste). ML-C acknowledges a post-doctoral fellowship from EGEE-III (FP7 INFSO-RI 222667). The authors are grateful to Raquel Fraga Encinas for reading carefully this paper and her style and grammatical suggestions and acknowledge the use of the PSM, developed by the Component Separation Working Group (WG2) of the Planck Collaboration. | es_ES |
dc.format.extent | 11 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Oxford University Press | es_ES |
dc.rights | This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2010 The Authors. Journal compilation ©2010 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | es_ES |
dc.source | Monthly Notices of the Royal Astronomical Society, 2010, 403(4), 2120-2130 | es_ES |
dc.subject.other | Methods: data analysis | es_ES |
dc.subject.other | Techniques: image processing | es_ES |
dc.subject.other | Surveys | es_ES |
dc.subject.other | Cosmic microwave background | es_ES |
dc.subject.other | Radio continuum: galaxies. | es_ES |
dc.title | A multifrequency method based on the matched multifilter for the detection of point sources in CMB maps | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1111/j.1365-2966.2010.16260.x | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1111/j.1365-2966.2010.16260.x | |
dc.type.version | publishedVersion | es_ES |