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dc.contributor.author | Alonso, P. | es_ES |
dc.contributor.author | Argüeso, F. | es_ES |
dc.contributor.author | Cortina, R. | es_ES |
dc.contributor.author | Ranilla, J. | es_ES |
dc.contributor.author | Vidal Maciá, Antonio Manuel | es_ES |
dc.date.accessioned | 2014-09-09T12:01:34Z | |
dc.date.issued | 2013-04 | |
dc.identifier.issn | 0259-9791 | |
dc.identifier.uri | http://hdl.handle.net/10251/39515 | |
dc.description.abstract | Abstract In this work we present a suitable computational tool to deal with large matrices and solve systems of non-linear equations. This technique is applied to a very interesting problem: the detection and flux estimation of point sources in Cos- mic Microwave Background (CMB) maps, which allows a good determination of CMB primordial fluctuations and leads to a better knowledge of the chemistry at the early stages of the Universe. The method uses previous information about the statis- tical properties of the sources, so that this knowledge is incorporated in a Bayesian scheme. Simulations show that our approach allows the detection of more sources than previous non-Bayesian techniques, with a small computation time | es_ES |
dc.description.sponsorship | This work was financially supported by the Spanish Ministerio de Ciencia e Innovacion and by FEDER Projects (TEC2012-38142-C04, TIN2010-14971, TEC2009-13741 and CAPAP-H4 TIN2011-15734-E) Universitat Politecnica de Valencia through Programa de Apoyo a la Investigacion y Desarrollo (PAID-05-11) and Generalitat Valenciana through project PROMETEO/2009/013. We thank Diego Herranz for his help with the CMB simulations. | en_EN |
dc.language | Inglés | es_ES |
dc.publisher | Springer Verlag (Germany) | es_ES |
dc.relation.ispartof | Journal of Mathematical Chemistry | es_ES |
dc.rights | Reserva de todos los derechos | es_ES |
dc.subject | Cosmic microwave background | es_ES |
dc.subject | Bayesian | es_ES |
dc.subject | Non-linear systems | es_ES |
dc.subject | Efficiency | es_ES |
dc.subject.classification | CIENCIAS DE LA COMPUTACION E INTELIGENCIA ARTIFICIAL | es_ES |
dc.title | Non-linear parallel solver for detecting point sources in CMB maps using Bayesian techniques | es_ES |
dc.type | Artículo | es_ES |
dc.identifier.doi | 10.1007/s10910-012-0078-7 | |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//TEC2009-13741/ES/Spatial Audio Systems Based On Massive Parallel Processing Of Multichannel Acoustic Signals With General Purpose-Graphics Processing Units (Gp-Gpu) And Multicores/ / | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/UPV//PAID-05-11/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/Generalitat Valenciana//PROMETEO09%2F2009%2F013/ES/Computacion de altas prestaciones sobre arquitecturas actuales en porblemas de procesado múltiple de señal/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//TIN2010-14971/ES/REDUCCION DE CARACTERISTICAS Y COMPUTACION DE ALTAS PRESTACIONES EN PROBLEMAS DE ALTA DIMENSIONALIDAD/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//TEC2012-38142-C04-01/ES/PROCESADO DISTRIBUIDO Y COLABORATIVO DE SEÑALES SONORAS: CONTROL ACTIVO/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//TIN2011-15734-E/ES/RED DE COMPUTACION DE ALTAS PRESTACIONES SOBRE ARQUITECTURAS PARALELAS HETEROGENEAS (CAPAP-H4) RENOVACION/ | es_ES |
dc.rights.accessRights | Cerrado | es_ES |
dc.contributor.affiliation | Universitat Politècnica de València. Departamento de Sistemas Informáticos y Computación - Departament de Sistemes Informàtics i Computació | es_ES |
dc.description.bibliographicCitation | Alonso, P.; Argüeso, F.; Cortina, R.; Ranilla, J.; Vidal Maciá, AM. (2013). Non-linear parallel solver for detecting point sources in CMB maps using Bayesian techniques. Journal of Mathematical Chemistry. 51(4):1153-1163. https://doi.org/10.1007/s10910-012-0078-7 | es_ES |
dc.description.accrualMethod | S | es_ES |
dc.relation.publisherversion | http://link.springer.com/article/10.1007%2Fs10910-012-0078-7 | es_ES |
dc.description.upvformatpinicio | 1153 | es_ES |
dc.description.upvformatpfin | 1163 | es_ES |
dc.type.version | info:eu-repo/semantics/publishedVersion | es_ES |
dc.description.volume | 51 | es_ES |
dc.description.issue | 4 | es_ES |
dc.relation.senia | 235694 | |
dc.contributor.funder | Generalitat Valenciana | es_ES |
dc.contributor.funder | Universitat Politècnica de València | es_ES |
dc.contributor.funder | Ministerio de Ciencia e Innovación | es_ES |
dc.description.references | P. Alonso, D. Argüelles, J. Ranilla, A.M. Vidal, The solution of Block-Toeplitz linear systems of equations in multicore computers. J. Supercomput. (2012). doi: 10.1007/s11227-012-0824-4 | es_ES |
dc.description.references | Alonso P., Argüeso F., Cortina R., Ranilla J., Vidal A.M.: Detecting point sources in CMB maps using an eficient parallel algorithm. J. Math. Chem. 50, 410–420 (2012) | es_ES |
dc.description.references | Argüeso F., Salerno E., Herranz D., Sanz J.L., Kuruoglu E.E., Kayabol K.: A Bayesian technique for the detection of point sources in CMB maps. Mon. Not. Roy. Astron. Soc. 414, 410–417 (2011) | es_ES |
dc.description.references | Carvalho P., Rocha G., Hobson M.: A fast Bayesian approach to discrete object detection in astronomical images. PowellSnakes I. Mon. Not. Roy. Astron. Soc. 393, 681 (2009) | es_ES |
dc.description.references | Planck Collaboration, P.A.R. Ade et al. Planck early results I. The Planck mission. Astron. Astrophys. 536, A1 (2011) | es_ES |
dc.description.references | De Zotti G. et al.: Predictions for high-frequency radio surveys of extragalactic sources. Astron. Astrophys. 431, 893–903 (2005) | es_ES |
dc.description.references | Dubrovich V.K.: Blurring of spatial microwave fluctuations by molecular last scattering. Astron. Lett. J. Astron. Space Astrophys. 19, 53 (1993) | es_ES |
dc.description.references | Golub G.H., Van Loan C.F.: Matrix Computations. Johns Hopkins University Press, Baltimore (1996) | es_ES |
dc.description.references | Herranz D., Vielva P.: Microwave backgound images. IEEE Signal Process. Mag. 27, 67–75 (2010) | es_ES |
dc.description.references | D. Herranz, F. Argüeso, P. Carvalho, Compact source detection in multichannel microwave surveys: from SZ clusters to polarized sources. Adv. Astron. (2012). doi: 10.1155/2012/410965 | es_ES |
dc.description.references | Maoli R., Melchiorri F., Tosti D.: Molecules in the postrecombination universe and microwave background anisotropies. Astrophys. J. 425, 372 (1994) | es_ES |
dc.description.references | Nolta M.R. et al.: Five-year wilkinson microwave anisotropy probe (WMAP) observations: angular power spectrum. Astrophys. J. Suppl. 180, 296 (2009) | es_ES |
dc.description.references | Penzias A.A., Wilson R.W.: A measurement of excess antenna temperature at 4,080 Mc/s. Astrophys. J. 142, 419–421 (1965) | es_ES |
dc.description.references | Schleicher D.R.G. et al.: Effects of primordial chemistry on the cosmic microwave background. Astron. Astrophys. 490, 521 (2008) | es_ES |
dc.description.references | Smoot G. et al.: Structure in the COBE differential microwave radiometer first-year maps. Astrophys. J. 396, L1–L5 (1992) | es_ES |
dc.description.references | Spergel D.N. et al.: First-year Wilkinson microwave anisotropy probe (WMAP) observations: determination of cosmological parameters. Astrophys. J. Suppl. 148, 175–194 (2003) | es_ES |
dc.description.references | StructPack: a high performance PACKage for STRUCTred Matrices. http://www.inco2.upv.es/structpack.html | es_ES |
dc.description.references | Wax M., Kailath T.: Efficient inversion of Toeplitz-block Toeplitz matrix. IEEE T. Acoust. Speech. 31, 5 (1983) | es_ES |