<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-19T16:16:45Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/9222" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/9222</identifier><datestamp>2025-12-05T16:41:17Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478823</setSpec><setSpec>col_2072_478917</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   <dc:title>Bayesian image reconstruction with space-variant noise suppression</dc:title>
   <dc:creator>Núñez de Murga, Jorge, 1955-</dc:creator>
   <dc:creator>Llacer, Jorge</dc:creator>
   <dc:subject>Processament de dades</dc:subject>
   <dc:subject>Anàlisi de dades</dc:subject>
   <dc:subject>Estadística bayesiana</dc:subject>
   <dc:subject>Image processing</dc:subject>
   <dc:subject>Data analysis</dc:subject>
   <dc:description>In this paper we present a Bayesian image reconstruction algorithm with entropy prior (FMAPE) that uses a space-variant hyperparameter. The spatial variation of the hyperparameter allows different degrees of resolution in areas of different statistical characteristics, thus avoiding the large residuals resulting from algorithms that use a constant hyperparameter. In the first implementation of the algorithm, we begin by segmenting a Maximum Likelihood Estimator (MLE) reconstruction. The segmentation method is based on using a wavelet decomposition and a self-organizing neural network. The result is a predetermined number of extended regions plus a small region for each star or bright object. To assign a different value of the hyperparameter to each extended region and star, we use either feasibility tests or cross-validation methods. Once the set of hyperparameters is obtained, we carried out the final Bayesian reconstruction, leading to a reconstruction with decreased bias and excellent visual characteristics. The method has been applied to data from the non-refurbished Hubble Space Telescope. The method can be also applied to ground-based images.</dc:description>
   <dc:date>2009-08-28T08:23:48Z</dc:date>
   <dc:date>2009-08-28T08:23:48Z</dc:date>
   <dc:date>1998</dc:date>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
   <dc:identifier>0365-0138</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2445/9222</dc:identifier>
   <dc:identifier>500848</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>Reproducció del document publicat a http://dx.doi.org/10.1051/aas:1998259</dc:relation>
   <dc:relation>Astronomy and Astrophysics Supplement Series, 1998, vol. 131, núm. 2, p. 167-180.</dc:relation>
   <dc:relation>http://dx.doi.org/10.1051/aas:1998259</dc:relation>
   <dc:rights>(c) The European Southern Observatory, 1998</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:format>14 p.</dc:format>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>EDP Sciences</dc:publisher>
   <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
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