<?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>2026-04-13T13:22:34Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/121016" metadataPrefix="qdc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/121016</identifier><datestamp>2025-12-05T17:01:16Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478823</setSpec><setSpec>col_2072_478904</setSpec><setSpec>col_2072_478917</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>HfS, Hyperfine Structure Fitting Tool</dc:title>
   <dc:creator>Estalella, Robert</dc:creator>
   <dc:subject>Molècules</dc:subject>
   <dc:subject>Estructura molecular</dc:subject>
   <dc:subject>Molecules</dc:subject>
   <dc:subject>Molecular structure</dc:subject>
   <dcterms:abstract>Hyperfine Structure Fitting (HfS) is a tool to fit the hyperfine structure of spectral lines with multiple velocity components. The HfS_nh3 procedures included in HfS simultaneously fit the hyperfine structure of the NH3 (J, K) = (1, 1) and (2, 2) transitions, and perform a standard analysis to derive ${T}_{\mathrm{ex}}$, NH3 column density, ${T}_{\mathrm{rot}}$, and ${T}_{{\rm{k}}}$. HfS uses a Monte Carlo approach for fitting the line parameters. Special attention is paid to the derivation of the parameter uncertainties. HfS includes procedures that make use of parallel computing for fitting spectra from a data cube.</dcterms:abstract>
   <dcterms:issued>2018-03-22T14:24:11Z</dcterms:issued>
   <dcterms:issued>2018-03-22T14:24:11Z</dcterms:issued>
   <dcterms:issued>2017-02</dcterms:issued>
   <dcterms:issued>2018-03-22T14:24:11Z</dcterms:issued>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
   <dc:relation>Reproducció del document publicat a: https://doi.org/10.1088/1538-3873/129/972/025003</dc:relation>
   <dc:relation>Publications of the Astronomical Society of the Pacific, 2017, vol. 129, num. 025003</dc:relation>
   <dc:relation>https://doi.org/10.1088/1538-3873/129/972/025003</dc:relation>
   <dc:rights>(c) Estalella, Robert, 2017</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:publisher>Astronomical Society of the Pacific</dc:publisher>
   <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
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