<?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>2026-06-08T01:04:15Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/59519" metadataPrefix="marc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/59519</identifier><datestamp>2023-08-25T19:48:53Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><record xmlns="http://www.loc.gov/MARC21/slim" 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://www.loc.gov/MARC21/slim http://www.loc.gov/standards/marcxml/schema/MARC21slim.xsd">
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      <subfield code="a">Cenarro, A. J.</subfield>
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      <subfield code="a">Gorgas García, Francisco Javier</subfield>
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      <subfield code="a">Cardiel López, Nicolás</subfield>
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      <subfield code="a">Pedraz, S.</subfield>
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      <subfield code="a">Peletier, R. F.</subfield>
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      <subfield code="a">Vazdekis, A.</subfield>
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   <datafield ind2=" " ind1=" " tag="260">
      <subfield code="c">2001-09-21</subfield>
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      <subfield code="a">We present a homogeneous set of stellar atmospheric parameters (T-eff, log g, [Fe/H]) for a sample of about 700 field and cluster stars which constitute a new stellar library in the near-IR developed for stellar population synthesis in this spectral region (lambda 8350-9020). Having compiled the available atmospheric data in the literature for field stars, we have found systematic deviations between the atmospheric parameters from different bibliographic references. The Soubiran, Katz &amp; Cayrel sample of stars with very well determined fundamental parameters has been taken as our standard reference system, and other papers have been calibrated and bootstrapped against it. The obtained transformations are provided in this paper. Once most of the data sets were on the same system, final parameters were derived by performing error weighted means. Atmospheric parameters for cluster stars have also been revised and updated according to recent metallicity scales and colour-temperature relations.</subfield>
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   <datafield ind1="8" ind2=" " tag="024">
      <subfield code="a">0035-8711</subfield>
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      <subfield code="a">10.1046/j.1365-8711.2001.04689.x</subfield>
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      <subfield code="a">https://hdl.handle.net/20.500.14352/59519</subfield>
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      <subfield code="a">http://dx.doi.org/10.1046/j.1365-8711.2001.04689.x</subfield>
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      <subfield code="a">http://mnras.oxfordjournals.org/</subfield>
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   <datafield ind2="0" ind1="0" tag="245">
      <subfield code="a">Empirical calibration of the near-infrared CaII triplet - II. The stellar atmospheric parameters</subfield>
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