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<ri:Resource created="2019-11-12T15:10:26Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>NGC 6397 stars MUSE spectra</title><shortName>J/A+A/588/A148</shortName><identifier>ivo://CDS.VizieR/J/A+A/588/A148</identifier><altIdentifier>doi:10.26093/cds/vizier.35880148</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Husser T.-O.</name></creator><creator><name>Kamann S.</name></creator><creator><name>Dreizler S.</name></creator><creator><name>Wendt M.</name></creator><creator><name>Wulff N.</name></creator><creator><name>Bacon R.,Wisotzki L.</name></creator><creator><name>Brinchmann J.</name></creator><creator><name>Weilbacher P.M.</name></creator><creator><name>Roth M.M.</name></creator><creator><name>Monreal-ibero A.</name></creator><date role="Updated">2022-03-23T16:26:54Z</date><date role="Created">2019-11-12T15:10:26Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>globular-star-clusters</subject><subject>stellar-populations</subject><subject>spectroscopy</subject><description>We demonstrate the high multiplex advantage of crowded field 3D spectroscopy with the new integral field spectrograph MUSE by means of a spectroscopic analysis of more than 12000 individual stars in the globular cluster NGC 6397. The stars are deblended with a point spread function fitting technique, using a photometric reference catalogue from HST as prior, including relative positions and brightnesses. This catalogue is also used for a first analysis of the extracted spectra, followed by an automatic in-depth analysis via a full-spectrum fitting method based on a large grid of PHOENIX spectra. We analysed the largest sample so far available for a single globular cluster of 18 932 spectra from 12 307 stars in NGC 6397. We derived a mean radial velocity of v_rad_=17.84+/-0.07km/s and a mean metallicity of [Fe/H]=-2.120+/-0.002, with the latter seemingly varying with temperature for stars on the red giant branch (RGB). We determine Teff and [Fe/H] from the spectra, and log g from HST photometry. This is the first very comprehensive Hertzsprung-Russell diagram (HRD) for a globular cluster based on the analysis of several thousands of stellar spectra, ranging from the main sequence to the tip of the RGB. 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