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<ri:Resource created="2025-03-11T09:35:24Z" status="active" updated="2025-05-19T20:01:23Z" 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>Mapping the Milky Way with Gaia Bp/Rp spectra</title><shortName>J/A+A/695/A75</shortName><identifier>ivo://CDS.VizieR/J/A+A/695/A75</identifier><altIdentifier>doi:10.26093/cds/vizier.36950075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ye X.</name></creator><creator><name>Wu W.</name></creator><creator><name>Allende Prieto C.</name></creator><creator><name>Aguado D.S.</name></creator><creator><name>Zhao J.,Gonzalez Hernandez J.I.</name></creator><creator><name>Rebolo R.</name></creator><creator><name>Zhao G.</name></creator><creator><name>Li Z.</name></creator><creator><name>del Burgo C.</name></creator><creator><name>Chen Y.</name></creator><date role="Updated">2025-05-19T20:01:23Z</date><date role="Created">2025-03-11T09:35:24Z</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>milky-way-galaxy</subject><subject>effective-temperature</subject><subject>metallicity</subject><subject>visible-astronomy</subject><description>Gaia Bp/Rp spectrophotometry for over two hundred million stars has been publicly released as part of Gaia Data Release 3 (DR3). These data have great potential for mapping metallicity across the Milky Way. Several recent studies have analyzed this data set to derive atmospheric parameters and identify new metal-poor stars. In addition, systematics in the fluxes of the Bp/Rp spectra have also been identified and characterized. We aim to construct an alternative catalog of atmospheric parameters from Gaia Bp/Rp spectra by fitting them with synthetic spectra based on model atmospheres, and provide corrections to the Bp/Rp fluxes according to stellar colors, magnitudes, and interstellar extinction. We use GaiaXPy to obtain calibrated spectra and apply FERR to match the corrected Bp/Rp spectra with models and infer atmospheric parameters. We train a neural network (NN) using stars in the Apache Point Observatory Galactic Evolution Experiment (APOGEE) to predict flux corrections as a function of wavelength for each target. Based on the comparison with APOGEE parameters, we conclude that our estimated parameters have systematic errors and uncertainties in Teff, logg, and [M/H] about -38+/-167K, 0.05+/-0.40dex, and -0.12+/-0.19dex, respectively, for stars in the range 4000&lt;=Teff&lt;=7000K. The corrected Bp/Rp spectra show improved agreement with both models and Hubble Space Telescope (HST) CALSPEC data. Our correction increases the precision of the relative spectrophotometry of the Bp/Rp data from 3.2-3.7% to 1.2-2.4%. We also compare our results with other similar catalogs from the literature and validate them using star clusters. Finally, we have built a catalog of atmospheric parameters for stars within 4000&lt;=Teff&lt;=7000K, comprising 68394431 sources, along with a subset of 124 188 stars with [M/H]&lt;=-2.5. Our catalogs and flux correction code are publicly available. Our results confirm that the Gaia Bp/Rp flux calibrated spectra show systematic patterns as a function of wavelength that are tightly related to colors, magnitudes, and extinction. Our optimization algorithm can give us accurate atmospheric parameters of stars with a clear and direct link to models of stellar atmospheres, and can be used to efficiently search for extremely metal-poor (EMP) stars.</description><source format="bibcode">2025A&amp;A...695A..75Y</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/695/A75</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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