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<ri:Resource created="2023-11-17T11:25:02Z" 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>FeI and FeII abundances with LOTUS</title><shortName>J/AJ/165/145</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/145</identifier><altIdentifier>doi:10.26093/cds/vizier.51650145</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li Y.</name></creator><creator><name>Ezzeddine R.</name></creator><date role="Updated">2024-02-13T12:09:40Z</date><date role="Created">2023-11-17T11:25:02Z</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>astronomical-models</subject><subject>stellar-atmospheres</subject><subject>metallicity</subject><subject>effective-temperature</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>Precise fundamental atmospheric stellar parameters and abundance determination of individual elements in stars are important for all stellar population studies. Non-local thermodynamic equilibrium (non-LTE; hereafter NLTE) models are often important for such high precision, however, can be computationally complex and expensive, which renders the models less utilized in spectroscopic analyses. To alleviate the computational burden of such models, we developed a robust 1D, NLTE fundamental atmospheric stellar parameter derivation tool, LOTUS, to determine the effective temperature Teff, surface gravity logg, metallicity [Fe/H], and microturbulent velocity v_mic_ for FGK-type stars, from equivalent width (EW) measurements of FeI and FeII lines. We utilize a generalized curve of growth method to take into account the EW dependencies of each FeI and FeII line on the corresponding atmospheric stellar parameters. A global differential evolution optimization algorithm is then used to derive the fundamental parameters. Additionally, LOTUS can determine precise uncertainties for each stellar parameter using a Markov Chain Monte Carlo algorithm. We test and apply LOTUS on a sample of benchmark stars, as well as stars with available asteroseismic surface gravities from the K2 survey, and metal-poor stars from the Gaia-ESO and R-Process Alliance surveys. We find very good agreement between our NLTE-derived parameters in LOTUS to nonspectroscopic values on average within Teff={+/-}30K, and logg={+/-}0.10dex for benchmark stars. We provide open access of our code, as well as of the interpolated precomputed NLTE EW grids available on Github (the software is available on GitHubunder an MIT License, and version 0.1.1 (as the persistent version) is archived in Zenodo) and documentation with working examples.</description><source format="bibcode">2023AJ....165..145L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/145</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/III/283">III/283 : RAVE 6th data release (Steinmetz+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16) (Ahumada+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/109">J/PASJ/57/109 : Late-G giants abundances (Takeda+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A54">J/A+A/512/A54 : Teff and Fbol from Infrared Flux Method (Casagrande+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A138">J/A+A/530/A138 : Geneva-Copenhagen survey re-analysis (Casagrande+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A38">J/A+A/558/A38 : FAMA code stellar parameters and abundances (Magrini+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/769/57">J/ApJ/769/57 : Equivalent widths of metal-poor stars (Frebel+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A119">J/A+A/564/A119 : CoRoT red giants abundances (Morel+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A133">J/A+A/564/A133 : Gaia FGK benchmark stars; metallicity (Jofre+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/575/A26">J/A+A/575/A26 : Properties of Population II star HD 140283 (Creevey+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/397">J/MNRAS/450/397 : Spectroscopic study of RGs in Kepler field (Takeda+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A2">J/A+A/587/A2 : SP_Ace derived data from stellar spectra (Boeche+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/592/A70">J/A+A/592/A70 : Gaia FGK stars; low-metallicities candidates (Hawkins+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/144">J/AJ/151/144 : ASPCAP weight for 15 APOGEE chemical elements (Garcia+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/608/A89">J/A+A/608/A89 : Very metal poor stars in MW halo (Mashonkina+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/847/142">J/ApJ/847/142 : Ultrametalpoor stars LTE &amp; NLTE abundances (Ezzeddine+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/612/A90">J/A+A/612/A90 : Inelastic Fe+H collision data (Barklem, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/18">J/AJ/156/18 : APOGEE DR14;Binary comp. evolved stars (Price-Whelan+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/92">J/ApJ/858/92 : RPA Southern Pilot Search of 107 Stars (Hansen+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/865/129">J/ApJ/865/129 : Abundance analysis of HD 222925 (Roederer+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/868/110">J/ApJ/868/110 : R-Process Alliance; DR1 in Galactic halo (Sakari+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/625/A33">J/A+A/625/A33 : Radial velocity time series of HD 122563 (Creevey+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/628/A54">J/A+A/628/A54 : Fe, Mg, Ti in Galactic clusters (Kovalev+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A25">J/A+A/640/A25 : Metal-poor stars limb-darkening coeff. 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