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<ri:Resource created="2020-12-25T10:30:16Z" 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>GIBS sources equivalent widths</title><shortName>J/A+A/645/A14</shortName><identifier>ivo://CDS.VizieR/J/A+A/645/A14</identifier><altIdentifier>doi:10.26093/cds/vizier.36450014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Zhao H.</name></creator><creator><name>Schultheis M.</name></creator><creator><name>Recio-Blanco A.</name></creator><creator><name>Kordopatis G.</name></creator><creator><name>de Laverny P.,Rojas-Arriagada A.</name></creator><creator><name>Zoccali M.</name></creator><creator><name>Surot F.</name></creator><creator><name>Valenti E.</name></creator><date role="Updated">2021-06-17T12:55:31Z</date><date role="Created">2020-12-25T10:30:16Z</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>interstellar-medium</subject><subject>line-intensities</subject><description>We developed a set of procedures to automatically detect and measure the DIB around 8620{AA} (the Gaia DIB) for a wide range of temperatures. The method was tested on about 5000 spectra from the Giraffe Inner Bulge Survey (GIBS; Zoccali et al., 2014A&amp;A...562A..66Z), and 4194 reasonable fitting results were got. We made use of the reddenings, E(J-Ks), from the extinction map developed by Surot et al. (2020arXiv201002723S). A linear correlation between the equivalent width (EW) and E(J-Ks) was derived as E(J-Ks)/EW = 1.875, according to E(B-V)/EW = 2.721, which is highly consistent with previous results toward similar sightlines. After a correction based on the Vista Variables in the Via Lactea (VVV; Minniti et al., 2010NewA...15..433M) database for both EW and E(J-Ks), the coefficient derived from individual GIBS fields, E(J-Ks)/EW=1.884, is also in perfect agreement with literature values. Based on a subsample of 1015 stars toward the Galactic center, we determined a rest-frame wavelength of the Gaia DIB as 8620.55{AA}. A Gaussian profile is proved to be a proper and stable assumption for the Gaia DIB as no intrinsic asymmetry is found.</description><source format="bibcode">2021A&amp;A...645A..14Z</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/645/A14</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/II/348">II/348 : VISTA Variable in the Via Lactea Survey DR2 (Minniti+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A66">J/A+A/562/A66 : GIRAFFE Inner Bulge Survey (GIBS). I. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GIBS</name><description>GIBS target name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>GLON</name><description>[] Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>EW</name><description>Measured equivalent width</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_EW</name><description>Error of equivalent width</description><unit>0.1nm</unit><ucd>stat.error;spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. 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