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<ri:Resource created="2019-05-24T08:28:55Z" 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>CIELO-RGS, soft X-ray ionized emission lines catalog</title><shortName>J/A+A/625/A122</shortName><identifier>ivo://CDS.VizieR/J/A+A/625/A122</identifier><altIdentifier>doi:10.26093/cds/vizier.36250122</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mao J.</name></creator><creator><name>Kaastra J.S.</name></creator><creator><name>Guainazzi M.</name></creator><creator><name>Gonzalez-Riestra R.,Santos-Lleo M.</name></creator><creator><name>Kretschmar P.</name></creator><creator><name>Grinberg V.</name></creator><creator><name>Kalfountzou E.</name></creator><creator><name>Ibarra A.,Matzeu G.</name></creator><creator><name>Parker M.</name></creator><creator><name>Rodriguez-Pascual P.</name></creator><date role="Updated">2019-07-24T11:31:32Z</date><date role="Created">2019-05-24T08:28:55Z</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>x-ray-sources</subject><subject>spectroscopy</subject><description>High-resolution X-ray spectroscopy has advanced our understanding of the hot Universe by revealing physical properties like kinematics, temperature, and abundances of the astrophysical plasmas. Despite technical and scientific achievements, the lack of scientific products at a level higher than count spectra is hampering complete scientific exploitation of high-quality data. This paper introduces the Catalog of Ionized Emission Lines Observed by the Reflection Grating Spectrometer (CIELO-RGS) onboard the XMM-Newton space observatory. The CIELO-RGS catalog aims to facilitate the exploitation of emission features in the public RGS spectra archive. In particular, we aim to analyze the relationship between X-ray spectral diagnostics parameters and measurements at other wavelengths. This paper focuses on the methodology of catalog generation, describing the automated line-detection algorithm. A moderate sample (~2400 observations) of high-quality RGS spectra available at XMM-Newton Science Archive is used as our starting point. A list of potential emission lines is selected based on a multi-scale peak-detection algorithm in a uniform and automated way without prior assumption on the underlying astrophysical model. The candidate line list is validated via spectral fitting with simple continuum and line profile models. We also compare the catalog content with published literature results on a small number of exemplary sources. We generate a catalog of emission lines (1.2x10^4^) detected in ~1600 observations toward stars, X-ray binaries, supernovae remnants, active galactic nuclei, and groups and clusters of galaxies. For each line, we report the observed wavelength, broadening, energy and photon flux, equivalent width, and so on.</description><source format="bibcode">2019A&amp;A...625A.122M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/625/A122</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/B/xmm">B/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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bname</description><ucd>obs.param;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>z</name><description>Redshift (1)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ObsIDs</name><description>Observation ID</description><ucd>meta.id;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>lambda</name><description>Observed wavelength of the line (1)</description><unit>0.1nm</unit><ucd>em.wl;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_lambda</name><description>The uncertainty of the wavelength (1)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_lambda</name><description>The uncertainty of the wavelength (1)</description><unit>0.1nm</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Width</name><description>Observed FWHM of the line (1)</description><unit>0.1nm</unit><ucd>spect.line.width;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Width</name><description>The uncertainty of the FWHM (1)</description><unit>0.1nm</unit><ucd>stat.error;spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Width</name><description>The uncertainty of the FWHM (1)</description><unit>0.1nm</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Norm</name><description>Observed normalization of the line (1)</description><unit>1e+44ph.s**-1</unit><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Norm</name><description>The uncertainty of the Norm (1)</description><unit>1e+44ph.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_Norm</name><description>The uncertainty of the Norm (1)</description><unit>1e+44ph.s**-1</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Fluxeng</name><description>Observed energy flux of the line (1)</description><unit>W.m**-2</unit><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Fluxph</name><description>Observed photon flux of the line (1)</description><ucd>phot.flux;spect.line</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>cFluxpho</name><description>Modeled (spline) continuum flux density at the line center (ph/m^2^/s/{AA}) (1)</description><ucd>phot.flux;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>EW</name><description>Equivalent width of the line (1)</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_RA</name><description>Position from XMM log (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Position from XMM log (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>