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<ri:Resource created="1999-12-19T21:24:44Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>The Optical Spectrum of RR Tel</title><shortName>J/A+AS/139/135</shortName><identifier>ivo://CDS.VizieR/J/A+AS/139/135</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Crawford F.L.</name></creator><creator><name>McKenna F.C.</name></creator><creator><name>Keenan F.P.</name></creator><creator><name>Aller L.H.</name></creator><creator><name>Feibelman W.A.,Ryan S.G.</name></creator><date role="Updated">1999-12-19T20:36:21Z</date><date role="Created">1999-12-19T21:24:44Z</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>variable-stars</subject><subject>novae</subject><subject>spectroscopy</subject><description>The symbiotic nova RR Telescopii has been observed with the 3.9 m telescope at the Anglo-Australian Observatory (AAO), using the University College London Echelle Spectrograph (UCLES) in conjunction with a Tek CCD. It displays a rich emission line spectrum, ranging in excitation from NI to NiVIII. We present a list of 811 measured lines, with their suggested identifications and absolute line intensities, covering a wavelength range from 3180 to 9455 A. The absolute line intensities have been derived by comparing the high resolution data with a flux-calibrated low resolution spectrum taken with the Australian National University 2.3 m telescope. All of the lines have been successfully identified. Comparing our results with those of previous studies indicates that the RR Tel system is advancing towards higher degrees of ionisation.</description><source format="bibcode">1999A&amp;AS..139..135C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/139/135</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/139/135</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/139/135</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/139/135</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/139/135</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/139/135</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/139/135</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+AS/139/135/table2</name><description>Line list for RR Telescopii, with absolute flux calibrated intensities shown, for the wavelength range 3490 - 5530{AA}</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LambdaMea</name><description>Measured wavelength</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DeltaV</name><description>Velocity FWHM</description><unit>km/s</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_DeltaV</name><description>[h] Note on DeltaV (2)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Int</name><description>Measured intensity</description><unit>1e-12mW.m**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Intc</name><description>Corrected intensity (1)</description><unit>1e-12mW.m**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_Intc</name><description>[efgkl] Note on Intc (2)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Line</name><description>Identity of line</description><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>n_Line</name><description>[j] Note on line (3)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>LambdaLab</name><description>Laboratory wavelength</description><unit>0.1nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>n_LambdaLab</name><description>[bcgi] Note on labLam (2)</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Mult</name><description>? Multiplet number</description><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>F</name><description>[F] F: forbidden line</description><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/A+AS/139/135/table3</name><description>Line list for RR Telescopii, in the wavelength range 3183 - 3488{AA} and 5550 - 9456{AA}, with intensities flux calibrated using the HeII recombination line ratios of Hummer and Storey (1987MNRAS.224..801H) and Storey and Hummer (1995MNRAS.272...41S)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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