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<ri:Resource created="2008-06-29T14:58:46Z" status="active" updated="2025-06-13T15:25:00Z" 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>Refractive index for silicon carbide (SiC)</title><shortName>J/A+A/483/661</shortName><identifier>ivo://CDS.VizieR/J/A+A/483/661</identifier><altIdentifier>doi:10.26093/cds/vizier.34830661</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pitman K.M.</name></creator><creator><name>Hofmeister A. M.</name></creator><creator><name>Corman A.B.</name></creator><creator><name>Speck A.K.</name></creator><date role="Updated">2008-06-29T15:01:53Z</date><date role="Created">2008-06-29T14:58:46Z</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>infrared-astronomy</subject><subject>spectroscopy</subject><subject>astronomical-models</subject><description>The SiC optical constants are fundamental inputs for radiative transfer (RT) models of astrophysical dust environments. However, previously published values contain errors and do not adequately represent the bulk physical properties of the cubic ({beta}) SiC polytype usually found around carbon stars. We provide new, uncompromised optical constants for {beta}- and {alpha}-SiC derived from single-crystal reflectance spectra and investigate quantitatively (i) whether there is any difference between {alpha}- and {beta}-SiC that can be seen in infrared (IR) spectra and optical functions and (ii) whether weak features from {lambda}~12.5-13.0{mu}m need to be fitted. We measured mid- and far-IR reflectance spectra for two samples of 3C ({beta}-)SiC and four samples of 6H ({alpha}-)SiC. For the latter group, we acquired polarized data (E{perpendicular.to}c, E{parallel.to}c orientations). 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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>lambda</name><description>Wavelength</description><unit>um</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>n</name><description>Real part of complex refractive index</description><ucd>phys.refractIndex</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>k</name><description>Imaginary part of complex refractive index</description><ucd>phys.refractIndex</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/A+A/483/661/grysicpa</name><description>Optical constants for gray 6H-SiC powder, extraordinary ray (table 4)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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