THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*
Identifieur interne : 001062 ( Istex/Corpus ); précédent : 001061; suivant : 001063THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*
Auteurs : A. Santagostino Barbone ; E. Gliozzo ; F. D Capito ; I. Memmi Turbanti ; M. Turchiano ; G. VolpeSource :
- Archaeometry [ 0003-813X ] ; 2008-06.
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Abstract
SEM–EDS, EMPA, ICP–MS and ICP–OES were applied to the study of three sectilia panels made of red, orange and yellow glass slabs. In order to determine the chemical state of Cu, XAS was also performed. The results indicate that, with the exception of the red samples, all slabs were made by mixing a siliceous sand with natron. The red slabs show significant compositional differences with respect to K2O and MgO contents, probably linked to the use of plant ashes as a source of alkali. The red, orange and yellow slabs are coloured by metallic copper, cuprite and Pb antimonates, respectively. The comparison between the chemical composition of the Faragola samples and several glass reference groups did not provide conclusive evidence of provenance.
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DOI: 10.1111/j.1475-4754.2007.00341.x
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ISTEX:F14745FAF550DAB1C406A9191BFB3B42CF8E3C86Le document en format XML
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D Capito</name><affiliation><mods:affiliation>GILDA CRG, c/o ESRF BP220, F‐38043 Grenoble, France</mods:affiliation></affiliation></author><author><name sortKey="Memmi Turbanti, I" sort="Memmi Turbanti, I" uniqKey="Memmi Turbanti I" first="I." last="Memmi Turbanti">I. Memmi Turbanti</name><affiliation><mods:affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</mods:affiliation></affiliation></author><author><name sortKey="Turchiano, M" sort="Turchiano, M" uniqKey="Turchiano M" first="M." last="Turchiano">M. Turchiano</name><affiliation><mods:affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</mods:affiliation></affiliation></author><author><name sortKey="Volpe, G" sort="Volpe, G" uniqKey="Volpe G" first="G." last="Volpe">G. Volpe</name><affiliation><mods:affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</mods:affiliation></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:F14745FAF550DAB1C406A9191BFB3B42CF8E3C86</idno><date when="2008" year="2008">2008</date><idno type="doi">10.1111/j.1475-4754.2007.00341.x</idno><idno type="url">https://api.istex.fr/document/F14745FAF550DAB1C406A9191BFB3B42CF8E3C86/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">001062</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">001062</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title><author><name sortKey="Santagostino Barbone, A" sort="Santagostino Barbone, A" uniqKey="Santagostino Barbone A" first="A." last="Santagostino Barbone">A. Santagostino Barbone</name><affiliation><mods:affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</mods:affiliation></affiliation></author><author><name sortKey="Gliozzo, E" sort="Gliozzo, E" uniqKey="Gliozzo E" first="E." last="Gliozzo">E. Gliozzo</name><affiliation><mods:affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</mods:affiliation></affiliation></author><author><name sortKey="D Capito, F" sort="D Capito, F" uniqKey="D Capito F" first="F." last="D Capito">F. D Capito</name><affiliation><mods:affiliation>GILDA CRG, c/o ESRF BP220, F‐38043 Grenoble, France</mods:affiliation></affiliation></author><author><name sortKey="Memmi Turbanti, I" sort="Memmi Turbanti, I" uniqKey="Memmi Turbanti I" first="I." last="Memmi Turbanti">I. Memmi Turbanti</name><affiliation><mods:affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</mods:affiliation></affiliation></author><author><name sortKey="Turchiano, M" sort="Turchiano, M" uniqKey="Turchiano M" first="M." last="Turchiano">M. Turchiano</name><affiliation><mods:affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</mods:affiliation></affiliation></author><author><name sortKey="Volpe, G" sort="Volpe, G" uniqKey="Volpe G" first="G." last="Volpe">G. Volpe</name><affiliation><mods:affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j">Archaeometry</title><idno type="ISSN">0003-813X</idno><idno type="eISSN">1475-4754</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2008-06">2008-06</date><biblScope unit="volume">50</biblScope><biblScope unit="issue">3</biblScope><biblScope unit="page" from="451">451</biblScope><biblScope unit="page" to="473">473</biblScope></imprint><idno type="ISSN">0003-813X</idno></series><idno type="istex">F14745FAF550DAB1C406A9191BFB3B42CF8E3C86</idno><idno type="DOI">10.1111/j.1475-4754.2007.00341.x</idno><idno type="ArticleID">ARCM341</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0003-813X</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>CUPRITE</term><term>FARAGOLA (ITALY)</term><term>GLASS SLABS</term><term>GLASS TECHNOLOGY AND PROVENANCE</term><term>METALLIC Cu</term><term>SECTILIA PANELS</term><term>X‐RAY ABSORPTION SPECTROSCOPY</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">SEM–EDS, EMPA, ICP–MS and ICP–OES were applied to the study of three sectilia panels made of red, orange and yellow glass slabs. In order to determine the chemical state of Cu, XAS was also performed. The results indicate that, with the exception of the red samples, all slabs were made by mixing a siliceous sand with natron. The red slabs show significant compositional differences with respect to K2O and MgO contents, probably linked to the use of plant ashes as a source of alkali. The red, orange and yellow slabs are coloured by metallic copper, cuprite and Pb antimonates, respectively. The comparison between the chemical composition of the Faragola samples and several glass reference groups did not provide conclusive evidence of provenance.</div></front></TEI><istex><corpusName>wiley</corpusName><author><json:item><name>A. SANTAGOSTINO BARBONE</name><affiliations><json:string>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</json:string></affiliations></json:item><json:item><name>E. GLIOZZO</name><affiliations><json:string>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</json:string></affiliations></json:item><json:item><name>F. D’ACAPITO</name><affiliations><json:string>GILDA CRG, c/o ESRF BP220, F‐38043 Grenoble, France</json:string></affiliations></json:item><json:item><name>I. MEMMI TURBANTI</name><affiliations><json:string>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</json:string></affiliations></json:item><json:item><name>M. TURCHIANO</name><affiliations><json:string>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</json:string></affiliations></json:item><json:item><name>G. 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In order to determine the chemical state of Cu, XAS was also performed. The results indicate that, with the exception of the red samples, all slabs were made by mixing a siliceous sand with natron. The red slabs show significant compositional differences with respect to K2O and MgO contents, probably linked to the use of plant ashes as a source of alkali. The red, orange and yellow slabs are coloured by metallic copper, cuprite and Pb antimonates, respectively. The comparison between the chemical composition of the Faragola samples and several glass reference groups did not provide conclusive evidence of provenance.</abstract><qualityIndicators><score>6.464</score><pdfVersion>1.3</pdfVersion><pdfPageSize>484.805 x 697.207 pts</pdfPageSize><refBibsNative>true</refBibsNative><keywordCount>7</keywordCount><abstractCharCount>752</abstractCharCount><pdfWordCount>9298</pdfWordCount><pdfCharCount>56826</pdfCharCount><pdfPageCount>23</pdfPageCount><abstractWordCount>122</abstractWordCount></qualityIndicators><title>THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title><genre><json:string>article</json:string></genre><host><volume>50</volume><publisherId><json:string>ARCM</json:string></publisherId><pages><total>23</total><last>473</last><first>451</first></pages><issn><json:string>0003-813X</json:string></issn><issue>3</issue><genre><json:string>journal</json:string></genre><language><json:string>unknown</json:string></language><eissn><json:string>1475-4754</json:string></eissn><title>Archaeometry</title><doi><json:string>10.1111/(ISSN)1475-4754</json:string></doi></host><publicationDate>2008</publicationDate><copyrightDate>2008</copyrightDate><doi><json:string>10.1111/j.1475-4754.2007.00341.x</json:string></doi><id>F14745FAF550DAB1C406A9191BFB3B42CF8E3C86</id><score>0.048889518</score><fulltext><json:item><original>true</original><mimetype>application/pdf</mimetype><extension>pdf</extension><uri>https://api.istex.fr/document/F14745FAF550DAB1C406A9191BFB3B42CF8E3C86/fulltext/pdf</uri></json:item><json:item><original>false</original><mimetype>application/zip</mimetype><extension>zip</extension><uri>https://api.istex.fr/document/F14745FAF550DAB1C406A9191BFB3B42CF8E3C86/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/F14745FAF550DAB1C406A9191BFB3B42CF8E3C86/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main" xml:lang="en">THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><availability><p>© University of Oxford, 2007</p></availability><date>2008</date></publicationStmt><sourceDesc><biblStruct type="inbook"><analytic><title level="a" type="main" xml:lang="en">THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title><author xml:id="author-1"><persName><forename type="first">A.</forename><surname>SANTAGOSTINO BARBONE</surname></persName><affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</affiliation></author><author xml:id="author-2"><persName><forename type="first">E.</forename><surname>GLIOZZO</surname></persName><affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</affiliation></author><author xml:id="author-3"><persName><forename type="first">F.</forename><surname>D’ACAPITO</surname></persName><affiliation>GILDA CRG, c/o ESRF BP220, F‐38043 Grenoble, France</affiliation></author><author xml:id="author-4"><persName><forename type="first">I.</forename><surname>MEMMI TURBANTI</surname></persName><affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</affiliation></author><author xml:id="author-5"><persName><forename type="first">M.</forename><surname>TURCHIANO</surname></persName><affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</affiliation></author><author xml:id="author-6"><persName><forename type="first">G.</forename><surname>VOLPE</surname></persName><affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</affiliation></author></analytic><monogr><title level="j">Archaeometry</title><idno type="pISSN">0003-813X</idno><idno type="eISSN">1475-4754</idno><idno type="DOI">10.1111/(ISSN)1475-4754</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2008-06"></date><biblScope unit="volume">50</biblScope><biblScope unit="issue">3</biblScope><biblScope unit="page" from="451">451</biblScope><biblScope unit="page" to="473">473</biblScope></imprint></monogr><idno type="istex">F14745FAF550DAB1C406A9191BFB3B42CF8E3C86</idno><idno type="DOI">10.1111/j.1475-4754.2007.00341.x</idno><idno type="ArticleID">ARCM341</idno></biblStruct></sourceDesc></fileDesc><profileDesc><creation><date>2008</date></creation><langUsage><language ident="en">en</language></langUsage><abstract xml:lang="en"><p>SEM–EDS, EMPA, ICP–MS and ICP–OES were applied to the study of three sectilia panels made of red, orange and yellow glass slabs. In order to determine the chemical state of Cu, XAS was also performed. The results indicate that, with the exception of the red samples, all slabs were made by mixing a siliceous sand with natron. The red slabs show significant compositional differences with respect to K2O and MgO contents, probably linked to the use of plant ashes as a source of alkali. The red, orange and yellow slabs are coloured by metallic copper, cuprite and Pb antimonates, respectively. The comparison between the chemical composition of the Faragola samples and several glass reference groups did not provide conclusive evidence of provenance.</p></abstract><textClass xml:lang="en"><keywords scheme="keyword"><list><head>keywords</head><item><term>SECTILIA PANELS</term></item><item><term>FARAGOLA (ITALY)</term></item><item><term>GLASS SLABS</term></item><item><term>X‐RAY ABSORPTION SPECTROSCOPY</term></item><item><term>METALLIC Cu</term></item><item><term>CUPRITE</term></item><item><term>GLASS TECHNOLOGY AND PROVENANCE</term></item></list></keywords></textClass></profileDesc><revisionDesc><change when="2008-06">Published</change></revisionDesc></teiHeader></istex:fulltextTEI><json:item><original>false</original><mimetype>text/plain</mimetype><extension>txt</extension><uri>https://api.istex.fr/document/F14745FAF550DAB1C406A9191BFB3B42CF8E3C86/fulltext/txt</uri></json:item></fulltext><metadata><istex:metadataXml wicri:clean="Wiley, elements deleted: body"><istex:xmlDeclaration>version="1.0" encoding="UTF-8" standalone="yes"</istex:xmlDeclaration><istex:document><component version="2.0" type="serialArticle" xml:lang="en"><header><publicationMeta level="product"><publisherInfo><publisherName>Blackwell Publishing Ltd</publisherName><publisherLoc>Oxford, UK</publisherLoc></publisherInfo><doi origin="wiley" registered="yes">10.1111/(ISSN)1475-4754</doi><issn type="print">0003-813X</issn><issn type="electronic">1475-4754</issn><idGroup><id type="product" value="ARCM"></id><id type="publisherDivision" value="ST"></id></idGroup><titleGroup><title type="main" sort="ARCHAEOMETRY">Archaeometry</title></titleGroup></publicationMeta><publicationMeta level="part" position="06003"><doi origin="wiley">10.1111/arch.2008.50.issue-3</doi><numberingGroup><numbering type="journalVolume" number="50">50</numbering><numbering type="journalIssue" number="3">3</numbering></numberingGroup><coverDate startDate="2008-06">June 2008</coverDate></publicationMeta><publicationMeta level="unit" type="article" position="4" status="forIssue"><doi origin="wiley">10.1111/j.1475-4754.2007.00341.x</doi><idGroup><id type="unit" value="ARCM341"></id></idGroup><countGroup><count type="pageTotal" number="23"></count></countGroup><titleGroup><title type="tocHeading1">Original Articles</title></titleGroup><copyright>© University of Oxford, 2007</copyright><eventGroup><event type="firstOnline" date="2007-10-25"></event><event type="publishedOnlineFinalForm" date="2007-10-25"></event><event type="xmlConverted" agent="Converter:BPG_TO_WML3G version:2.3.5 mode:FullText source:FullText result:FullText" date="2010-04-06"></event><event type="xmlConverted" agent="Converter:WILEY_ML3G_TO_WILEY_ML3GV2 version:3.8.8" date="2014-01-05"></event><event type="xmlConverted" agent="Converter:WML3G_To_WML3G version:4.1.7 mode:FullText,remove_FC" date="2014-10-15"></event></eventGroup><numberingGroup><numbering type="pageFirst" number="451">451</numbering><numbering type="pageLast" number="473">473</numbering></numberingGroup><linkGroup><link type="toTypesetVersion" href="file:ARCM.ARCM341.pdf"></link></linkGroup></publicationMeta><contentMeta><unparsedEditorialHistory>*Received 12 May 2006; accepted 28 November 2006</unparsedEditorialHistory><countGroup><count type="figureTotal" number="9"></count><count type="tableTotal" number="4"></count><count type="formulaTotal" number="0"></count><count type="referenceTotal" number="64"></count><count type="wordTotal" number="8079"></count></countGroup><titleGroup><title type="main">THE <i>SECTILIA</i> PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title><title type="shortAuthors"><i>A. Santagostino Barbone </i>et al.</title><title type="short"><i>The</i> sectilia <i>panels of Faragola (Ascoli Satriano, southern Italy)</i></title></titleGroup><creators><creator creatorRole="author" xml:id="cr1" affiliationRef="#a1"><personName><givenNames>A.</givenNames><familyName>SANTAGOSTINO BARBONE</familyName></personName></creator><creator creatorRole="author" xml:id="cr2" affiliationRef="#a1"><personName><givenNames>E.</givenNames><familyName>GLIOZZO</familyName></personName></creator><creator creatorRole="author" xml:id="cr3" affiliationRef="#a2"><personName><givenNames>F.</givenNames><familyName>D’ACAPITO</familyName></personName></creator><creator creatorRole="author" xml:id="cr4" affiliationRef="#a1"><personName><givenNames>I.</givenNames><familyName>MEMMI TURBANTI</familyName></personName></creator><creator creatorRole="author" xml:id="cr5" affiliationRef="#a3"><personName><givenNames>M.</givenNames><familyName>TURCHIANO</familyName></personName></creator><creator creatorRole="author" xml:id="cr6" affiliationRef="#a3"><personName><givenNames>G.</givenNames><familyName>VOLPE</familyName></personName></creator></creators><affiliationGroup><affiliation xml:id="a1" countryCode="IT"><unparsedAffiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</unparsedAffiliation></affiliation><affiliation xml:id="a2" countryCode="FR"><unparsedAffiliation>GILDA CRG, c/o ESRF BP220, F‐38043 Grenoble, France</unparsedAffiliation></affiliation><affiliation xml:id="a3" countryCode="IT"><unparsedAffiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</unparsedAffiliation></affiliation></affiliationGroup><keywordGroup xml:lang="en"><keyword xml:id="k1"><i>SECTILIA </i>PANELS</keyword><keyword xml:id="k2">FARAGOLA (ITALY)</keyword><keyword xml:id="k3">GLASS SLABS</keyword><keyword xml:id="k4">X‐RAY ABSORPTION SPECTROSCOPY</keyword><keyword xml:id="k5">METALLIC Cu</keyword><keyword xml:id="k6">CUPRITE</keyword><keyword xml:id="k7">GLASS TECHNOLOGY AND PROVENANCE</keyword></keywordGroup><abstractGroup><abstract type="main" xml:lang="en"><p> <i>SEM–EDS, EMPA, ICP–MS and ICP–OES were applied to the study of three</i> sectilia <i>panels made of red, orange and yellow glass slabs. In order to determine the chemical state of Cu, XAS was also performed. The results indicate that, with the exception of the red samples, all slabs were made by mixing a siliceous sand with natron. The red slabs show significant compositional differences with respect to K<sub>2</sub>O and MgO contents, probably linked to the use of plant ashes as a source of alkali. The red, orange and yellow slabs are coloured by metallic copper, cuprite and Pb antimonates, respectively. The comparison between the chemical composition of the Faragola samples and several glass reference groups did not provide conclusive evidence of provenance.</i></p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>The sectilia panels of Faragola (Ascoli Satriano, southern Italy)</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>THE SECTILIA PANELS OF FARAGOLA (ASCOLI SATRIANO, SOUTHERN ITALY): A MULTI‐ANALYTICAL STUDY OF THE RED, ORANGE AND YELLOW GLASS SLABS*</title></titleInfo><name type="personal"><namePart type="given">A.</namePart><namePart type="family">SANTAGOSTINO BARBONE</namePart><affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">E.</namePart><namePart type="family">GLIOZZO</namePart><affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">F.</namePart><namePart type="family">D’ACAPITO</namePart><affiliation>GILDA CRG, c/o ESRF BP220, F‐38043 Grenoble, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">I.</namePart><namePart type="family">MEMMI TURBANTI</namePart><affiliation>Department of Earth Sciences, University of Siena, via Laterina 8, 53100 Siena, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">M.</namePart><namePart type="family">TURCHIANO</namePart><affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">G.</namePart><namePart type="family">VOLPE</namePart><affiliation>Department of Human Sciences, University of Foggia, via Arpi 155, 71100 Foggia, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article"></genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><place><placeTerm type="text">Oxford, UK</placeTerm></place><dateIssued encoding="w3cdtf">2008-06</dateIssued><edition>*Received 12 May 2006; accepted 28 November 2006</edition><copyrightDate encoding="w3cdtf">2008</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><internetMediaType>text/html</internetMediaType><extent unit="figures">9</extent><extent unit="tables">4</extent><extent unit="references">64</extent><extent unit="words">8079</extent></physicalDescription><abstract lang="en">SEM–EDS, EMPA, ICP–MS and ICP–OES were applied to the study of three sectilia panels made of red, orange and yellow glass slabs. In order to determine the chemical state of Cu, XAS was also performed. The results indicate that, with the exception of the red samples, all slabs were made by mixing a siliceous sand with natron. The red slabs show significant compositional differences with respect to K2O and MgO contents, probably linked to the use of plant ashes as a source of alkali. The red, orange and yellow slabs are coloured by metallic copper, cuprite and Pb antimonates, respectively. The comparison between the chemical composition of the Faragola samples and several glass reference groups did not provide conclusive evidence of provenance.</abstract><subject lang="en"><genre>keywords</genre><topic>SECTILIA PANELS</topic><topic>FARAGOLA (ITALY)</topic><topic>GLASS SLABS</topic><topic>X‐RAY ABSORPTION SPECTROSCOPY</topic><topic>METALLIC Cu</topic><topic>CUPRITE</topic><topic>GLASS TECHNOLOGY AND PROVENANCE</topic></subject><relatedItem type="host"><titleInfo><title>Archaeometry</title></titleInfo><genre type="journal">journal</genre><identifier type="ISSN">0003-813X</identifier><identifier type="eISSN">1475-4754</identifier><identifier type="DOI">10.1111/(ISSN)1475-4754</identifier><identifier type="PublisherID">ARCM</identifier><part><date>2008</date><detail type="volume"><caption>vol.</caption><number>50</number></detail><detail type="issue"><caption>no.</caption><number>3</number></detail><extent unit="pages"><start>451</start><end>473</end><total>23</total></extent></part></relatedItem><identifier type="istex">F14745FAF550DAB1C406A9191BFB3B42CF8E3C86</identifier><identifier type="DOI">10.1111/j.1475-4754.2007.00341.x</identifier><identifier type="ArticleID">ARCM341</identifier><accessCondition type="use and reproduction" contentType="copyright">© University of Oxford, 2007</accessCondition><recordInfo><recordContentSource>WILEY</recordContentSource><recordOrigin>Blackwell Publishing Ltd</recordOrigin></recordInfo></mods></metadata><serie></serie></istex></record>Pour manipuler ce document sous Unix (Dilib)
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