{"@context":"http://schema.org","@id":"https://doi.org/10.17182/hepdata.133217.v1/t3","@reverse":{"isBasedOn":[{"@type":"ScholarlyArticle","identifier":{"@type":"PropertyValue","propertyID":"URL","value":"https://inspirehep.net/literature/2112341"}},{"@id":"https://doi.org/10.1103/PhysRevLett.130.112301","@type":"JournalArticle"}]},"@type":"Dataset","additionalType":"Dataset","author":{"@type":"Organization","name":"STAR Collaboration"},"creator":{"@type":"Organization","name":"STAR Collaboration"},"datePublished":"2023","description":"Upper limit of inclusive Y(3S) $R_{AA}$ with 95% confidence level in 0-60% Au+Au collisions at 200 GeV","distribution":[{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/1465950/root","description":"ROOT file","encodingFormat":"https://root.cern"},{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/1465950/yaml","description":"YAML file","encodingFormat":"https://yaml.org"},{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/1465950/csv","description":"CSV file","encodingFormat":"text/csv"},{"@type":"DataDownload","contentUrl":"https://www.hepdata.net/download/table/1465950/yoda","description":"YODA file","encodingFormat":"https://yoda.hepforge.org"}],"identifier":[{"@type":"PropertyValue","propertyID":"HEPDataRecord","value":"https://www.hepdata.net/record/ins2112341?version=1"},{"@type":"PropertyValue","propertyID":"HEPDataRecordAlt","value":"https://www.hepdata.net/record/133217"}],"inLanguage":"en","includedInDataCatalog":{"@id":"https://doi.org/10.17182/hepdata.133217.v1","@type":"DataCatalog","url":"https://www.hepdata.net/record/ins2112341?version=1"},"isPartOf":{"@id":"https://doi.org/10.17182/hepdata.133217.v1","@type":"Dataset","description":"We report on measurements of sequential $\\Upsilon$ suppression in Au+Au collisions at $\\sqrt{s_{_\\mathrm{NN}}}$ = 200 GeV with the STAR detector at the Relativistic Heavy Ion Collider (RHIC) through both the dielectron and dimuon decay channels. In the 0-60\\% centrality class, the nuclear modification factors ($R_{\\mathrm{AA}}$), which quantify the level of yield suppression in heavy-ion collisions compared to p+p collisions, for $\\Upsilon$(1S) and $\\Upsilon$(2S) are $0.40 \\pm 0.03~\\textrm{(stat.)} \\pm 0.03~\\textrm{(sys.)} \\pm 0.09~\\textrm{(norm.)}$ and $0.26 \\pm 0.08~\\textrm{(stat.)} \\pm 0.02~\\textrm{(sys.)} \\pm 0.06~\\textrm{(norm.)}$, respectively, while the upper limit of the $\\Upsilon$(3S) $R_{\\mathrm{AA}}$ is 0.17 at a 95\\% confidence level. This provides experimental evidence that the $\\Upsilon$(3S) is significantly more suppressed than the $\\Upsilon$(1S) at RHIC. The level of suppression for $\\Upsilon$(1S) is comparable to that observed at the much higher collision energy at the Large Hadron Collider. These results point to the creation of a medium at RHIC whose temperature is sufficiently high to strongly suppress excited $\\Upsilon$ states.","name":"Observation of sequential $\\Upsilon$ suppression in Au+Au collisions at $\\sqrt{s_{_\\mathrm{NN}}}$ = 200 GeV with the STAR experiment","url":"https://www.hepdata.net/record/ins2112341?version=1"},"keywords":"$R_{AA}$, Au+Au --> Y(3S) + X","name":"Figure 2.3","provider":{"@type":"Organization","name":"HEPData"},"publisher":{"@type":"Organization","name":"HEPData"},"url":"https://www.hepdata.net/record/138362","version":1}