@prefix prodottidellaricerca: . @prefix istituto: . @prefix prodotto: . istituto:CDS036 prodottidellaricerca:prodotto prodotto:ID24468 . @prefix rdf: . prodotto:ID24468 rdf:type prodotto:TIPO1101 . @prefix retescientifica: . prodotto:ID24468 rdf:type retescientifica:ProdottoDellaRicerca . @prefix rdfs: . prodotto:ID24468 rdfs:label "Search for correlation between GRB's detected by bepposax (Articolo in rivista)"@en . @prefix xsd: . @prefix pubblicazioni: . prodotto:ID24468 pubblicazioni:anno "2002-01-01T00:00:00+01:00"^^xsd:gYear . @prefix skos: . prodotto:ID24468 skos:altLabel "
Astone P., Bassan M., Bonifazi P., Carelli P., Castellano G., Coccia E., Cosmelli C., D'Agostini G., D'Antonio S., Fafone V., Federici G., Frontera F., Guidorzi C., Marini A., Minenkov Y., Modena I., Modestino G., Moleti A., Pallottino G. V., Torrioli G. (2002)
Search for correlation between GRB's detected by bepposax
"^^rdf:HTML ; pubblicazioni:autori "Astone P., Bassan M., Bonifazi P., Carelli P., Castellano G., Coccia E., Cosmelli C., D'Agostini G., D'Antonio S., Fafone V., Federici G., Frontera F., Guidorzi C., Marini A., Minenkov Y., Modena I., Modestino G., Moleti A., Pallottino G. V., Torrioli G."^^xsd:string ; pubblicazioni:paginaInizio "102002"^^xsd:string ; pubblicazioni:numeroVolume "66"^^xsd:string ; skos:note "ISI Web of Science (WOS)"^^xsd:string ; pubblicazioni:titolo "Search for correlation between GRB's detected by bepposax"^^xsd:string ; prodottidellaricerca:abstract "Data obtained during five months of 2001 with the gravitational wave (GW) \ndetectors EXPLORER and NAUTILUS, operating with a bandwidth of a few Hz at \nfrequencies near 900 Hz, were studied in correlation with the gamma ray \nburst data (GRB) obtained with the BeppoSAX satellite. During this period \nBeppoSAX was the only GRB satellite in operation, while EXPLORER and \nNAUTILUS were the only GW detectors in operation. No correlation between \nthe GW data and the GRB bursts was found. The analysis, performed over 47 \nGRB's, excludes the presence of signals of amplitude h>=6.5\u00D710\u009619, with \n95% probability, if we allow a time delay between GW bursts and GRB within \n\u00B15 s, and h>=1.2\u00D710\u009618, if the time delay is within \u00B1400 s. The result is \nalso provided in the form of scaled likelihood for unbiased interpretation \nand easier use for further analysis." ; prodottidellaricerca:prodottoDi istituto:CDS036 .