<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Kambali, I.</author>
             <author>Astarina, H.</author>
             <author>Huda, N.</author>
             <author>Ismuha, R.R.</author>
             <author>Kardinah, K.</author>
             <author>Listiawadi, F.D.</author>
             <author>Marlina, M.</author>
             <author>Parwanto, P.</author>
             <author>Rajiman, R.</author>
             <author>Suryanto, H.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Production of F-18 and Tc-99m Radionuclides using an 11 MeV Proton Accelerating Cyclotron
          </title>
       </titles>
		 <publisher>JACoW</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>978-3-95450-167-0</isbn>
		 <electronic-resource-num>10.18429/JACoW-Cyclotrons2016-MOP13</electronic-resource-num>
		 <language>English</language>
		 <pages>83-86</pages>
       <pages>MOP13</pages>
       <keywords>
          <keyword>target</keyword>
          <keyword>proton</keyword>
          <keyword>cyclotron</keyword>
          <keyword>positron</keyword>
          <keyword>radioactivity</keyword>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2017</year>
          <pub-dates>
             <date>2017-01</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>http://dx.doi.org/10.18429/JACoW-Cyclotrons2016-MOP13</url>
              <url>http://jacow.org/cyclotrons2016/papers/mop13.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          An 11-MeV proton-accelerating cyclotron has been employed to produce F-18 and Tc-99m radionuclides. In this report, F-18 radionuclide was produced from enriched-water target whereas Tc-99m was generated from natural molybdenum trioxide (MoO3) target. Two recoiled radioactive impurities such as Co-56 and Ag-110m are identified in the F-18 solution whereas N-13 was recognized as an impurity in the Tc-99m production. The Co-56 radionuclidic impurity is presumably sputtered off the havar window in the target system whereas Ag-110m is originally from a silver body housing the enriched water target which is generated by secondary neutron irradiated Ag-10⁹. In addition, N-13 impurity found in the post-irradiated MoO3 target occurs presumably via (p,He-4) nuclear reaction.
       </abstract>
    </record>
  </records>
</xml>
