<?xml version='1.0' encoding='UTF-8'?>
<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd">
  <responseDate>2026-03-12T13:57:27Z</responseDate>
  <request verb="GetRecord" metadataPrefix="jpcoar_1.0" identifier="oai:fut.repo.nii.ac.jp:00000742">https://fut.repo.nii.ac.jp/oai</request>
  <GetRecord>
    <record>
      <header>
        <identifier>oai:fut.repo.nii.ac.jp:00000742</identifier>
        <datestamp>2023-06-20T14:26:14Z</datestamp>
        <setSpec>1</setSpec>
      </header>
      <metadata>
        <jpcoar:jpcoar xmlns:datacite="https://schema.datacite.org/meta/kernel-4/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcndl="http://ndl.go.jp/dcndl/terms/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:jpcoar="https://github.com/JPCOAR/schema/blob/master/1.0/" xmlns:oaire="http://namespace.openaire.eu/schema/oaire/" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:rioxxterms="http://www.rioxx.net/schema/v2.0/rioxxterms/" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns="https://github.com/JPCOAR/schema/blob/master/1.0/" xsi:schemaLocation="https://github.com/JPCOAR/schema/blob/master/1.0/jpcoar_scm.xsd">
          <dc:title>Discovery of Decimeter Radio Wave Pulses from Super Massive Black Holes in the Center Region of Our Galaxy : First Preliminary Results</dc:title>
          <jpcoar:creator>
            <jpcoar:creatorName>Oya, Hiroshi</jpcoar:creatorName>
          </jpcoar:creator>
          <datacite:description descriptionType="Abstract">Pulses of decimeter wavelength radio waves, in the frequency bands of 1.4GHz and 1.6GHz, arriving from the center part of our Galaxy have been discovered by observations made from July 25 to August 26,2005 at Awara Space and Cosmic Radio wave Observatory of Space Communication Science and Technology in Fukui University of Technology, The identified pulse periods are 129.99, 104.55 and 52.003 sec which correspond, respectively to Gaa, Gab, and Gac that had been already detected in decameter wavelength range. Because the decameter wave pulses have been considered to be from the rotating super massive black holes, the origins of decimeter radio pulses detected in the present study can also be considered to be radiated from the same black holes in the center part of our Galaxy.</datacite:description>
          <dc:publisher>福井工業大学</dc:publisher>
          <datacite:date dateType="Issued">2006-03-18</datacite:date>
          <dc:language>eng</dc:language>
          <dc:type rdf:resource="http://purl.org/coar/resource_type/c_6501">departmental bulletin paper</dc:type>
          <oaire:version rdf:resource="http://purl.org/coar/version/c_970fb48d4fbd8a85">VoR</oaire:version>
          <jpcoar:identifier identifierType="DOI">https://doi.org/10.57375/00000736</jpcoar:identifier>
          <jpcoar:identifier identifierType="URI">https://fut.repo.nii.ac.jp/records/742</jpcoar:identifier>
          <jpcoar:identifierRegistration identifierType="JaLC">10.57375/00000736</jpcoar:identifierRegistration>
          <jpcoar:relation>
            <jpcoar:relatedIdentifier identifierType="NCID">TF00009195</jpcoar:relatedIdentifier>
          </jpcoar:relation>
          <jpcoar:sourceIdentifier identifierType="ISSN">2868571</jpcoar:sourceIdentifier>
          <jpcoar:sourceTitle>福井工業大学研究紀要. 第一部</jpcoar:sourceTitle>
          <jpcoar:issue>36</jpcoar:issue>
          <jpcoar:pageStart>221</jpcoar:pageStart>
          <jpcoar:pageEnd>228</jpcoar:pageEnd>
          <jpcoar:file>
            <jpcoar:URI label="KJ00004437943.pdf">https://fut.repo.nii.ac.jp/record/742/files/KJ00004437943.pdf</jpcoar:URI>
            <jpcoar:mimeType>application/pdf</jpcoar:mimeType>
            <jpcoar:extent>637.1 kB</jpcoar:extent>
            <datacite:date dateType="Available">2023-04-12</datacite:date>
          </jpcoar:file>
        </jpcoar:jpcoar>
      </metadata>
    </record>
  </GetRecord>
</OAI-PMH>
