<?xml version="1.0" encoding="UTF-8"?>

<?xml-stylesheet type="text/xsl" href="/static/oaitohtml.xsl"?>

<!--
<?xml-stylesheet type="text/xsl" href="/oaitohtml.xsl"?>
-->

<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
    <responseDate>2026-10-10T16:15:06Z</responseDate>
    <request verb="GetRecord" metadataPrefix="oai_dc" identifier="10.57760/sciencedb.20581" >https://www.scidb.cn/oai</request>
<GetRecord>
    <record>
    <header >
    <identifier>10.57760/sciencedb.20581</identifier>
    <datestamp>2025-02-06T10:02:20Z</datestamp>
</header>
    <metadata>
        
<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:date>2025-02-06</dc:date>
  <dc:title>A Catalog of 13CO Clumps from the MWISP</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.20581</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>The dataset is a catalog of the dense structures obtained by using the FacetClumps algorithm (version 0.0.8, https://pypi.org/project/FacetClumps/) to analyze the MWISP 13CO (J = 1 &amp;minus; 0) data.The data covers the Milky Way within the longitude range 10&amp;deg; &amp;lt; l &amp;lt; 230&amp;deg; and the latitude range of |b| &amp;lt; 5&amp;deg;.25.The velocity range is -200 to 200&amp;nbsp;km s&amp;minus;1.The data to be detected are signal-to-noise ratio (SNR) data.The detection parameters are as follows:RMS: The global noise level of the data, measured in intensity units. When the detection target is SNR data, the RMS is set to 1.Threshold: The threshold for truncating the signal, measured in intensity units. It is set to 5 * RMS.SWindow: The scale of the window function, measured in voxels. It is set to 3.KBins: The coefficient used to calculate the number of feature value intervals, unitless. It is set to 35.FwhmBeam: The full width at half maximum (FWHM) of the device beam, measured in voxels. It is set to 2.VeloRes: The resolution of the device's velocity channel, measured in voxels. It is set to 2.SRecursionLBV: The minimum area in the spatial direction and the minimum length in the velocity channel when recursion terminates, measured in voxels: [SRecursionLB, SRecursionV]. It is set to [16, 5].A total of 71,604 molecular cloud clumps were detected.</dc:description>
  <dc:subject>CO; clumps; MWISP</dc:subject>
  <dc:creator>Zheng Sheng</dc:creator>
  <dc:creator>Jiang Zhibo</dc:creator>
  <dc:creator>huang yao</dc:creator>
  <dc:creator>Chen Zhiwei</dc:creator>
  <dc:creator>Liu Dejian</dc:creator>
  <dc:creator>Luo Xiaoyu</dc:creator>
  <dc:creator>Jiang Yu</dc:creator>
  <dc:rights>RESTRICTED</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
</oai_dc:dc>

    </metadata>
</record>
</GetRecord>
</OAI-PMH>