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    <responseDate>2026-10-12T15:34:43Z</responseDate>
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    <identifier>10.57760/sciencedb.0135a</identifier>
    <datestamp>2026-09-28T10:45:58Z</datestamp>
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<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>2026-09-28</dc:date>
  <dc:title>Catalog of 4916 &amp;sup1;&amp;sup3;CO Molecular Clouds from the MWISP Survey Identified with GDCluster</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.0135a</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>This dataset provides the catalog of 4916 &amp;sup1;&amp;sup3;CO (J = 1&amp;ndash;0) molecular clouds used in &amp;quot;How Intensity Threshold Shapes the Velocity Dispersion&amp;ndash;Size Relation in Molecular Clouds&amp;quot; (Qi, Liu &amp;amp; Du, [journal/DOI to be added]). The clouds were identified from the Milky Way Imaging Scroll Painting (MWISP) survey, covering the second Galactic quadrant (104.75&amp;deg; &amp;le; l &amp;le; 150.25&amp;deg;, &amp;minus;5.25&amp;deg; &amp;le; b &amp;le; 5.25&amp;deg;), using the GDCluster algorithm (Liu &amp;amp; Du 2025), which incorporates spatial-continuity constraints during Gaussian decomposition and clustering to separate kinematically blended velocity components.Kinematic distances were derived from the line-of-sight velocity (VLSR) using the Galactic rotation curve model of Reid et al. (2019). Clouds with |VLSR| &amp;lt; 10 km/s were excluded to ensure reliable distance estimates, leaving the final sample of 4916 clouds reported here.Each entry corresponds to a cloud's native GDCluster boundary (prior to any intensity-threshold reprocessing described in the paper) and includes its Galactic coordinates, centroid velocity, kinematic distance, effective radius, velocity dispersion, peak brightness temperature, voxel count, and a velocity-group label (corresponding to the two spiral-arm subgroups defined by VLSR = &amp;minus;23.55 km/s in the paper).&amp;nbsp;</dc:description>
  <dc:subject> Molecular clouds; Scaling relations;  Interstellar dynamics; co line emission</dc:subject>
  <dc:creator>Yaru Qi</dc:creator>
  <dc:creator>Fujun Du</dc:creator>
  <dc:creator>Xin Liu</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by-nc-nd/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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