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    <responseDate>2026-10-11T10:26:15Z</responseDate>
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    <identifier>10.57760/sciencedb.12869</identifier>
    <datestamp>2025-10-13T10:51:04Z</datestamp>
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    <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>2025-10-13</dc:date>
  <dc:title>Dust extinction map of the Galactic plane based on the UKIDSS survey data</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.12869</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>We have generated 2D dust extinction maps with spatial resolutions ranging from 30 arcsec to 300 arcsec using the UKIDSS/GPS photometric catalog. These maps cover the entire about 1800 deg2 area of the Galactic plane surveyed by UKIDSS/GPS. The maps were produced utilizing the XPNICER technique, an advancement of the previous PNICER and Xpercentile methods. Here we released all extinction maps and associated uncertainty and number density maps at different spatial resolutions and X0 configurations.</dc:description>
  <dc:subject>infrared ; extinction map; dust; photomery;  survey</dc:subject>
  <dc:creator>Miaomiao Zhang</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by-nc/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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