<?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>2026-10-13T11:01:52Z</responseDate>
    <request verb="GetRecord" metadataPrefix="oai_dc" identifier="10.57760/sciencedb.j00167.00012" >https://www.scidb.cn/oai</request>
<GetRecord>
    <record>
    <header >
    <identifier>10.57760/sciencedb.j00167.00012</identifier>
    <datestamp>2025-03-07T10:11:03Z</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>2025-03-07</dc:date>
  <dc:title>Chemical Abundances of OCs in the Current Sample (Extract). The full table is available at the ScienceDB</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.j00167.00012</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>| **Column** | **字段名** | **解释** | **单位/备注** ||-----------|-----------|---------|--------------|| **Column 1**&amp;nbsp;| **Cluster** | 疏散星团名称 |&amp;nbsp;|| **Column 2**&amp;nbsp;| **RA_ICRS** | 赤经（ICRS 坐标） |&amp;nbsp;|| **Column 3**&amp;nbsp;| **DE_ICRS** | 赤纬（ICRS 坐标） |&amp;nbsp;|| **Column 4**&amp;nbsp;| **RV** | 径向速度 | km/s || **Column 5**&amp;nbsp;| **Rgc** | 银心距离 | pc || **Column 6**&amp;nbsp;| **log age50** | 对数年龄 |&amp;nbsp;|| **Column 7**&amp;nbsp;| **[O/Fe]mean** | [O/Fe] 均值 |&amp;nbsp;|| **Column 8**&amp;nbsp;| **[O/Fe]std** | [O/Fe] 标准差 |&amp;nbsp;|| **Column 9**&amp;nbsp;| **[Mg/Fe]mean** | [Mg/Fe] 均值 |&amp;nbsp;|| **Column 10** | **[Mg/Fe]std** | [Mg/Fe] 标准差 |&amp;nbsp;|| **Column 11** | **[Si/Fe]mean** | [Si/Fe] 均值 |&amp;nbsp;|| **Column 12** | **[Si/Fe]std** | [Si/Fe] 标准差 |&amp;nbsp;|| **Column 13** | **[Ca/Fe]mean** | [Ca/Fe] 均值 |&amp;nbsp;|| **Column 14** | **[Ca/Fe]std** | [Ca/Fe] 标准差 |&amp;nbsp;|| **Column 15** | **[Ti/Fe]mean** | [Ti/Fe] 均值 |&amp;nbsp;|| **Column 16** | **[Ti/Fe]std** | [Ti/Fe] 标准差 |&amp;nbsp;|</dc:description>
  <dc:subject>echniques:XGBoost model; LAMOST DR11 — stars:Open clusters — stars: individual: α-elements abundances; chemical gradients; galactic chemical evolution</dc:subject>
  <dc:creator>Chengyuan Wu</dc:creator>
  <dc:creator>Ruyuan Zhang</dc:creator>
  <dc:creator>Jianxing Chen</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/publicdomain/zero/1.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:relation>http://www.doi.org/10.1088/1674-4527/adba29</dc:relation>
  <dc:publisher>Science Data Bank</dc:publisher>
</oai_dc:dc>

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