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    <identifier>10.57760/sciencedb.j00167.00002</identifier>
    <datestamp>2023-11-13T12:49:06Z</datestamp>
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  <dc:date>2023-11-13</dc:date>
  <dc:title>FAST experimental data for paper &amp;quot;Applying hybrid clustering in pulsar candidate sifting with multi-modality for FAST survey&amp;quot;</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.j00167.00002</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>The FAST data set was used to further verify the robustness and efficiency of our proposed algorithm. At first, to change the class imbalance ratio between pulsar and non-pulsar samples in a single block, 1600 known pulsar samples from multiple types were prepared as a known sample set s&amp;prime; and added to this data set. Some of the pulsar samples in s&amp;prime; are known pulsars searched by CRAFTS during synchronization testing, and they can be found in the linked star catalog:http://groups.bao.ac.cn/ism/CRAFTS/CRAFTS/. More over, the dispersion measurement (DM) range of these pulsar samples is often set to [2,1000](cm&amp;minus;3pc). The remaining in s&amp;prime; were collected from foreign surveys such as HTRU.&amp;nbsp;All the new candidates in FAST data&amp;nbsp;(containing the above known sample set s&amp;prime; ) were formed by the DCA fusion of the 1-D feature arrays and related 2-D TVP arrays, which were extracted from corresponding pfd files by the feature extraction programs of HTRU2 and PICS. Moreover, the known sample set s &amp;prime; (1600 real pulsar samples) and 10000 non-pulsar samples were used for DCA algorithm training. Next, the sliding window size was also set to Batchsize = 2 and the unit-size was 1251, then the original data set was divided into (g1, g2, &amp;middot; &amp;middot; &amp;middot;, g125, g126) , where g1, g2, &amp;middot; &amp;middot; &amp;middot;, g125 = 1251 but g126 = 1241 . As a result, the experimental data set consisted of 126 data blocks, i.e.Block(1):[ s&amp;prime; , g1, g2], Block(2):[ s&amp;prime; , g2, g3],..., Block(125):[ s &amp;prime; ,g125, g126], Block(126):[ s&amp;prime; , g126, g1]. Note that, the original 78 pulsar samples from FAST data were randomly distributed in (g1, g2, &amp;middot;&amp;middot;&amp;middot;, g125, g126).&amp;nbsp;</dc:description>
  <dc:subject>astronomy data analysis;  radio pulsars; multivariate analysis</dc:subject>
  <dc:creator>Ziyi You</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:relation>http://www.doi.org/10.1088/1674-4527/ad0c28</dc:relation>
  <dc:publisher>Science Data Bank</dc:publisher>
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