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    <identifier>10.11922/sciencedb.o00069.00003</identifier>
    <datestamp>2023-08-18T16:12:57Z</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>2023-08-18</dc:date>
  <dc:title>Photometric redshifts and galaxy clusters for DES DR2, DESI DR9 and HSC-SSP PDR3</dc:title>
  <dc:identifier>doi:10.11922/sciencedb.o00069.00003</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>Photometric redshift (photo-z) is a fundamental parameter for multi-wavelength photometric surveys, while galaxy clusters are important cosmological probers and ideal objects for exploring the dense environmental impact on galaxy evolution. We extend our previous work on estimating photo-z and detecting galaxy clusters to the latest data releases of the Dark Energy Spectroscopic Instrument (DESI) imaging surveys, Dark Energy Survey (DES), and Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) imaging surveys and make corresponding catalogs publicly available for more extensive scientific applications. The photo-z catalogs include accurate measurements of photo-z and stellar mass for about 320, 293, and 134 million galaxies with r&amp;lt;23, i&amp;lt;24, and i&amp;lt;25 in DESI DR9, DES DR2, and HSC-SSP PDR3 data, respectively. The photo-z accuracy is about 0.017, 0.024, and 0.029 and the general redshift coverage is z&amp;lt;1, z&amp;lt;1.2, and z&amp;lt;1.6, respectively for those three surveys. The uncertainties of the logarithmic stellar mass that is inferred from stellar population synthesis fitting is about 0.2 dex. With the above photo-z catalogs, galaxy clusters are detected using a fast cluster-finding algorithm. A total of 532,810, 86,963, and 36,566 galaxy clusters with the number of members larger than 10 are discovered for DESI, DES, and HSC-SSP, respectively. Their photo-z accuracy is at the level of 0.01. The total mass of our clusters are also estimated by using the calibration relations between the optical richness and the mass measurement from X-ray and radio observations.&amp;nbsp;The catalogs including(A) Photo-z and stellar mass1. desdr2_galaxy_cspcat: total catalog of photo-z and stellar mass for DES DR2&amp;nbsp;&amp;nbsp;photoz_desdr2: dividing the catalog into smaller files&amp;nbsp;&amp;nbsp;filename: desdr2_galaxy_cspcat_raXXX_YYY.fits, where XXX and YYY is the lower and upper limits of R.A in degrees2. desidr9_galaxy_cspcat.fits: total catalog of photo-z and stellar mass for DESI DR9&amp;nbsp;&amp;nbsp;photoz_desidr9: dividing the catalog into smaller files&amp;nbsp;&amp;nbsp;filename: desidr9_galaxy_cspcat_raXXX_YYY.fits, where XXX and YYY is the lower and upper limits of R.A in degrees3. hscpdr3_wide_galaxy_cspcat.fits: total catalog of photo-z and stellar mass for HSC-SSP PDR3&amp;nbsp;&amp;nbsp;photoz_hscpdr3: dividing the catalog into smaller files&amp;nbsp;&amp;nbsp;filename: hscpdr3_wide_galaxy_cspcat_raXXX_YYY.fits, where XXX and YYY is the lower and upper limits of R.A in degrees(B) Galaxy clusters1. galaxy_clusters_desdr2.fits: catalog of galaxy clusters for DES DR22. galaxy_clusters_desidr9.fits: catalog of galaxy clusters for DESI DR93. galaxy_clusters_hscpdr3_wide.fits: catalog of galaxy clusters for HSC-SSP PDR3</dc:description>
  <dc:subject>survey; photometric redshifts; galaxy cluster; stellar mass</dc:subject>
  <dc:creator>Hu Zou</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/publicdomain/zero/1.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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