A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys
Based on the DESI Legacy Imaging Surveys released data and available spectroscopic redshifts, we identify 1.58 million clusters of galaxies by searching for the overdensity of the stellar mass distribution of galaxies within redshift slices around preselected massive galaxies, with 877,806 clusters...
| Published in: | The Astrophysical Journal Supplement Series |
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| Main Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
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| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4365/ad409d |
| _version_ | 1850269195267211264 |
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| author | Z. L. Wen J. L. Han |
| author_facet | Z. L. Wen J. L. Han |
| author_sort | Z. L. Wen |
| collection | DOAJ |
| container_title | The Astrophysical Journal Supplement Series |
| description | Based on the DESI Legacy Imaging Surveys released data and available spectroscopic redshifts, we identify 1.58 million clusters of galaxies by searching for the overdensity of the stellar mass distribution of galaxies within redshift slices around preselected massive galaxies, with 877,806 clusters being found for the first time. The identified clusters have an equivalent mass of M _500 ≥ 0.47 × 10 ^14 M _⊙ with an uncertainty of 0.2 dex. The redshift distribution of clusters extends to z ∼ 1.5, and 338,841 clusters have spectroscopic redshifts. Our cluster sample includes most of the rich optical clusters in previous catalogs, more than 95% of the massive Sunyaev–Zeldovich clusters, and 90% of the ROSAT and eROSITA X-ray clusters. From the light distributions of the member galaxies, we derive the dynamical state parameters for 27,685 rich clusters and find no significant evolution of the dynamical state with redshift. We find that the stellar mass of the brightest cluster galaxies grows by a factor of 2 since z = 1. |
| format | Article |
| id | doaj-art-2ddff00a1c8e40dbabf8339576767d0b |
| institution | Directory of Open Access Journals |
| issn | 0067-0049 |
| language | English |
| publishDate | 2024-01-01 |
| publisher | IOP Publishing |
| record_format | Article |
| spelling | doaj-art-2ddff00a1c8e40dbabf8339576767d0b2025-08-19T23:43:29ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492024-01-0127223910.3847/1538-4365/ad409dA Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging SurveysZ. L. Wen0J. L. Han1https://orcid.org/0000-0002-9274-3092National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing 100101, People's Republic of China ; hjl@nao.cas.cn; CAS Key Laboratory of FAST, NAOC, Chinese Academy of Sciences , Chaoyang District, Beijing 100101, People's Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing 100101, People's Republic of China ; hjl@nao.cas.cn; CAS Key Laboratory of FAST, NAOC, Chinese Academy of Sciences , Chaoyang District, Beijing 100101, People's Republic of China; School of Astronomy and Space Sciences, University of Chinese Academy of Sciences , Beijing 100049, People's Republic of ChinaBased on the DESI Legacy Imaging Surveys released data and available spectroscopic redshifts, we identify 1.58 million clusters of galaxies by searching for the overdensity of the stellar mass distribution of galaxies within redshift slices around preselected massive galaxies, with 877,806 clusters being found for the first time. The identified clusters have an equivalent mass of M _500 ≥ 0.47 × 10 ^14 M _⊙ with an uncertainty of 0.2 dex. The redshift distribution of clusters extends to z ∼ 1.5, and 338,841 clusters have spectroscopic redshifts. Our cluster sample includes most of the rich optical clusters in previous catalogs, more than 95% of the massive Sunyaev–Zeldovich clusters, and 90% of the ROSAT and eROSITA X-ray clusters. From the light distributions of the member galaxies, we derive the dynamical state parameters for 27,685 rich clusters and find no significant evolution of the dynamical state with redshift. We find that the stellar mass of the brightest cluster galaxies grows by a factor of 2 since z = 1.https://doi.org/10.3847/1538-4365/ad409dGalaxy clustersGalaxy evolutionCatalogs |
| spellingShingle | Z. L. Wen J. L. Han A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys Galaxy clusters Galaxy evolution Catalogs |
| title | A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys |
| title_full | A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys |
| title_fullStr | A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys |
| title_full_unstemmed | A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys |
| title_short | A Catalog of 1.58 Million Clusters of Galaxies Identified from the DESI Legacy Imaging Surveys |
| title_sort | catalog of 1 58 million clusters of galaxies identified from the desi legacy imaging surveys |
| topic | Galaxy clusters Galaxy evolution Catalogs |
| url | https://doi.org/10.3847/1538-4365/ad409d |
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