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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2507.05360 |
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| _version_ | 1866913938789105664 |
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| author | Benoist, C. Aguena, M. da Costa, L. Gschwend, J. Allam, S. Alves, O. Andrade-Oliveira, F. Bacon, D. Bleem, L. Brooks, D. Rosell, A. Carnero Carretero, J. Castander, F. J. Costanzi, M. De Vicente, J. Desai, S. Dodelson, S. Doel, P. Everett, S. Flaugher, B. Frieman, J. Garcia-Bellido, J. Giannini, G. Giles, P. Gruendl, R. Gutierrez, G. Hinton, S. Hollowood, D. L. Honscheid, K. James, D. Kuehn, K. Lee, S. Marshall, J. Mena-Fernández, J. Miquel, R. Malagón, A. Plazas Romer, K. Sanchez, E. Santiago, B. Sevilla, I. Smith, M. Suchyta, E. Tarle, G. Weaverdyck, N. Weller, J. Pereira, M. E. da Silva |
| author_facet | Benoist, C. Aguena, M. da Costa, L. Gschwend, J. Allam, S. Alves, O. Andrade-Oliveira, F. Bacon, D. Bleem, L. Brooks, D. Rosell, A. Carnero Carretero, J. Castander, F. J. Costanzi, M. De Vicente, J. Desai, S. Dodelson, S. Doel, P. Everett, S. Flaugher, B. Frieman, J. Garcia-Bellido, J. Giannini, G. Giles, P. Gruendl, R. Gutierrez, G. Hinton, S. Hollowood, D. L. Honscheid, K. James, D. Kuehn, K. Lee, S. Marshall, J. Mena-Fernández, J. Miquel, R. Malagón, A. Plazas Romer, K. Sanchez, E. Santiago, B. Sevilla, I. Smith, M. Suchyta, E. Tarle, G. Weaverdyck, N. Weller, J. Pereira, M. E. da Silva |
| contents | In this work, we present and characterize the galaxy cluster catalog detected by the WaZP cluster finder, which is not based on red-sequence identification, on the full six years of observations of the Dark Energy Survey (DES-Y6). The full catalog contains over 400k detected clusters with richnesses, Ngals, above 5 and that reach redshifts up to 1.3. We also provide a version of the catalog where the observation depth and richness computation are homogenized to be used for cosmology, containing 33k rich (Ngals >25) clusters. We compare our results with the previous WaZP catalog obtained from the DES first-year data release (DES-Y1). We find that essentially all clusters within the common footprint and depth limit are recovered. The deeper observations on DES-Y6 and the more complete available spectroscopic redshift sample lead to improvements in the redshifts of the clusters, resulting in an average scatter of 1.4% and offset of 0.2%. The optical clusters are also cross-matched with Sunyaev Zel'dovich Effect (SZE) cluster samples detected by the South Pole Telescope (SPT) and the Atacama Cosmology Telescope (ACT). We find that essentially all SZE clusters with reasonable overlapping footprint have a corresponding WaZP cluster. Conversely, 90% of the optical detections with richness greater than 150 have a counterpart in the deeper regions of the SZE surveys. Based on cross-match with the SZE catalogs, we also find that 15-20% of the SZE matched systems have more than one possible WaZP counterpart at the same redshift and within the SZE R500c, indicating possible interacting or unrelaxed systems. Finally, given the optical and SZE beams, WaZP and SZE centerings are found to be consistent. A more detailed study of the SZE-WaZP mass-richness relation will be presented in a separate paper. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_05360 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The final WaZP galaxy cluster catalog of the Dark Energy Survey and comparison with SZE data Benoist, C. Aguena, M. da Costa, L. Gschwend, J. Allam, S. Alves, O. Andrade-Oliveira, F. Bacon, D. Bleem, L. Brooks, D. Rosell, A. Carnero Carretero, J. Castander, F. J. Costanzi, M. De Vicente, J. Desai, S. Dodelson, S. Doel, P. Everett, S. Flaugher, B. Frieman, J. Garcia-Bellido, J. Giannini, G. Giles, P. Gruendl, R. Gutierrez, G. Hinton, S. Hollowood, D. L. Honscheid, K. James, D. Kuehn, K. Lee, S. Marshall, J. Mena-Fernández, J. Miquel, R. Malagón, A. Plazas Romer, K. Sanchez, E. Santiago, B. Sevilla, I. Smith, M. Suchyta, E. Tarle, G. Weaverdyck, N. Weller, J. Pereira, M. E. da Silva Cosmology and Nongalactic Astrophysics In this work, we present and characterize the galaxy cluster catalog detected by the WaZP cluster finder, which is not based on red-sequence identification, on the full six years of observations of the Dark Energy Survey (DES-Y6). The full catalog contains over 400k detected clusters with richnesses, Ngals, above 5 and that reach redshifts up to 1.3. We also provide a version of the catalog where the observation depth and richness computation are homogenized to be used for cosmology, containing 33k rich (Ngals >25) clusters. We compare our results with the previous WaZP catalog obtained from the DES first-year data release (DES-Y1). We find that essentially all clusters within the common footprint and depth limit are recovered. The deeper observations on DES-Y6 and the more complete available spectroscopic redshift sample lead to improvements in the redshifts of the clusters, resulting in an average scatter of 1.4% and offset of 0.2%. The optical clusters are also cross-matched with Sunyaev Zel'dovich Effect (SZE) cluster samples detected by the South Pole Telescope (SPT) and the Atacama Cosmology Telescope (ACT). We find that essentially all SZE clusters with reasonable overlapping footprint have a corresponding WaZP cluster. Conversely, 90% of the optical detections with richness greater than 150 have a counterpart in the deeper regions of the SZE surveys. Based on cross-match with the SZE catalogs, we also find that 15-20% of the SZE matched systems have more than one possible WaZP counterpart at the same redshift and within the SZE R500c, indicating possible interacting or unrelaxed systems. Finally, given the optical and SZE beams, WaZP and SZE centerings are found to be consistent. A more detailed study of the SZE-WaZP mass-richness relation will be presented in a separate paper. |
| title | The final WaZP galaxy cluster catalog of the Dark Energy Survey and comparison with SZE data |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2507.05360 |