{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:SRURJCU4HSJMLAYSUPCJ7IPS5W","short_pith_number":"pith:SRURJCU4","schema_version":"1.0","canonical_sha256":"9469148a9c3c92c58312a3c49fa1f2ed907f6a4a79f07a94699d109e823032fe","source":{"kind":"arxiv","id":"2207.11937","version":4},"attestation_state":"computed","paper":{"title":"A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas Malag\\'on, A. Carnero Rosell, A. Cukierman, A. E. Gambrel, A. E. Lowitz, A. Fert\\'e, A. Foster, A. J. Anderson, A. K. Romer, A. N. Bender, A. Pieres, A. Rahlin, A. Suzuki, A. T. Lee, B. A. Benson, B. Flaugher, B. Thorne, C. Daley, C. Doux, C. Feng, C. L. Chang, C. Lidman, C.-L. Kuo, C. L. Reichardt, C. Lu, C. To, C. Tucker, C. Umilta, D. Bacon, D. Brooks, D. Dutcher, D. Gruen, D. J. James, D. L. Burke, D. L. Hollowood, D. Thomas, E. Bertin, E. Hivon, E. Rozo, E. Sanchez, E. Schiappucci, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. Bianchini, F. Menanteau, F. Paz-Chinch\\'on, F. R. Bouchet, G. Gutierrez, G. I. Noble, G. M. Bernstein, G. P. Holder, G. Smecher, G. Tarle, G. Wang, H. T. Diehl, I. Ferrero, J. Annis, J. A. Sobrin, J. Carretero, J. C. Hood, J. D. Vieira, J. E. Carlstrom, J. E. Ruhl, J. Frieman, J. Garc\\'ia-Bellido, J. J. Mohr, J. Mena-Fern\\'andez, J. Montgomery, J. Muir, J. Prat, J. S. Avva, J. Weller, K. Benabed, K. Honscheid, K. Kuehn, K. L. Thompson, K. Prabhu, K. R. Dibert, K. R. Ferguson, L. Balkenhol, L. E. Bleem, L. Knox, L. N. da Costa, M. A. Dobbs, M. Aguena, M. Archipley, M. Carrasco Kind, M. Costanzi, M. E. S. Pereira, M. Gatti, M. Korman, M. Lima, M. March, M. Millea, M. Raveri, M. Rodriguez-Monroy, M. Rouble, M. R. Young, M. Schubnell, M. Smith, M. Soares-Santos, M. Vincenzi, N. Goeckner-Wald, N. Huang, N. Weaverdyck, N. W. Halverson, N. Whitehorn, O. Alves, O. Lahav, P. A. R. Ade, P. Chaubal, P. Doel, P. M. Chichura, R. Gualtieri, R. L. C. Ogando, R. Miquel, R. W. Gardner, S. Bocquet, S. Desai, S. Everett, S. Galli, S. Grandis, S. Guns, S. Padin, S. R. Hinton, T. de Haan, T. Giannantonio, T.-L. Chou, T. M. C. Abbott, T. M. Crawford, T. Natoli, T. W. Cecil, V. Novosad, V. Scarpine, V. Yefremenko, W. Everett, W. L. Holzapfel, W. L. K. Wu, W. Quan, Y. Omori, Z. Pan","submitted_at":"2022-07-25T07:06:15Z","abstract_excerpt":"We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The pairwise kSZ signal between pairs of clusters drawn from the DES Year-3 cluster catalog is detected at $4.1 \\sigma$ in cosmic microwave background (CMB) temperature maps from two years of observations with the SPT-3G camera on the South Pole Telescope. After cuts, there are 24,580 clusters in the $\\sim 1,400$ deg$^2$ of the southern sky observed by both experiments. We infer the mean optical depth of the cluster samp"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2207.11937","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-07-25T07:06:15Z","cross_cats_sorted":[],"title_canon_sha256":"d2a5adaf664466011b48579cc9ad3d8735910d4205ecad30481bcc584ef0ec70","abstract_canon_sha256":"2dd1b26997f481120078b556191d32b9616fd72adbd7d74bccab490ec9745108"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:21:28.838626Z","signature_b64":"dAW4nN2SQYgKi7neVa/tCXaOAs7h9+V0hS8lXuTcuULIMtoc3Pu6cZLyBhS7dV3l165qrrbs6fNQj9xzg0beCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9469148a9c3c92c58312a3c49fa1f2ed907f6a4a79f07a94699d109e823032fe","last_reissued_at":"2026-07-05T06:21:28.838136Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:21:28.838136Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas Malag\\'on, A. Carnero Rosell, A. Cukierman, A. E. Gambrel, A. E. Lowitz, A. Fert\\'e, A. Foster, A. J. Anderson, A. K. Romer, A. N. Bender, A. Pieres, A. Rahlin, A. Suzuki, A. T. Lee, B. A. Benson, B. Flaugher, B. Thorne, C. Daley, C. Doux, C. Feng, C. L. Chang, C. Lidman, C.-L. Kuo, C. L. Reichardt, C. Lu, C. To, C. Tucker, C. Umilta, D. Bacon, D. Brooks, D. Dutcher, D. Gruen, D. J. James, D. L. Burke, D. L. Hollowood, D. Thomas, E. Bertin, E. Hivon, E. Rozo, E. Sanchez, E. Schiappucci, E. S. Rykoff, E. Suchyta, F. Andrade-Oliveira, F. Bianchini, F. Menanteau, F. Paz-Chinch\\'on, F. R. Bouchet, G. Gutierrez, G. I. Noble, G. M. Bernstein, G. P. Holder, G. Smecher, G. Tarle, G. Wang, H. T. Diehl, I. Ferrero, J. Annis, J. A. Sobrin, J. Carretero, J. C. Hood, J. D. Vieira, J. E. Carlstrom, J. E. Ruhl, J. Frieman, J. Garc\\'ia-Bellido, J. J. Mohr, J. Mena-Fern\\'andez, J. Montgomery, J. Muir, J. Prat, J. S. Avva, J. Weller, K. Benabed, K. Honscheid, K. Kuehn, K. L. Thompson, K. Prabhu, K. R. Dibert, K. R. Ferguson, L. Balkenhol, L. E. Bleem, L. Knox, L. N. da Costa, M. A. Dobbs, M. Aguena, M. Archipley, M. Carrasco Kind, M. Costanzi, M. E. S. Pereira, M. Gatti, M. Korman, M. Lima, M. March, M. Millea, M. Raveri, M. Rodriguez-Monroy, M. Rouble, M. R. Young, M. Schubnell, M. Smith, M. Soares-Santos, M. Vincenzi, N. Goeckner-Wald, N. Huang, N. Weaverdyck, N. W. Halverson, N. Whitehorn, O. Alves, O. Lahav, P. A. R. Ade, P. Chaubal, P. Doel, P. M. Chichura, R. Gualtieri, R. L. C. Ogando, R. Miquel, R. W. Gardner, S. Bocquet, S. Desai, S. Everett, S. Galli, S. Grandis, S. Guns, S. Padin, S. R. Hinton, T. de Haan, T. Giannantonio, T.-L. Chou, T. M. C. Abbott, T. M. Crawford, T. Natoli, T. W. Cecil, V. Novosad, V. Scarpine, V. Yefremenko, W. Everett, W. L. Holzapfel, W. L. K. Wu, W. Quan, Y. Omori, Z. Pan","submitted_at":"2022-07-25T07:06:15Z","abstract_excerpt":"We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The pairwise kSZ signal between pairs of clusters drawn from the DES Year-3 cluster catalog is detected at $4.1 \\sigma$ in cosmic microwave background (CMB) temperature maps from two years of observations with the SPT-3G camera on the South Pole Telescope. After cuts, there are 24,580 clusters in the $\\sim 1,400$ deg$^2$ of the southern sky observed by both experiments. We infer the mean optical depth of the cluster samp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2207.11937","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2207.11937/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2207.11937","created_at":"2026-07-05T06:21:28.838196+00:00"},{"alias_kind":"arxiv_version","alias_value":"2207.11937v4","created_at":"2026-07-05T06:21:28.838196+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2207.11937","created_at":"2026-07-05T06:21:28.838196+00:00"},{"alias_kind":"pith_short_12","alias_value":"SRURJCU4HSJM","created_at":"2026-07-05T06:21:28.838196+00:00"},{"alias_kind":"pith_short_16","alias_value":"SRURJCU4HSJMLAYS","created_at":"2026-07-05T06:21:28.838196+00:00"},{"alias_kind":"pith_short_8","alias_value":"SRURJCU4","created_at":"2026-07-05T06:21:28.838196+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.13913","citing_title":"The Cosmic Microwave Background -- Secondary Anisotropies","ref_index":169,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W","json":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W.json","graph_json":"https://pith.science/api/pith-number/SRURJCU4HSJMLAYSUPCJ7IPS5W/graph.json","events_json":"https://pith.science/api/pith-number/SRURJCU4HSJMLAYSUPCJ7IPS5W/events.json","paper":"https://pith.science/paper/SRURJCU4"},"agent_actions":{"view_html":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W","download_json":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W.json","view_paper":"https://pith.science/paper/SRURJCU4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2207.11937&json=true","fetch_graph":"https://pith.science/api/pith-number/SRURJCU4HSJMLAYSUPCJ7IPS5W/graph.json","fetch_events":"https://pith.science/api/pith-number/SRURJCU4HSJMLAYSUPCJ7IPS5W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W/action/storage_attestation","attest_author":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W/action/author_attestation","sign_citation":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W/action/citation_signature","submit_replication":"https://pith.science/pith/SRURJCU4HSJMLAYSUPCJ7IPS5W/action/replication_record"}},"created_at":"2026-07-05T06:21:28.838196+00:00","updated_at":"2026-07-05T06:21:28.838196+00:00"}