{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:FBLYUGI3BNXX6J4BPKTYSI6RUT","short_pith_number":"pith:FBLYUGI3","schema_version":"1.0","canonical_sha256":"28578a191b0b6f7f27817aa78923d1a4e5f245a9c8da990c8eadaf0ab15ac9ba","source":{"kind":"arxiv","id":"2506.18231","version":1},"attestation_state":"computed","paper":{"title":"NIKA2 Cosmological Legacy Survey: Blind detection of galaxy clusters in the COSMOS field via the Sunyaev-Zel'dovich effect","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Beelen, A. Benoit, A. Bongiovanni, A. Catalano, A. Ferragamo, A. Gomez, A.J. Rigby, A. Maury, A. Monfardini, A. Moyer-Anin, A. Paliwal, A. Ritacco, A. Sievers, B. Ladjelate, C. Hanser, C. Kramer, C. Tucker, D. Ch\\'erouvrier, E.F.C. Driessen, E. Pointecouteau, F. K\\'eruzor\\'e, F. Mayet, F. Ruppin, F.X. D\\'esert, G. Ejlali, G. Lagache, G. Pisano, G.W. Pratt, H. Ajeddig, H. Aussel, H. Roussel, I. Myserlis, J. -B. Melin, J. Bounmy, J.-F. Lestrade, J.F. Macias-Perez, J. Goupy, K. Schuster, L. -J. Bing, L. Perotto, M. B\\'ethermin, M. Calvo, M. De Petris, M. Fernandez-Torreiro, M. Mu noz-Echeverria, M. Sanchez-Portal, N. Ponthieu, O. Bourrion, P. Ade, P. Andr\\'e, R. Adam, R. Barrena, R. Neri, R. Zylka, S. Amarantidis, S. Berta, S.C. Madden, S. Doyle, S. Katsioli, S. Leclercq, S. Savorgnano, V. Reveret","submitted_at":"2025-06-23T01:41:18Z","abstract_excerpt":"(Abridged) Clusters of galaxies, formed in the latest stages of structure formation, are unique cosmological probes. With the advent of large CMB surveys like those from the Planck satellite, the ACT and SPT telescopes, we now have access to a large number of galaxy clusters detected at millimeter wavelengths via the thermal Sunyaev-Zel'dovich (tSZ) effect. Nevertheless, it is interesting to complement them with high-angular-resolution (tens of arcseconds) observations to target the lowest-mass and highest-redshift clusters. This is the case of observations with the NIKA2 camera, which is inst"},"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":"2506.18231","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-06-23T01:41:18Z","cross_cats_sorted":[],"title_canon_sha256":"92eec0dfac7f046651e734a6c3ab74483ff6a4019b3131c78d18e9436201eb9a","abstract_canon_sha256":"ac37f5a0f97ea8df3042bb80faad2557d138c03a30593120b1d856d077f0cca3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:25:31.117934Z","signature_b64":"SbpmCeNkDH9rqULmPixCN3/uI0nXikBMcNR40bVKmDtK89ddGgEb94aAkiujI7GpogfaHyu2f1I78a34rH16Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"28578a191b0b6f7f27817aa78923d1a4e5f245a9c8da990c8eadaf0ab15ac9ba","last_reissued_at":"2026-07-05T11:25:31.117443Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:25:31.117443Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"NIKA2 Cosmological Legacy Survey: Blind detection of galaxy clusters in the COSMOS field via the Sunyaev-Zel'dovich effect","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Beelen, A. Benoit, A. Bongiovanni, A. Catalano, A. Ferragamo, A. Gomez, A.J. Rigby, A. Maury, A. Monfardini, A. Moyer-Anin, A. Paliwal, A. Ritacco, A. Sievers, B. Ladjelate, C. Hanser, C. Kramer, C. Tucker, D. Ch\\'erouvrier, E.F.C. Driessen, E. Pointecouteau, F. K\\'eruzor\\'e, F. Mayet, F. Ruppin, F.X. D\\'esert, G. Ejlali, G. Lagache, G. Pisano, G.W. Pratt, H. Ajeddig, H. Aussel, H. Roussel, I. Myserlis, J. -B. Melin, J. Bounmy, J.-F. Lestrade, J.F. Macias-Perez, J. Goupy, K. Schuster, L. -J. Bing, L. Perotto, M. B\\'ethermin, M. Calvo, M. De Petris, M. Fernandez-Torreiro, M. Mu noz-Echeverria, M. Sanchez-Portal, N. Ponthieu, O. Bourrion, P. Ade, P. Andr\\'e, R. Adam, R. Barrena, R. Neri, R. Zylka, S. Amarantidis, S. Berta, S.C. Madden, S. Doyle, S. Katsioli, S. Leclercq, S. Savorgnano, V. Reveret","submitted_at":"2025-06-23T01:41:18Z","abstract_excerpt":"(Abridged) Clusters of galaxies, formed in the latest stages of structure formation, are unique cosmological probes. With the advent of large CMB surveys like those from the Planck satellite, the ACT and SPT telescopes, we now have access to a large number of galaxy clusters detected at millimeter wavelengths via the thermal Sunyaev-Zel'dovich (tSZ) effect. Nevertheless, it is interesting to complement them with high-angular-resolution (tens of arcseconds) observations to target the lowest-mass and highest-redshift clusters. This is the case of observations with the NIKA2 camera, which is inst"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.18231","kind":"arxiv","version":1},"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/2506.18231/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":"2506.18231","created_at":"2026-07-05T11:25:31.117498+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.18231v1","created_at":"2026-07-05T11:25:31.117498+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.18231","created_at":"2026-07-05T11:25:31.117498+00:00"},{"alias_kind":"pith_short_12","alias_value":"FBLYUGI3BNXX","created_at":"2026-07-05T11:25:31.117498+00:00"},{"alias_kind":"pith_short_16","alias_value":"FBLYUGI3BNXX6J4B","created_at":"2026-07-05T11:25:31.117498+00:00"},{"alias_kind":"pith_short_8","alias_value":"FBLYUGI3","created_at":"2026-07-05T11:25:31.117498+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT","json":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT.json","graph_json":"https://pith.science/api/pith-number/FBLYUGI3BNXX6J4BPKTYSI6RUT/graph.json","events_json":"https://pith.science/api/pith-number/FBLYUGI3BNXX6J4BPKTYSI6RUT/events.json","paper":"https://pith.science/paper/FBLYUGI3"},"agent_actions":{"view_html":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT","download_json":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT.json","view_paper":"https://pith.science/paper/FBLYUGI3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.18231&json=true","fetch_graph":"https://pith.science/api/pith-number/FBLYUGI3BNXX6J4BPKTYSI6RUT/graph.json","fetch_events":"https://pith.science/api/pith-number/FBLYUGI3BNXX6J4BPKTYSI6RUT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT/action/storage_attestation","attest_author":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT/action/author_attestation","sign_citation":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT/action/citation_signature","submit_replication":"https://pith.science/pith/FBLYUGI3BNXX6J4BPKTYSI6RUT/action/replication_record"}},"created_at":"2026-07-05T11:25:31.117498+00:00","updated_at":"2026-07-05T11:25:31.117498+00:00"}