{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:EY6FVKW2EIH7P4SVKCBAMFU3OZ","short_pith_number":"pith:EY6FVKW2","schema_version":"1.0","canonical_sha256":"263c5aaada220ff7f255508206169b7654159db3f00a7a933afd55964e1a50ca","source":{"kind":"arxiv","id":"2602.12332","version":1},"attestation_state":"computed","paper":{"title":"A tight relation between the distribution of globular clusters and dark matter in AS1063","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C. Goolsby, C.J. Conselice, J.M. Diego, J.M. Palencia","submitted_at":"2026-02-12T19:00:04Z","abstract_excerpt":"Based on deep high resolution JWST images of AS1063, and after a careful masking of artifacts, extended features in the cluster, and background galaxies (including known lensed ones), we have identified tens of thousands of unresolved point sources in the central region of the galaxy cluster. We extended the identification of these point sources up to 1.18 Mpc from the center of the cluster using data in the second module. Most of these sources are expected to be globular clusters orbiting in the deep potential well of the cluster, but also the surviving compact cores of satellite galaxies. We"},"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":"2602.12332","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-02-12T19:00:04Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"cd7ab57ed001e139a9a79bc3f5eb39faadd9d55e0145aa651f3a1dd0f7952875","abstract_canon_sha256":"deb7de22e99042e34b9eadcc7cccfc7d1c53fd38e713f28eded1d1a83be85126"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-27T14:06:40.857989Z","signature_b64":"uDqrCbiYVXS/8qeLNRGnJ8Q4fhWxZtoRNP7wX9pAtD59TQ1JiDrU1CEpaj+DJo80BJEeMmivhiisXjv7D2TvBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"263c5aaada220ff7f255508206169b7654159db3f00a7a933afd55964e1a50ca","last_reissued_at":"2026-05-27T14:06:40.856887Z","signature_status":"signed_v1","first_computed_at":"2026-05-27T14:06:40.856887Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A tight relation between the distribution of globular clusters and dark matter in AS1063","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"C. Goolsby, C.J. Conselice, J.M. Diego, J.M. Palencia","submitted_at":"2026-02-12T19:00:04Z","abstract_excerpt":"Based on deep high resolution JWST images of AS1063, and after a careful masking of artifacts, extended features in the cluster, and background galaxies (including known lensed ones), we have identified tens of thousands of unresolved point sources in the central region of the galaxy cluster. We extended the identification of these point sources up to 1.18 Mpc from the center of the cluster using data in the second module. Most of these sources are expected to be globular clusters orbiting in the deep potential well of the cluster, but also the surviving compact cores of satellite galaxies. We"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2602.12332","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/2602.12332/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":"2602.12332","created_at":"2026-05-27T14:06:40.857056+00:00"},{"alias_kind":"arxiv_version","alias_value":"2602.12332v1","created_at":"2026-05-27T14:06:40.857056+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2602.12332","created_at":"2026-05-27T14:06:40.857056+00:00"},{"alias_kind":"pith_short_12","alias_value":"EY6FVKW2EIH7","created_at":"2026-05-27T14:06:40.857056+00:00"},{"alias_kind":"pith_short_16","alias_value":"EY6FVKW2EIH7P4SV","created_at":"2026-05-27T14:06:40.857056+00:00"},{"alias_kind":"pith_short_8","alias_value":"EY6FVKW2","created_at":"2026-05-27T14:06:40.857056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.20352","citing_title":"On the correlation between globular clusters and the distribution of dark matter in galaxy clusters: the case of Abell 2744","ref_index":17,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15189","citing_title":"Strong Gravitational Lensing with the James Webb Space Telescope","ref_index":230,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ","json":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ.json","graph_json":"https://pith.science/api/pith-number/EY6FVKW2EIH7P4SVKCBAMFU3OZ/graph.json","events_json":"https://pith.science/api/pith-number/EY6FVKW2EIH7P4SVKCBAMFU3OZ/events.json","paper":"https://pith.science/paper/EY6FVKW2"},"agent_actions":{"view_html":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ","download_json":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ.json","view_paper":"https://pith.science/paper/EY6FVKW2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2602.12332&json=true","fetch_graph":"https://pith.science/api/pith-number/EY6FVKW2EIH7P4SVKCBAMFU3OZ/graph.json","fetch_events":"https://pith.science/api/pith-number/EY6FVKW2EIH7P4SVKCBAMFU3OZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ/action/storage_attestation","attest_author":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ/action/author_attestation","sign_citation":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ/action/citation_signature","submit_replication":"https://pith.science/pith/EY6FVKW2EIH7P4SVKCBAMFU3OZ/action/replication_record"}},"created_at":"2026-05-27T14:06:40.857056+00:00","updated_at":"2026-05-27T14:06:40.857056+00:00"}