{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:TMJ45GDMO4YMLZIGMRUOFC4CTU","short_pith_number":"pith:TMJ45GDM","schema_version":"1.0","canonical_sha256":"9b13ce986c7730c5e5066468e28b829d16ad56cb86d3bcb319ab651fa7e5d22f","source":{"kind":"arxiv","id":"1604.03554","version":1},"attestation_state":"computed","paper":{"title":"Globular clusters hosting intermediate-mass black-holes: no mass-segregation based candidates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bong Won Sohn, Mario Pasquato, Paolo Miocchi, Young-Wook Lee","submitted_at":"2016-04-12T20:00:05Z","abstract_excerpt":"Recently, both stellar mass-segregation and binary-fractions were uniformly measured on relatively large samples of Galactic Globular Clusters (GCs). Simulations show that both sizeable binary-star populations and Intermediate-Mass Black Holes (IMBHs) quench mass-segregation in relaxed GCs. Thus mass-segregation in GCs with a reliable binary-fraction measurement is a valuable probe to constrain IMBHs. In this paper we combine mass-segregation and binary-fraction measurements from the literature to build a sample of 33 GCs (with measured core-binary fractions), and a sample of 43 GCs (with a bi"},"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":"1604.03554","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-04-12T20:00:05Z","cross_cats_sorted":[],"title_canon_sha256":"52852f07c2682c3bb739450364aa9818458161e18b5b82f8394d5c6fb0170d23","abstract_canon_sha256":"ff4a6513e51f8f1dfbd682d963a728474f1cdb7989505260a0707b0f9bbf5512"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:12:48.454725Z","signature_b64":"jX0i8m/WrlzUKSPr96NZUHYQpdbMFZNrexjvgzeklbkNoFCVwV9XscAGdbHU6gDUY3/L7jTPe7GVPzUA9HpTAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b13ce986c7730c5e5066468e28b829d16ad56cb86d3bcb319ab651fa7e5d22f","last_reissued_at":"2026-05-18T01:12:48.454377Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:12:48.454377Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Globular clusters hosting intermediate-mass black-holes: no mass-segregation based candidates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bong Won Sohn, Mario Pasquato, Paolo Miocchi, Young-Wook Lee","submitted_at":"2016-04-12T20:00:05Z","abstract_excerpt":"Recently, both stellar mass-segregation and binary-fractions were uniformly measured on relatively large samples of Galactic Globular Clusters (GCs). Simulations show that both sizeable binary-star populations and Intermediate-Mass Black Holes (IMBHs) quench mass-segregation in relaxed GCs. Thus mass-segregation in GCs with a reliable binary-fraction measurement is a valuable probe to constrain IMBHs. In this paper we combine mass-segregation and binary-fraction measurements from the literature to build a sample of 33 GCs (with measured core-binary fractions), and a sample of 43 GCs (with a bi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.03554","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":""},"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":"1604.03554","created_at":"2026-05-18T01:12:48.454434+00:00"},{"alias_kind":"arxiv_version","alias_value":"1604.03554v1","created_at":"2026-05-18T01:12:48.454434+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.03554","created_at":"2026-05-18T01:12:48.454434+00:00"},{"alias_kind":"pith_short_12","alias_value":"TMJ45GDMO4YM","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"TMJ45GDMO4YMLZIG","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"TMJ45GDM","created_at":"2026-05-18T12:30:44.179134+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/TMJ45GDMO4YMLZIGMRUOFC4CTU","json":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU.json","graph_json":"https://pith.science/api/pith-number/TMJ45GDMO4YMLZIGMRUOFC4CTU/graph.json","events_json":"https://pith.science/api/pith-number/TMJ45GDMO4YMLZIGMRUOFC4CTU/events.json","paper":"https://pith.science/paper/TMJ45GDM"},"agent_actions":{"view_html":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU","download_json":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU.json","view_paper":"https://pith.science/paper/TMJ45GDM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1604.03554&json=true","fetch_graph":"https://pith.science/api/pith-number/TMJ45GDMO4YMLZIGMRUOFC4CTU/graph.json","fetch_events":"https://pith.science/api/pith-number/TMJ45GDMO4YMLZIGMRUOFC4CTU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU/action/storage_attestation","attest_author":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU/action/author_attestation","sign_citation":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU/action/citation_signature","submit_replication":"https://pith.science/pith/TMJ45GDMO4YMLZIGMRUOFC4CTU/action/replication_record"}},"created_at":"2026-05-18T01:12:48.454434+00:00","updated_at":"2026-05-18T01:12:48.454434+00:00"}