{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:VX5EEQ6JCCVSVUMO5PAUSWCNHY","short_pith_number":"pith:VX5EEQ6J","schema_version":"1.0","canonical_sha256":"adfa4243c910ab2ad18eebc149584d3e1d985bf310b52de3f3a3217e89b8c2dc","source":{"kind":"arxiv","id":"astro-ph/0106005","version":1},"attestation_state":"computed","paper":{"title":"Dynamics of the Globular Cluster System Associated with M87 (NGC 4486). II. Analysis","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"David A. Hanes (Queens), David Merritt (Rutgers), Dean E. McLaughlin (Berkeley), Doug Geisler (Concepcion), Gretchen L.H. Harris (Waterloo), James E. Hesser (HIA/DAO), Myung Gyoon Lee (Seoul), Patrick Cote (Rutgers), Terry J. Bridges (AAO)","submitted_at":"2001-05-31T23:13:07Z","abstract_excerpt":"We present a dynamical analysis of the globular cluster system associated with M87 (= NGC 4486), the cD galaxy near the dynamical center of the Virgo cluster. The analysis utilizes a new spectroscopic and photometric database which is described in a companion paper (Hanes et al. 2001). Using a sample of 278 globular clusters with measured radial velocities and metallicities, and new surface density profiles based on wide-field Washington photometry, we study the dynamics of the M87 globular cluster system both globally --- for the entire cluster sample --- and separately --- for the metal-rich"},"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":"astro-ph/0106005","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-05-31T23:13:07Z","cross_cats_sorted":[],"title_canon_sha256":"9de2001625b0aa5d0a2bf4ff972e217540077dc1684ec44ca09f154ed9df46fe","abstract_canon_sha256":"99374120625d131d4b048d0f30a55f5ff954e59262dc4e0de026f9bc0cd558a6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:23:28.765257Z","signature_b64":"DHjLg0RiymlGGPcp/lNDOaqq4Sm7PGeDG0XpMvHUye5Ln5WE0Byhl6bcR6Ojb3RhBEP/cvziPE516MRpbvXXBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"adfa4243c910ab2ad18eebc149584d3e1d985bf310b52de3f3a3217e89b8c2dc","last_reissued_at":"2026-07-04T16:23:28.764722Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:23:28.764722Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamics of the Globular Cluster System Associated with M87 (NGC 4486). II. Analysis","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"David A. Hanes (Queens), David Merritt (Rutgers), Dean E. McLaughlin (Berkeley), Doug Geisler (Concepcion), Gretchen L.H. Harris (Waterloo), James E. Hesser (HIA/DAO), Myung Gyoon Lee (Seoul), Patrick Cote (Rutgers), Terry J. Bridges (AAO)","submitted_at":"2001-05-31T23:13:07Z","abstract_excerpt":"We present a dynamical analysis of the globular cluster system associated with M87 (= NGC 4486), the cD galaxy near the dynamical center of the Virgo cluster. The analysis utilizes a new spectroscopic and photometric database which is described in a companion paper (Hanes et al. 2001). Using a sample of 278 globular clusters with measured radial velocities and metallicities, and new surface density profiles based on wide-field Washington photometry, we study the dynamics of the M87 globular cluster system both globally --- for the entire cluster sample --- and separately --- for the metal-rich"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0106005","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/astro-ph/0106005/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":"astro-ph/0106005","created_at":"2026-07-04T16:23:28.764784+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0106005v1","created_at":"2026-07-04T16:23:28.764784+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0106005","created_at":"2026-07-04T16:23:28.764784+00:00"},{"alias_kind":"pith_short_12","alias_value":"VX5EEQ6JCCVS","created_at":"2026-07-04T16:23:28.764784+00:00"},{"alias_kind":"pith_short_16","alias_value":"VX5EEQ6JCCVSVUMO","created_at":"2026-07-04T16:23:28.764784+00:00"},{"alias_kind":"pith_short_8","alias_value":"VX5EEQ6J","created_at":"2026-07-04T16:23:28.764784+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.02480","citing_title":"The Merger-Driven Origin of the Vast Extended Stellar Disc Around the Andromeda Galaxy","ref_index":48,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY","json":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY.json","graph_json":"https://pith.science/api/pith-number/VX5EEQ6JCCVSVUMO5PAUSWCNHY/graph.json","events_json":"https://pith.science/api/pith-number/VX5EEQ6JCCVSVUMO5PAUSWCNHY/events.json","paper":"https://pith.science/paper/VX5EEQ6J"},"agent_actions":{"view_html":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY","download_json":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY.json","view_paper":"https://pith.science/paper/VX5EEQ6J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0106005&json=true","fetch_graph":"https://pith.science/api/pith-number/VX5EEQ6JCCVSVUMO5PAUSWCNHY/graph.json","fetch_events":"https://pith.science/api/pith-number/VX5EEQ6JCCVSVUMO5PAUSWCNHY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY/action/storage_attestation","attest_author":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY/action/author_attestation","sign_citation":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY/action/citation_signature","submit_replication":"https://pith.science/pith/VX5EEQ6JCCVSVUMO5PAUSWCNHY/action/replication_record"}},"created_at":"2026-07-04T16:23:28.764784+00:00","updated_at":"2026-07-04T16:23:28.764784+00:00"}