{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:KMGVDAGZXYRTOPZHS4HZMYEA5N","short_pith_number":"pith:KMGVDAGZ","schema_version":"1.0","canonical_sha256":"530d5180d9be23373f27970f966080eb64635dd382b2117a6dec00ec0913b949","source":{"kind":"arxiv","id":"1501.07064","version":2},"attestation_state":"computed","paper":{"title":"A New Dynamical Mass Measurement for the Virgo Cluster using the Radial Velocity Profile of the Filament Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Chungnam National University), Jounghun Lee (1), Soo-Chang Rey (2) ((1) Seoul National University, Suk Kim (2)","submitted_at":"2015-01-28T10:58:46Z","abstract_excerpt":"The radial velocities of the galaxies in the vicinity of a cluster shows deviation from the pure Hubble flow due to their gravitational interaction with the cluster. According to a recent study of Falco et al. (2014) based on a high-resolution N-body simulation, the radial velocity profile of the galaxies located at distances larger than three times the virial radius of a neighbor cluster can be well approximated by a universal formula and could be reconstructed from direct observables provided that the galaxies are distributed along one dimensional filament. They suggested an algorithm for th"},"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":"1501.07064","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-01-28T10:58:46Z","cross_cats_sorted":[],"title_canon_sha256":"96138285091523d33f92afc7191d6e5cb73830028edc4c76f4470125ec46a5f9","abstract_canon_sha256":"103cca9c5831b4c808114c675df31f48185a8394215815dc0eb954be951097c4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:54.495654Z","signature_b64":"tobNmfqgOM+6wZ6LGlHhxNf0xjkQ3KrFzMjh9m53HXEasjpuGzzmQ3cOauY2Pqv4zANgQ1e4L5mM3sPwomF8Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"530d5180d9be23373f27970f966080eb64635dd382b2117a6dec00ec0913b949","last_reissued_at":"2026-05-18T01:36:54.494900Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:54.494900Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A New Dynamical Mass Measurement for the Virgo Cluster using the Radial Velocity Profile of the Filament Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) Chungnam National University), Jounghun Lee (1), Soo-Chang Rey (2) ((1) Seoul National University, Suk Kim (2)","submitted_at":"2015-01-28T10:58:46Z","abstract_excerpt":"The radial velocities of the galaxies in the vicinity of a cluster shows deviation from the pure Hubble flow due to their gravitational interaction with the cluster. According to a recent study of Falco et al. (2014) based on a high-resolution N-body simulation, the radial velocity profile of the galaxies located at distances larger than three times the virial radius of a neighbor cluster can be well approximated by a universal formula and could be reconstructed from direct observables provided that the galaxies are distributed along one dimensional filament. They suggested an algorithm for th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.07064","kind":"arxiv","version":2},"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":"1501.07064","created_at":"2026-05-18T01:36:54.495021+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.07064v2","created_at":"2026-05-18T01:36:54.495021+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.07064","created_at":"2026-05-18T01:36:54.495021+00:00"},{"alias_kind":"pith_short_12","alias_value":"KMGVDAGZXYRT","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_16","alias_value":"KMGVDAGZXYRTOPZH","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_8","alias_value":"KMGVDAGZ","created_at":"2026-05-18T12:29:29.992203+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/KMGVDAGZXYRTOPZHS4HZMYEA5N","json":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N.json","graph_json":"https://pith.science/api/pith-number/KMGVDAGZXYRTOPZHS4HZMYEA5N/graph.json","events_json":"https://pith.science/api/pith-number/KMGVDAGZXYRTOPZHS4HZMYEA5N/events.json","paper":"https://pith.science/paper/KMGVDAGZ"},"agent_actions":{"view_html":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N","download_json":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N.json","view_paper":"https://pith.science/paper/KMGVDAGZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.07064&json=true","fetch_graph":"https://pith.science/api/pith-number/KMGVDAGZXYRTOPZHS4HZMYEA5N/graph.json","fetch_events":"https://pith.science/api/pith-number/KMGVDAGZXYRTOPZHS4HZMYEA5N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N/action/storage_attestation","attest_author":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N/action/author_attestation","sign_citation":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N/action/citation_signature","submit_replication":"https://pith.science/pith/KMGVDAGZXYRTOPZHS4HZMYEA5N/action/replication_record"}},"created_at":"2026-05-18T01:36:54.495021+00:00","updated_at":"2026-05-18T01:36:54.495021+00:00"}