{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:RQ2YH4QX4YUYTHPAGHJRNPZBBT","short_pith_number":"pith:RQ2YH4QX","schema_version":"1.0","canonical_sha256":"8c3583f217e629899de031d316bf210ccb9c3c10585abdfa2b6af645fdcf05b0","source":{"kind":"arxiv","id":"1312.4799","version":1},"attestation_state":"computed","paper":{"title":"The Black Hole Mass and the Stellar Ring in NGC 3706","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Douglas O. Richstone, John Kormendy, Karl Gebhardt, Kayhan G\\\"ultekin, Ralf Bender, Scott Tremaine, Tod R. Lauer","submitted_at":"2013-12-17T14:27:51Z","abstract_excerpt":"We determine the mass of the nuclear black hole ($M$) in NGC 3706, an early type galaxy with a central surface brightness minimum arising from an apparent stellar ring, which is misaligned with respect to the galaxy's major axis at larger radii. We fit new HST/STIS and archival data with axisymmetric orbit models to determine $M$, mass-to-light ratio ($\\Upsilon_V$), and dark matter halo profile. The best-fit model parameters with 1$\\sigma$ uncertainties are $M = (6.0^{+0.7}_{-0.9}) \\times 10^8\\ M_{\\scriptscriptstyle \\odot}$ and $\\Upsilon_V = 6.0 \\pm 0.2\\ M_{\\scriptscriptstyle \\odot}\\ L_{{\\scri"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1312.4799","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-12-17T14:27:51Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"f8c1705b2b54e7f6feb3ce6aa09f2d13bf59050dad388ecc945080888044fb32","abstract_canon_sha256":"95c9dfafd2dba0eccc79644706e71be87df0a506d35d9d5d3ee0d8f2ec0ccbf9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:49.763451Z","signature_b64":"v0ZHAkpHmAILtB5nhhvEX9zTc59ma0rFuCZJ0zIk9DOQ+QWCCFKp/xlOo7yAEHkspeVVYFlf8wOrXT283CKDAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8c3583f217e629899de031d316bf210ccb9c3c10585abdfa2b6af645fdcf05b0","last_reissued_at":"2026-05-18T01:45:49.762924Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:49.762924Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Black Hole Mass and the Stellar Ring in NGC 3706","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Douglas O. Richstone, John Kormendy, Karl Gebhardt, Kayhan G\\\"ultekin, Ralf Bender, Scott Tremaine, Tod R. Lauer","submitted_at":"2013-12-17T14:27:51Z","abstract_excerpt":"We determine the mass of the nuclear black hole ($M$) in NGC 3706, an early type galaxy with a central surface brightness minimum arising from an apparent stellar ring, which is misaligned with respect to the galaxy's major axis at larger radii. We fit new HST/STIS and archival data with axisymmetric orbit models to determine $M$, mass-to-light ratio ($\\Upsilon_V$), and dark matter halo profile. The best-fit model parameters with 1$\\sigma$ uncertainties are $M = (6.0^{+0.7}_{-0.9}) \\times 10^8\\ M_{\\scriptscriptstyle \\odot}$ and $\\Upsilon_V = 6.0 \\pm 0.2\\ M_{\\scriptscriptstyle \\odot}\\ L_{{\\scri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.4799","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":"1312.4799","created_at":"2026-05-18T01:45:49.763013+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.4799v1","created_at":"2026-05-18T01:45:49.763013+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.4799","created_at":"2026-05-18T01:45:49.763013+00:00"},{"alias_kind":"pith_short_12","alias_value":"RQ2YH4QX4YUY","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_16","alias_value":"RQ2YH4QX4YUYTHPA","created_at":"2026-05-18T12:27:59.945178+00:00"},{"alias_kind":"pith_short_8","alias_value":"RQ2YH4QX","created_at":"2026-05-18T12:27:59.945178+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/RQ2YH4QX4YUYTHPAGHJRNPZBBT","json":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT.json","graph_json":"https://pith.science/api/pith-number/RQ2YH4QX4YUYTHPAGHJRNPZBBT/graph.json","events_json":"https://pith.science/api/pith-number/RQ2YH4QX4YUYTHPAGHJRNPZBBT/events.json","paper":"https://pith.science/paper/RQ2YH4QX"},"agent_actions":{"view_html":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT","download_json":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT.json","view_paper":"https://pith.science/paper/RQ2YH4QX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.4799&json=true","fetch_graph":"https://pith.science/api/pith-number/RQ2YH4QX4YUYTHPAGHJRNPZBBT/graph.json","fetch_events":"https://pith.science/api/pith-number/RQ2YH4QX4YUYTHPAGHJRNPZBBT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT/action/storage_attestation","attest_author":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT/action/author_attestation","sign_citation":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT/action/citation_signature","submit_replication":"https://pith.science/pith/RQ2YH4QX4YUYTHPAGHJRNPZBBT/action/replication_record"}},"created_at":"2026-05-18T01:45:49.763013+00:00","updated_at":"2026-05-18T01:45:49.763013+00:00"}