{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:FEIJ6P2RATIM535OB6QJNV6GGN","short_pith_number":"pith:FEIJ6P2R","schema_version":"1.0","canonical_sha256":"29109f3f5104d0ceefae0fa096d7c633481d941961b030a6591adb059bc0f19e","source":{"kind":"arxiv","id":"1508.02399","version":3},"attestation_state":"computed","paper":{"title":"Optical Thermonuclear Transients From Tidal Compression of White Dwarfs as Tracers of the Low End of the Massive Black Hole Mass Function","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Daniel Kasen, Enrico Ramirez-Ruiz, James Guillochon, Morgan MacLeod, Stephan Rosswog","submitted_at":"2015-08-10T20:07:50Z","abstract_excerpt":"In this paper, we model the observable signatures of tidal disruptions of white dwarf (WD) stars by massive black holes (MBHs) of moderate mass, $\\approx 10^3 - 10^5 M_\\odot$. When the WD passes deep enough within the MBH's tidal field, these signatures include thermonuclear transients from burning during maximum compression. We combine a hydrodynamic simulation that includes nuclear burning of the disruption of a $0.6 M_\\odot$ C/O WD with a Monte Carlo radiative transfer calculation to synthesize the properties of a representative transient. The transient's emission emerges in the optical, wi"},"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":"1508.02399","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-08-10T20:07:50Z","cross_cats_sorted":[],"title_canon_sha256":"a9c7b723088f91e4e565f7adabe73531391a31236b8ba297bc5bb92de52fc95f","abstract_canon_sha256":"d73fefd0bec1293d80acf952674b01dd20e095316c85ff47e1aa10ecf34bb208"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:42:22.104262Z","signature_b64":"TksR2/BNVs2Xzr1mPX9WFYyMGiETVD+dmfWuSIdBVY+u+bBToONz4/OHbzeaayEFzG21CcmIoiyVS6UuEngpBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"29109f3f5104d0ceefae0fa096d7c633481d941961b030a6591adb059bc0f19e","last_reissued_at":"2026-05-18T00:42:22.103763Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:42:22.103763Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Optical Thermonuclear Transients From Tidal Compression of White Dwarfs as Tracers of the Low End of the Massive Black Hole Mass Function","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Daniel Kasen, Enrico Ramirez-Ruiz, James Guillochon, Morgan MacLeod, Stephan Rosswog","submitted_at":"2015-08-10T20:07:50Z","abstract_excerpt":"In this paper, we model the observable signatures of tidal disruptions of white dwarf (WD) stars by massive black holes (MBHs) of moderate mass, $\\approx 10^3 - 10^5 M_\\odot$. When the WD passes deep enough within the MBH's tidal field, these signatures include thermonuclear transients from burning during maximum compression. We combine a hydrodynamic simulation that includes nuclear burning of the disruption of a $0.6 M_\\odot$ C/O WD with a Monte Carlo radiative transfer calculation to synthesize the properties of a representative transient. The transient's emission emerges in the optical, wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.02399","kind":"arxiv","version":3},"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":"1508.02399","created_at":"2026-05-18T00:42:22.103840+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.02399v3","created_at":"2026-05-18T00:42:22.103840+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.02399","created_at":"2026-05-18T00:42:22.103840+00:00"},{"alias_kind":"pith_short_12","alias_value":"FEIJ6P2RATIM","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_16","alias_value":"FEIJ6P2RATIM535O","created_at":"2026-05-18T12:29:19.899920+00:00"},{"alias_kind":"pith_short_8","alias_value":"FEIJ6P2R","created_at":"2026-05-18T12:29:19.899920+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/FEIJ6P2RATIM535OB6QJNV6GGN","json":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN.json","graph_json":"https://pith.science/api/pith-number/FEIJ6P2RATIM535OB6QJNV6GGN/graph.json","events_json":"https://pith.science/api/pith-number/FEIJ6P2RATIM535OB6QJNV6GGN/events.json","paper":"https://pith.science/paper/FEIJ6P2R"},"agent_actions":{"view_html":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN","download_json":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN.json","view_paper":"https://pith.science/paper/FEIJ6P2R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.02399&json=true","fetch_graph":"https://pith.science/api/pith-number/FEIJ6P2RATIM535OB6QJNV6GGN/graph.json","fetch_events":"https://pith.science/api/pith-number/FEIJ6P2RATIM535OB6QJNV6GGN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN/action/storage_attestation","attest_author":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN/action/author_attestation","sign_citation":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN/action/citation_signature","submit_replication":"https://pith.science/pith/FEIJ6P2RATIM535OB6QJNV6GGN/action/replication_record"}},"created_at":"2026-05-18T00:42:22.103840+00:00","updated_at":"2026-05-18T00:42:22.103840+00:00"}