{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:7QBRY2T6SIACWVKWVNSHYO3R62","short_pith_number":"pith:7QBRY2T6","schema_version":"1.0","canonical_sha256":"fc031c6a7e92002b5556ab647c3b71f69c17b002b4a36309c594f0755c3511e1","source":{"kind":"arxiv","id":"1801.08221","version":3},"attestation_state":"computed","paper":{"title":"Weighing Black Holes using Tidal Disruption Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Brenna Mockler, Enrico Ramirez-Ruiz, James Guillochon","submitted_at":"2018-01-24T22:20:42Z","abstract_excerpt":"While once rare, observations of stars being tidally disrupted by supermassive black holes are quickly becoming commonplace. To continue to learn from these events it is necessary to robustly and systematically compare our growing number of observations with theory. We present a tidal disruption module for the Modular Open Source Fitter for Transients (MOSFiT) and the results from fitting 14 tidal disruption events (TDEs). Our model uses FLASH simulations of TDEs to generate bolometric luminosities and passes these luminosities through viscosity and reprocessing transformation functions to cre"},"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":"1801.08221","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-01-24T22:20:42Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"9fbd4489376aea1762845696c01c1bd70be88f35f7f03083f567aad79bc90fb8","abstract_canon_sha256":"9ddbc0c2233717c9f645deb7ad8adf2859efd40436f540e953cd814b46e22ffd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:44.311390Z","signature_b64":"Sln167PJN0wmPhIiC6oG2JrrdEfammWhjNFILc5RNC5q/ffIjSSfDnTBJxECOj+AM8/CtjIFxluGOAACnbJeAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fc031c6a7e92002b5556ab647c3b71f69c17b002b4a36309c594f0755c3511e1","last_reissued_at":"2026-05-17T23:52:44.310833Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:44.310833Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Weighing Black Holes using Tidal Disruption Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Brenna Mockler, Enrico Ramirez-Ruiz, James Guillochon","submitted_at":"2018-01-24T22:20:42Z","abstract_excerpt":"While once rare, observations of stars being tidally disrupted by supermassive black holes are quickly becoming commonplace. To continue to learn from these events it is necessary to robustly and systematically compare our growing number of observations with theory. We present a tidal disruption module for the Modular Open Source Fitter for Transients (MOSFiT) and the results from fitting 14 tidal disruption events (TDEs). Our model uses FLASH simulations of TDEs to generate bolometric luminosities and passes these luminosities through viscosity and reprocessing transformation functions to cre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.08221","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":"1801.08221","created_at":"2026-05-17T23:52:44.310945+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.08221v3","created_at":"2026-05-17T23:52:44.310945+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.08221","created_at":"2026-05-17T23:52:44.310945+00:00"},{"alias_kind":"pith_short_12","alias_value":"7QBRY2T6SIAC","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_16","alias_value":"7QBRY2T6SIACWVKW","created_at":"2026-05-18T12:32:11.075285+00:00"},{"alias_kind":"pith_short_8","alias_value":"7QBRY2T6","created_at":"2026-05-18T12:32:11.075285+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2606.31434","citing_title":"Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04090","citing_title":"Mapping the nuclear environments of extreme coronal line emitting galaxies","ref_index":74,"is_internal_anchor":true},{"citing_arxiv_id":"2606.04740","citing_title":"TDEs on FIRE: Illuminating the Cosmic Evolution of Tidal Disruption Rates","ref_index":159,"is_internal_anchor":true},{"citing_arxiv_id":"2606.22919","citing_title":"Are most detected tidal disruption events partial?","ref_index":49,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62","json":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62.json","graph_json":"https://pith.science/api/pith-number/7QBRY2T6SIACWVKWVNSHYO3R62/graph.json","events_json":"https://pith.science/api/pith-number/7QBRY2T6SIACWVKWVNSHYO3R62/events.json","paper":"https://pith.science/paper/7QBRY2T6"},"agent_actions":{"view_html":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62","download_json":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62.json","view_paper":"https://pith.science/paper/7QBRY2T6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.08221&json=true","fetch_graph":"https://pith.science/api/pith-number/7QBRY2T6SIACWVKWVNSHYO3R62/graph.json","fetch_events":"https://pith.science/api/pith-number/7QBRY2T6SIACWVKWVNSHYO3R62/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62/action/storage_attestation","attest_author":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62/action/author_attestation","sign_citation":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62/action/citation_signature","submit_replication":"https://pith.science/pith/7QBRY2T6SIACWVKWVNSHYO3R62/action/replication_record"}},"created_at":"2026-05-17T23:52:44.310945+00:00","updated_at":"2026-05-17T23:52:44.310945+00:00"}