{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:I2KDETWNMUERTZGZXIQDMHQUF3","short_pith_number":"pith:I2KDETWN","schema_version":"1.0","canonical_sha256":"4694324ecd650919e4d9ba20361e142ee9881c0db5cb6a20bdda922d9b8cfc06","source":{"kind":"arxiv","id":"1812.04803","version":3},"attestation_state":"computed","paper":{"title":"Multi-messenger Bayesian parameter inference of a binary neutron-star merger","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ben Margalit, Brian D. Metzger, Michael W. Coughlin, Tim Dietrich","submitted_at":"2018-12-12T04:23:11Z","abstract_excerpt":"The combined detection of a binary neutron-star merger in both gravitational waves (GWs) and electromagnetic (EM) radiation spanning the entire spectrum -- GW170817 / AT2017gfo / GRB170817A -- marks a breakthrough in the field of multi-messenger astronomy. Between the plethora of modeling and observations, the rich synergy that exists among the available data sets creates a unique opportunity to constrain the binary parameters, the equation of state of supranuclear density matter, and the physical processes at work during the kilonova and gamma-ray burst. We report, for the first time, Bayesia"},"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":"1812.04803","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-12-12T04:23:11Z","cross_cats_sorted":[],"title_canon_sha256":"8481aca3405c9998048d4a871564cffc550272db674cfb1e2cab09b941e9045b","abstract_canon_sha256":"a4535235fc9fb4267d3c19b86cef988ad66c0ecb51ad676ed5761591e6e1bf06"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:12:38.975052Z","signature_b64":"Ojl802w2m0DahAxO4P1zJJvKDzi2nf5/rwvLCvlXT/CTJJCrIlPh/BIxCu0tL4DfD2qdeTel+c/Q7r7Zoh+XCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4694324ecd650919e4d9ba20361e142ee9881c0db5cb6a20bdda922d9b8cfc06","last_reissued_at":"2026-07-05T02:12:38.974634Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:12:38.974634Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Multi-messenger Bayesian parameter inference of a binary neutron-star merger","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Ben Margalit, Brian D. Metzger, Michael W. Coughlin, Tim Dietrich","submitted_at":"2018-12-12T04:23:11Z","abstract_excerpt":"The combined detection of a binary neutron-star merger in both gravitational waves (GWs) and electromagnetic (EM) radiation spanning the entire spectrum -- GW170817 / AT2017gfo / GRB170817A -- marks a breakthrough in the field of multi-messenger astronomy. Between the plethora of modeling and observations, the rich synergy that exists among the available data sets creates a unique opportunity to constrain the binary parameters, the equation of state of supranuclear density matter, and the physical processes at work during the kilonova and gamma-ray burst. We report, for the first time, Bayesia"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.04803","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1812.04803/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":"1812.04803","created_at":"2026-07-05T02:12:38.974689+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.04803v3","created_at":"2026-07-05T02:12:38.974689+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.04803","created_at":"2026-07-05T02:12:38.974689+00:00"},{"alias_kind":"pith_short_12","alias_value":"I2KDETWNMUER","created_at":"2026-07-05T02:12:38.974689+00:00"},{"alias_kind":"pith_short_16","alias_value":"I2KDETWNMUERTZGZ","created_at":"2026-07-05T02:12:38.974689+00:00"},{"alias_kind":"pith_short_8","alias_value":"I2KDETWN","created_at":"2026-07-05T02:12:38.974689+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07120","citing_title":"Prospect for Detection of Strongly Lensed Multi-messenger Signals of Binary Neutron Star Mergers","ref_index":147,"is_internal_anchor":true},{"citing_arxiv_id":"2606.11299","citing_title":"A magnetar formation in binary neutron star merger","ref_index":13,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3","json":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3.json","graph_json":"https://pith.science/api/pith-number/I2KDETWNMUERTZGZXIQDMHQUF3/graph.json","events_json":"https://pith.science/api/pith-number/I2KDETWNMUERTZGZXIQDMHQUF3/events.json","paper":"https://pith.science/paper/I2KDETWN"},"agent_actions":{"view_html":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3","download_json":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3.json","view_paper":"https://pith.science/paper/I2KDETWN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.04803&json=true","fetch_graph":"https://pith.science/api/pith-number/I2KDETWNMUERTZGZXIQDMHQUF3/graph.json","fetch_events":"https://pith.science/api/pith-number/I2KDETWNMUERTZGZXIQDMHQUF3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3/action/storage_attestation","attest_author":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3/action/author_attestation","sign_citation":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3/action/citation_signature","submit_replication":"https://pith.science/pith/I2KDETWNMUERTZGZXIQDMHQUF3/action/replication_record"}},"created_at":"2026-07-05T02:12:38.974689+00:00","updated_at":"2026-07-05T02:12:38.974689+00:00"}