{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:U5PJRWRY3RXU65JTP7DFO7STEW","short_pith_number":"pith:U5PJRWRY","schema_version":"1.0","canonical_sha256":"a75e98da38dc6f4f75337fc6577e5325b185ec5fca326a423919e4897b24201a","source":{"kind":"arxiv","id":"1604.05205","version":1},"attestation_state":"computed","paper":{"title":"Maximizing the Probability of Detecting an Electromagnetic Counterpart of Gravitational-wave Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Christopher W. Stubbs, Michael W. Coughlin","submitted_at":"2016-04-18T15:21:14Z","abstract_excerpt":"Compact binary coalescences are a promising source of gravitational waves for second-generation interferometric gravitational-wave detectors such as advanced LIGO and advanced Virgo. These are among the most promising sources for joint detection of electromagnetic (EM) and gravitational-wave (GW) emission. To maximize the science performed with these objects, it is essential to undertake a followup observing strategy that maximizes the likelihood of detecting the EM counterpart. We present a follow-up strategy that maximizes the counterpart detection probability, given a fixed investment of te"},"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":"1604.05205","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2016-04-18T15:21:14Z","cross_cats_sorted":[],"title_canon_sha256":"1b3181bdd315575900aaf68324a50058d27a6123efeea32a7a25689bf42e6d96","abstract_canon_sha256":"9d8cc2a8a6abe529a6167f34397e326ed64afc1d71a87c4ef276ce89cb04c3fb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:10:05.659372Z","signature_b64":"ZyYRi6cC6SpbiqxF2RC3Gie5g/DT7TfQIpv0hbrwwQGFx9sNu4LVmwD38+tSlwEzsE/a7djPL3n/kZlYQka3Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a75e98da38dc6f4f75337fc6577e5325b185ec5fca326a423919e4897b24201a","last_reissued_at":"2026-05-18T01:10:05.658717Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:10:05.658717Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Maximizing the Probability of Detecting an Electromagnetic Counterpart of Gravitational-wave Events","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Christopher W. Stubbs, Michael W. Coughlin","submitted_at":"2016-04-18T15:21:14Z","abstract_excerpt":"Compact binary coalescences are a promising source of gravitational waves for second-generation interferometric gravitational-wave detectors such as advanced LIGO and advanced Virgo. These are among the most promising sources for joint detection of electromagnetic (EM) and gravitational-wave (GW) emission. To maximize the science performed with these objects, it is essential to undertake a followup observing strategy that maximizes the likelihood of detecting the EM counterpart. We present a follow-up strategy that maximizes the counterpart detection probability, given a fixed investment of te"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.05205","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":"1604.05205","created_at":"2026-05-18T01:10:05.658808+00:00"},{"alias_kind":"arxiv_version","alias_value":"1604.05205v1","created_at":"2026-05-18T01:10:05.658808+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.05205","created_at":"2026-05-18T01:10:05.658808+00:00"},{"alias_kind":"pith_short_12","alias_value":"U5PJRWRY3RXU","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"U5PJRWRY3RXU65JT","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"U5PJRWRY","created_at":"2026-05-18T12:30:46.583412+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/U5PJRWRY3RXU65JTP7DFO7STEW","json":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW.json","graph_json":"https://pith.science/api/pith-number/U5PJRWRY3RXU65JTP7DFO7STEW/graph.json","events_json":"https://pith.science/api/pith-number/U5PJRWRY3RXU65JTP7DFO7STEW/events.json","paper":"https://pith.science/paper/U5PJRWRY"},"agent_actions":{"view_html":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW","download_json":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW.json","view_paper":"https://pith.science/paper/U5PJRWRY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1604.05205&json=true","fetch_graph":"https://pith.science/api/pith-number/U5PJRWRY3RXU65JTP7DFO7STEW/graph.json","fetch_events":"https://pith.science/api/pith-number/U5PJRWRY3RXU65JTP7DFO7STEW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW/action/storage_attestation","attest_author":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW/action/author_attestation","sign_citation":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW/action/citation_signature","submit_replication":"https://pith.science/pith/U5PJRWRY3RXU65JTP7DFO7STEW/action/replication_record"}},"created_at":"2026-05-18T01:10:05.658808+00:00","updated_at":"2026-05-18T01:10:05.658808+00:00"}