{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:RNTIACBG3UA75DVFGEGFSTPVJI","short_pith_number":"pith:RNTIACBG","schema_version":"1.0","canonical_sha256":"8b66800826dd01fe8ea5310c594df54a3797e755dc054e6df2cf6c6957709fc8","source":{"kind":"arxiv","id":"1603.06611","version":2},"attestation_state":"computed","paper":{"title":"Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","gr-qc","physics.data-an"],"primary_cat":"astro-ph.HE","authors_text":"D. Sz\\'ecsi, I. Csabai, I. Horv\\'ath, J. Lichtenberger, L. Dobos, L.G. Bal\\'azs, L.V. T\\'oth, Z. Bagoly","submitted_at":"2016-03-21T20:55:03Z","abstract_excerpt":"The Fermi collaboration identified a possible electromagnetic counterpart of the gravitational wave event of September 14, 2015. Our goal is to provide an unsupervised data analysis algorithm to identify similar events in Fermi's Gamma-ray Burst Monitor CTTE data stream. We are looking for signals that are typically weak. Therefore, they can only be found by a careful analysis of count rates of all detectors and energy channels simultaneously. Our Automatized Detector Weight Optimization (ADWO) method consists of a search for the signal, and a test of its significance. We developed ADWO, a vir"},"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":"1603.06611","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-21T20:55:03Z","cross_cats_sorted":["astro-ph.IM","gr-qc","physics.data-an"],"title_canon_sha256":"01d14026450c153264535d1b8956c3f0c749de8988bb8d91085eb83607102654","abstract_canon_sha256":"1a60c6934c3c41845e002f7ed6e1c89c2e9bedf42ee46507c858e534b21f3f26"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:04:45.108544Z","signature_b64":"82W2KUhzd8GxCQ6tbJSG5NwFwFimkyNmMux1AxIHDXn1eyRW9zEBFXpHBLbT/2vLhVofnVU34zUl8w5XN+FKAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b66800826dd01fe8ea5310c594df54a3797e755dc054e6df2cf6c6957709fc8","last_reissued_at":"2026-05-18T01:04:45.108022Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:04:45.108022Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searching for electromagnetic counterpart of LIGO gravitational waves in the Fermi GBM data with ADWO","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","gr-qc","physics.data-an"],"primary_cat":"astro-ph.HE","authors_text":"D. Sz\\'ecsi, I. Csabai, I. Horv\\'ath, J. Lichtenberger, L. Dobos, L.G. Bal\\'azs, L.V. T\\'oth, Z. Bagoly","submitted_at":"2016-03-21T20:55:03Z","abstract_excerpt":"The Fermi collaboration identified a possible electromagnetic counterpart of the gravitational wave event of September 14, 2015. Our goal is to provide an unsupervised data analysis algorithm to identify similar events in Fermi's Gamma-ray Burst Monitor CTTE data stream. We are looking for signals that are typically weak. Therefore, they can only be found by a careful analysis of count rates of all detectors and energy channels simultaneously. Our Automatized Detector Weight Optimization (ADWO) method consists of a search for the signal, and a test of its significance. We developed ADWO, a vir"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.06611","kind":"arxiv","version":2},"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":"1603.06611","created_at":"2026-05-18T01:04:45.108115+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.06611v2","created_at":"2026-05-18T01:04:45.108115+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.06611","created_at":"2026-05-18T01:04:45.108115+00:00"},{"alias_kind":"pith_short_12","alias_value":"RNTIACBG3UA7","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"RNTIACBG3UA75DVF","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"RNTIACBG","created_at":"2026-05-18T12:30:41.710351+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/RNTIACBG3UA75DVFGEGFSTPVJI","json":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI.json","graph_json":"https://pith.science/api/pith-number/RNTIACBG3UA75DVFGEGFSTPVJI/graph.json","events_json":"https://pith.science/api/pith-number/RNTIACBG3UA75DVFGEGFSTPVJI/events.json","paper":"https://pith.science/paper/RNTIACBG"},"agent_actions":{"view_html":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI","download_json":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI.json","view_paper":"https://pith.science/paper/RNTIACBG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.06611&json=true","fetch_graph":"https://pith.science/api/pith-number/RNTIACBG3UA75DVFGEGFSTPVJI/graph.json","fetch_events":"https://pith.science/api/pith-number/RNTIACBG3UA75DVFGEGFSTPVJI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI/action/storage_attestation","attest_author":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI/action/author_attestation","sign_citation":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI/action/citation_signature","submit_replication":"https://pith.science/pith/RNTIACBG3UA75DVFGEGFSTPVJI/action/replication_record"}},"created_at":"2026-05-18T01:04:45.108115+00:00","updated_at":"2026-05-18T01:04:45.108115+00:00"}