{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:PLXBZLQITVJL3SMW5F477L7LFG","short_pith_number":"pith:PLXBZLQI","schema_version":"1.0","canonical_sha256":"7aee1cae089d52bdc996e979ffafeb29957bf7313c57f5f345ea5fd418b3ccb3","source":{"kind":"arxiv","id":"1408.6536","version":1},"attestation_state":"computed","paper":{"title":"The LOFT Burst Alert System and its Burst On-board Trigger","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"((a) CEA Saclay/IRFU/Service d'Astrophysique, (b) CEA Saclay/IRFU/Service Electronique, (c) ISDC, (d) DTU Space, Denmark), D. G\\\"otz (a), E. Bozzo (c), F. Ch\\^ateau (b), France, H. Le Provost (b), Lyngby, S. Brandt (d), S. Schanne (a), Switzerland, University of Geneva","submitted_at":"2014-08-27T20:00:22Z","abstract_excerpt":"The ESA M3 candidate mission LOFT (Large Observatory For x-ray Timing) has been designed to study strong gravitational fields by observing compact objects, such as black-hole binaries or neutron-star systems and supermassive black-holes, based on the temporal analysis of photons collected by the primary instrument LAD (Large Area Detector), sensitive to X-rays from 2 to 50 keV, offering a very large effective area (>10 m 2 ), but a small field of view ({\\o}<1{\\deg}). Simultaneously the second instrument WFM (Wide Field Monitor), composed of 5 coded-mask camera pairs (2-50 keV), monitors a larg"},"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":"1408.6536","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2014-08-27T20:00:22Z","cross_cats_sorted":[],"title_canon_sha256":"24026997d4c7f9c0384c93a7b6fae5cf41e8824e8f17ac1b0af9e7683eb4a6a2","abstract_canon_sha256":"5f81196a60660860a7985600d27494e58c89d872cbe85b28c49af1445c895060"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:44:01.396252Z","signature_b64":"3HzvhkeYVabreFu4EMgkONnBxw/9B/QQzMNYvrw/ZKMhiub4SG+usFiEXEae0OtJoGHMyK6imY8fHqNDNVMgAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7aee1cae089d52bdc996e979ffafeb29957bf7313c57f5f345ea5fd418b3ccb3","last_reissued_at":"2026-05-18T02:44:01.395586Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:44:01.395586Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The LOFT Burst Alert System and its Burst On-board Trigger","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"((a) CEA Saclay/IRFU/Service d'Astrophysique, (b) CEA Saclay/IRFU/Service Electronique, (c) ISDC, (d) DTU Space, Denmark), D. G\\\"otz (a), E. Bozzo (c), F. Ch\\^ateau (b), France, H. Le Provost (b), Lyngby, S. Brandt (d), S. Schanne (a), Switzerland, University of Geneva","submitted_at":"2014-08-27T20:00:22Z","abstract_excerpt":"The ESA M3 candidate mission LOFT (Large Observatory For x-ray Timing) has been designed to study strong gravitational fields by observing compact objects, such as black-hole binaries or neutron-star systems and supermassive black-holes, based on the temporal analysis of photons collected by the primary instrument LAD (Large Area Detector), sensitive to X-rays from 2 to 50 keV, offering a very large effective area (>10 m 2 ), but a small field of view ({\\o}<1{\\deg}). Simultaneously the second instrument WFM (Wide Field Monitor), composed of 5 coded-mask camera pairs (2-50 keV), monitors a larg"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.6536","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":"1408.6536","created_at":"2026-05-18T02:44:01.395693+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.6536v1","created_at":"2026-05-18T02:44:01.395693+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.6536","created_at":"2026-05-18T02:44:01.395693+00:00"},{"alias_kind":"pith_short_12","alias_value":"PLXBZLQITVJL","created_at":"2026-05-18T12:28:43.426989+00:00"},{"alias_kind":"pith_short_16","alias_value":"PLXBZLQITVJL3SMW","created_at":"2026-05-18T12:28:43.426989+00:00"},{"alias_kind":"pith_short_8","alias_value":"PLXBZLQI","created_at":"2026-05-18T12:28:43.426989+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/PLXBZLQITVJL3SMW5F477L7LFG","json":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG.json","graph_json":"https://pith.science/api/pith-number/PLXBZLQITVJL3SMW5F477L7LFG/graph.json","events_json":"https://pith.science/api/pith-number/PLXBZLQITVJL3SMW5F477L7LFG/events.json","paper":"https://pith.science/paper/PLXBZLQI"},"agent_actions":{"view_html":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG","download_json":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG.json","view_paper":"https://pith.science/paper/PLXBZLQI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.6536&json=true","fetch_graph":"https://pith.science/api/pith-number/PLXBZLQITVJL3SMW5F477L7LFG/graph.json","fetch_events":"https://pith.science/api/pith-number/PLXBZLQITVJL3SMW5F477L7LFG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG/action/storage_attestation","attest_author":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG/action/author_attestation","sign_citation":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG/action/citation_signature","submit_replication":"https://pith.science/pith/PLXBZLQITVJL3SMW5F477L7LFG/action/replication_record"}},"created_at":"2026-05-18T02:44:01.395693+00:00","updated_at":"2026-05-18T02:44:01.395693+00:00"}