{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:IL7CXKNEYLIHPLHK4TGR3CC5JB","short_pith_number":"pith:IL7CXKNE","schema_version":"1.0","canonical_sha256":"42fe2ba9a4c2d077aceae4cd1d885d486d50ba3a5e7440624a3488aaeeb51e16","source":{"kind":"arxiv","id":"1612.00158","version":1},"attestation_state":"computed","paper":{"title":"X-ray/GeV emissions from Crab-like pulsars in LMC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"(2) The University of Hong Kong), J. Takata (1), K.S. Cheng (2) ((1) Huazhong University of Science, Technology","submitted_at":"2016-12-01T06:16:18Z","abstract_excerpt":"We discuss X-ray and gamma-ray emissions from Crab-like pulsars, PSRs~J0537-6910 and~J0540-6919, in Large Magellanic Cloud. Fermi-LAT observations have resolved the gamma-ray emissions from these two pulsars and found the pulsed emissions from PSR~J0540-6919. The total pulsed radiation in the X-ray/gamma-ray energy bands of PSR~J0540-6919 is observed with the efficiency $\\eta_{J0540}\\sim 0.06$ (in 4$\\pi$ sr), which is about a factor of ten larger than $\\eta_{Crab}\\sim 0.006$ of the Crab pulsar. Although PSR~J0537-6910 has the highest spin-down power among currently known pulsars, the efficienc"},"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":"1612.00158","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-01T06:16:18Z","cross_cats_sorted":[],"title_canon_sha256":"687a626d48f67645d4956c9a9e514a95151a73a5259523a08c65a1639ca8cdff","abstract_canon_sha256":"358a53aa65e5c847edab4230bb8a3eda0bb6fdb6ba0e79b41e9e0eac853323a9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:57.564347Z","signature_b64":"KikX9EhZ6pcbK5hECSMALamQDm2t5xJSJpLmb0SVCbh9dQPpLxkP26E9iOijcwvFRjo3+6JyFU7Zc9Msves6Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"42fe2ba9a4c2d077aceae4cd1d885d486d50ba3a5e7440624a3488aaeeb51e16","last_reissued_at":"2026-05-18T00:53:57.563742Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:57.563742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray/GeV emissions from Crab-like pulsars in LMC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"(2) The University of Hong Kong), J. Takata (1), K.S. Cheng (2) ((1) Huazhong University of Science, Technology","submitted_at":"2016-12-01T06:16:18Z","abstract_excerpt":"We discuss X-ray and gamma-ray emissions from Crab-like pulsars, PSRs~J0537-6910 and~J0540-6919, in Large Magellanic Cloud. Fermi-LAT observations have resolved the gamma-ray emissions from these two pulsars and found the pulsed emissions from PSR~J0540-6919. The total pulsed radiation in the X-ray/gamma-ray energy bands of PSR~J0540-6919 is observed with the efficiency $\\eta_{J0540}\\sim 0.06$ (in 4$\\pi$ sr), which is about a factor of ten larger than $\\eta_{Crab}\\sim 0.006$ of the Crab pulsar. Although PSR~J0537-6910 has the highest spin-down power among currently known pulsars, the efficienc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.00158","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":"1612.00158","created_at":"2026-05-18T00:53:57.563846+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.00158v1","created_at":"2026-05-18T00:53:57.563846+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.00158","created_at":"2026-05-18T00:53:57.563846+00:00"},{"alias_kind":"pith_short_12","alias_value":"IL7CXKNEYLIH","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_16","alias_value":"IL7CXKNEYLIHPLHK","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_8","alias_value":"IL7CXKNE","created_at":"2026-05-18T12:30:22.444734+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/IL7CXKNEYLIHPLHK4TGR3CC5JB","json":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB.json","graph_json":"https://pith.science/api/pith-number/IL7CXKNEYLIHPLHK4TGR3CC5JB/graph.json","events_json":"https://pith.science/api/pith-number/IL7CXKNEYLIHPLHK4TGR3CC5JB/events.json","paper":"https://pith.science/paper/IL7CXKNE"},"agent_actions":{"view_html":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB","download_json":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB.json","view_paper":"https://pith.science/paper/IL7CXKNE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.00158&json=true","fetch_graph":"https://pith.science/api/pith-number/IL7CXKNEYLIHPLHK4TGR3CC5JB/graph.json","fetch_events":"https://pith.science/api/pith-number/IL7CXKNEYLIHPLHK4TGR3CC5JB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB/action/storage_attestation","attest_author":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB/action/author_attestation","sign_citation":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB/action/citation_signature","submit_replication":"https://pith.science/pith/IL7CXKNEYLIHPLHK4TGR3CC5JB/action/replication_record"}},"created_at":"2026-05-18T00:53:57.563846+00:00","updated_at":"2026-05-18T00:53:57.563846+00:00"}