{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:TNNSOCQ3E2DEYF5PZ7TDSU64MP","short_pith_number":"pith:TNNSOCQ3","schema_version":"1.0","canonical_sha256":"9b5b270a1b26864c17afcfe63953dc63c200f4bbd5515aca022f7303480dc612","source":{"kind":"arxiv","id":"1109.1590","version":1},"attestation_state":"computed","paper":{"title":"Observations of Energetic High Magnetic Field Pulsars with the Fermi Large Area Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. A. Abdo, A. G. Lyne, A. K. Harding, A. Noutsos, A. Possenti, B. W. Stappers, C. M. Espinoza, D. A. Smith, D. Parent, E. V. Gotthelf, F. Camilo, F. Giordano, G. Hobbs, H. A. Craig, K. Watters, L. Guillemot, M. Burgay, M. E. DeCesar, M. G. Baring, M. Keith, M. Kerr, M. Kramer, M. Livingstone, P. C. C. Freire, P. R. den Hartog, P. Weltevrede, R. N. Manchester, R. W. Romani, S. Johnston, V. M. Kaspi","submitted_at":"2011-09-07T22:14:53Z","abstract_excerpt":"We report the detection of gamma-ray pulsations from the high-magnetic-field rotation-powered pulsar PSR J1119-6127 using data from the Fermi Large Area Telescope. The gamma-ray light curve of PSR J1119-6127 shows a single, wide peak offset from the radio peak by 0.43 pm 0.02 in phase. Spectral analysis suggests a power law of index 1.0 pm 0.3 with an energy cut-off at 0.8 pm 0.2 GeV. The first uncertainty is statistical and the second is systematic. We discuss the emission models of PSR J1119-6127 and demonstrate that despite the object's high surface magnetic field---near that of magnetars--"},"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":"1109.1590","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-09-07T22:14:53Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"bb8691a08d6336c833159597054aa0029b63c6c9fe5f0055851eac36e9150b14","abstract_canon_sha256":"92f4df173289056a2b6c6ef40d66b9541045cd547016e298b5c4dbb4d553ca90"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:00:38.131014Z","signature_b64":"oUEnWjZLRCTD093NkcOYfRNxIH0NNS7Qcv5jY3SDrjSwR3Qd+S5oHCezKusBkhitUKnhocs6Q8KnaJGQ0fUiAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b5b270a1b26864c17afcfe63953dc63c200f4bbd5515aca022f7303480dc612","last_reissued_at":"2026-05-18T02:00:38.130457Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:00:38.130457Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Observations of Energetic High Magnetic Field Pulsars with the Fermi Large Area Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. A. Abdo, A. G. Lyne, A. K. Harding, A. Noutsos, A. Possenti, B. W. Stappers, C. M. Espinoza, D. A. Smith, D. Parent, E. V. Gotthelf, F. Camilo, F. Giordano, G. Hobbs, H. A. Craig, K. Watters, L. Guillemot, M. Burgay, M. E. DeCesar, M. G. Baring, M. Keith, M. Kerr, M. Kramer, M. Livingstone, P. C. C. Freire, P. R. den Hartog, P. Weltevrede, R. N. Manchester, R. W. Romani, S. Johnston, V. M. Kaspi","submitted_at":"2011-09-07T22:14:53Z","abstract_excerpt":"We report the detection of gamma-ray pulsations from the high-magnetic-field rotation-powered pulsar PSR J1119-6127 using data from the Fermi Large Area Telescope. The gamma-ray light curve of PSR J1119-6127 shows a single, wide peak offset from the radio peak by 0.43 pm 0.02 in phase. Spectral analysis suggests a power law of index 1.0 pm 0.3 with an energy cut-off at 0.8 pm 0.2 GeV. The first uncertainty is statistical and the second is systematic. We discuss the emission models of PSR J1119-6127 and demonstrate that despite the object's high surface magnetic field---near that of magnetars--"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.1590","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":"1109.1590","created_at":"2026-05-18T02:00:38.130546+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.1590v1","created_at":"2026-05-18T02:00:38.130546+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.1590","created_at":"2026-05-18T02:00:38.130546+00:00"},{"alias_kind":"pith_short_12","alias_value":"TNNSOCQ3E2DE","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_16","alias_value":"TNNSOCQ3E2DEYF5P","created_at":"2026-05-18T12:26:42.757692+00:00"},{"alias_kind":"pith_short_8","alias_value":"TNNSOCQ3","created_at":"2026-05-18T12:26:42.757692+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/TNNSOCQ3E2DEYF5PZ7TDSU64MP","json":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP.json","graph_json":"https://pith.science/api/pith-number/TNNSOCQ3E2DEYF5PZ7TDSU64MP/graph.json","events_json":"https://pith.science/api/pith-number/TNNSOCQ3E2DEYF5PZ7TDSU64MP/events.json","paper":"https://pith.science/paper/TNNSOCQ3"},"agent_actions":{"view_html":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP","download_json":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP.json","view_paper":"https://pith.science/paper/TNNSOCQ3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.1590&json=true","fetch_graph":"https://pith.science/api/pith-number/TNNSOCQ3E2DEYF5PZ7TDSU64MP/graph.json","fetch_events":"https://pith.science/api/pith-number/TNNSOCQ3E2DEYF5PZ7TDSU64MP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP/action/storage_attestation","attest_author":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP/action/author_attestation","sign_citation":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP/action/citation_signature","submit_replication":"https://pith.science/pith/TNNSOCQ3E2DEYF5PZ7TDSU64MP/action/replication_record"}},"created_at":"2026-05-18T02:00:38.130546+00:00","updated_at":"2026-05-18T02:00:38.130546+00:00"}