{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:QRBAHYXEKPTJAXTBNGNKLHHCYN","short_pith_number":"pith:QRBAHYXE","schema_version":"1.0","canonical_sha256":"844203e2e453e6905e61699aa59ce2c35d320a777008c0cae770112e84c60c00","source":{"kind":"arxiv","id":"1410.2332","version":1},"attestation_state":"computed","paper":{"title":"Discovery of X-ray Pulsations from the INTEGRAL Source IGR J11014-6103","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bodaghee, C.-Y. Ng, E. V. Gotthelf, F. Camilo, F. Rahoui, J. A. Tomsick, J. P. Halpern, J. Rodriguez, S. Chaty","submitted_at":"2014-10-09T01:32:22Z","abstract_excerpt":"We report the discovery of PSR J1101-6101, a 62.8 ms pulsar in IGR J11014-6103, a hard X-ray source with a jet and a cometary tail that strongly suggests it is moving away from the center of the supernova remnant (SNR) MSH 11-61A at v>1000 km/s. Two XMM-Newton observations were obtained with the EPIC pn in small window mode, resulting in the measurement of its spin-down luminosity E_dot = 1.36e36 erg/s, characteristic age Tau_c = 116 kyr, and surface magnetic field strength B_s = 7.4e11 G. In comparison to Tau_c, the 10-30 kyr age estimated for MSH 11-61A suggests that the pulsar was born in t"},"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":"1410.2332","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-10-09T01:32:22Z","cross_cats_sorted":[],"title_canon_sha256":"34859d1f0233137e535386e89fb7aec4a743a46b019ecda2daf2ecd4c5088691","abstract_canon_sha256":"007e5cc1410e40c0353df4968b5052eeab351de4857c8b15ae8ba0716570b5dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:49.781910Z","signature_b64":"XUSoBuztQDQvqgGpB0MgsRdlvDdBhQgcyDITj0eof5SnxlvX3CtC6vG3NMdPVF7vYSqil9NIv0k31ADeyNQ2Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"844203e2e453e6905e61699aa59ce2c35d320a777008c0cae770112e84c60c00","last_reissued_at":"2026-05-18T01:41:49.781384Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:49.781384Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of X-ray Pulsations from the INTEGRAL Source IGR J11014-6103","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Bodaghee, C.-Y. Ng, E. V. Gotthelf, F. Camilo, F. Rahoui, J. A. Tomsick, J. P. Halpern, J. Rodriguez, S. Chaty","submitted_at":"2014-10-09T01:32:22Z","abstract_excerpt":"We report the discovery of PSR J1101-6101, a 62.8 ms pulsar in IGR J11014-6103, a hard X-ray source with a jet and a cometary tail that strongly suggests it is moving away from the center of the supernova remnant (SNR) MSH 11-61A at v>1000 km/s. Two XMM-Newton observations were obtained with the EPIC pn in small window mode, resulting in the measurement of its spin-down luminosity E_dot = 1.36e36 erg/s, characteristic age Tau_c = 116 kyr, and surface magnetic field strength B_s = 7.4e11 G. In comparison to Tau_c, the 10-30 kyr age estimated for MSH 11-61A suggests that the pulsar was born in t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.2332","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":"1410.2332","created_at":"2026-05-18T01:41:49.781480+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.2332v1","created_at":"2026-05-18T01:41:49.781480+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.2332","created_at":"2026-05-18T01:41:49.781480+00:00"},{"alias_kind":"pith_short_12","alias_value":"QRBAHYXEKPTJ","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"QRBAHYXEKPTJAXTB","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"QRBAHYXE","created_at":"2026-05-18T12:28:46.137349+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/QRBAHYXEKPTJAXTBNGNKLHHCYN","json":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN.json","graph_json":"https://pith.science/api/pith-number/QRBAHYXEKPTJAXTBNGNKLHHCYN/graph.json","events_json":"https://pith.science/api/pith-number/QRBAHYXEKPTJAXTBNGNKLHHCYN/events.json","paper":"https://pith.science/paper/QRBAHYXE"},"agent_actions":{"view_html":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN","download_json":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN.json","view_paper":"https://pith.science/paper/QRBAHYXE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.2332&json=true","fetch_graph":"https://pith.science/api/pith-number/QRBAHYXEKPTJAXTBNGNKLHHCYN/graph.json","fetch_events":"https://pith.science/api/pith-number/QRBAHYXEKPTJAXTBNGNKLHHCYN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN/action/storage_attestation","attest_author":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN/action/author_attestation","sign_citation":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN/action/citation_signature","submit_replication":"https://pith.science/pith/QRBAHYXEKPTJAXTBNGNKLHHCYN/action/replication_record"}},"created_at":"2026-05-18T01:41:49.781480+00:00","updated_at":"2026-05-18T01:41:49.781480+00:00"}