{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2003:BPRHEITKMQNBKWOLBWTLL5ZDEO","short_pith_number":"pith:BPRHEITK","schema_version":"1.0","canonical_sha256":"0be272226a641a1559cb0da6b5f7232396e7ad7e1796c2441ae4ac20b114c257","source":{"kind":"arxiv","id":"astro-ph/0310455","version":1},"attestation_state":"computed","paper":{"title":"Two Radio Pulsars with Magnetar Fields","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. G. Lyne, A. J. Faulkner, A. Possenti & N. D'Amico, D. R. Lorimer, F. Camilo, G. Hobbs, I. H. Stairs, M. A. McLaughlin, M. Kramer, R. N. Manchester, V. M. Kaspi","submitted_at":"2003-10-16T13:10:31Z","abstract_excerpt":"PSRs J1847-0130 and J1718-37184 have inferred surface dipole magnetic fields greater than those of any other known pulsars and well above the ``quantum critical field'' above which some models predict radio emission should not occur.These fields are similar to those of the anomalous X-ray pulsars (AXPs), which growing evidence suggests are ``magnetars''. The lack of AXP-like X-ray emission from these radio pulsars (and the non-detection of radio emission from the AXPs) creates new challenges for understanding pulsar emission physics and the relationship between these classes of apparently youn"},"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":"astro-ph/0310455","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2003-10-16T13:10:31Z","cross_cats_sorted":[],"title_canon_sha256":"1f24d512bc655094ac672b9f689fa465925a403bb6a209e38881b5fc8cccf4f3","abstract_canon_sha256":"c2fcb96ef5504e1040e802f578b7c0c68678e33ea80d01f1dbfeb8bb812ac4ee"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:13:06.254453Z","signature_b64":"KD79CylWB+6d3Mp/FGcuZJbdsKFacIoQPiAiHpfTOzPuendaFp4gfGO6f6lTjF+jVR/iO8HCv6LhUcJZ7dLAAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0be272226a641a1559cb0da6b5f7232396e7ad7e1796c2441ae4ac20b114c257","last_reissued_at":"2026-07-04T14:13:06.253934Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:13:06.253934Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Two Radio Pulsars with Magnetar Fields","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. G. Lyne, A. J. Faulkner, A. Possenti & N. D'Amico, D. R. Lorimer, F. Camilo, G. Hobbs, I. H. Stairs, M. A. McLaughlin, M. Kramer, R. N. Manchester, V. M. Kaspi","submitted_at":"2003-10-16T13:10:31Z","abstract_excerpt":"PSRs J1847-0130 and J1718-37184 have inferred surface dipole magnetic fields greater than those of any other known pulsars and well above the ``quantum critical field'' above which some models predict radio emission should not occur.These fields are similar to those of the anomalous X-ray pulsars (AXPs), which growing evidence suggests are ``magnetars''. The lack of AXP-like X-ray emission from these radio pulsars (and the non-detection of radio emission from the AXPs) creates new challenges for understanding pulsar emission physics and the relationship between these classes of apparently youn"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0310455","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0310455/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0310455","created_at":"2026-07-04T14:13:06.253994+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0310455v1","created_at":"2026-07-04T14:13:06.253994+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0310455","created_at":"2026-07-04T14:13:06.253994+00:00"},{"alias_kind":"pith_short_12","alias_value":"BPRHEITKMQNB","created_at":"2026-07-04T14:13:06.253994+00:00"},{"alias_kind":"pith_short_16","alias_value":"BPRHEITKMQNBKWOL","created_at":"2026-07-04T14:13:06.253994+00:00"},{"alias_kind":"pith_short_8","alias_value":"BPRHEITK","created_at":"2026-07-04T14:13:06.253994+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/BPRHEITKMQNBKWOLBWTLL5ZDEO","json":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO.json","graph_json":"https://pith.science/api/pith-number/BPRHEITKMQNBKWOLBWTLL5ZDEO/graph.json","events_json":"https://pith.science/api/pith-number/BPRHEITKMQNBKWOLBWTLL5ZDEO/events.json","paper":"https://pith.science/paper/BPRHEITK"},"agent_actions":{"view_html":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO","download_json":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO.json","view_paper":"https://pith.science/paper/BPRHEITK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0310455&json=true","fetch_graph":"https://pith.science/api/pith-number/BPRHEITKMQNBKWOLBWTLL5ZDEO/graph.json","fetch_events":"https://pith.science/api/pith-number/BPRHEITKMQNBKWOLBWTLL5ZDEO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO/action/storage_attestation","attest_author":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO/action/author_attestation","sign_citation":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO/action/citation_signature","submit_replication":"https://pith.science/pith/BPRHEITKMQNBKWOLBWTLL5ZDEO/action/replication_record"}},"created_at":"2026-07-04T14:13:06.253994+00:00","updated_at":"2026-07-04T14:13:06.253994+00:00"}