{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:FHZOIWOHDM4546AZURIPIZ63BT","short_pith_number":"pith:FHZOIWOH","schema_version":"1.0","canonical_sha256":"29f2e459c71b39de7819a450f467db0cca64edad0032fc43be11129f8c529ba1","source":{"kind":"arxiv","id":"2111.09788","version":1},"attestation_state":"computed","paper":{"title":"VLA proper motion constraints on the origin, age, and potential magnetar future of PSR J1734$-$3333","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Deller, C. M. Espinoza, M. Vidal-Navarro, S. Chatterjee, W. C. G. Ho","submitted_at":"2021-11-18T16:38:45Z","abstract_excerpt":"The characteristic age of PSR J1734$-$3333 estimated from its current spin down rate implies that it is a young pulsar ($\\tau_c<10$ kyr). But the time derivative of its spin down rate differs markedly from that assumed for normal radio pulsars, meaning its actual age is uncertain. G354.8$-$0.8 is a supernova remnant (SNR) whose centre is located 21 arcmin away of the pulsar, and with a morphology that suggests an association with the pulsar. We want to assess the likelihood of the association between PSR J1734$-$3333 and G354.8$-$0.8 or other nearby supernova remnants quantitatively, with the "},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2111.09788","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2021-11-18T16:38:45Z","cross_cats_sorted":[],"title_canon_sha256":"82869db1ebb032332ba3ce5cb57101b725a997f066e19097e61368e8bc34149f","abstract_canon_sha256":"0cbdd8730dcdd9742ffedbc1d4609748af808560dde79e0748899e09a728c744"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:04:25.090371Z","signature_b64":"UvZfxalTa3n3okiKc691CGUbVVh+1s6z7RtyuOQgSx9fYdQZVU7sN3+b9trzysNLBO84M+0Es9KIGJfpf8+WCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"29f2e459c71b39de7819a450f467db0cca64edad0032fc43be11129f8c529ba1","last_reissued_at":"2026-07-05T04:04:25.089959Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:04:25.089959Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"VLA proper motion constraints on the origin, age, and potential magnetar future of PSR J1734$-$3333","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Deller, C. M. Espinoza, M. Vidal-Navarro, S. Chatterjee, W. C. G. Ho","submitted_at":"2021-11-18T16:38:45Z","abstract_excerpt":"The characteristic age of PSR J1734$-$3333 estimated from its current spin down rate implies that it is a young pulsar ($\\tau_c<10$ kyr). But the time derivative of its spin down rate differs markedly from that assumed for normal radio pulsars, meaning its actual age is uncertain. G354.8$-$0.8 is a supernova remnant (SNR) whose centre is located 21 arcmin away of the pulsar, and with a morphology that suggests an association with the pulsar. We want to assess the likelihood of the association between PSR J1734$-$3333 and G354.8$-$0.8 or other nearby supernova remnants quantitatively, with the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.09788","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/2111.09788/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":"2111.09788","created_at":"2026-07-05T04:04:25.090015+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.09788v1","created_at":"2026-07-05T04:04:25.090015+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.09788","created_at":"2026-07-05T04:04:25.090015+00:00"},{"alias_kind":"pith_short_12","alias_value":"FHZOIWOHDM45","created_at":"2026-07-05T04:04:25.090015+00:00"},{"alias_kind":"pith_short_16","alias_value":"FHZOIWOHDM4546AZ","created_at":"2026-07-05T04:04:25.090015+00:00"},{"alias_kind":"pith_short_8","alias_value":"FHZOIWOH","created_at":"2026-07-05T04:04:25.090015+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/FHZOIWOHDM4546AZURIPIZ63BT","json":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT.json","graph_json":"https://pith.science/api/pith-number/FHZOIWOHDM4546AZURIPIZ63BT/graph.json","events_json":"https://pith.science/api/pith-number/FHZOIWOHDM4546AZURIPIZ63BT/events.json","paper":"https://pith.science/paper/FHZOIWOH"},"agent_actions":{"view_html":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT","download_json":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT.json","view_paper":"https://pith.science/paper/FHZOIWOH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.09788&json=true","fetch_graph":"https://pith.science/api/pith-number/FHZOIWOHDM4546AZURIPIZ63BT/graph.json","fetch_events":"https://pith.science/api/pith-number/FHZOIWOHDM4546AZURIPIZ63BT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT/action/storage_attestation","attest_author":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT/action/author_attestation","sign_citation":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT/action/citation_signature","submit_replication":"https://pith.science/pith/FHZOIWOHDM4546AZURIPIZ63BT/action/replication_record"}},"created_at":"2026-07-05T04:04:25.090015+00:00","updated_at":"2026-07-05T04:04:25.090015+00:00"}