{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:IVNYCLFSZ4G4VO373WWVBIUQSF","short_pith_number":"pith:IVNYCLFS","schema_version":"1.0","canonical_sha256":"455b812cb2cf0dcabb7fddad50a290914aa267a0f799618f673cb0efeeabc79f","source":{"kind":"arxiv","id":"2606.04232","version":1},"attestation_state":"computed","paper":{"title":"Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. J. M. Thomson, A. Zic, B. N. Barlow, D. Dobie, D. Huber, D. L. Kaplan, E. Lenc, F. Zahedy, G. Heald, G. J. Yang, G. R. Sivakoff, I. Andreoni, I. de Ruiter, J. Carney, J. K. Leung, Joshua Pritchard, Kovi Rose, K. Shaji, L. N. Driessen, M. Caleb, M. G. Pedersen, M. Gu, N. Rea, R. Momose, Tara Murphy, W. Lu, Y. L. Wang, Y. Qu, Ziteng Wang","submitted_at":"2026-06-02T21:32:49Z","abstract_excerpt":"Long period radio transients (LPTs) are coherent bursts of polarised radio emission that repeat periodically on timescales of minutes to hours. Little is known about the physical origins of these systems. Astronomers have proposed magnetars that rotate slowly and white dwarfs that rapidly orbit with a companion star as potential explanations. While several recent examples appear to support the latter hypothesis, the mechanism generating these bright radio pulses remains poorly understood. Here we report our discovery and classification of the LPT ASKAP J174508.9-505149 as an accreting white dw"},"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":"2606.04232","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2026-06-02T21:32:49Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"7e78d31e1927ee9a96fdf66cfc3a67abc7da6a7faee0a96a9e898a767d91415b","abstract_canon_sha256":"4ed6307022370a79890dda7eae70aca1fe653deac66caebd1425272398fd79dc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-04T01:08:59.531351Z","signature_b64":"0n+DzImZokz+5mb92+HprcwetcJIEDgybrXhfMk31A+iRPLsDcVd78D6S7QiMAaH7eWgnMcV+cVWEO1JhZYYCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"455b812cb2cf0dcabb7fddad50a290914aa267a0f799618f673cb0efeeabc79f","last_reissued_at":"2026-06-04T01:08:59.530821Z","signature_status":"signed_v1","first_computed_at":"2026-06-04T01:08:59.530821Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. J. M. Thomson, A. Zic, B. N. Barlow, D. Dobie, D. Huber, D. L. Kaplan, E. Lenc, F. Zahedy, G. Heald, G. J. Yang, G. R. Sivakoff, I. Andreoni, I. de Ruiter, J. Carney, J. K. Leung, Joshua Pritchard, Kovi Rose, K. Shaji, L. N. Driessen, M. Caleb, M. G. Pedersen, M. Gu, N. Rea, R. Momose, Tara Murphy, W. Lu, Y. L. Wang, Y. Qu, Ziteng Wang","submitted_at":"2026-06-02T21:32:49Z","abstract_excerpt":"Long period radio transients (LPTs) are coherent bursts of polarised radio emission that repeat periodically on timescales of minutes to hours. Little is known about the physical origins of these systems. Astronomers have proposed magnetars that rotate slowly and white dwarfs that rapidly orbit with a companion star as potential explanations. While several recent examples appear to support the latter hypothesis, the mechanism generating these bright radio pulses remains poorly understood. Here we report our discovery and classification of the LPT ASKAP J174508.9-505149 as an accreting white dw"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.04232","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/2606.04232/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":"2606.04232","created_at":"2026-06-04T01:08:59.530919+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.04232v1","created_at":"2026-06-04T01:08:59.530919+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.04232","created_at":"2026-06-04T01:08:59.530919+00:00"},{"alias_kind":"pith_short_12","alias_value":"IVNYCLFSZ4G4","created_at":"2026-06-04T01:08:59.530919+00:00"},{"alias_kind":"pith_short_16","alias_value":"IVNYCLFSZ4G4VO37","created_at":"2026-06-04T01:08:59.530919+00:00"},{"alias_kind":"pith_short_8","alias_value":"IVNYCLFS","created_at":"2026-06-04T01:08:59.530919+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/IVNYCLFSZ4G4VO373WWVBIUQSF","json":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF.json","graph_json":"https://pith.science/api/pith-number/IVNYCLFSZ4G4VO373WWVBIUQSF/graph.json","events_json":"https://pith.science/api/pith-number/IVNYCLFSZ4G4VO373WWVBIUQSF/events.json","paper":"https://pith.science/paper/IVNYCLFS"},"agent_actions":{"view_html":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF","download_json":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF.json","view_paper":"https://pith.science/paper/IVNYCLFS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.04232&json=true","fetch_graph":"https://pith.science/api/pith-number/IVNYCLFSZ4G4VO373WWVBIUQSF/graph.json","fetch_events":"https://pith.science/api/pith-number/IVNYCLFSZ4G4VO373WWVBIUQSF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF/action/storage_attestation","attest_author":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF/action/author_attestation","sign_citation":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF/action/citation_signature","submit_replication":"https://pith.science/pith/IVNYCLFSZ4G4VO373WWVBIUQSF/action/replication_record"}},"created_at":"2026-06-04T01:08:59.530919+00:00","updated_at":"2026-06-04T01:08:59.530919+00:00"}