{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:KCWYV5ALLTWM4ZLS3VSTWROWN6","short_pith_number":"pith:KCWYV5AL","schema_version":"1.0","canonical_sha256":"50ad8af40b5cecce6572dd653b45d66fb0b140881d5b9591d48c78d4c74fee56","source":{"kind":"arxiv","id":"1709.08574","version":1},"attestation_state":"computed","paper":{"title":"Simultaneous Chandra and VLA Observations of the Transitional Millisecond Pulsar PSR J1023+0038: Anti-correlated X-ray and Radio Variability","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Adam T. Deller, Alessandro Patruno, Amruta Jaodand, Anne M. Archibald, Caroline D'Angelo, Cees Bassa, James C. A. Miller-Jones, Jason W. T. Hessels, Slavko Bogdanov","submitted_at":"2017-09-25T16:28:52Z","abstract_excerpt":"We present coordinated Chandra X-ray Observatory and Karl G. Jansky Very Large Array observations of the transitional millisecond pulsar PSR J1023+0038 in its low-luminosity accreting state. The unprecedented five hours of strictly simultaneous X-ray and radio continuum coverage for the first time unambiguously show a highly reproducible, anti-correlated variability pattern. The characteristic switches from the X-ray high mode into a low mode are always accompanied by a radio brightening with duration that closely matches the X-ray low mode interval. This behavior cannot be explained by a cano"},"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":"1709.08574","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-09-25T16:28:52Z","cross_cats_sorted":[],"title_canon_sha256":"b2baeae376efcf0ec82791a2c9a8720ac9427f7fdb68b3ad303c716bc982d460","abstract_canon_sha256":"e8c94c9a4df858eeed692911e7f4fcca331f06c04ff3c187cd59013283870c8c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:18:53.295792Z","signature_b64":"RUPr0WCcdAqWWbFielbkVFiKZUKObUGwBmtcR1GgarC/VEHtNmq8RmlcndE8TxkVMieeMHaUcDzu4rN0T1BpAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"50ad8af40b5cecce6572dd653b45d66fb0b140881d5b9591d48c78d4c74fee56","last_reissued_at":"2026-05-18T00:18:53.295393Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:18:53.295393Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simultaneous Chandra and VLA Observations of the Transitional Millisecond Pulsar PSR J1023+0038: Anti-correlated X-ray and Radio Variability","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Adam T. Deller, Alessandro Patruno, Amruta Jaodand, Anne M. Archibald, Caroline D'Angelo, Cees Bassa, James C. A. Miller-Jones, Jason W. T. Hessels, Slavko Bogdanov","submitted_at":"2017-09-25T16:28:52Z","abstract_excerpt":"We present coordinated Chandra X-ray Observatory and Karl G. Jansky Very Large Array observations of the transitional millisecond pulsar PSR J1023+0038 in its low-luminosity accreting state. The unprecedented five hours of strictly simultaneous X-ray and radio continuum coverage for the first time unambiguously show a highly reproducible, anti-correlated variability pattern. The characteristic switches from the X-ray high mode into a low mode are always accompanied by a radio brightening with duration that closely matches the X-ray low mode interval. This behavior cannot be explained by a cano"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.08574","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":"1709.08574","created_at":"2026-05-18T00:18:53.295460+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.08574v1","created_at":"2026-05-18T00:18:53.295460+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.08574","created_at":"2026-05-18T00:18:53.295460+00:00"},{"alias_kind":"pith_short_12","alias_value":"KCWYV5ALLTWM","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"KCWYV5ALLTWM4ZLS","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"KCWYV5AL","created_at":"2026-05-18T12:31:24.725408+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/KCWYV5ALLTWM4ZLS3VSTWROWN6","json":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6.json","graph_json":"https://pith.science/api/pith-number/KCWYV5ALLTWM4ZLS3VSTWROWN6/graph.json","events_json":"https://pith.science/api/pith-number/KCWYV5ALLTWM4ZLS3VSTWROWN6/events.json","paper":"https://pith.science/paper/KCWYV5AL"},"agent_actions":{"view_html":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6","download_json":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6.json","view_paper":"https://pith.science/paper/KCWYV5AL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.08574&json=true","fetch_graph":"https://pith.science/api/pith-number/KCWYV5ALLTWM4ZLS3VSTWROWN6/graph.json","fetch_events":"https://pith.science/api/pith-number/KCWYV5ALLTWM4ZLS3VSTWROWN6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6/action/storage_attestation","attest_author":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6/action/author_attestation","sign_citation":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6/action/citation_signature","submit_replication":"https://pith.science/pith/KCWYV5ALLTWM4ZLS3VSTWROWN6/action/replication_record"}},"created_at":"2026-05-18T00:18:53.295460+00:00","updated_at":"2026-05-18T00:18:53.295460+00:00"}