{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:XEJG6EZSZOITGQHXQVMLAWYS2Z","short_pith_number":"pith:XEJG6EZS","schema_version":"1.0","canonical_sha256":"b9126f1332cb913340f78558b05b12d653d60ab39b4c3a5ab8a76c0857ee46f1","source":{"kind":"arxiv","id":"2211.13407","version":1},"attestation_state":"computed","paper":{"title":"X-ray emission of radio-loud quasar SDSS J121426.52+140258.9: independent variations between optical/UV and X-ray emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Mai Liao, Minfeng Gu, Minhua Zhou, Muhammad S. Anjum","submitted_at":"2022-11-24T04:14:46Z","abstract_excerpt":"To understand the X-ray emission of active galactic nuclei (AGNs), we explored the optical-to-X-ray variation correlation of a radio-loud quasar (RLQ) SDSS J121426.52+140258.9 (hereafter J1214+1402) with multi-epoch observations of Swift and XMM-Newton telescopes. With the historical multi-band data, we found that the infrared to X-ray flux of RLQ J1214+1402 should not be dominated by the beamed jet emission. The Swift optical/UV and X-ray light curves showed that J1214+1402 has two optical states with low flux before 2014 April 08 and high flux after 2014 June 11, but has no significant X-ray"},"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":"2211.13407","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-11-24T04:14:46Z","cross_cats_sorted":[],"title_canon_sha256":"e5998202ba15902585d38435a8adf015f3281664454f12471332780eec3a4831","abstract_canon_sha256":"cd17fb4bbbac286e79b679c905f12ccccd46de8e53b3ff7ba469c6c1ae5d62b5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:30:18.937092Z","signature_b64":"GYYXvDkK7lqkDNylqcie7TldpmsqGAw8dbSfhZH1YH/wjTNoVuG5g4luL4y7Hl2KYsrRqpPgzdytZHkKUUXyDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b9126f1332cb913340f78558b05b12d653d60ab39b4c3a5ab8a76c0857ee46f1","last_reissued_at":"2026-07-05T05:30:18.936682Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:30:18.936682Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray emission of radio-loud quasar SDSS J121426.52+140258.9: independent variations between optical/UV and X-ray emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Mai Liao, Minfeng Gu, Minhua Zhou, Muhammad S. Anjum","submitted_at":"2022-11-24T04:14:46Z","abstract_excerpt":"To understand the X-ray emission of active galactic nuclei (AGNs), we explored the optical-to-X-ray variation correlation of a radio-loud quasar (RLQ) SDSS J121426.52+140258.9 (hereafter J1214+1402) with multi-epoch observations of Swift and XMM-Newton telescopes. With the historical multi-band data, we found that the infrared to X-ray flux of RLQ J1214+1402 should not be dominated by the beamed jet emission. The Swift optical/UV and X-ray light curves showed that J1214+1402 has two optical states with low flux before 2014 April 08 and high flux after 2014 June 11, but has no significant X-ray"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.13407","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/2211.13407/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":"2211.13407","created_at":"2026-07-05T05:30:18.936739+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.13407v1","created_at":"2026-07-05T05:30:18.936739+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.13407","created_at":"2026-07-05T05:30:18.936739+00:00"},{"alias_kind":"pith_short_12","alias_value":"XEJG6EZSZOIT","created_at":"2026-07-05T05:30:18.936739+00:00"},{"alias_kind":"pith_short_16","alias_value":"XEJG6EZSZOITGQHX","created_at":"2026-07-05T05:30:18.936739+00:00"},{"alias_kind":"pith_short_8","alias_value":"XEJG6EZS","created_at":"2026-07-05T05:30:18.936739+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/XEJG6EZSZOITGQHXQVMLAWYS2Z","json":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z.json","graph_json":"https://pith.science/api/pith-number/XEJG6EZSZOITGQHXQVMLAWYS2Z/graph.json","events_json":"https://pith.science/api/pith-number/XEJG6EZSZOITGQHXQVMLAWYS2Z/events.json","paper":"https://pith.science/paper/XEJG6EZS"},"agent_actions":{"view_html":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z","download_json":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z.json","view_paper":"https://pith.science/paper/XEJG6EZS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.13407&json=true","fetch_graph":"https://pith.science/api/pith-number/XEJG6EZSZOITGQHXQVMLAWYS2Z/graph.json","fetch_events":"https://pith.science/api/pith-number/XEJG6EZSZOITGQHXQVMLAWYS2Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z/action/storage_attestation","attest_author":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z/action/author_attestation","sign_citation":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z/action/citation_signature","submit_replication":"https://pith.science/pith/XEJG6EZSZOITGQHXQVMLAWYS2Z/action/replication_record"}},"created_at":"2026-07-05T05:30:18.936739+00:00","updated_at":"2026-07-05T05:30:18.936739+00:00"}