{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:XMANMKUSHNW7ENX67AUC6IRHGE","short_pith_number":"pith:XMANMKUS","schema_version":"1.0","canonical_sha256":"bb00d62a923b6df236fef8282f2227310e5b9fd39c51f389bb6e56c6447ad7df","source":{"kind":"arxiv","id":"2506.04371","version":1},"attestation_state":"computed","paper":{"title":"Precise Timing Analysis of Four Magnetic Cataclysmic Variables with TESS","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Ajay Kumar Singh, Arti Joshi, Jeewan C Pandey, Nikita Rawat, Srinivas M Rao","submitted_at":"2025-06-04T18:37:01Z","abstract_excerpt":"We analysed high time-resolution optical photometric data from the Transiting Exoplanet Survey Satellite (TESS) to study the timing behaviour of four intermediate polar-like objects, namely, V1460 Her, 1RXS J045707.4+452751, Swift J0958.0-4208, and V842 Cen. In the case of V1460 Her, we refined the measurement of its orbital period. Long-term observations suggest a gradual decrease in the orbital period of V1460 Her, and the stable light curve during the TESS observations indicates its quiescent state. We detected a beat period of 1290.6 $\\pm$ 0.5 s for the first time for the source 1RXS J0457"},"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":"2506.04371","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2025-06-04T18:37:01Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"f3cfa952e047ac9f00fb2274f270286aa6bd667f12e132106d93e72a2dbe7763","abstract_canon_sha256":"78b5b3524018aa58a70560567daa9eb35bcd0d1246a114070783d5c9f0d5e792"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:16:13.396337Z","signature_b64":"0P4QWbg3A3WDV5R/rWdYChvtijMh/Fdl4/vSJklb3VM6Wz7KdCqmtjQ5Y40zwtA9Ij+d29rkquqZ4GxY6DaCBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bb00d62a923b6df236fef8282f2227310e5b9fd39c51f389bb6e56c6447ad7df","last_reissued_at":"2026-07-05T11:16:13.395876Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:16:13.395876Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Precise Timing Analysis of Four Magnetic Cataclysmic Variables with TESS","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Ajay Kumar Singh, Arti Joshi, Jeewan C Pandey, Nikita Rawat, Srinivas M Rao","submitted_at":"2025-06-04T18:37:01Z","abstract_excerpt":"We analysed high time-resolution optical photometric data from the Transiting Exoplanet Survey Satellite (TESS) to study the timing behaviour of four intermediate polar-like objects, namely, V1460 Her, 1RXS J045707.4+452751, Swift J0958.0-4208, and V842 Cen. In the case of V1460 Her, we refined the measurement of its orbital period. Long-term observations suggest a gradual decrease in the orbital period of V1460 Her, and the stable light curve during the TESS observations indicates its quiescent state. We detected a beat period of 1290.6 $\\pm$ 0.5 s for the first time for the source 1RXS J0457"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.04371","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/2506.04371/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":"2506.04371","created_at":"2026-07-05T11:16:13.395934+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.04371v1","created_at":"2026-07-05T11:16:13.395934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.04371","created_at":"2026-07-05T11:16:13.395934+00:00"},{"alias_kind":"pith_short_12","alias_value":"XMANMKUSHNW7","created_at":"2026-07-05T11:16:13.395934+00:00"},{"alias_kind":"pith_short_16","alias_value":"XMANMKUSHNW7ENX6","created_at":"2026-07-05T11:16:13.395934+00:00"},{"alias_kind":"pith_short_8","alias_value":"XMANMKUS","created_at":"2026-07-05T11:16:13.395934+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08727","citing_title":"Cataclysmic Variables Photometric Periods from TESS","ref_index":231,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE","json":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE.json","graph_json":"https://pith.science/api/pith-number/XMANMKUSHNW7ENX67AUC6IRHGE/graph.json","events_json":"https://pith.science/api/pith-number/XMANMKUSHNW7ENX67AUC6IRHGE/events.json","paper":"https://pith.science/paper/XMANMKUS"},"agent_actions":{"view_html":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE","download_json":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE.json","view_paper":"https://pith.science/paper/XMANMKUS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.04371&json=true","fetch_graph":"https://pith.science/api/pith-number/XMANMKUSHNW7ENX67AUC6IRHGE/graph.json","fetch_events":"https://pith.science/api/pith-number/XMANMKUSHNW7ENX67AUC6IRHGE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE/action/storage_attestation","attest_author":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE/action/author_attestation","sign_citation":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE/action/citation_signature","submit_replication":"https://pith.science/pith/XMANMKUSHNW7ENX67AUC6IRHGE/action/replication_record"}},"created_at":"2026-07-05T11:16:13.395934+00:00","updated_at":"2026-07-05T11:16:13.395934+00:00"}