{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:VZUQO2EPNYJ2F22FFPM46QWL65","short_pith_number":"pith:VZUQO2EP","schema_version":"1.0","canonical_sha256":"ae6907688f6e13a2eb452bd9cf42cbf74de81d9d506d5b1a13b0a6e123f1e1c8","source":{"kind":"arxiv","id":"2206.10625","version":1},"attestation_state":"computed","paper":{"title":"1RXH J082623.6-505741: a new long-period cataclysmic variable with an evolved donor and a low mass transfer rate","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Allison K. Hughes, Arash Bahramian, Craig O. Heinke, David J. Sand, Elias Aydi, Evangelia Tremou, James C. A. Miller-Jones, Jay Strader, Karina Voggel, Kirill V. Sokolovsky, Koji Mukai, Kwan-Lok Li, Laura Chomiuk, Laura Shishkovsky, Raimundo Lopes de Oliveira, Samuel J. Swihart","submitted_at":"2022-06-21T18:00:00Z","abstract_excerpt":"We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a $\\sim 0.4 M_{\\odot}$ K-type secondary transferring mass through a low-state accretion disk to a non-magnetic $\\sim 0.8 M_{\\odot}$ white dwarf. The secondary is overluminous for its mass and dominates the optical spectra at all epochs, and must be evolved to fill its Roche Lobe at this orbital period. The X-ray luminosity $L_X \\sim 1$-$2 \\times 10^{32}$ erg s$^{-1}$ derived from both new XMM-Newton and archival observations, although high co"},"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":"2206.10625","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2022-06-21T18:00:00Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"a1a50a99cc183fdce11f910a2ea753e8221392812c5f381e35289ede0f94323e","abstract_canon_sha256":"f4ff65953baf339c77d2793852d9df4776f72ba95b460d3a802a89e62e9a3194"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:48:56.745476Z","signature_b64":"uTuWHOSpNfLt+SS1DlTEvYcKoHlaN/A47Ha3YZ2WEsbqkK087Rr7bxWQ0z8Cca7XSXbFODmz3ysEhhFwYLf8DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae6907688f6e13a2eb452bd9cf42cbf74de81d9d506d5b1a13b0a6e123f1e1c8","last_reissued_at":"2026-07-05T04:48:56.744873Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:48:56.744873Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"1RXH J082623.6-505741: a new long-period cataclysmic variable with an evolved donor and a low mass transfer rate","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Allison K. Hughes, Arash Bahramian, Craig O. Heinke, David J. Sand, Elias Aydi, Evangelia Tremou, James C. A. Miller-Jones, Jay Strader, Karina Voggel, Kirill V. Sokolovsky, Koji Mukai, Kwan-Lok Li, Laura Chomiuk, Laura Shishkovsky, Raimundo Lopes de Oliveira, Samuel J. Swihart","submitted_at":"2022-06-21T18:00:00Z","abstract_excerpt":"We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a $\\sim 0.4 M_{\\odot}$ K-type secondary transferring mass through a low-state accretion disk to a non-magnetic $\\sim 0.8 M_{\\odot}$ white dwarf. The secondary is overluminous for its mass and dominates the optical spectra at all epochs, and must be evolved to fill its Roche Lobe at this orbital period. The X-ray luminosity $L_X \\sim 1$-$2 \\times 10^{32}$ erg s$^{-1}$ derived from both new XMM-Newton and archival observations, although high co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2206.10625","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/2206.10625/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":"2206.10625","created_at":"2026-07-05T04:48:56.744962+00:00"},{"alias_kind":"arxiv_version","alias_value":"2206.10625v1","created_at":"2026-07-05T04:48:56.744962+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2206.10625","created_at":"2026-07-05T04:48:56.744962+00:00"},{"alias_kind":"pith_short_12","alias_value":"VZUQO2EPNYJ2","created_at":"2026-07-05T04:48:56.744962+00:00"},{"alias_kind":"pith_short_16","alias_value":"VZUQO2EPNYJ2F22F","created_at":"2026-07-05T04:48:56.744962+00:00"},{"alias_kind":"pith_short_8","alias_value":"VZUQO2EP","created_at":"2026-07-05T04:48:56.744962+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/VZUQO2EPNYJ2F22FFPM46QWL65","json":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65.json","graph_json":"https://pith.science/api/pith-number/VZUQO2EPNYJ2F22FFPM46QWL65/graph.json","events_json":"https://pith.science/api/pith-number/VZUQO2EPNYJ2F22FFPM46QWL65/events.json","paper":"https://pith.science/paper/VZUQO2EP"},"agent_actions":{"view_html":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65","download_json":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65.json","view_paper":"https://pith.science/paper/VZUQO2EP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2206.10625&json=true","fetch_graph":"https://pith.science/api/pith-number/VZUQO2EPNYJ2F22FFPM46QWL65/graph.json","fetch_events":"https://pith.science/api/pith-number/VZUQO2EPNYJ2F22FFPM46QWL65/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65/action/storage_attestation","attest_author":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65/action/author_attestation","sign_citation":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65/action/citation_signature","submit_replication":"https://pith.science/pith/VZUQO2EPNYJ2F22FFPM46QWL65/action/replication_record"}},"created_at":"2026-07-05T04:48:56.744962+00:00","updated_at":"2026-07-05T04:48:56.744962+00:00"}