{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3CXSWIMZEA7R5CV3QF2VU4R3FC","short_pith_number":"pith:3CXSWIMZ","schema_version":"1.0","canonical_sha256":"d8af2b2199203f1e8abb81755a723b289f76e795f2b22bb22f3a3f79cb48ca9b","source":{"kind":"arxiv","id":"1708.00325","version":1},"attestation_state":"computed","paper":{"title":"Modifying the Standard Disk Model for the Ultraviolet Spectral Analysis of Disk-dominated Cataclysmic Variables. I. The Novalikes MV Lyrae, BZ Camelopardalis, and V592 Cassiopeiae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Edward M. Sion, Patrick Godon, Solen Balman, William P. Blair","submitted_at":"2017-08-01T13:53:17Z","abstract_excerpt":"The standard disk is often inadequate to model disk-dominated cataclysmic variables (CVs) and generates a spectrum that is bluer than the observed UV spectra [Puebla et al 2007]. X-ray observations of these systems reveal an optically thin boundary layer (BL) expected to appear as an inner hole in the disk. Consequently, we truncate the inner disk. However, instead of removing the inner disk, we impose the no-shear boundary condition at the truncation radius, thereby lowering the disk temperature and generating a spectrum that better fits the UV data. With our modified disk, we analyze the arc"},"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":"1708.00325","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2017-08-01T13:53:17Z","cross_cats_sorted":[],"title_canon_sha256":"573ae7bfe658f31a3650f1cbcd4a184a0952be0430c582c6fca1c630abb4cddc","abstract_canon_sha256":"5750580f23b0b53da96fbebff95a52b631557d612f154131a3fc20a4f737db47"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:02.800141Z","signature_b64":"/SfRPreznrsFhZGh7I/avOT+gnymYGoygq1qbnz2QjuYd0NgZXMnFs/TIzFmSLBZa0D3pOkLCs1QcbHERSgfCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d8af2b2199203f1e8abb81755a723b289f76e795f2b22bb22f3a3f79cb48ca9b","last_reissued_at":"2026-05-18T00:36:02.799667Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:02.799667Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modifying the Standard Disk Model for the Ultraviolet Spectral Analysis of Disk-dominated Cataclysmic Variables. I. The Novalikes MV Lyrae, BZ Camelopardalis, and V592 Cassiopeiae","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Edward M. Sion, Patrick Godon, Solen Balman, William P. Blair","submitted_at":"2017-08-01T13:53:17Z","abstract_excerpt":"The standard disk is often inadequate to model disk-dominated cataclysmic variables (CVs) and generates a spectrum that is bluer than the observed UV spectra [Puebla et al 2007]. X-ray observations of these systems reveal an optically thin boundary layer (BL) expected to appear as an inner hole in the disk. Consequently, we truncate the inner disk. However, instead of removing the inner disk, we impose the no-shear boundary condition at the truncation radius, thereby lowering the disk temperature and generating a spectrum that better fits the UV data. With our modified disk, we analyze the arc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.00325","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":"1708.00325","created_at":"2026-05-18T00:36:02.799730+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.00325v1","created_at":"2026-05-18T00:36:02.799730+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.00325","created_at":"2026-05-18T00:36:02.799730+00:00"},{"alias_kind":"pith_short_12","alias_value":"3CXSWIMZEA7R","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3CXSWIMZEA7R5CV3","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3CXSWIMZ","created_at":"2026-05-18T12:30:58.224056+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/3CXSWIMZEA7R5CV3QF2VU4R3FC","json":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC.json","graph_json":"https://pith.science/api/pith-number/3CXSWIMZEA7R5CV3QF2VU4R3FC/graph.json","events_json":"https://pith.science/api/pith-number/3CXSWIMZEA7R5CV3QF2VU4R3FC/events.json","paper":"https://pith.science/paper/3CXSWIMZ"},"agent_actions":{"view_html":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC","download_json":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC.json","view_paper":"https://pith.science/paper/3CXSWIMZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.00325&json=true","fetch_graph":"https://pith.science/api/pith-number/3CXSWIMZEA7R5CV3QF2VU4R3FC/graph.json","fetch_events":"https://pith.science/api/pith-number/3CXSWIMZEA7R5CV3QF2VU4R3FC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC/action/storage_attestation","attest_author":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC/action/author_attestation","sign_citation":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC/action/citation_signature","submit_replication":"https://pith.science/pith/3CXSWIMZEA7R5CV3QF2VU4R3FC/action/replication_record"}},"created_at":"2026-05-18T00:36:02.799730+00:00","updated_at":"2026-05-18T00:36:02.799730+00:00"}