{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:6YKFKP777BXOXHCTK36CZJVLRT","short_pith_number":"pith:6YKFKP77","schema_version":"1.0","canonical_sha256":"f614553ffff86eeb9c5356fc2ca6ab8cf287ece0eebcb8a4fd3ed93b2173f736","source":{"kind":"arxiv","id":"1006.0485","version":1},"attestation_state":"computed","paper":{"title":"X-ray reflected spectra from accretion disk models. I. Constant density atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Javier Garcia, Timothy Kallman","submitted_at":"2010-06-02T20:00:12Z","abstract_excerpt":"We present new models for illuminated accretion disks, their structure and reprocessed emission. We consider the effects of incident X-rays on the surface of an accretion disk by solving simultaneously the equations of radiative transfer, energy balance and ionization equilibrium over a large range of column densities. We assume plane-parallel geometry and azimuthal symmetry, such that each calculation corresponds to a ring at a given distance from the central object. Our models include recent and complete atomic data for K-shell processes of the iron and oxygen isonuclear sequences. We examin"},"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":"1006.0485","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-06-02T20:00:12Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"330fe0a0c7b6c34678550a191c4be66781424093fca68ed2407a72d17fd02392","abstract_canon_sha256":"a9b698bc3dd38f16feb858d45642aab346aa9ec4f1932e3fda8dca9e828f6fd8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:07:05.442154Z","signature_b64":"qH8EZVmn7qoB7kc70s30T2OOHPd84Engg78wFYvRSumDaaY6LVJ5e/BUA+gUpv6sEoiegZalNI2wDDoqys1aAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f614553ffff86eeb9c5356fc2ca6ab8cf287ece0eebcb8a4fd3ed93b2173f736","last_reissued_at":"2026-05-18T02:07:05.441572Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:07:05.441572Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray reflected spectra from accretion disk models. I. Constant density atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Javier Garcia, Timothy Kallman","submitted_at":"2010-06-02T20:00:12Z","abstract_excerpt":"We present new models for illuminated accretion disks, their structure and reprocessed emission. We consider the effects of incident X-rays on the surface of an accretion disk by solving simultaneously the equations of radiative transfer, energy balance and ionization equilibrium over a large range of column densities. We assume plane-parallel geometry and azimuthal symmetry, such that each calculation corresponds to a ring at a given distance from the central object. Our models include recent and complete atomic data for K-shell processes of the iron and oxygen isonuclear sequences. We examin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.0485","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":"1006.0485","created_at":"2026-05-18T02:07:05.441668+00:00"},{"alias_kind":"arxiv_version","alias_value":"1006.0485v1","created_at":"2026-05-18T02:07:05.441668+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.0485","created_at":"2026-05-18T02:07:05.441668+00:00"},{"alias_kind":"pith_short_12","alias_value":"6YKFKP777BXO","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_16","alias_value":"6YKFKP777BXOXHCT","created_at":"2026-05-18T12:26:04.259169+00:00"},{"alias_kind":"pith_short_8","alias_value":"6YKFKP77","created_at":"2026-05-18T12:26:04.259169+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.20317","citing_title":"Simulation-Based Prediction of Black Hole Fe K$\\alpha$ Line Profiles","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT","json":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT.json","graph_json":"https://pith.science/api/pith-number/6YKFKP777BXOXHCTK36CZJVLRT/graph.json","events_json":"https://pith.science/api/pith-number/6YKFKP777BXOXHCTK36CZJVLRT/events.json","paper":"https://pith.science/paper/6YKFKP77"},"agent_actions":{"view_html":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT","download_json":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT.json","view_paper":"https://pith.science/paper/6YKFKP77","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1006.0485&json=true","fetch_graph":"https://pith.science/api/pith-number/6YKFKP777BXOXHCTK36CZJVLRT/graph.json","fetch_events":"https://pith.science/api/pith-number/6YKFKP777BXOXHCTK36CZJVLRT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT/action/storage_attestation","attest_author":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT/action/author_attestation","sign_citation":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT/action/citation_signature","submit_replication":"https://pith.science/pith/6YKFKP777BXOXHCTK36CZJVLRT/action/replication_record"}},"created_at":"2026-05-18T02:07:05.441668+00:00","updated_at":"2026-05-18T02:07:05.441668+00:00"}