{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:IBBAKF5YNLBNA7RB5VJS2TILJW","short_pith_number":"pith:IBBAKF5Y","schema_version":"1.0","canonical_sha256":"40420517b86ac2d07e21ed532d4d0b4d8471a234c1aa1309b238c154a7e301fa","source":{"kind":"arxiv","id":"1209.2915","version":1},"attestation_state":"computed","paper":{"title":"Modeling optical and UV polarization of AGNs II. Polarization imaging and complex reprocessing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"C. M. Gaskell, D. Porquet, F. Marin, M. Dovciak, R. W. Goosmann","submitted_at":"2012-09-13T14:50:03Z","abstract_excerpt":"We model the spectropolarimetric signature resulting from the radiative coupling between the innermost parts of active galactic nuclei (AGNs). We use a new public version of STOKES, a Monte Carlo radiative transfer code presented in the first paper of this series. The code has been significantly improved for computational speed and polarization imaging has been implemented. We couple continuum sources with equatorial scattering regions, polar outflows, and toroidal obscuring dust and we study the resulting polarization. We compute a grid of thermal AGN models for different half-opening angles "},"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":"1209.2915","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-09-13T14:50:03Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"8dea154343a7a26a9447598aae6d194d1e7c6905ac865655e659f133094bab00","abstract_canon_sha256":"869befea7c27ee1fb40579ff3789f0e0724f5a7a7b59116c13aef53d6bba8b30"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:29.473000Z","signature_b64":"G2nnA8JSaqNbLs7qVzXna0sKT5X2GiE4UIu1BI9g89aMsW64pt64hCNgvEg3CzxEZRX6te9rAjTQyB5OlHbLDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40420517b86ac2d07e21ed532d4d0b4d8471a234c1aa1309b238c154a7e301fa","last_reissued_at":"2026-05-18T01:54:29.472360Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:29.472360Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling optical and UV polarization of AGNs II. Polarization imaging and complex reprocessing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"C. M. Gaskell, D. Porquet, F. Marin, M. Dovciak, R. W. Goosmann","submitted_at":"2012-09-13T14:50:03Z","abstract_excerpt":"We model the spectropolarimetric signature resulting from the radiative coupling between the innermost parts of active galactic nuclei (AGNs). We use a new public version of STOKES, a Monte Carlo radiative transfer code presented in the first paper of this series. The code has been significantly improved for computational speed and polarization imaging has been implemented. We couple continuum sources with equatorial scattering regions, polar outflows, and toroidal obscuring dust and we study the resulting polarization. We compute a grid of thermal AGN models for different half-opening angles "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.2915","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":"1209.2915","created_at":"2026-05-18T01:54:29.472471+00:00"},{"alias_kind":"arxiv_version","alias_value":"1209.2915v1","created_at":"2026-05-18T01:54:29.472471+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1209.2915","created_at":"2026-05-18T01:54:29.472471+00:00"},{"alias_kind":"pith_short_12","alias_value":"IBBAKF5YNLBN","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"IBBAKF5YNLBNA7RB","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"IBBAKF5Y","created_at":"2026-05-18T12:27:09.501522+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/IBBAKF5YNLBNA7RB5VJS2TILJW","json":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW.json","graph_json":"https://pith.science/api/pith-number/IBBAKF5YNLBNA7RB5VJS2TILJW/graph.json","events_json":"https://pith.science/api/pith-number/IBBAKF5YNLBNA7RB5VJS2TILJW/events.json","paper":"https://pith.science/paper/IBBAKF5Y"},"agent_actions":{"view_html":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW","download_json":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW.json","view_paper":"https://pith.science/paper/IBBAKF5Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1209.2915&json=true","fetch_graph":"https://pith.science/api/pith-number/IBBAKF5YNLBNA7RB5VJS2TILJW/graph.json","fetch_events":"https://pith.science/api/pith-number/IBBAKF5YNLBNA7RB5VJS2TILJW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW/action/storage_attestation","attest_author":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW/action/author_attestation","sign_citation":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW/action/citation_signature","submit_replication":"https://pith.science/pith/IBBAKF5YNLBNA7RB5VJS2TILJW/action/replication_record"}},"created_at":"2026-05-18T01:54:29.472471+00:00","updated_at":"2026-05-18T01:54:29.472471+00:00"}