{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1999:JQM2LXYW3UEWUMF2GGULK5C72B","short_pith_number":"pith:JQM2LXYW","schema_version":"1.0","canonical_sha256":"4c19a5df16dd096a30ba31a8b5745fd056e083d268217de2bc00db69b5aa0b6c","source":{"kind":"arxiv","id":"astro-ph/9909137","version":1},"attestation_state":"computed","paper":{"title":"Ultraviolet Imaging Polarimetry of the Large Magellanic Cloud. II. Models","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Andrew A. Cole, Kenneth H. Nordsieck, Kenneth Wood","submitted_at":"1999-09-08T01:05:04Z","abstract_excerpt":"Motivated by new sounding-rocket wide-field polarimetric images of the Large Magellanic Cloud, we have used a three-dimensional Monte Carlo radiation transfer code to investigate the escape of near-ultraviolet photons from young stellar associations embedded within a disk of dusty material (i.e. a galaxy). As photons propagate through the disk, they may be scattered or absorbed by dust. Scattered photons are polarized and tracked until they escape to be observed; absorbed photons heat the dust, which radiates isotropically in the far-infrared, where the galaxy is optically thin. The code produ"},"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":"astro-ph/9909137","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1999-09-08T01:05:04Z","cross_cats_sorted":[],"title_canon_sha256":"40d0e576ce409bf9aa5795132ca2d63f52ce51a282eef5dbb00f29b8ba60283c","abstract_canon_sha256":"111a913d77b32ab157a18e8b6b16c5f16d3587c3fd1e3743262347464cb8be6b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:07:36.081126Z","signature_b64":"n8YaYZ/nObJ096I1u5b+lVRjRbAX5boCBmBeoq1kCPnHivU9ue9ECCrjBUkOnDyis1r+n9W6t1C15cj3JAgDBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4c19a5df16dd096a30ba31a8b5745fd056e083d268217de2bc00db69b5aa0b6c","last_reissued_at":"2026-05-18T01:07:36.080537Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:07:36.080537Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ultraviolet Imaging Polarimetry of the Large Magellanic Cloud. II. Models","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Andrew A. Cole, Kenneth H. Nordsieck, Kenneth Wood","submitted_at":"1999-09-08T01:05:04Z","abstract_excerpt":"Motivated by new sounding-rocket wide-field polarimetric images of the Large Magellanic Cloud, we have used a three-dimensional Monte Carlo radiation transfer code to investigate the escape of near-ultraviolet photons from young stellar associations embedded within a disk of dusty material (i.e. a galaxy). As photons propagate through the disk, they may be scattered or absorbed by dust. Scattered photons are polarized and tracked until they escape to be observed; absorbed photons heat the dust, which radiates isotropically in the far-infrared, where the galaxy is optically thin. The code produ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9909137","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":"astro-ph/9909137","created_at":"2026-05-18T01:07:36.080634+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9909137v1","created_at":"2026-05-18T01:07:36.080634+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9909137","created_at":"2026-05-18T01:07:36.080634+00:00"},{"alias_kind":"pith_short_12","alias_value":"JQM2LXYW3UEW","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_16","alias_value":"JQM2LXYW3UEWUMF2","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_8","alias_value":"JQM2LXYW","created_at":"2026-05-18T12:25:49.631198+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/JQM2LXYW3UEWUMF2GGULK5C72B","json":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B.json","graph_json":"https://pith.science/api/pith-number/JQM2LXYW3UEWUMF2GGULK5C72B/graph.json","events_json":"https://pith.science/api/pith-number/JQM2LXYW3UEWUMF2GGULK5C72B/events.json","paper":"https://pith.science/paper/JQM2LXYW"},"agent_actions":{"view_html":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B","download_json":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B.json","view_paper":"https://pith.science/paper/JQM2LXYW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9909137&json=true","fetch_graph":"https://pith.science/api/pith-number/JQM2LXYW3UEWUMF2GGULK5C72B/graph.json","fetch_events":"https://pith.science/api/pith-number/JQM2LXYW3UEWUMF2GGULK5C72B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B/action/storage_attestation","attest_author":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B/action/author_attestation","sign_citation":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B/action/citation_signature","submit_replication":"https://pith.science/pith/JQM2LXYW3UEWUMF2GGULK5C72B/action/replication_record"}},"created_at":"2026-05-18T01:07:36.080634+00:00","updated_at":"2026-05-18T01:07:36.080634+00:00"}