{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1995:SMGH3KAWB4GF4QNOLP37AM4CS6","short_pith_number":"pith:SMGH3KAW","schema_version":"1.0","canonical_sha256":"930c7da8160f0c5e41ae5bf7f03382978becd9d8f196e60b41c111cf78aeda9e","source":{"kind":"arxiv","id":"astro-ph/9512154","version":2},"attestation_state":"computed","paper":{"title":"Infrared Imaging of Late-Type Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Moshe Elitzur (University of Kentucky), Zeljko Ivezic","submitted_at":"1995-12-22T20:46:08Z","abstract_excerpt":"Infrared imaging properties of dusty winds around late-type stars are investigated in detail, employing a self-consistent model that couples the equations of motion and radiative transfer. Because of general scaling properties, the angular profiles of surface brightness are self-similar. In any given star, the profile shape is determined essentially by overall optical depth at each wavelength and it is self-similarly scaled by the size of the dust condensation zone. We find that the mid-IR is the best wavelength range to measure directly the angular size of this zone, and from {\\it IRAS} data "},"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/9512154","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1995-12-22T20:46:08Z","cross_cats_sorted":[],"title_canon_sha256":"b6ccc3e76a6dd5ff4c8e8ce9b3f5c975be5cc519ef0a15b1ff8683a6fb2a5968","abstract_canon_sha256":"0fc4cb55cc7ebbc404cf1afd198f7266a834873ca3fdaf55044ef4267247aed1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:22.045538Z","signature_b64":"ACHLqf7IT+9Vwd9WQnxYYMDumwn7vVmIoq7Rc98FxI7O9ZpX53pUS7+xOz3KzrcKFJrWlR9mgeXiyIWy8ALaAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"930c7da8160f0c5e41ae5bf7f03382978becd9d8f196e60b41c111cf78aeda9e","last_reissued_at":"2026-05-18T01:40:22.044880Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:22.044880Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Infrared Imaging of Late-Type Stars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Moshe Elitzur (University of Kentucky), Zeljko Ivezic","submitted_at":"1995-12-22T20:46:08Z","abstract_excerpt":"Infrared imaging properties of dusty winds around late-type stars are investigated in detail, employing a self-consistent model that couples the equations of motion and radiative transfer. Because of general scaling properties, the angular profiles of surface brightness are self-similar. In any given star, the profile shape is determined essentially by overall optical depth at each wavelength and it is self-similarly scaled by the size of the dust condensation zone. We find that the mid-IR is the best wavelength range to measure directly the angular size of this zone, and from {\\it IRAS} data "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9512154","kind":"arxiv","version":2},"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/9512154","created_at":"2026-05-18T01:40:22.044970+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9512154v2","created_at":"2026-05-18T01:40:22.044970+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9512154","created_at":"2026-05-18T01:40:22.044970+00:00"},{"alias_kind":"pith_short_12","alias_value":"SMGH3KAWB4GF","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_16","alias_value":"SMGH3KAWB4GF4QNO","created_at":"2026-05-18T12:25:47.700082+00:00"},{"alias_kind":"pith_short_8","alias_value":"SMGH3KAW","created_at":"2026-05-18T12:25:47.700082+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/SMGH3KAWB4GF4QNOLP37AM4CS6","json":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6.json","graph_json":"https://pith.science/api/pith-number/SMGH3KAWB4GF4QNOLP37AM4CS6/graph.json","events_json":"https://pith.science/api/pith-number/SMGH3KAWB4GF4QNOLP37AM4CS6/events.json","paper":"https://pith.science/paper/SMGH3KAW"},"agent_actions":{"view_html":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6","download_json":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6.json","view_paper":"https://pith.science/paper/SMGH3KAW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9512154&json=true","fetch_graph":"https://pith.science/api/pith-number/SMGH3KAWB4GF4QNOLP37AM4CS6/graph.json","fetch_events":"https://pith.science/api/pith-number/SMGH3KAWB4GF4QNOLP37AM4CS6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6/action/storage_attestation","attest_author":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6/action/author_attestation","sign_citation":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6/action/citation_signature","submit_replication":"https://pith.science/pith/SMGH3KAWB4GF4QNOLP37AM4CS6/action/replication_record"}},"created_at":"2026-05-18T01:40:22.044970+00:00","updated_at":"2026-05-18T01:40:22.044970+00:00"}