{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:6CWHADSBUNFC6CDNADIQM3P7AU","short_pith_number":"pith:6CWHADSB","schema_version":"1.0","canonical_sha256":"f0ac700e41a34a2f086d00d1066dff0524399bbdd8e70ba6d0b76c1ebd715116","source":{"kind":"arxiv","id":"1303.4950","version":1},"attestation_state":"computed","paper":{"title":"Optical Properties of Iron Silicates in the Infrared to Millimeter as a Function of Temperatures and Wavelength","license":"http://creativecommons.org/licenses/publicdomain/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"C. R. Richey, D. J. Benford, E. J. Wollack, G. Cataldo, J. A. Nuth, R. E. Kinzer, R. F. Silverberg, S. A. Rinehart","submitted_at":"2013-03-20T14:26:46Z","abstract_excerpt":"The Optical Properties of Astronomical Silicates with Infrared Techniques (OPASI-T) program utilizes multiple instruments to provide spectral data over a wide range of temperature and wavelengths. Experimental methods include Vector Network Analyzer (VNA) and Fourier Transform Spectroscopy (FTS) transmission, and reflection/scattering measurements. From this data, we can determine the optical parameters for the index of refraction, \\textit{n}, and the absorption coefficient, \\textit{k}. The analysis of the laboratory transmittance data for each sample type is based upon different mathematical "},"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":"1303.4950","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/publicdomain/","primary_cat":"astro-ph.GA","submitted_at":"2013-03-20T14:26:46Z","cross_cats_sorted":["astro-ph.CO","astro-ph.IM"],"title_canon_sha256":"49e4350f20c2a80002bee093d1329a3f8432cc6f0d2bfda86ac937b0be983ef4","abstract_canon_sha256":"3d17ab5628613b04b1d069036aafc2e70392a8cdd81a9a1ee378f5764652108b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:51:00.336377Z","signature_b64":"fKyoUvL+l020Ds6nM9eY65Sc8o97hwGeyVLsUkFdMkGZ2EX/QAIrEIptWRtlr9ANztxlmWkrje/DDDBhEgF0CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f0ac700e41a34a2f086d00d1066dff0524399bbdd8e70ba6d0b76c1ebd715116","last_reissued_at":"2026-05-18T01:51:00.335707Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:51:00.335707Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Optical Properties of Iron Silicates in the Infrared to Millimeter as a Function of Temperatures and Wavelength","license":"http://creativecommons.org/licenses/publicdomain/","headline":"","cross_cats":["astro-ph.CO","astro-ph.IM"],"primary_cat":"astro-ph.GA","authors_text":"C. R. Richey, D. J. Benford, E. J. Wollack, G. Cataldo, J. A. Nuth, R. E. Kinzer, R. F. Silverberg, S. A. Rinehart","submitted_at":"2013-03-20T14:26:46Z","abstract_excerpt":"The Optical Properties of Astronomical Silicates with Infrared Techniques (OPASI-T) program utilizes multiple instruments to provide spectral data over a wide range of temperature and wavelengths. Experimental methods include Vector Network Analyzer (VNA) and Fourier Transform Spectroscopy (FTS) transmission, and reflection/scattering measurements. From this data, we can determine the optical parameters for the index of refraction, \\textit{n}, and the absorption coefficient, \\textit{k}. The analysis of the laboratory transmittance data for each sample type is based upon different mathematical "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.4950","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":"1303.4950","created_at":"2026-05-18T01:51:00.335811+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.4950v1","created_at":"2026-05-18T01:51:00.335811+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.4950","created_at":"2026-05-18T01:51:00.335811+00:00"},{"alias_kind":"pith_short_12","alias_value":"6CWHADSBUNFC","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_16","alias_value":"6CWHADSBUNFC6CDN","created_at":"2026-05-18T12:27:36.564083+00:00"},{"alias_kind":"pith_short_8","alias_value":"6CWHADSB","created_at":"2026-05-18T12:27:36.564083+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/6CWHADSBUNFC6CDNADIQM3P7AU","json":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU.json","graph_json":"https://pith.science/api/pith-number/6CWHADSBUNFC6CDNADIQM3P7AU/graph.json","events_json":"https://pith.science/api/pith-number/6CWHADSBUNFC6CDNADIQM3P7AU/events.json","paper":"https://pith.science/paper/6CWHADSB"},"agent_actions":{"view_html":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU","download_json":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU.json","view_paper":"https://pith.science/paper/6CWHADSB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.4950&json=true","fetch_graph":"https://pith.science/api/pith-number/6CWHADSBUNFC6CDNADIQM3P7AU/graph.json","fetch_events":"https://pith.science/api/pith-number/6CWHADSBUNFC6CDNADIQM3P7AU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU/action/storage_attestation","attest_author":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU/action/author_attestation","sign_citation":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU/action/citation_signature","submit_replication":"https://pith.science/pith/6CWHADSBUNFC6CDNADIQM3P7AU/action/replication_record"}},"created_at":"2026-05-18T01:51:00.335811+00:00","updated_at":"2026-05-18T01:51:00.335811+00:00"}