{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:KN75T6CDDQ3JAK7YATB2SYNFUH","short_pith_number":"pith:KN75T6CD","schema_version":"1.0","canonical_sha256":"537fd9f8431c36902bf804c3a961a5a1cda4b21de9e2a982d6f1e8d8a0d8eb8a","source":{"kind":"arxiv","id":"2205.04815","version":1},"attestation_state":"computed","paper":{"title":"Polarimetric investigation of selected cloud compositions in exoplanetary atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Moritz Lietzow, Sebastian Wolf","submitted_at":"2022-05-10T11:32:16Z","abstract_excerpt":"We investigated the impact of selected cloud condensates in exoplanetary atmospheres on the polarization of scattered stellar radiation. We considered a selection of 25 cloud condensates that are expected to be present in extrasolar planetary atmospheres. Using the three-dimensional Monte Carlo radiative transfer code POLARIS and assuming Mie scattering theory, we calculated and studied the net polarization of scattered radiation as a function of planetary phase angle at optical to near-infrared wavelengths. In addition to the well-known characteristics in the state of polarization, such as th"},"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":"2205.04815","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2022-05-10T11:32:16Z","cross_cats_sorted":[],"title_canon_sha256":"6109ebb4fde67df60b9944d730c5fee7405c3428a07759a18cd0ca50c75261e0","abstract_canon_sha256":"e362754dc71f53467ded23808451de56a438669838d4d73435f60c4e62d31f05"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:39:36.998055Z","signature_b64":"uzuHRzzGfLhGki4+jySIb6aLslHeGCZjPQcLBKT7cuT/25/W/NnUAZeN2BxvxDUuqSnXBgFkU6fjSNiQcKszCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"537fd9f8431c36902bf804c3a961a5a1cda4b21de9e2a982d6f1e8d8a0d8eb8a","last_reissued_at":"2026-07-05T04:39:36.997688Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:39:36.997688Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Polarimetric investigation of selected cloud compositions in exoplanetary atmospheres","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Moritz Lietzow, Sebastian Wolf","submitted_at":"2022-05-10T11:32:16Z","abstract_excerpt":"We investigated the impact of selected cloud condensates in exoplanetary atmospheres on the polarization of scattered stellar radiation. We considered a selection of 25 cloud condensates that are expected to be present in extrasolar planetary atmospheres. Using the three-dimensional Monte Carlo radiative transfer code POLARIS and assuming Mie scattering theory, we calculated and studied the net polarization of scattered radiation as a function of planetary phase angle at optical to near-infrared wavelengths. In addition to the well-known characteristics in the state of polarization, such as th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.04815","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2205.04815/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2205.04815","created_at":"2026-07-05T04:39:36.997751+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.04815v1","created_at":"2026-07-05T04:39:36.997751+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.04815","created_at":"2026-07-05T04:39:36.997751+00:00"},{"alias_kind":"pith_short_12","alias_value":"KN75T6CDDQ3J","created_at":"2026-07-05T04:39:36.997751+00:00"},{"alias_kind":"pith_short_16","alias_value":"KN75T6CDDQ3JAK7Y","created_at":"2026-07-05T04:39:36.997751+00:00"},{"alias_kind":"pith_short_8","alias_value":"KN75T6CD","created_at":"2026-07-05T04:39:36.997751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.04837","citing_title":"Circular polarization as a probe of cloud properties and asymmetries in giant exoplanet atmospheres","ref_index":74,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH","json":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH.json","graph_json":"https://pith.science/api/pith-number/KN75T6CDDQ3JAK7YATB2SYNFUH/graph.json","events_json":"https://pith.science/api/pith-number/KN75T6CDDQ3JAK7YATB2SYNFUH/events.json","paper":"https://pith.science/paper/KN75T6CD"},"agent_actions":{"view_html":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH","download_json":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH.json","view_paper":"https://pith.science/paper/KN75T6CD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.04815&json=true","fetch_graph":"https://pith.science/api/pith-number/KN75T6CDDQ3JAK7YATB2SYNFUH/graph.json","fetch_events":"https://pith.science/api/pith-number/KN75T6CDDQ3JAK7YATB2SYNFUH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH/action/storage_attestation","attest_author":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH/action/author_attestation","sign_citation":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH/action/citation_signature","submit_replication":"https://pith.science/pith/KN75T6CDDQ3JAK7YATB2SYNFUH/action/replication_record"}},"created_at":"2026-07-05T04:39:36.997751+00:00","updated_at":"2026-07-05T04:39:36.997751+00:00"}