{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:Y3HL4YU7NMOLNGTSWRSLQJEZPN","short_pith_number":"pith:Y3HL4YU7","schema_version":"1.0","canonical_sha256":"c6cebe629f6b1cb69a72b464b824997b5f3bfb18e11df814eaf7f594800bfd7a","source":{"kind":"arxiv","id":"1804.08357","version":1},"attestation_state":"computed","paper":{"title":"PyMieDAP: a Python--Fortran tool to compute fluxes and polarization signals of (exo)planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Daphne M. Stam, Javier Berzosa-Molina, Lo\\\"ic Rossi","submitted_at":"2018-04-23T12:00:49Z","abstract_excerpt":"PyMieDAP (the Python Mie Doubling-Adding Programme) is a Python--based tool for computing the total, linearly, and circularly polarized fluxes of incident unpolarized sun- or starlight that is reflected by, respectively, Solar System planets or moons, or exoplanets at a range of wavelengths. The radiative transfer computations are based on an adding--doubling Fortran algorithm and fully include polarization for all orders of scattering. The model (exo)planets are described by a model atmosphere composed of a stack of homogeneous layers containing gas and/or aerosol and/or cloud particles bound"},"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":"1804.08357","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-04-23T12:00:49Z","cross_cats_sorted":[],"title_canon_sha256":"ab08f49bb2a73efcf8298a6fc417adb3ae785a29f4ecd64923bed09b238ba491","abstract_canon_sha256":"ea8da1ea027c5a7424c04908a8379f541a36ec1ee4e4f5d893da66329b72f3f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:06:40.088782Z","signature_b64":"MHLpmdkFIOjHebtYE2W8QZ0z3KfUMlem73CwMTc77IBXIfJMAu0C++gf/fe98XU+JYus77Jh2qtPLxm2F15aBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c6cebe629f6b1cb69a72b464b824997b5f3bfb18e11df814eaf7f594800bfd7a","last_reissued_at":"2026-05-18T00:06:40.088408Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:06:40.088408Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"PyMieDAP: a Python--Fortran tool to compute fluxes and polarization signals of (exo)planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Daphne M. Stam, Javier Berzosa-Molina, Lo\\\"ic Rossi","submitted_at":"2018-04-23T12:00:49Z","abstract_excerpt":"PyMieDAP (the Python Mie Doubling-Adding Programme) is a Python--based tool for computing the total, linearly, and circularly polarized fluxes of incident unpolarized sun- or starlight that is reflected by, respectively, Solar System planets or moons, or exoplanets at a range of wavelengths. The radiative transfer computations are based on an adding--doubling Fortran algorithm and fully include polarization for all orders of scattering. The model (exo)planets are described by a model atmosphere composed of a stack of homogeneous layers containing gas and/or aerosol and/or cloud particles bound"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.08357","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":"1804.08357","created_at":"2026-05-18T00:06:40.088467+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.08357v1","created_at":"2026-05-18T00:06:40.088467+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.08357","created_at":"2026-05-18T00:06:40.088467+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y3HL4YU7NMOL","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y3HL4YU7NMOLNGTS","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y3HL4YU7","created_at":"2026-05-18T12:33:04.347982+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/Y3HL4YU7NMOLNGTSWRSLQJEZPN","json":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN.json","graph_json":"https://pith.science/api/pith-number/Y3HL4YU7NMOLNGTSWRSLQJEZPN/graph.json","events_json":"https://pith.science/api/pith-number/Y3HL4YU7NMOLNGTSWRSLQJEZPN/events.json","paper":"https://pith.science/paper/Y3HL4YU7"},"agent_actions":{"view_html":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN","download_json":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN.json","view_paper":"https://pith.science/paper/Y3HL4YU7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.08357&json=true","fetch_graph":"https://pith.science/api/pith-number/Y3HL4YU7NMOLNGTSWRSLQJEZPN/graph.json","fetch_events":"https://pith.science/api/pith-number/Y3HL4YU7NMOLNGTSWRSLQJEZPN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN/action/storage_attestation","attest_author":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN/action/author_attestation","sign_citation":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN/action/citation_signature","submit_replication":"https://pith.science/pith/Y3HL4YU7NMOLNGTSWRSLQJEZPN/action/replication_record"}},"created_at":"2026-05-18T00:06:40.088467+00:00","updated_at":"2026-05-18T00:06:40.088467+00:00"}