{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:CXZPMZX2H3HSETVGFSPI4SBFSR","short_pith_number":"pith:CXZPMZX2","schema_version":"1.0","canonical_sha256":"15f2f666fa3ecf224ea62c9e8e4825947f74549c8712c860765df826ba81beab","source":{"kind":"arxiv","id":"1505.08013","version":2},"attestation_state":"computed","paper":{"title":"Tables of phase functions, opacities, albedos, equilibrium temperatures, and radiative accelerations of dust grains in exoplanets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Ivan Hubeny, Jan Budaj, Miroslav Kocifaj, Raquel Salmeron","submitted_at":"2015-05-29T12:27:05Z","abstract_excerpt":"There has been growing observational evidence for the presence of condensates in the atmospheres and/or comet-like tails of extrasolar planets. As a result, systematic and homogeneous tables of dust properties are useful in order to facilitate further observational and theoretical studies. In this paper we present calculations and analysis of non-isotropic phase functions, asymmetry parameter (mean cosine of the scattering angle), absorption and scattering opacities, single scattering albedos, equilibrium temperatures, and radiative accelerations of dust grains relevant for extrasolar planets."},"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":"1505.08013","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-05-29T12:27:05Z","cross_cats_sorted":[],"title_canon_sha256":"5b7b4134947ade3d5bca479f9dc7ffabddfa08664f4677476645f8eb8f94c9ec","abstract_canon_sha256":"fa6da1435208969b361d8025cf371d8347f9b39530e66b07d527b06eb9875c0f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:26:57.614877Z","signature_b64":"Td3VwHpzgLonW37gDTX0qq7QQsybMEUeqcd7AqF9Nrx+6OsEi7nhpB2MhiTUMIyPvWYtAo+ClyFMwNwjZxN8DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"15f2f666fa3ecf224ea62c9e8e4825947f74549c8712c860765df826ba81beab","last_reissued_at":"2026-05-18T01:26:57.614209Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:26:57.614209Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tables of phase functions, opacities, albedos, equilibrium temperatures, and radiative accelerations of dust grains in exoplanets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Ivan Hubeny, Jan Budaj, Miroslav Kocifaj, Raquel Salmeron","submitted_at":"2015-05-29T12:27:05Z","abstract_excerpt":"There has been growing observational evidence for the presence of condensates in the atmospheres and/or comet-like tails of extrasolar planets. As a result, systematic and homogeneous tables of dust properties are useful in order to facilitate further observational and theoretical studies. In this paper we present calculations and analysis of non-isotropic phase functions, asymmetry parameter (mean cosine of the scattering angle), absorption and scattering opacities, single scattering albedos, equilibrium temperatures, and radiative accelerations of dust grains relevant for extrasolar planets."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.08013","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":"1505.08013","created_at":"2026-05-18T01:26:57.614326+00:00"},{"alias_kind":"arxiv_version","alias_value":"1505.08013v2","created_at":"2026-05-18T01:26:57.614326+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.08013","created_at":"2026-05-18T01:26:57.614326+00:00"},{"alias_kind":"pith_short_12","alias_value":"CXZPMZX2H3HS","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_16","alias_value":"CXZPMZX2H3HSETVG","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_8","alias_value":"CXZPMZX2","created_at":"2026-05-18T12:29:17.054201+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/CXZPMZX2H3HSETVGFSPI4SBFSR","json":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR.json","graph_json":"https://pith.science/api/pith-number/CXZPMZX2H3HSETVGFSPI4SBFSR/graph.json","events_json":"https://pith.science/api/pith-number/CXZPMZX2H3HSETVGFSPI4SBFSR/events.json","paper":"https://pith.science/paper/CXZPMZX2"},"agent_actions":{"view_html":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR","download_json":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR.json","view_paper":"https://pith.science/paper/CXZPMZX2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1505.08013&json=true","fetch_graph":"https://pith.science/api/pith-number/CXZPMZX2H3HSETVGFSPI4SBFSR/graph.json","fetch_events":"https://pith.science/api/pith-number/CXZPMZX2H3HSETVGFSPI4SBFSR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/action/storage_attestation","attest_author":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/action/author_attestation","sign_citation":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/action/citation_signature","submit_replication":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/action/replication_record"}},"created_at":"2026-05-18T01:26:57.614326+00:00","updated_at":"2026-05-18T01:26:57.614326+00:00"}