{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:CXZPMZX2H3HSETVGFSPI4SBFSR","short_pith_number":"pith:CXZPMZX2","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"},"canonical_sha256":"15f2f666fa3ecf224ea62c9e8e4825947f74549c8712c860765df826ba81beab","source":{"kind":"arxiv","id":"1505.08013","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1505.08013","created_at":"2026-05-18T01:26:57Z"},{"alias_kind":"arxiv_version","alias_value":"1505.08013v2","created_at":"2026-05-18T01:26:57Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.08013","created_at":"2026-05-18T01:26:57Z"},{"alias_kind":"pith_short_12","alias_value":"CXZPMZX2H3HS","created_at":"2026-05-18T12:29:17Z"},{"alias_kind":"pith_short_16","alias_value":"CXZPMZX2H3HSETVG","created_at":"2026-05-18T12:29:17Z"},{"alias_kind":"pith_short_8","alias_value":"CXZPMZX2","created_at":"2026-05-18T12:29:17Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:CXZPMZX2H3HSETVGFSPI4SBFSR","target":"record","payload":{"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"},"canonical_sha256":"15f2f666fa3ecf224ea62c9e8e4825947f74549c8712c860765df826ba81beab","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"},"source_kind":"arxiv","source_id":"1505.08013","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:26:57Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1mUd49OM2JC2iU/0E0sopBbQGQsB2LNEnstF/euPwF6OUBdAffmjOE0ckfwtQIL7NvbwTOL7HBUhnT7fX69/DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T05:32:58.179829Z"},"content_sha256":"5c49a08e5d97cb31816f3be468bd64e52fe5b3ee8e3c4507a13a4afeb0a9f0bb","schema_version":"1.0","event_id":"sha256:5c49a08e5d97cb31816f3be468bd64e52fe5b3ee8e3c4507a13a4afeb0a9f0bb"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:CXZPMZX2H3HSETVGFSPI4SBFSR","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:26:57Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"FIZ+Hw2uBiMkqCkkLGhLflcXbJ/52Pb1mRFHYbwCF/HFiAVlplOF15UwiuhArhzEoUgHGPNJLO0fXT56PH2BBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T05:32:58.180178Z"},"content_sha256":"9f35e54e9f0abf84b10c32cc6a96f461a57359d177afba9c1a3ceebff452a7d6","schema_version":"1.0","event_id":"sha256:9f35e54e9f0abf84b10c32cc6a96f461a57359d177afba9c1a3ceebff452a7d6"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/bundle.json","state_url":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-03T05:32:58Z","links":{"resolver":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR","bundle":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/bundle.json","state":"https://pith.science/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CXZPMZX2H3HSETVGFSPI4SBFSR/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:CXZPMZX2H3HSETVGFSPI4SBFSR","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"fa6da1435208969b361d8025cf371d8347f9b39530e66b07d527b06eb9875c0f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-05-29T12:27:05Z","title_canon_sha256":"5b7b4134947ade3d5bca479f9dc7ffabddfa08664f4677476645f8eb8f94c9ec"},"schema_version":"1.0","source":{"id":"1505.08013","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1505.08013","created_at":"2026-05-18T01:26:57Z"},{"alias_kind":"arxiv_version","alias_value":"1505.08013v2","created_at":"2026-05-18T01:26:57Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.08013","created_at":"2026-05-18T01:26:57Z"},{"alias_kind":"pith_short_12","alias_value":"CXZPMZX2H3HS","created_at":"2026-05-18T12:29:17Z"},{"alias_kind":"pith_short_16","alias_value":"CXZPMZX2H3HSETVG","created_at":"2026-05-18T12:29:17Z"},{"alias_kind":"pith_short_8","alias_value":"CXZPMZX2","created_at":"2026-05-18T12:29:17Z"}],"graph_snapshots":[{"event_id":"sha256:9f35e54e9f0abf84b10c32cc6a96f461a57359d177afba9c1a3ceebff452a7d6","target":"graph","created_at":"2026-05-18T01:26:57Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"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.","authors_text":"Ivan Hubeny, Jan Budaj, Miroslav Kocifaj, Raquel Salmeron","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-05-29T12:27:05Z","title":"Tables of phase functions, opacities, albedos, equilibrium temperatures, and radiative accelerations of dust grains in exoplanets"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.08013","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:5c49a08e5d97cb31816f3be468bd64e52fe5b3ee8e3c4507a13a4afeb0a9f0bb","target":"record","created_at":"2026-05-18T01:26:57Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"fa6da1435208969b361d8025cf371d8347f9b39530e66b07d527b06eb9875c0f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-05-29T12:27:05Z","title_canon_sha256":"5b7b4134947ade3d5bca479f9dc7ffabddfa08664f4677476645f8eb8f94c9ec"},"schema_version":"1.0","source":{"id":"1505.08013","kind":"arxiv","version":2}},"canonical_sha256":"15f2f666fa3ecf224ea62c9e8e4825947f74549c8712c860765df826ba81beab","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"15f2f666fa3ecf224ea62c9e8e4825947f74549c8712c860765df826ba81beab","first_computed_at":"2026-05-18T01:26:57.614209Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:26:57.614209Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Td3VwHpzgLonW37gDTX0qq7QQsybMEUeqcd7AqF9Nrx+6OsEi7nhpB2MhiTUMIyPvWYtAo+ClyFMwNwjZxN8DA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:26:57.614877Z","signed_message":"canonical_sha256_bytes"},"source_id":"1505.08013","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:5c49a08e5d97cb31816f3be468bd64e52fe5b3ee8e3c4507a13a4afeb0a9f0bb","sha256:9f35e54e9f0abf84b10c32cc6a96f461a57359d177afba9c1a3ceebff452a7d6"],"state_sha256":"e574147effecfaa1868e5c0ce1f57a3eb07c9f3be21dd9605d41bd5152aefaf1"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KM7IqDW6okyE3VnaU4TINDi8Iz7YM5vffSusjO7EKba/AxlOrzqx0t4OxTQ++HEgqNClOBCtpmOxPbZoOFX2DA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-03T05:32:58.182145Z","bundle_sha256":"42c1a5df2fcc98d0301f9d7d7daa7c240ca13052f588d4e8a759610ac9e50599"}}