{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2005:NTAYXGEVMSMVY3HI3JG7WJD7AR","short_pith_number":"pith:NTAYXGEV","canonical_record":{"source":{"id":"astro-ph/0503554","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-03-24T21:05:04Z","cross_cats_sorted":[],"title_canon_sha256":"3b25aa5080e9692a42d5121f620f90703e6c6d2813ad39bf184151ec2a934fc1","abstract_canon_sha256":"3bbb2ab24ff7acef05470459b0fa0797b0398d180d6a2c30178d5177125d87f7"},"schema_version":"1.0"},"canonical_sha256":"6cc18b989564995c6ce8da4dfb247f045b8b772e33a620a7d39c6feda53395bd","source":{"kind":"arxiv","id":"astro-ph/0503554","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0503554","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0503554v1","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0503554","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"pith_short_12","alias_value":"NTAYXGEVMSMV","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"pith_short_16","alias_value":"NTAYXGEVMSMVY3HI","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"pith_short_8","alias_value":"NTAYXGEV","created_at":"2026-07-04T16:51:04Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2005:NTAYXGEVMSMVY3HI3JG7WJD7AR","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/0503554","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-03-24T21:05:04Z","cross_cats_sorted":[],"title_canon_sha256":"3b25aa5080e9692a42d5121f620f90703e6c6d2813ad39bf184151ec2a934fc1","abstract_canon_sha256":"3bbb2ab24ff7acef05470459b0fa0797b0398d180d6a2c30178d5177125d87f7"},"schema_version":"1.0"},"canonical_sha256":"6cc18b989564995c6ce8da4dfb247f045b8b772e33a620a7d39c6feda53395bd","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:51:04.534339Z","signature_b64":"nmOp4AL4A3gM78hnfNPx/ZILaw/d3I34mArCZ0BIdmCnwwlGoRcSCwV7C1BP8iOkeBjERfktoyK4bCwXyrCUDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6cc18b989564995c6ce8da4dfb247f045b8b772e33a620a7d39c6feda53395bd","last_reissued_at":"2026-07-04T16:51:04.533895Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:51:04.533895Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/0503554","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:51:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"PRx5cOZGwwbYmkV1/HHFZ+jSf4nycWvpIazl0gPOgbcV/I4eNnhEg2bMzemrWmEqVsbPkXtBxmcE+z5ZgKodAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T12:24:56.510508Z"},"content_sha256":"db2e4fc428f5330651c92c8366b31eaeefcee872adf1f8b807152128fd339740","schema_version":"1.0","event_id":"sha256:db2e4fc428f5330651c92c8366b31eaeefcee872adf1f8b807152128fd339740"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2005:NTAYXGEVMSMVY3HI3JG7WJD7AR","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Infrared radiation from an extrasolar planet","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Drake Deming, Joseph Harrington, L. Jeremy Richardson, Sara Seager","submitted_at":"2005-03-24T21:05:04Z","abstract_excerpt":"A class of extrasolar giant planets - the so-called `hot Jupiters' - orbit within 0.05 AU of their primary stars. These planets should be hot and so emit detectable infrared radiation. The planet HD 209458b is an ideal candidate for the detection and characterization of this infrared light because it is eclipsed by the star. This planet has an anomalously large radius (1.35 times that of Jupiter), which may be the result of ongoing tidal dissipation, but this explanation requires a non-zero orbital eccentricity (~0.03), maintained by interaction with a hypothetical second planet. Here we repor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0503554","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/astro-ph/0503554/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:51:04Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"r5uoW/BDqla4h5mgvYClqB2zk6RYwqfOvNLfDboYCbB0e/SfZemBEw51pClTgiKQWffNmgGPvdZ/AXm+wYe/CA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T12:24:56.510987Z"},"content_sha256":"2b89ae3e817252525618c21e65eb6cd044519a0757f1ac2f6ba8aacd41a6a06e","schema_version":"1.0","event_id":"sha256:2b89ae3e817252525618c21e65eb6cd044519a0757f1ac2f6ba8aacd41a6a06e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR/bundle.json","state_url":"https://pith.science/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR/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":"2026-08-04T12:24:56Z","links":{"resolver":"https://pith.science/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR","bundle":"https://pith.science/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR/bundle.json","state":"https://pith.science/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR/state.json","well_known_bundle":"https://pith.science/.well-known/pith/NTAYXGEVMSMVY3HI3JG7WJD7AR/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2005:NTAYXGEVMSMVY3HI3JG7WJD7AR","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":"3bbb2ab24ff7acef05470459b0fa0797b0398d180d6a2c30178d5177125d87f7","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2005-03-24T21:05:04Z","title_canon_sha256":"3b25aa5080e9692a42d5121f620f90703e6c6d2813ad39bf184151ec2a934fc1"},"schema_version":"1.0","source":{"id":"astro-ph/0503554","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0503554","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0503554v1","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0503554","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"pith_short_12","alias_value":"NTAYXGEVMSMV","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"pith_short_16","alias_value":"NTAYXGEVMSMVY3HI","created_at":"2026-07-04T16:51:04Z"},{"alias_kind":"pith_short_8","alias_value":"NTAYXGEV","created_at":"2026-07-04T16:51:04Z"}],"graph_snapshots":[{"event_id":"sha256:2b89ae3e817252525618c21e65eb6cd044519a0757f1ac2f6ba8aacd41a6a06e","target":"graph","created_at":"2026-07-04T16:51:04Z","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"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/astro-ph/0503554/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"A class of extrasolar giant planets - the so-called `hot Jupiters' - orbit within 0.05 AU of their primary stars. These planets should be hot and so emit detectable infrared radiation. The planet HD 209458b is an ideal candidate for the detection and characterization of this infrared light because it is eclipsed by the star. This planet has an anomalously large radius (1.35 times that of Jupiter), which may be the result of ongoing tidal dissipation, but this explanation requires a non-zero orbital eccentricity (~0.03), maintained by interaction with a hypothetical second planet. Here we repor","authors_text":"Drake Deming, Joseph Harrington, L. Jeremy Richardson, Sara Seager","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"2005-03-24T21:05:04Z","title":"Infrared radiation from an extrasolar planet"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0503554","kind":"arxiv","version":1},"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:db2e4fc428f5330651c92c8366b31eaeefcee872adf1f8b807152128fd339740","target":"record","created_at":"2026-07-04T16:51:04Z","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":"3bbb2ab24ff7acef05470459b0fa0797b0398d180d6a2c30178d5177125d87f7","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"2005-03-24T21:05:04Z","title_canon_sha256":"3b25aa5080e9692a42d5121f620f90703e6c6d2813ad39bf184151ec2a934fc1"},"schema_version":"1.0","source":{"id":"astro-ph/0503554","kind":"arxiv","version":1}},"canonical_sha256":"6cc18b989564995c6ce8da4dfb247f045b8b772e33a620a7d39c6feda53395bd","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6cc18b989564995c6ce8da4dfb247f045b8b772e33a620a7d39c6feda53395bd","first_computed_at":"2026-07-04T16:51:04.533895Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T16:51:04.533895Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"nmOp4AL4A3gM78hnfNPx/ZILaw/d3I34mArCZ0BIdmCnwwlGoRcSCwV7C1BP8iOkeBjERfktoyK4bCwXyrCUDQ==","signature_status":"signed_v1","signed_at":"2026-07-04T16:51:04.534339Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/0503554","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:db2e4fc428f5330651c92c8366b31eaeefcee872adf1f8b807152128fd339740","sha256:2b89ae3e817252525618c21e65eb6cd044519a0757f1ac2f6ba8aacd41a6a06e"],"state_sha256":"3e907b43aba75fa0f7e86c805937f3c7741f09fcbc64b2f050ec96d4a3422a55"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iJNriG2DySLW1a1yNNOpfyX1nrjajgGmF7UZbCWJ6x7BN+wyk/GStC6CjGJgTuPW7I0xgmYM9leVfwg0EjIDCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-04T12:24:56.515097Z","bundle_sha256":"ecc09572c149c148e552e9e977caf14054b552426cfce9eb082abba340e487af"}}