{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:26IZCAH47JZT2PQESNY77DII7I","short_pith_number":"pith:26IZCAH4","schema_version":"1.0","canonical_sha256":"d7919100fcfa733d3e049371ff8d08fa24ba0ededa6ad1ff16a53e380337bd18","source":{"kind":"arxiv","id":"1810.02172","version":2},"attestation_state":"computed","paper":{"title":"Deciphering the atmosphere of HAT-P-12b: solving discrepant results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"C. Denker, C. von Essen, E. Dineva, E. Keles, J. D. Turner, J. Southworth, K. G. Strassmeier, L. Mancini, M. Mallonn, S. Ciceri, T. Granzer, X. Alexoudi","submitted_at":"2018-10-04T12:32:26Z","abstract_excerpt":"Two independent investigations of the atmosphere of the hot Jupiter HAT-P-12b by two different groups resulted in discrepant solutions. Using broad-band photometry from the ground, one study found a flat and featureless transmission spectrum which was interpreted as a gray absorption by dense cloud coverage. The second study made use of the Hubble Space Telescope (HST) observations and found Rayleigh scattering at optical wavelengths caused by haze. The main purpose of this work is to find the source of this inconsistency and provide feedback to prevent similar discrepancies in future analyses"},"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":"1810.02172","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-10-04T12:32:26Z","cross_cats_sorted":[],"title_canon_sha256":"1f9061d0554fec3288dfcd4581896bbf976a46bc61ca054d3211f098171b19a4","abstract_canon_sha256":"4c407e7547d5b157b4f7db28cabccaf79f5b084afb0aa541e1aed320f4fb007f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:49:57.444379Z","signature_b64":"sHe3ow9FuZzhL8zXME35xlGlhbZ+2gKed0qzrTkoI1BxIBjZNw/JGooXjKz25x9iUBkgFS4g5w8WeigNh8E2AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d7919100fcfa733d3e049371ff8d08fa24ba0ededa6ad1ff16a53e380337bd18","last_reissued_at":"2026-07-05T03:49:57.444014Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:49:57.444014Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Deciphering the atmosphere of HAT-P-12b: solving discrepant results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"C. Denker, C. von Essen, E. Dineva, E. Keles, J. D. Turner, J. Southworth, K. G. Strassmeier, L. Mancini, M. Mallonn, S. Ciceri, T. Granzer, X. Alexoudi","submitted_at":"2018-10-04T12:32:26Z","abstract_excerpt":"Two independent investigations of the atmosphere of the hot Jupiter HAT-P-12b by two different groups resulted in discrepant solutions. Using broad-band photometry from the ground, one study found a flat and featureless transmission spectrum which was interpreted as a gray absorption by dense cloud coverage. The second study made use of the Hubble Space Telescope (HST) observations and found Rayleigh scattering at optical wavelengths caused by haze. The main purpose of this work is to find the source of this inconsistency and provide feedback to prevent similar discrepancies in future analyses"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.02172","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1810.02172/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":"1810.02172","created_at":"2026-07-05T03:49:57.444069+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.02172v2","created_at":"2026-07-05T03:49:57.444069+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.02172","created_at":"2026-07-05T03:49:57.444069+00:00"},{"alias_kind":"pith_short_12","alias_value":"26IZCAH47JZT","created_at":"2026-07-05T03:49:57.444069+00:00"},{"alias_kind":"pith_short_16","alias_value":"26IZCAH47JZT2PQE","created_at":"2026-07-05T03:49:57.444069+00:00"},{"alias_kind":"pith_short_8","alias_value":"26IZCAH4","created_at":"2026-07-05T03:49:57.444069+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/26IZCAH47JZT2PQESNY77DII7I","json":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I.json","graph_json":"https://pith.science/api/pith-number/26IZCAH47JZT2PQESNY77DII7I/graph.json","events_json":"https://pith.science/api/pith-number/26IZCAH47JZT2PQESNY77DII7I/events.json","paper":"https://pith.science/paper/26IZCAH4"},"agent_actions":{"view_html":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I","download_json":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I.json","view_paper":"https://pith.science/paper/26IZCAH4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.02172&json=true","fetch_graph":"https://pith.science/api/pith-number/26IZCAH47JZT2PQESNY77DII7I/graph.json","fetch_events":"https://pith.science/api/pith-number/26IZCAH47JZT2PQESNY77DII7I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I/action/storage_attestation","attest_author":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I/action/author_attestation","sign_citation":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I/action/citation_signature","submit_replication":"https://pith.science/pith/26IZCAH47JZT2PQESNY77DII7I/action/replication_record"}},"created_at":"2026-07-05T03:49:57.444069+00:00","updated_at":"2026-07-05T03:49:57.444069+00:00"}