{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:QMTUFJEP5EZBOYZGOFUYDFIRTD","short_pith_number":"pith:QMTUFJEP","schema_version":"1.0","canonical_sha256":"832742a48fe932176326716981951198c9a3f1a3ec5fd6a28f048f153d7e3165","source":{"kind":"arxiv","id":"2105.11034","version":2},"attestation_state":"computed","paper":{"title":"Decomposing the Iron Cross-Correlation Signal of the Ultra-Hot Jupiter WASP-76b in Transmission using 3D Monte-Carlo Radiative Transfer","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Ehsan Gharib-Nezhad, Elspeth K.H. Lee, Joost P. Wardenier, Michael R. Line, Vivien Parmentier","submitted_at":"2021-05-23T22:42:30Z","abstract_excerpt":"Ultra-hot Jupiters are tidally locked gas giants with dayside temperatures high enough to dissociate hydrogen and other molecules. Their atmospheres are vastly non-uniform in terms of chemistry, temperature and dynamics, and this makes their high-resolution transmission spectra and cross-correlation signal difficult to interpret. In this work, we use the SPARC/MITgcm global circulation model to simulate the atmosphere of the ultra-hot Jupiter WASP-76b under different conditions, such as atmospheric drag and the absence of TiO and VO. We then employ a 3D Monte-Carlo radiative transfer code, HIR"},"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":"2105.11034","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2021-05-23T22:42:30Z","cross_cats_sorted":[],"title_canon_sha256":"097fe588ded44b22a00a4d61739466ff678a14e0d7801c8cf7bd7a6193d0b64e","abstract_canon_sha256":"9e0b9e2db4cd785d5c51473042724287e04a8eb8d58e265f7ae0d8e01efc3539"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:55:15.189495Z","signature_b64":"6Biz/rli1ZEIfG7XlDlW1oI7NbETvXcHG9zegyTPQ505eY9a2H5pobEMfGxoLldjwJJJ/YbYWCBo1bScLSAWCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"832742a48fe932176326716981951198c9a3f1a3ec5fd6a28f048f153d7e3165","last_reissued_at":"2026-07-05T02:55:15.189092Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:55:15.189092Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Decomposing the Iron Cross-Correlation Signal of the Ultra-Hot Jupiter WASP-76b in Transmission using 3D Monte-Carlo Radiative Transfer","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Ehsan Gharib-Nezhad, Elspeth K.H. Lee, Joost P. Wardenier, Michael R. Line, Vivien Parmentier","submitted_at":"2021-05-23T22:42:30Z","abstract_excerpt":"Ultra-hot Jupiters are tidally locked gas giants with dayside temperatures high enough to dissociate hydrogen and other molecules. Their atmospheres are vastly non-uniform in terms of chemistry, temperature and dynamics, and this makes their high-resolution transmission spectra and cross-correlation signal difficult to interpret. In this work, we use the SPARC/MITgcm global circulation model to simulate the atmosphere of the ultra-hot Jupiter WASP-76b under different conditions, such as atmospheric drag and the absence of TiO and VO. We then employ a 3D Monte-Carlo radiative transfer code, HIR"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2105.11034","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/2105.11034/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":"2105.11034","created_at":"2026-07-05T02:55:15.189149+00:00"},{"alias_kind":"arxiv_version","alias_value":"2105.11034v2","created_at":"2026-07-05T02:55:15.189149+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2105.11034","created_at":"2026-07-05T02:55:15.189149+00:00"},{"alias_kind":"pith_short_12","alias_value":"QMTUFJEP5EZB","created_at":"2026-07-05T02:55:15.189149+00:00"},{"alias_kind":"pith_short_16","alias_value":"QMTUFJEP5EZBOYZG","created_at":"2026-07-05T02:55:15.189149+00:00"},{"alias_kind":"pith_short_8","alias_value":"QMTUFJEP","created_at":"2026-07-05T02:55:15.189149+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/QMTUFJEP5EZBOYZGOFUYDFIRTD","json":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD.json","graph_json":"https://pith.science/api/pith-number/QMTUFJEP5EZBOYZGOFUYDFIRTD/graph.json","events_json":"https://pith.science/api/pith-number/QMTUFJEP5EZBOYZGOFUYDFIRTD/events.json","paper":"https://pith.science/paper/QMTUFJEP"},"agent_actions":{"view_html":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD","download_json":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD.json","view_paper":"https://pith.science/paper/QMTUFJEP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2105.11034&json=true","fetch_graph":"https://pith.science/api/pith-number/QMTUFJEP5EZBOYZGOFUYDFIRTD/graph.json","fetch_events":"https://pith.science/api/pith-number/QMTUFJEP5EZBOYZGOFUYDFIRTD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD/action/storage_attestation","attest_author":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD/action/author_attestation","sign_citation":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD/action/citation_signature","submit_replication":"https://pith.science/pith/QMTUFJEP5EZBOYZGOFUYDFIRTD/action/replication_record"}},"created_at":"2026-07-05T02:55:15.189149+00:00","updated_at":"2026-07-05T02:55:15.189149+00:00"}