{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:UOPC2RAR5JV3UIDL33OYFKZ6NH","short_pith_number":"pith:UOPC2RAR","schema_version":"1.0","canonical_sha256":"a39e2d4411ea6bba206bdedd82ab3e69cf27444969b4b32f2a63e196c4e85aea","source":{"kind":"arxiv","id":"2309.04042","version":1},"attestation_state":"computed","paper":{"title":"Methane Throughout the Atmosphere of the Warm Exoplanet WASP-80b","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Emily Rauscher, Everett Schlawin, John A. Stansberry, Jonathan J. Fortney, Kazumasa Ohno, Lindsey S. Wiser, Luis Welbanks, Marcia J. Rieke, Martha L. Boyer, Michael R. Line, Sagnick Mukherjee, Taylor J. Bell, Thomas G. Beatty, Thomas P. Greene, Vivien Parmentier","submitted_at":"2023-09-07T23:13:09Z","abstract_excerpt":"The abundances of major carbon and oxygen bearing gases in the atmospheres of giant exoplanets provide insights into atmospheric chemistry and planet formation processes. Thermochemistry suggests that methane should be the dominant carbon-bearing species below $\\sim$1000 K over a range of plausible atmospheric compositions; this is the case for the Solar System planets and has been confirmed in the atmospheres of brown dwarfs and self-luminous directly imaged exoplanets. However, methane has not yet been definitively detected with space-based spectroscopy in the atmosphere of a transiting exop"},"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":"2309.04042","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-09-07T23:13:09Z","cross_cats_sorted":[],"title_canon_sha256":"d9a8e7eb44bd3b60041305a5cfd51386e09b2e310a9574e15d75a43cbc549bbe","abstract_canon_sha256":"90fd87c3a760bfe845e98519f6bfdb258aa89e72a444635824cf7ab99baf80e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:48:54.062426Z","signature_b64":"9jSD8JeZcG1twNIZUDp+1sAKaqWwuEWCAvhvQ71k3acImBcYLMqBsKB9pJJ+Bgjhl0Y5EN1/3JNypgvQI36ADw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a39e2d4411ea6bba206bdedd82ab3e69cf27444969b4b32f2a63e196c4e85aea","last_reissued_at":"2026-07-05T06:48:54.062010Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:48:54.062010Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Methane Throughout the Atmosphere of the Warm Exoplanet WASP-80b","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Emily Rauscher, Everett Schlawin, John A. Stansberry, Jonathan J. Fortney, Kazumasa Ohno, Lindsey S. Wiser, Luis Welbanks, Marcia J. Rieke, Martha L. Boyer, Michael R. Line, Sagnick Mukherjee, Taylor J. Bell, Thomas G. Beatty, Thomas P. Greene, Vivien Parmentier","submitted_at":"2023-09-07T23:13:09Z","abstract_excerpt":"The abundances of major carbon and oxygen bearing gases in the atmospheres of giant exoplanets provide insights into atmospheric chemistry and planet formation processes. Thermochemistry suggests that methane should be the dominant carbon-bearing species below $\\sim$1000 K over a range of plausible atmospheric compositions; this is the case for the Solar System planets and has been confirmed in the atmospheres of brown dwarfs and self-luminous directly imaged exoplanets. However, methane has not yet been definitively detected with space-based spectroscopy in the atmosphere of a transiting exop"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.04042","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/2309.04042/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":"2309.04042","created_at":"2026-07-05T06:48:54.062060+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.04042v1","created_at":"2026-07-05T06:48:54.062060+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.04042","created_at":"2026-07-05T06:48:54.062060+00:00"},{"alias_kind":"pith_short_12","alias_value":"UOPC2RAR5JV3","created_at":"2026-07-05T06:48:54.062060+00:00"},{"alias_kind":"pith_short_16","alias_value":"UOPC2RAR5JV3UIDL","created_at":"2026-07-05T06:48:54.062060+00:00"},{"alias_kind":"pith_short_8","alias_value":"UOPC2RAR","created_at":"2026-07-05T06:48:54.062060+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.08486","citing_title":"Phase-dependent chemistry of WASP-43 b revealed with a suite of one-, two-, and three-dimensional models","ref_index":29,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH","json":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH.json","graph_json":"https://pith.science/api/pith-number/UOPC2RAR5JV3UIDL33OYFKZ6NH/graph.json","events_json":"https://pith.science/api/pith-number/UOPC2RAR5JV3UIDL33OYFKZ6NH/events.json","paper":"https://pith.science/paper/UOPC2RAR"},"agent_actions":{"view_html":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH","download_json":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH.json","view_paper":"https://pith.science/paper/UOPC2RAR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.04042&json=true","fetch_graph":"https://pith.science/api/pith-number/UOPC2RAR5JV3UIDL33OYFKZ6NH/graph.json","fetch_events":"https://pith.science/api/pith-number/UOPC2RAR5JV3UIDL33OYFKZ6NH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH/action/storage_attestation","attest_author":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH/action/author_attestation","sign_citation":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH/action/citation_signature","submit_replication":"https://pith.science/pith/UOPC2RAR5JV3UIDL33OYFKZ6NH/action/replication_record"}},"created_at":"2026-07-05T06:48:54.062060+00:00","updated_at":"2026-07-05T06:48:54.062060+00:00"}