{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:FDVB2TQH56E42DNHI76UXU7ZDP","short_pith_number":"pith:FDVB2TQH","schema_version":"1.0","canonical_sha256":"28ea1d4e07ef89cd0da747fd4bd3f91bd5cb78dc79168c0bff06010fb7aa9161","source":{"kind":"arxiv","id":"2109.11460","version":2},"attestation_state":"computed","paper":{"title":"The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI). Part III: Simulated Observables -- The return of the spectrum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ao-ph"],"primary_cat":"astro-ph.EP","authors_text":"Denis E. Sergeev, Eric T. Wolf, Francois Forget, Geronimo L. Villanueva, Ian A. Boutle, Jacob Haqq-Misra, James Manners, Kostas Tsigaridis, Martin Turbet, Michael J. Way, Nathan J. Mayne, Ravi K. Kopparapu, Shawn D. Domagal-Goldman, Thomas J. Fauchez","submitted_at":"2021-09-23T16:04:38Z","abstract_excerpt":"The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI) is a community project that aims to quantify how dfferences in general circulation models (GCMs) could impact the climate prediction for TRAPPIST-1e and, subsequently its atmospheric characterization in transit. Four GCMs have participated in THAI so far: ExoCAM, LMD-Generic, ROCKE-3D and the UM. This paper, focused on the simulated observations, is the third part of a trilogy, following the analysis of two land planet scenarios (part I) and two aquaplanet scenarios (part II). Here, we show a robust agreement between the simulated spec"},"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":"2109.11460","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2021-09-23T16:04:38Z","cross_cats_sorted":["physics.ao-ph"],"title_canon_sha256":"5a0c08a36f92fe6c583beb6736a9e72081ad20902ad5c0a36028eac71a382b46","abstract_canon_sha256":"b6eed944fd99143df0459ebb5e9f993aaa5f4714f527fb2fdc484bda33004ee0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:57:43.191869Z","signature_b64":"snMq9uRC/fNqlYRzZsaWjcMhtrD5Wkn5002XdWwXH2gNoalem7FVo+cYlnGjSA+1Zerov4ua7fc1uSzVbMjQAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"28ea1d4e07ef89cd0da747fd4bd3f91bd5cb78dc79168c0bff06010fb7aa9161","last_reissued_at":"2026-07-05T04:57:43.191401Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:57:43.191401Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI). Part III: Simulated Observables -- The return of the spectrum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ao-ph"],"primary_cat":"astro-ph.EP","authors_text":"Denis E. Sergeev, Eric T. Wolf, Francois Forget, Geronimo L. Villanueva, Ian A. Boutle, Jacob Haqq-Misra, James Manners, Kostas Tsigaridis, Martin Turbet, Michael J. Way, Nathan J. Mayne, Ravi K. Kopparapu, Shawn D. Domagal-Goldman, Thomas J. Fauchez","submitted_at":"2021-09-23T16:04:38Z","abstract_excerpt":"The TRAPPIST-1 Habitable Atmosphere Intercomparison (THAI) is a community project that aims to quantify how dfferences in general circulation models (GCMs) could impact the climate prediction for TRAPPIST-1e and, subsequently its atmospheric characterization in transit. Four GCMs have participated in THAI so far: ExoCAM, LMD-Generic, ROCKE-3D and the UM. This paper, focused on the simulated observations, is the third part of a trilogy, following the analysis of two land planet scenarios (part I) and two aquaplanet scenarios (part II). Here, we show a robust agreement between the simulated spec"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2109.11460","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/2109.11460/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":"2109.11460","created_at":"2026-07-05T04:57:43.191449+00:00"},{"alias_kind":"arxiv_version","alias_value":"2109.11460v2","created_at":"2026-07-05T04:57:43.191449+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2109.11460","created_at":"2026-07-05T04:57:43.191449+00:00"},{"alias_kind":"pith_short_12","alias_value":"FDVB2TQH56E4","created_at":"2026-07-05T04:57:43.191449+00:00"},{"alias_kind":"pith_short_16","alias_value":"FDVB2TQH56E42DNH","created_at":"2026-07-05T04:57:43.191449+00:00"},{"alias_kind":"pith_short_8","alias_value":"FDVB2TQH","created_at":"2026-07-05T04:57:43.191449+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06366","citing_title":"A generalised microbial cell model for methane biosignature predictions","ref_index":79,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP","json":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP.json","graph_json":"https://pith.science/api/pith-number/FDVB2TQH56E42DNHI76UXU7ZDP/graph.json","events_json":"https://pith.science/api/pith-number/FDVB2TQH56E42DNHI76UXU7ZDP/events.json","paper":"https://pith.science/paper/FDVB2TQH"},"agent_actions":{"view_html":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP","download_json":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP.json","view_paper":"https://pith.science/paper/FDVB2TQH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2109.11460&json=true","fetch_graph":"https://pith.science/api/pith-number/FDVB2TQH56E42DNHI76UXU7ZDP/graph.json","fetch_events":"https://pith.science/api/pith-number/FDVB2TQH56E42DNHI76UXU7ZDP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP/action/storage_attestation","attest_author":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP/action/author_attestation","sign_citation":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP/action/citation_signature","submit_replication":"https://pith.science/pith/FDVB2TQH56E42DNHI76UXU7ZDP/action/replication_record"}},"created_at":"2026-07-05T04:57:43.191449+00:00","updated_at":"2026-07-05T04:57:43.191449+00:00"}