{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ","short_pith_number":"pith:ZWVPNIU4","schema_version":"1.0","canonical_sha256":"cdaaf6a29cc6a2764a640e79619ef1064a476f44f37a5dee267db926487c364a","source":{"kind":"arxiv","id":"1704.05878","version":2},"attestation_state":"computed","paper":{"title":"NIR-Driven Moist Upper Atmospheres of Synchronously Rotating Temperate Terrestrial Exoplanets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Anthony D. Del Genio, David S. Amundsen, Yuka Fujii","submitted_at":"2017-04-19T18:17:42Z","abstract_excerpt":"H$_2$O is a key molecule in characterizing atmospheres of temperate terrestrial planets, and observations of transmission spectra are expected to play a primary role in detecting its signatures in the near future. The detectability of H$_2$O absorption features in transmission spectra depends on the abundance of water vapor in the upper part of the atmosphere. We study the three-dimensional distribution of atmospheric H$_2$O for synchronously rotating Earth-sized aquaplanets using the general circulation model (GCM) ROCKE-3D, and examine the effects of total incident flux and stellar spectral "},"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":"1704.05878","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2017-04-19T18:17:42Z","cross_cats_sorted":[],"title_canon_sha256":"35b61602317b5b3dcb179477e8b0fa253a0b51702be3f7b6270b4f6b02d57867","abstract_canon_sha256":"9456adf00bdc1674ced467fdcecc1fb2551b9d49ab176924e9ca8b46af6dcab6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:31:51.222766Z","signature_b64":"J1v/SHaCJfW/4asOZThuR6onleKYgo6ezZusbuia7gOn9nyRjQKg0yP19qQKcJ4ypB0+fZ+SoNuNfCMYa3KDDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cdaaf6a29cc6a2764a640e79619ef1064a476f44f37a5dee267db926487c364a","last_reissued_at":"2026-05-18T00:31:51.222311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:31:51.222311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"NIR-Driven Moist Upper Atmospheres of Synchronously Rotating Temperate Terrestrial Exoplanets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Anthony D. Del Genio, David S. Amundsen, Yuka Fujii","submitted_at":"2017-04-19T18:17:42Z","abstract_excerpt":"H$_2$O is a key molecule in characterizing atmospheres of temperate terrestrial planets, and observations of transmission spectra are expected to play a primary role in detecting its signatures in the near future. The detectability of H$_2$O absorption features in transmission spectra depends on the abundance of water vapor in the upper part of the atmosphere. We study the three-dimensional distribution of atmospheric H$_2$O for synchronously rotating Earth-sized aquaplanets using the general circulation model (GCM) ROCKE-3D, and examine the effects of total incident flux and stellar spectral "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.05878","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":""},"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":"1704.05878","created_at":"2026-05-18T00:31:51.222387+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.05878v2","created_at":"2026-05-18T00:31:51.222387+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.05878","created_at":"2026-05-18T00:31:51.222387+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZWVPNIU4Y2RH","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZWVPNIU4Y2RHMSTE","created_at":"2026-05-18T12:31:59.375834+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZWVPNIU4","created_at":"2026-05-18T12:31:59.375834+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/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ","json":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ.json","graph_json":"https://pith.science/api/pith-number/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/graph.json","events_json":"https://pith.science/api/pith-number/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/events.json","paper":"https://pith.science/paper/ZWVPNIU4"},"agent_actions":{"view_html":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ","download_json":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ.json","view_paper":"https://pith.science/paper/ZWVPNIU4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.05878&json=true","fetch_graph":"https://pith.science/api/pith-number/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/graph.json","fetch_events":"https://pith.science/api/pith-number/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/action/storage_attestation","attest_author":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/action/author_attestation","sign_citation":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/action/citation_signature","submit_replication":"https://pith.science/pith/ZWVPNIU4Y2RHMSTEBZ4WDHXRAZ/action/replication_record"}},"created_at":"2026-05-18T00:31:51.222387+00:00","updated_at":"2026-05-18T00:31:51.222387+00:00"}