{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:CQJU5TEEVXGDHHOIBF57YREYR5","short_pith_number":"pith:CQJU5TEE","schema_version":"1.0","canonical_sha256":"14134ecc84adcc339dc8097bfc44988f7301f90f4ddc680dfbf66515205bee74","source":{"kind":"arxiv","id":"2501.02081","version":1},"attestation_state":"computed","paper":{"title":"Statistical trends in JWST transiting exoplanet atmospheres","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrew W. Mann, Cyril Gapp, Daniel Thorngren, David K. Sing, Guangwei Fu, Joshua Lothringer, Kevin B. Stevenson, Luis Welbanks, Pa Chia Thao, Peter Gao, Romain Allart, Sagnick Mukherjee, Shang-Min Tsai, Stefan Pelletier, Thomas G. Beatty, Thomas M. Evans-Soma","submitted_at":"2025-01-03T19:55:19Z","abstract_excerpt":"Our brains are hardwired for pattern recognition as correlations are useful for predicting and understanding nature. As more exoplanet atmospheres are being characterized with JWST, we are starting to unveil their properties on a population level. Here we present a framework for comparing exoplanet transmission spectroscopy from 3 to 5$\\mu$m with four bands: L (2.9 - 3.7$\\mu$m), SO$_2$ (3.95 - 4.1$\\mu$m), CO$_2$ (4.25 - 4.4$\\mu$m) and CO (4.5 - 4.9$\\mu$m). Together, the four bands cover the major carbon, oxygen, nitrogen, and sulfur-bearing molecules including H$_2$O, CH$_4$, NH$_3$, H$_2$S, S"},"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":"2501.02081","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-01-03T19:55:19Z","cross_cats_sorted":[],"title_canon_sha256":"209d76eeab8d23fd82308e0e3349ae08fb5948a00088a5125547f6ba5fe6ce2d","abstract_canon_sha256":"10611d464b0a05c82336a6815e90e216ad0e59f4789885e2ee706bf645195712"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:57:01.862186Z","signature_b64":"TO186KX+x4oXVgO6/VadupW7zfGbIob7LBvzdlIWtftbL6bvE2j7No3GGzygew8GutyCQ1+9jOJ2tdD/b2rpBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14134ecc84adcc339dc8097bfc44988f7301f90f4ddc680dfbf66515205bee74","last_reissued_at":"2026-07-05T09:57:01.861729Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:57:01.861729Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Statistical trends in JWST transiting exoplanet atmospheres","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrew W. Mann, Cyril Gapp, Daniel Thorngren, David K. Sing, Guangwei Fu, Joshua Lothringer, Kevin B. Stevenson, Luis Welbanks, Pa Chia Thao, Peter Gao, Romain Allart, Sagnick Mukherjee, Shang-Min Tsai, Stefan Pelletier, Thomas G. Beatty, Thomas M. Evans-Soma","submitted_at":"2025-01-03T19:55:19Z","abstract_excerpt":"Our brains are hardwired for pattern recognition as correlations are useful for predicting and understanding nature. As more exoplanet atmospheres are being characterized with JWST, we are starting to unveil their properties on a population level. Here we present a framework for comparing exoplanet transmission spectroscopy from 3 to 5$\\mu$m with four bands: L (2.9 - 3.7$\\mu$m), SO$_2$ (3.95 - 4.1$\\mu$m), CO$_2$ (4.25 - 4.4$\\mu$m) and CO (4.5 - 4.9$\\mu$m). Together, the four bands cover the major carbon, oxygen, nitrogen, and sulfur-bearing molecules including H$_2$O, CH$_4$, NH$_3$, H$_2$S, S"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.02081","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/2501.02081/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":"2501.02081","created_at":"2026-07-05T09:57:01.861788+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.02081v1","created_at":"2026-07-05T09:57:01.861788+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.02081","created_at":"2026-07-05T09:57:01.861788+00:00"},{"alias_kind":"pith_short_12","alias_value":"CQJU5TEEVXGD","created_at":"2026-07-05T09:57:01.861788+00:00"},{"alias_kind":"pith_short_16","alias_value":"CQJU5TEEVXGDHHOI","created_at":"2026-07-05T09:57:01.861788+00:00"},{"alias_kind":"pith_short_8","alias_value":"CQJU5TEE","created_at":"2026-07-05T09:57:01.861788+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.21770","citing_title":"Radiatively Controlled Thermal Stability of High-Altitude Clouds in Exoplanetary Atmospheres","ref_index":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5","json":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5.json","graph_json":"https://pith.science/api/pith-number/CQJU5TEEVXGDHHOIBF57YREYR5/graph.json","events_json":"https://pith.science/api/pith-number/CQJU5TEEVXGDHHOIBF57YREYR5/events.json","paper":"https://pith.science/paper/CQJU5TEE"},"agent_actions":{"view_html":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5","download_json":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5.json","view_paper":"https://pith.science/paper/CQJU5TEE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.02081&json=true","fetch_graph":"https://pith.science/api/pith-number/CQJU5TEEVXGDHHOIBF57YREYR5/graph.json","fetch_events":"https://pith.science/api/pith-number/CQJU5TEEVXGDHHOIBF57YREYR5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5/action/storage_attestation","attest_author":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5/action/author_attestation","sign_citation":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5/action/citation_signature","submit_replication":"https://pith.science/pith/CQJU5TEEVXGDHHOIBF57YREYR5/action/replication_record"}},"created_at":"2026-07-05T09:57:01.861788+00:00","updated_at":"2026-07-05T09:57:01.861788+00:00"}