{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:WEOWAOWINY2VV6DPDSQ4DTSMVT","short_pith_number":"pith:WEOWAOWI","schema_version":"1.0","canonical_sha256":"b11d603ac86e355af86f1ca1c1ce4cacc4747d9a28e2af5d1b82b4c61247784d","source":{"kind":"arxiv","id":"astro-ph/0505359","version":1},"attestation_state":"computed","paper":{"title":"Comparative Planetary Atmospheres: Models of TrES-1 and HD209458b","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Saumon, J.J. Fortney, K. Lodders, M.S. Marley, R. Freedman","submitted_at":"2005-05-17T20:13:27Z","abstract_excerpt":"We present new self-consistent atmosphere models for transiting planets TrES-1 and HD209458b. The planets were recently observed with the Spitzer Space Telescope in bands centered on 4.5 and 8.0 $\\mu$m, for TrES-1, and 24 $\\mu$m, for HD209458b. We find that standard solar metallicity models fit the observations for HD209458b. For TrES-1, which has an T_eff ~300 K cooler, we find that models with a metallicity 3-5 times enhanced over solar abundances can match the 1$\\sigma$ error bar at 4.5 $\\mu$m and 2$\\sigma$ at 8.0$\\mu$m. Models with solar abundances that included energy deposition into the "},"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":"astro-ph/0505359","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-05-17T20:13:27Z","cross_cats_sorted":[],"title_canon_sha256":"2011c6c3485c52ffc6695bc99c2833c3f89155d4ef32492f3ba1dc884f506f3e","abstract_canon_sha256":"2658e4eea9c0cf0b47b76eb8129f32f576c439ca7b8a8551e9b0f13d743611da"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:52:23.925569Z","signature_b64":"OPrxphJa8GlIfYYcuxIkM9Y4a5TB+7IdQqPpZDMJ55YCWJPTkKAVY9J/tLVj0zkLxjzLLX5GoGVkwJtSbvIjBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b11d603ac86e355af86f1ca1c1ce4cacc4747d9a28e2af5d1b82b4c61247784d","last_reissued_at":"2026-07-04T16:52:23.925210Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:52:23.925210Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comparative Planetary Atmospheres: Models of TrES-1 and HD209458b","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Saumon, J.J. Fortney, K. Lodders, M.S. Marley, R. Freedman","submitted_at":"2005-05-17T20:13:27Z","abstract_excerpt":"We present new self-consistent atmosphere models for transiting planets TrES-1 and HD209458b. The planets were recently observed with the Spitzer Space Telescope in bands centered on 4.5 and 8.0 $\\mu$m, for TrES-1, and 24 $\\mu$m, for HD209458b. We find that standard solar metallicity models fit the observations for HD209458b. For TrES-1, which has an T_eff ~300 K cooler, we find that models with a metallicity 3-5 times enhanced over solar abundances can match the 1$\\sigma$ error bar at 4.5 $\\mu$m and 2$\\sigma$ at 8.0$\\mu$m. Models with solar abundances that included energy deposition into the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0505359","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/astro-ph/0505359/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":"astro-ph/0505359","created_at":"2026-07-04T16:52:23.925270+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0505359v1","created_at":"2026-07-04T16:52:23.925270+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0505359","created_at":"2026-07-04T16:52:23.925270+00:00"},{"alias_kind":"pith_short_12","alias_value":"WEOWAOWINY2V","created_at":"2026-07-04T16:52:23.925270+00:00"},{"alias_kind":"pith_short_16","alias_value":"WEOWAOWINY2VV6DP","created_at":"2026-07-04T16:52:23.925270+00:00"},{"alias_kind":"pith_short_8","alias_value":"WEOWAOWI","created_at":"2026-07-04T16:52:23.925270+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/WEOWAOWINY2VV6DPDSQ4DTSMVT","json":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT.json","graph_json":"https://pith.science/api/pith-number/WEOWAOWINY2VV6DPDSQ4DTSMVT/graph.json","events_json":"https://pith.science/api/pith-number/WEOWAOWINY2VV6DPDSQ4DTSMVT/events.json","paper":"https://pith.science/paper/WEOWAOWI"},"agent_actions":{"view_html":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT","download_json":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT.json","view_paper":"https://pith.science/paper/WEOWAOWI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0505359&json=true","fetch_graph":"https://pith.science/api/pith-number/WEOWAOWINY2VV6DPDSQ4DTSMVT/graph.json","fetch_events":"https://pith.science/api/pith-number/WEOWAOWINY2VV6DPDSQ4DTSMVT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT/action/storage_attestation","attest_author":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT/action/author_attestation","sign_citation":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT/action/citation_signature","submit_replication":"https://pith.science/pith/WEOWAOWINY2VV6DPDSQ4DTSMVT/action/replication_record"}},"created_at":"2026-07-04T16:52:23.925270+00:00","updated_at":"2026-07-04T16:52:23.925270+00:00"}