{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:GDAOMYCGBYCMULG7CYAOLP4DIU","short_pith_number":"pith:GDAOMYCG","schema_version":"1.0","canonical_sha256":"30c0e660460e04ca2cdf1600e5bf83450203f718beaca20cdbf4bb786b244904","source":{"kind":"arxiv","id":"2410.11643","version":1},"attestation_state":"computed","paper":{"title":"Spectroscopically resolved partial phase curve of the rapid heating and cooling of the highly-eccentric Hot Jupiter HAT-P-2b with WFC3","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Bob Jacobs, Jean-Michel D\\'esert, Jonathan Fortney, Julien de Wit, Kevin B. Stevenson, L. C. Mayorga, Michael Line, Nikole Lewis, Ryan C. Challener, Saugata Barat, Tiffany Kataria, Vivien Parmentier, Zo\\\"e de Beurs","submitted_at":"2024-10-14T16:00:16Z","abstract_excerpt":"The extreme environments of transiting close-in exoplanets in highly-eccentric orbits are ideal for testing exo-climate physics. Spectroscopically resolved phase curves not only allow for the characterization of their thermal response to irradiation changes but also unveil phase-dependent atmospheric chemistry and dynamics. We observed a partial phase curve of the highly-eccentric close-in giant planet HAT-P-2b ($e=0.51,M=9M_{\\rm{Jup}}$) with the Wide Field Camera 3 aboard the Hubble Space Telescope. Using these data, we updated the planet's orbital parameters and radius, and retrieved high-fr"},"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":"2410.11643","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-10-14T16:00:16Z","cross_cats_sorted":[],"title_canon_sha256":"1a8dc623225c9862bcf059ca0944111f80bf3d35e044d0ad8d7aa0c5d3afaa0b","abstract_canon_sha256":"4eea4f2c0b77e880f0e5505191824a6bcc3b4acaeca363aba34146e74f58fd58"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:32:48.784813Z","signature_b64":"bzQlEEM4cnqGAAP++hSzaeGXp68FA5+zIumM2HtyoHRiOUwVaAINzMT6HLIIXnoBgO6x9uy63ken9gDSymQVDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"30c0e660460e04ca2cdf1600e5bf83450203f718beaca20cdbf4bb786b244904","last_reissued_at":"2026-07-05T09:32:48.784241Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:32:48.784241Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spectroscopically resolved partial phase curve of the rapid heating and cooling of the highly-eccentric Hot Jupiter HAT-P-2b with WFC3","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Bob Jacobs, Jean-Michel D\\'esert, Jonathan Fortney, Julien de Wit, Kevin B. Stevenson, L. C. Mayorga, Michael Line, Nikole Lewis, Ryan C. Challener, Saugata Barat, Tiffany Kataria, Vivien Parmentier, Zo\\\"e de Beurs","submitted_at":"2024-10-14T16:00:16Z","abstract_excerpt":"The extreme environments of transiting close-in exoplanets in highly-eccentric orbits are ideal for testing exo-climate physics. Spectroscopically resolved phase curves not only allow for the characterization of their thermal response to irradiation changes but also unveil phase-dependent atmospheric chemistry and dynamics. We observed a partial phase curve of the highly-eccentric close-in giant planet HAT-P-2b ($e=0.51,M=9M_{\\rm{Jup}}$) with the Wide Field Camera 3 aboard the Hubble Space Telescope. Using these data, we updated the planet's orbital parameters and radius, and retrieved high-fr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2410.11643","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/2410.11643/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":"2410.11643","created_at":"2026-07-05T09:32:48.784311+00:00"},{"alias_kind":"arxiv_version","alias_value":"2410.11643v1","created_at":"2026-07-05T09:32:48.784311+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2410.11643","created_at":"2026-07-05T09:32:48.784311+00:00"},{"alias_kind":"pith_short_12","alias_value":"GDAOMYCGBYCM","created_at":"2026-07-05T09:32:48.784311+00:00"},{"alias_kind":"pith_short_16","alias_value":"GDAOMYCGBYCMULG7","created_at":"2026-07-05T09:32:48.784311+00:00"},{"alias_kind":"pith_short_8","alias_value":"GDAOMYCG","created_at":"2026-07-05T09:32:48.784311+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/GDAOMYCGBYCMULG7CYAOLP4DIU","json":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU.json","graph_json":"https://pith.science/api/pith-number/GDAOMYCGBYCMULG7CYAOLP4DIU/graph.json","events_json":"https://pith.science/api/pith-number/GDAOMYCGBYCMULG7CYAOLP4DIU/events.json","paper":"https://pith.science/paper/GDAOMYCG"},"agent_actions":{"view_html":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU","download_json":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU.json","view_paper":"https://pith.science/paper/GDAOMYCG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2410.11643&json=true","fetch_graph":"https://pith.science/api/pith-number/GDAOMYCGBYCMULG7CYAOLP4DIU/graph.json","fetch_events":"https://pith.science/api/pith-number/GDAOMYCGBYCMULG7CYAOLP4DIU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU/action/storage_attestation","attest_author":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU/action/author_attestation","sign_citation":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU/action/citation_signature","submit_replication":"https://pith.science/pith/GDAOMYCGBYCMULG7CYAOLP4DIU/action/replication_record"}},"created_at":"2026-07-05T09:32:48.784311+00:00","updated_at":"2026-07-05T09:32:48.784311+00:00"}