{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:SN2Q6YHPHECTXJDXUOWTWS4Z2L","short_pith_number":"pith:SN2Q6YHP","schema_version":"1.0","canonical_sha256":"93750f60ef39053ba477a3ad3b4b99d2c8fd329cebc2c587ea5cc3e20c085f33","source":{"kind":"arxiv","id":"2305.01000","version":2},"attestation_state":"computed","paper":{"title":"Revised Properties and Dynamical History for the HD 17156 System","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrew W. Howard, Crystal L. Gnilka, Gregory W. Henry, Howard Isaacson, Michelle L. Hill, Paul A. Dalba, Sergio B. Fajardo-Acosta, Stephen R. Kane, Steve B. Howell, Tara Fetherolf","submitted_at":"2023-05-01T18:00:03Z","abstract_excerpt":"From the thousands of known exoplanets, those that transit bright host stars provide the greatest accessibility toward detailed system characterization. The first known such planets were generally discovered using the radial velocity technique, then later found to transit. HD 17156b is particularly notable among these initial discoveries because it diverged from the typical hot Jupiter population, occupying a 21.2 day eccentric ($e = 0.68$) orbit, offering preliminary insights into the evolution of planets in extreme orbits. Here we present new data for this system, including ground and space-"},"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":"2305.01000","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2023-05-01T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"07dce02f7b641a9350fd0beb89be641f6e5cae19cba0353cc392a13471b31242","abstract_canon_sha256":"b8a59e6c40a3074b1dbb2f14826a2e91862599c2bbc0eaa8185e938ba6e5c232"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:15:30.330180Z","signature_b64":"D7rIsL2C9RwFD/oLhVCyjhNy5ppdiGrXPQJ7BbhSfWGndpz9Vu37ceC1vH5dxfxs4HluqaL0QdefQ0uZy8dJAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"93750f60ef39053ba477a3ad3b4b99d2c8fd329cebc2c587ea5cc3e20c085f33","last_reissued_at":"2026-07-05T06:15:30.329745Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:15:30.329745Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revised Properties and Dynamical History for the HD 17156 System","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Andrew W. Howard, Crystal L. Gnilka, Gregory W. Henry, Howard Isaacson, Michelle L. Hill, Paul A. Dalba, Sergio B. Fajardo-Acosta, Stephen R. Kane, Steve B. Howell, Tara Fetherolf","submitted_at":"2023-05-01T18:00:03Z","abstract_excerpt":"From the thousands of known exoplanets, those that transit bright host stars provide the greatest accessibility toward detailed system characterization. The first known such planets were generally discovered using the radial velocity technique, then later found to transit. HD 17156b is particularly notable among these initial discoveries because it diverged from the typical hot Jupiter population, occupying a 21.2 day eccentric ($e = 0.68$) orbit, offering preliminary insights into the evolution of planets in extreme orbits. Here we present new data for this system, including ground and space-"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.01000","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/2305.01000/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":"2305.01000","created_at":"2026-07-05T06:15:30.329800+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.01000v2","created_at":"2026-07-05T06:15:30.329800+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.01000","created_at":"2026-07-05T06:15:30.329800+00:00"},{"alias_kind":"pith_short_12","alias_value":"SN2Q6YHPHECT","created_at":"2026-07-05T06:15:30.329800+00:00"},{"alias_kind":"pith_short_16","alias_value":"SN2Q6YHPHECTXJDX","created_at":"2026-07-05T06:15:30.329800+00:00"},{"alias_kind":"pith_short_8","alias_value":"SN2Q6YHP","created_at":"2026-07-05T06:15:30.329800+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/SN2Q6YHPHECTXJDXUOWTWS4Z2L","json":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L.json","graph_json":"https://pith.science/api/pith-number/SN2Q6YHPHECTXJDXUOWTWS4Z2L/graph.json","events_json":"https://pith.science/api/pith-number/SN2Q6YHPHECTXJDXUOWTWS4Z2L/events.json","paper":"https://pith.science/paper/SN2Q6YHP"},"agent_actions":{"view_html":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L","download_json":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L.json","view_paper":"https://pith.science/paper/SN2Q6YHP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.01000&json=true","fetch_graph":"https://pith.science/api/pith-number/SN2Q6YHPHECTXJDXUOWTWS4Z2L/graph.json","fetch_events":"https://pith.science/api/pith-number/SN2Q6YHPHECTXJDXUOWTWS4Z2L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L/action/storage_attestation","attest_author":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L/action/author_attestation","sign_citation":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L/action/citation_signature","submit_replication":"https://pith.science/pith/SN2Q6YHPHECTXJDXUOWTWS4Z2L/action/replication_record"}},"created_at":"2026-07-05T06:15:30.329800+00:00","updated_at":"2026-07-05T06:15:30.329800+00:00"}