{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:NKUHGADKOCU4J7V37TL2GHDSIY","short_pith_number":"pith:NKUHGADK","schema_version":"1.0","canonical_sha256":"6aa873006a70a9c4febbfcd7a31c724616b75d7c9d3c524e42ae3af4c0014e19","source":{"kind":"arxiv","id":"2205.10549","version":2},"attestation_state":"computed","paper":{"title":"The GAPS Programme at TNG: XXXVI. Measurement of the Rossiter-McLaughlin effect and revising the physical and orbital parameters of the HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, HAT-P-29 eccentric planetary systems","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bignamini, A. F. Lanza, A. F. M. Fiorenzano, A. Harutyunyan, A. Maggio, A. S. Bonomo, A. Sozzetti, C. Knapic, D. Barbato, D. F. Evans, E. Covino, E. Molinari, E. Poretti, G. Andreuzzi, G. Micela, G. Piotto, I. Bruni, I. Pagano, J. Southworth, J. Tregloan-Reed, K. Biazzo, L. Borsato, L. Di Fabrizio, L. Mancini, L. Naponiello, M. Basilicata, M. Damasso, M. Esposito, M. Pedani, M. Pinamonti, P. Giacobbe, R. Claudi, R. Cosentino, S. Desidera, Th. Henning, V. Granata, V. Nascimbeni","submitted_at":"2022-05-21T09:50:41Z","abstract_excerpt":"Aim: We aim to refine the orbital and physical parameters and determine the sky-projected planet orbital obliquity of five eccentric transiting planetary systems: HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, and HAT-P-29. Each of the systems hosts a hot Jupiter, except for HAT-P-26 which hosts a Neptune-mass planet. Methods: We observed transit events of these planets with the HARPS-N spectrograph, obtaining high-precision radial velocity measurements that allow us to measure the Rossiter-McLaughlin effect for each of the target systems. We used these new HARPS-N spectra and archival data, includin"},"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":"2205.10549","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2022-05-21T09:50:41Z","cross_cats_sorted":[],"title_canon_sha256":"83b5e74363ce51f8d82d8f61a5e7183a07c8b155bdde3f93ce65b56680b6928d","abstract_canon_sha256":"0909e3778755e39db78e526f6871252bef428743bbac659e7db83bb42c66edb3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:56:44.909357Z","signature_b64":"DoRO2OnpAcbocDhkZumKGZb5IYUhBTZ3tjja2ubK7Hbnx1/shdYB40jKQWaaO5pEtpoFsai8hA8HW3HWflucDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6aa873006a70a9c4febbfcd7a31c724616b75d7c9d3c524e42ae3af4c0014e19","last_reissued_at":"2026-07-05T04:56:44.908892Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:56:44.908892Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The GAPS Programme at TNG: XXXVI. Measurement of the Rossiter-McLaughlin effect and revising the physical and orbital parameters of the HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, HAT-P-29 eccentric planetary systems","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bignamini, A. F. Lanza, A. F. M. Fiorenzano, A. Harutyunyan, A. Maggio, A. S. Bonomo, A. Sozzetti, C. Knapic, D. Barbato, D. F. Evans, E. Covino, E. Molinari, E. Poretti, G. Andreuzzi, G. Micela, G. Piotto, I. Bruni, I. Pagano, J. Southworth, J. Tregloan-Reed, K. Biazzo, L. Borsato, L. Di Fabrizio, L. Mancini, L. Naponiello, M. Basilicata, M. Damasso, M. Esposito, M. Pedani, M. Pinamonti, P. Giacobbe, R. Claudi, R. Cosentino, S. Desidera, Th. Henning, V. Granata, V. Nascimbeni","submitted_at":"2022-05-21T09:50:41Z","abstract_excerpt":"Aim: We aim to refine the orbital and physical parameters and determine the sky-projected planet orbital obliquity of five eccentric transiting planetary systems: HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, and HAT-P-29. Each of the systems hosts a hot Jupiter, except for HAT-P-26 which hosts a Neptune-mass planet. Methods: We observed transit events of these planets with the HARPS-N spectrograph, obtaining high-precision radial velocity measurements that allow us to measure the Rossiter-McLaughlin effect for each of the target systems. We used these new HARPS-N spectra and archival data, includin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.10549","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/2205.10549/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":"2205.10549","created_at":"2026-07-05T04:56:44.908950+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.10549v2","created_at":"2026-07-05T04:56:44.908950+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.10549","created_at":"2026-07-05T04:56:44.908950+00:00"},{"alias_kind":"pith_short_12","alias_value":"NKUHGADKOCU4","created_at":"2026-07-05T04:56:44.908950+00:00"},{"alias_kind":"pith_short_16","alias_value":"NKUHGADKOCU4J7V3","created_at":"2026-07-05T04:56:44.908950+00:00"},{"alias_kind":"pith_short_8","alias_value":"NKUHGADK","created_at":"2026-07-05T04:56:44.908950+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.09656","citing_title":"HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna","ref_index":122,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY","json":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY.json","graph_json":"https://pith.science/api/pith-number/NKUHGADKOCU4J7V37TL2GHDSIY/graph.json","events_json":"https://pith.science/api/pith-number/NKUHGADKOCU4J7V37TL2GHDSIY/events.json","paper":"https://pith.science/paper/NKUHGADK"},"agent_actions":{"view_html":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY","download_json":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY.json","view_paper":"https://pith.science/paper/NKUHGADK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.10549&json=true","fetch_graph":"https://pith.science/api/pith-number/NKUHGADKOCU4J7V37TL2GHDSIY/graph.json","fetch_events":"https://pith.science/api/pith-number/NKUHGADKOCU4J7V37TL2GHDSIY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY/action/storage_attestation","attest_author":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY/action/author_attestation","sign_citation":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY/action/citation_signature","submit_replication":"https://pith.science/pith/NKUHGADKOCU4J7V37TL2GHDSIY/action/replication_record"}},"created_at":"2026-07-05T04:56:44.908950+00:00","updated_at":"2026-07-05T04:56:44.908950+00:00"}