{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:SPC2DL4L2PGKMZDXJDJS77F5E2","short_pith_number":"pith:SPC2DL4L","schema_version":"1.0","canonical_sha256":"93c5a1af8bd3cca6647748d32ffcbd2685f5e272dd3eb6d5b22673f09d274269","source":{"kind":"arxiv","id":"2403.00608","version":3},"attestation_state":"computed","paper":{"title":"The GAPS Programme at TNG: LIV. A HeI survey of close-in giant planets hosted by M-K dwarf stars with GIANO-B","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bignamini, A. F. Lanza, A. Ghedina, A. Maggio, A. Petralia, A. S. Bonomo, A. Sozzetti, C. Knapic, D. Sicilia, F. Biassoni, F. Borsa, G. Andreuzzi, G. Guilluy, G. Mantovan, G. Micela, G. Scandariato, I. Carleo, L. Affer, L. Fossati, L. Mancini, L. Pino, M. C. D'Arpa, M. Cecconi, M. Pedani, M. Rainer, M. Stangret, P. Giacobbe, R. Spinelli, S. Desidera, T. Zingales, V. Fardella, V. Nascimbeni, W. Boschin","submitted_at":"2024-03-01T15:32:58Z","abstract_excerpt":"Atmospheric escape plays a fundamental role in shaping the properties of exoplanets. The metastable near-infrared helium triplet at 1083.3 nm (HeI) is a powerful proxy of extended and evaporating atmospheres. We used the GIARPS (GIANO-B+HARPS-N) observing mode of the Telescopio Nazionale Galileo to search for HeI absorption in the upper atmosphere of five close-in giant planets hosted by the K and M dwarf stars of our sample, namely WASP-69b, WASP-107b, HAT-P-11b, GJ436b, and GJ3470b. We focused our analysis on the HeI triplet by performing high-resolution transmission spectroscopy. When night"},"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":"2403.00608","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-03-01T15:32:58Z","cross_cats_sorted":[],"title_canon_sha256":"d74527c8addd435a1b19b0049e960b538d56987d52ac447ff2a25dae26059c7a","abstract_canon_sha256":"afd31c51ba8ba850d7acfdbf9ddf145cb0da18811a85804e69dfa031abc93d31"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:04:18.459976Z","signature_b64":"3HBBCxH+ZBH7q/ESbhv75YyD9KFI6vNCEKci0Zb4vTzlHdPxIcLmyvJsyZ0XTQV3F8fyyGitM/DMw8D2h4BICg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"93c5a1af8bd3cca6647748d32ffcbd2685f5e272dd3eb6d5b22673f09d274269","last_reissued_at":"2026-07-05T08:04:18.459499Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:04:18.459499Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The GAPS Programme at TNG: LIV. A HeI survey of close-in giant planets hosted by M-K dwarf stars with GIANO-B","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bignamini, A. F. Lanza, A. Ghedina, A. Maggio, A. Petralia, A. S. Bonomo, A. Sozzetti, C. Knapic, D. Sicilia, F. Biassoni, F. Borsa, G. Andreuzzi, G. Guilluy, G. Mantovan, G. Micela, G. Scandariato, I. Carleo, L. Affer, L. Fossati, L. Mancini, L. Pino, M. C. D'Arpa, M. Cecconi, M. Pedani, M. Rainer, M. Stangret, P. Giacobbe, R. Spinelli, S. Desidera, T. Zingales, V. Fardella, V. Nascimbeni, W. Boschin","submitted_at":"2024-03-01T15:32:58Z","abstract_excerpt":"Atmospheric escape plays a fundamental role in shaping the properties of exoplanets. The metastable near-infrared helium triplet at 1083.3 nm (HeI) is a powerful proxy of extended and evaporating atmospheres. We used the GIARPS (GIANO-B+HARPS-N) observing mode of the Telescopio Nazionale Galileo to search for HeI absorption in the upper atmosphere of five close-in giant planets hosted by the K and M dwarf stars of our sample, namely WASP-69b, WASP-107b, HAT-P-11b, GJ436b, and GJ3470b. We focused our analysis on the HeI triplet by performing high-resolution transmission spectroscopy. When night"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.00608","kind":"arxiv","version":3},"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/2403.00608/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":"2403.00608","created_at":"2026-07-05T08:04:18.459556+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.00608v3","created_at":"2026-07-05T08:04:18.459556+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.00608","created_at":"2026-07-05T08:04:18.459556+00:00"},{"alias_kind":"pith_short_12","alias_value":"SPC2DL4L2PGK","created_at":"2026-07-05T08:04:18.459556+00:00"},{"alias_kind":"pith_short_16","alias_value":"SPC2DL4L2PGKMZDX","created_at":"2026-07-05T08:04:18.459556+00:00"},{"alias_kind":"pith_short_8","alias_value":"SPC2DL4L","created_at":"2026-07-05T08:04:18.459556+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/SPC2DL4L2PGKMZDXJDJS77F5E2","json":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2.json","graph_json":"https://pith.science/api/pith-number/SPC2DL4L2PGKMZDXJDJS77F5E2/graph.json","events_json":"https://pith.science/api/pith-number/SPC2DL4L2PGKMZDXJDJS77F5E2/events.json","paper":"https://pith.science/paper/SPC2DL4L"},"agent_actions":{"view_html":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2","download_json":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2.json","view_paper":"https://pith.science/paper/SPC2DL4L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.00608&json=true","fetch_graph":"https://pith.science/api/pith-number/SPC2DL4L2PGKMZDXJDJS77F5E2/graph.json","fetch_events":"https://pith.science/api/pith-number/SPC2DL4L2PGKMZDXJDJS77F5E2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2/action/storage_attestation","attest_author":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2/action/author_attestation","sign_citation":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2/action/citation_signature","submit_replication":"https://pith.science/pith/SPC2DL4L2PGKMZDXJDJS77F5E2/action/replication_record"}},"created_at":"2026-07-05T08:04:18.459556+00:00","updated_at":"2026-07-05T08:04:18.459556+00:00"}