{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:GAFPZUFR4EKAMOFP7ORBJT5HUM","short_pith_number":"pith:GAFPZUFR","schema_version":"1.0","canonical_sha256":"300afcd0b1e1140638affba214cfa7a300eb1d35acfdbecb752533b2ee5a931d","source":{"kind":"arxiv","id":"2606.27221","version":1},"attestation_state":"computed","paper":{"title":"Cross-correlation transmission spectroscopy of ultra-hot Jupiters WASP-189b, HAT-P-57b, KELT-17b, and KELT-21b with GIANO-B","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"E. Pall\\'e, Gareb Fern\\'andez-Rodr\\'iguez, H. Parviainen, I. Carleo, J. Orell-Miquel, M. Basilicata, M. Stangret, P. Giacobbe, P. Meni-Gallardo","submitted_at":"2026-06-25T16:08:27Z","abstract_excerpt":"Since the discovery of the first exoplanet, significant efforts have been made to characterise their atmospheres. Ultra-hot Jupiters (UHJs) are of particular interest due to their extended and hot atmospheres. Although previous studies have focused on the detection of atomic species at optical wavelengths, near-infrared (NIR) observations offer the potential to detect molecules. In our study, we applied the cross-correlation technique to NIR transmission spectra from \\giano. The analysis focuses on the search for H$_2$O, CO, CO$_2$, CH$_4$, HCN, and FeH molecular signals in the atmospheres of "},"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":"2606.27221","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2026-06-25T16:08:27Z","cross_cats_sorted":[],"title_canon_sha256":"76d718b508ac07be7900854e21e16c813c30646dec3ea6eab5258553c1098930","abstract_canon_sha256":"272f16685a5824c7bd8a72938ed8995a674fd21ca985709d1a1e40c3fb786efc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-26T01:16:15.454460Z","signature_b64":"rOt0IK16HZKCdp6YCnslzITYXWeeEGPacxzZbvbs9kRrHEvvE/M2zw46+KcE5iA/EhFRCkd80WW1tHm0qEBUAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"300afcd0b1e1140638affba214cfa7a300eb1d35acfdbecb752533b2ee5a931d","last_reissued_at":"2026-06-26T01:16:15.454046Z","signature_status":"signed_v1","first_computed_at":"2026-06-26T01:16:15.454046Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cross-correlation transmission spectroscopy of ultra-hot Jupiters WASP-189b, HAT-P-57b, KELT-17b, and KELT-21b with GIANO-B","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"E. Pall\\'e, Gareb Fern\\'andez-Rodr\\'iguez, H. Parviainen, I. Carleo, J. Orell-Miquel, M. Basilicata, M. Stangret, P. Giacobbe, P. Meni-Gallardo","submitted_at":"2026-06-25T16:08:27Z","abstract_excerpt":"Since the discovery of the first exoplanet, significant efforts have been made to characterise their atmospheres. Ultra-hot Jupiters (UHJs) are of particular interest due to their extended and hot atmospheres. Although previous studies have focused on the detection of atomic species at optical wavelengths, near-infrared (NIR) observations offer the potential to detect molecules. In our study, we applied the cross-correlation technique to NIR transmission spectra from \\giano. The analysis focuses on the search for H$_2$O, CO, CO$_2$, CH$_4$, HCN, and FeH molecular signals in the atmospheres of "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.27221","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/2606.27221/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":"2606.27221","created_at":"2026-06-26T01:16:15.454104+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.27221v1","created_at":"2026-06-26T01:16:15.454104+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.27221","created_at":"2026-06-26T01:16:15.454104+00:00"},{"alias_kind":"pith_short_12","alias_value":"GAFPZUFR4EKA","created_at":"2026-06-26T01:16:15.454104+00:00"},{"alias_kind":"pith_short_16","alias_value":"GAFPZUFR4EKAMOFP","created_at":"2026-06-26T01:16:15.454104+00:00"},{"alias_kind":"pith_short_8","alias_value":"GAFPZUFR","created_at":"2026-06-26T01:16:15.454104+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/GAFPZUFR4EKAMOFP7ORBJT5HUM","json":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM.json","graph_json":"https://pith.science/api/pith-number/GAFPZUFR4EKAMOFP7ORBJT5HUM/graph.json","events_json":"https://pith.science/api/pith-number/GAFPZUFR4EKAMOFP7ORBJT5HUM/events.json","paper":"https://pith.science/paper/GAFPZUFR"},"agent_actions":{"view_html":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM","download_json":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM.json","view_paper":"https://pith.science/paper/GAFPZUFR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.27221&json=true","fetch_graph":"https://pith.science/api/pith-number/GAFPZUFR4EKAMOFP7ORBJT5HUM/graph.json","fetch_events":"https://pith.science/api/pith-number/GAFPZUFR4EKAMOFP7ORBJT5HUM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM/action/storage_attestation","attest_author":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM/action/author_attestation","sign_citation":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM/action/citation_signature","submit_replication":"https://pith.science/pith/GAFPZUFR4EKAMOFP7ORBJT5HUM/action/replication_record"}},"created_at":"2026-06-26T01:16:15.454104+00:00","updated_at":"2026-06-26T01:16:15.454104+00:00"}