{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:A42OCBF6FCU6EAKO4QOXT5RD2I","short_pith_number":"pith:A42OCBF6","schema_version":"1.0","canonical_sha256":"0734e104be28a9e2014ee41d79f623d2081662bba2c324db3a80d9a33eff7ba6","source":{"kind":"arxiv","id":"2104.12414","version":1},"attestation_state":"computed","paper":{"title":"The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic ormolecular absorptions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bello-Arufe, A. Harutyunyan, A. S. Bonomo, A. Sozzetti, B. C. Addison, D. A. Fischer, D. Sicilia, E. Pall\\'e, F. Borsa, F. Yan, G. Nowak, H. Parviainen, J. M. Mendon\\c{c}a, J. Orell-Miquel, L. A. Buchhave, L. Malavolta, M. Cecconi, M. Oshagh, M. Stangret, N. Casasayas-Barris, R. Luque, R. Tronsgaard, S.H. C. Cabot, V. Nascimbeni","submitted_at":"2021-04-26T09:13:07Z","abstract_excerpt":"Ultra-hot Jupiters are defined as giant planets with equilibrium temperatures larger than 2000 K. Most of them are found orbiting bright A-F type stars, making them extremely suitable objects to study their atmospheres using high-resolution spectroscopy. Recent studies show a variety of atoms and molecules detected in the atmospheres of this type of planets. Here we present our analysis of the newly discovered ultra-hot Jupiter TOI-1431b/MASCARA-5b, using two transit observations with the HARPS-N spectrograph and one transit observation with the EXPRES spectrograph. Analysis of the Rossiter-Mc"},"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":"2104.12414","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2021-04-26T09:13:07Z","cross_cats_sorted":[],"title_canon_sha256":"288fe136afaa4568ba5bc7d7c6e069d5a7ee0bcee395e809076906f7c8298daa","abstract_canon_sha256":"e1041e35e1034eda3743e04a56ffc7a948c0efd55aaf1f89a32a466e26413c49"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:21:47.458110Z","signature_b64":"BXSbSrk+1PvJ1GFt+JXTxzr0CuPwNITeUgqKn1GdNKW0JdUSA38cWariBiSVHMYQeh7ARpAffgcI2DHcsWVxDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0734e104be28a9e2014ee41d79f623d2081662bba2c324db3a80d9a33eff7ba6","last_reissued_at":"2026-07-05T03:21:47.457645Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:21:47.457645Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic ormolecular absorptions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Bello-Arufe, A. Harutyunyan, A. S. Bonomo, A. Sozzetti, B. C. Addison, D. A. Fischer, D. Sicilia, E. Pall\\'e, F. Borsa, F. Yan, G. Nowak, H. Parviainen, J. M. Mendon\\c{c}a, J. Orell-Miquel, L. A. Buchhave, L. Malavolta, M. Cecconi, M. Oshagh, M. Stangret, N. Casasayas-Barris, R. Luque, R. Tronsgaard, S.H. C. Cabot, V. Nascimbeni","submitted_at":"2021-04-26T09:13:07Z","abstract_excerpt":"Ultra-hot Jupiters are defined as giant planets with equilibrium temperatures larger than 2000 K. Most of them are found orbiting bright A-F type stars, making them extremely suitable objects to study their atmospheres using high-resolution spectroscopy. Recent studies show a variety of atoms and molecules detected in the atmospheres of this type of planets. Here we present our analysis of the newly discovered ultra-hot Jupiter TOI-1431b/MASCARA-5b, using two transit observations with the HARPS-N spectrograph and one transit observation with the EXPRES spectrograph. Analysis of the Rossiter-Mc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2104.12414","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/2104.12414/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":"2104.12414","created_at":"2026-07-05T03:21:47.457703+00:00"},{"alias_kind":"arxiv_version","alias_value":"2104.12414v1","created_at":"2026-07-05T03:21:47.457703+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2104.12414","created_at":"2026-07-05T03:21:47.457703+00:00"},{"alias_kind":"pith_short_12","alias_value":"A42OCBF6FCU6","created_at":"2026-07-05T03:21:47.457703+00:00"},{"alias_kind":"pith_short_16","alias_value":"A42OCBF6FCU6EAKO","created_at":"2026-07-05T03:21:47.457703+00:00"},{"alias_kind":"pith_short_8","alias_value":"A42OCBF6","created_at":"2026-07-05T03:21:47.457703+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/A42OCBF6FCU6EAKO4QOXT5RD2I","json":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I.json","graph_json":"https://pith.science/api/pith-number/A42OCBF6FCU6EAKO4QOXT5RD2I/graph.json","events_json":"https://pith.science/api/pith-number/A42OCBF6FCU6EAKO4QOXT5RD2I/events.json","paper":"https://pith.science/paper/A42OCBF6"},"agent_actions":{"view_html":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I","download_json":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I.json","view_paper":"https://pith.science/paper/A42OCBF6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2104.12414&json=true","fetch_graph":"https://pith.science/api/pith-number/A42OCBF6FCU6EAKO4QOXT5RD2I/graph.json","fetch_events":"https://pith.science/api/pith-number/A42OCBF6FCU6EAKO4QOXT5RD2I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I/action/storage_attestation","attest_author":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I/action/author_attestation","sign_citation":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I/action/citation_signature","submit_replication":"https://pith.science/pith/A42OCBF6FCU6EAKO4QOXT5RD2I/action/replication_record"}},"created_at":"2026-07-05T03:21:47.457703+00:00","updated_at":"2026-07-05T03:21:47.457703+00:00"}