{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:Y7BLKJGSWRFYETA6JIUG3HPWPP","short_pith_number":"pith:Y7BLKJGS","schema_version":"1.0","canonical_sha256":"c7c2b524d2b44b824c1e4a286d9df67bfe68af315691045ddbd4df3369ec58e8","source":{"kind":"arxiv","id":"2502.00576","version":3},"attestation_state":"computed","paper":{"title":"A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Allyson Bieryla, Andrew W. Mann, Annabelle E. Niblett, Catherine A. Clark, Chelsea X. Huang, Colin Littlefield, Cristilyn N. Watkins, David W. Latham, Duncan Wright, George Zhou, Jack M. Nelson, James G. Rogers, Jessie L. Christiansen, Joachim Kr\\\"uger, Joshua N. Winn, Karen A. Collins, Keith Horne, Kevin I. Collins, Luke G. Bouma, Madyson G. Barber, Michelle Kunimoto, Ramotholo Sefako, Richard P. Schwarz, Samuel N. Quinn, Steve B. Howell, Sydney Vach, Tyler R. Fairnington, Zahra Essack","submitted_at":"2025-02-01T22:00:55Z","abstract_excerpt":"Measuring the properties of planets younger than about 50 Myr helps to test different planetary formation and evolution models. NASA's Transiting Exoplanet Survey Satellite (TESS) has observed nearly the entire sky, including a wide range of star-forming regions and young stellar clusters, expanding our census of the newborn planet population. In this work, we present the discovery of the TIC 88785435 planetary system located in the Upper-Centaurus Lupus (UCL) region of the Scorpius-Centaurus OB association (Sco-Cen) and a preliminary survey of the planet population within Sco-Cen. TIC 8878543"},"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":"2502.00576","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-02-01T22:00:55Z","cross_cats_sorted":[],"title_canon_sha256":"3367a2a2a0e45f4783b4cc1f06e291b05c3ad9c55b044ecb56b0582e2e65c754","abstract_canon_sha256":"aa4b6c2419a409f752915297d735bbe32d5f57de6ad25731489bc91967c45a96"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:23:23.008877Z","signature_b64":"PC4tNccbr8gPf98V0ZgOJH0kSzwfIYb5fl6lkIPlwdbLqDIEZCPva1B0vaz7wgbKfnjq5s5AivxFqNUAwpxOAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c7c2b524d2b44b824c1e4a286d9df67bfe68af315691045ddbd4df3369ec58e8","last_reissued_at":"2026-07-05T11:23:23.005638Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:23:23.005638Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Allyson Bieryla, Andrew W. Mann, Annabelle E. Niblett, Catherine A. Clark, Chelsea X. Huang, Colin Littlefield, Cristilyn N. Watkins, David W. Latham, Duncan Wright, George Zhou, Jack M. Nelson, James G. Rogers, Jessie L. Christiansen, Joachim Kr\\\"uger, Joshua N. Winn, Karen A. Collins, Keith Horne, Kevin I. Collins, Luke G. Bouma, Madyson G. Barber, Michelle Kunimoto, Ramotholo Sefako, Richard P. Schwarz, Samuel N. Quinn, Steve B. Howell, Sydney Vach, Tyler R. Fairnington, Zahra Essack","submitted_at":"2025-02-01T22:00:55Z","abstract_excerpt":"Measuring the properties of planets younger than about 50 Myr helps to test different planetary formation and evolution models. NASA's Transiting Exoplanet Survey Satellite (TESS) has observed nearly the entire sky, including a wide range of star-forming regions and young stellar clusters, expanding our census of the newborn planet population. In this work, we present the discovery of the TIC 88785435 planetary system located in the Upper-Centaurus Lupus (UCL) region of the Scorpius-Centaurus OB association (Sco-Cen) and a preliminary survey of the planet population within Sco-Cen. TIC 8878543"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.00576","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/2502.00576/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":"2502.00576","created_at":"2026-07-05T11:23:23.008328+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.00576v3","created_at":"2026-07-05T11:23:23.008328+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.00576","created_at":"2026-07-05T11:23:23.008328+00:00"},{"alias_kind":"pith_short_12","alias_value":"Y7BLKJGSWRFY","created_at":"2026-07-05T11:23:23.008328+00:00"},{"alias_kind":"pith_short_16","alias_value":"Y7BLKJGSWRFYETA6","created_at":"2026-07-05T11:23:23.008328+00:00"},{"alias_kind":"pith_short_8","alias_value":"Y7BLKJGS","created_at":"2026-07-05T11:23:23.008328+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09973","citing_title":"Stellar Obliquities of Young Systems, Atmospheres Undergoing Contraction and Escape (SOYSAUCE) II: a 135 Myr planet on an aligned orbit with transit timing variations","ref_index":224,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP","json":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP.json","graph_json":"https://pith.science/api/pith-number/Y7BLKJGSWRFYETA6JIUG3HPWPP/graph.json","events_json":"https://pith.science/api/pith-number/Y7BLKJGSWRFYETA6JIUG3HPWPP/events.json","paper":"https://pith.science/paper/Y7BLKJGS"},"agent_actions":{"view_html":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP","download_json":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP.json","view_paper":"https://pith.science/paper/Y7BLKJGS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.00576&json=true","fetch_graph":"https://pith.science/api/pith-number/Y7BLKJGSWRFYETA6JIUG3HPWPP/graph.json","fetch_events":"https://pith.science/api/pith-number/Y7BLKJGSWRFYETA6JIUG3HPWPP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP/action/storage_attestation","attest_author":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP/action/author_attestation","sign_citation":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP/action/citation_signature","submit_replication":"https://pith.science/pith/Y7BLKJGSWRFYETA6JIUG3HPWPP/action/replication_record"}},"created_at":"2026-07-05T11:23:23.008328+00:00","updated_at":"2026-07-05T11:23:23.008328+00:00"}