{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:5XPB2JZYJER4KTZMNEVEAVHHLW","short_pith_number":"pith:5XPB2JZY","schema_version":"1.0","canonical_sha256":"edde1d27384923c54f2c692a4054e75d9b9cea89d616cfa0b4e64b76eaf75c9a","source":{"kind":"arxiv","id":"1203.6271","version":1},"attestation_state":"computed","paper":{"title":"Circumstellar disks and planets. Science cases for next-generation optical/infrared long-baseline interferometers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Anne Dutrey, Christophe Mordasini, Eric Pantin, Eric Tatulli, Fabien Malbet, Frederic Pont, Gaspard Duchene, Jean-Philippe Berger, Joerg-Uwe Pott, Leonardo Testi, Michelle Creech-Eakman, Richard Alexander, Sebastian Wolf","submitted_at":"2012-03-28T14:01:56Z","abstract_excerpt":"We present a review of the interplay between the evolution of circumstellar disks and the formation of planets, both from the perspective of theoretical models and dedicated observations. Based on this, we identify and discuss fundamental questions concerning the formation and evolution of circumstellar disks and planets which can be addressed in the near future with optical and infrared long-baseline interferometers. Furthermore, the importance of complementary observations with long-baseline (sub)millimeter interferometers and high-sensitivity infrared observatories is outlined."},"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":"1203.6271","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2012-03-28T14:01:56Z","cross_cats_sorted":["astro-ph.EP","astro-ph.SR"],"title_canon_sha256":"6c971071615080f6b52f24cd26fca0c0354899569757b100e2d8b5a6eba33ebf","abstract_canon_sha256":"a35b3141fad0373a5cd83f47895dee3e1854fd4396fb7296f8ce5058f1cf4c6e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:59:03.769378Z","signature_b64":"GwgTe/+HvM51mVodZKgQ5NtIv7T68NpGgS1S4f5J7k4CcoChfaW5sd8EXE3+43M0qUqPzocYI2Qh3JBjRFCWCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"edde1d27384923c54f2c692a4054e75d9b9cea89d616cfa0b4e64b76eaf75c9a","last_reissued_at":"2026-05-18T03:59:03.768669Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:59:03.768669Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Circumstellar disks and planets. Science cases for next-generation optical/infrared long-baseline interferometers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.SR"],"primary_cat":"astro-ph.IM","authors_text":"Anne Dutrey, Christophe Mordasini, Eric Pantin, Eric Tatulli, Fabien Malbet, Frederic Pont, Gaspard Duchene, Jean-Philippe Berger, Joerg-Uwe Pott, Leonardo Testi, Michelle Creech-Eakman, Richard Alexander, Sebastian Wolf","submitted_at":"2012-03-28T14:01:56Z","abstract_excerpt":"We present a review of the interplay between the evolution of circumstellar disks and the formation of planets, both from the perspective of theoretical models and dedicated observations. Based on this, we identify and discuss fundamental questions concerning the formation and evolution of circumstellar disks and planets which can be addressed in the near future with optical and infrared long-baseline interferometers. Furthermore, the importance of complementary observations with long-baseline (sub)millimeter interferometers and high-sensitivity infrared observatories is outlined."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.6271","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":""},"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":"1203.6271","created_at":"2026-05-18T03:59:03.768778+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.6271v1","created_at":"2026-05-18T03:59:03.768778+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.6271","created_at":"2026-05-18T03:59:03.768778+00:00"},{"alias_kind":"pith_short_12","alias_value":"5XPB2JZYJER4","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"5XPB2JZYJER4KTZM","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"5XPB2JZY","created_at":"2026-05-18T12:26:56.085431+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/5XPB2JZYJER4KTZMNEVEAVHHLW","json":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW.json","graph_json":"https://pith.science/api/pith-number/5XPB2JZYJER4KTZMNEVEAVHHLW/graph.json","events_json":"https://pith.science/api/pith-number/5XPB2JZYJER4KTZMNEVEAVHHLW/events.json","paper":"https://pith.science/paper/5XPB2JZY"},"agent_actions":{"view_html":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW","download_json":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW.json","view_paper":"https://pith.science/paper/5XPB2JZY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.6271&json=true","fetch_graph":"https://pith.science/api/pith-number/5XPB2JZYJER4KTZMNEVEAVHHLW/graph.json","fetch_events":"https://pith.science/api/pith-number/5XPB2JZYJER4KTZMNEVEAVHHLW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW/action/storage_attestation","attest_author":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW/action/author_attestation","sign_citation":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW/action/citation_signature","submit_replication":"https://pith.science/pith/5XPB2JZYJER4KTZMNEVEAVHHLW/action/replication_record"}},"created_at":"2026-05-18T03:59:03.768778+00:00","updated_at":"2026-05-18T03:59:03.768778+00:00"}