{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:XFMMEYZB3MCK4E23LL2VYHALHZ","short_pith_number":"pith:XFMMEYZB","schema_version":"1.0","canonical_sha256":"b958c26321db04ae135b5af55c1c0b3e42635f5e84280793f8bfa27c235ba59f","source":{"kind":"arxiv","id":"1309.5098","version":1},"attestation_state":"computed","paper":{"title":"Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modeling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andres Carmona, Benjamin Montesinos, Carlos Eiroa, Christophe Pinte, Claire Martin-Za\\\"idi, David Ardila, Eric Pantin, Francois Menard, Giambattista Aresu, Glenn White, Goran Sandell, Gwendolyn Meeus, Ignacio Mendigutia, Inga Kamp, Jean-Charles Augereau, Jeremy Lebreton, Marco Spaans, Pablo Riviere-Marichalar, Peter Woitke, Rowin Meijerink, Sean Brittain, Williams Dent, Wing-Fai Thi","submitted_at":"2013-09-19T20:46:29Z","abstract_excerpt":"At the distance of 99-116 pc, HD141569A is one of the nearest HerbigAe stars that is surrounded by a tenuous disk, probably in transition between a massive primordial disk and a debris disk. We observed the fine-structure lines of OI at 63 and 145 micron and the CII line at 157 micron with the PACS instrument onboard the Herschel Space Telescope as part of the open-time large programme GASPS. We complemented the atomic line observations with archival Spitzer spectroscopic and photometric continuum data, a ground-based VLT-VISIR image at 8.6 micron, and 12CO fundamental ro-vibrational and pure "},"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":"1309.5098","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-09-19T20:46:29Z","cross_cats_sorted":[],"title_canon_sha256":"2ba05382ff60a435bde53200d495285aaba5fde7acd3a2fb261b3a55e8583b4d","abstract_canon_sha256":"9eb7a8f1f082a9846a006fb796f19a53e8e8e583e5e0980e073eeb826bcec8cb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:35.308825Z","signature_b64":"KJkBeATmhJkomdjYSRwlGqOJLqPEPgh8ugq4BrpoDwxRn47+uvcNKhwG81Ww4tIQNTnVPys6I5z6j7jV17L1Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b958c26321db04ae135b5af55c1c0b3e42635f5e84280793f8bfa27c235ba59f","last_reissued_at":"2026-05-18T01:47:35.308275Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:35.308275Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modeling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andres Carmona, Benjamin Montesinos, Carlos Eiroa, Christophe Pinte, Claire Martin-Za\\\"idi, David Ardila, Eric Pantin, Francois Menard, Giambattista Aresu, Glenn White, Goran Sandell, Gwendolyn Meeus, Ignacio Mendigutia, Inga Kamp, Jean-Charles Augereau, Jeremy Lebreton, Marco Spaans, Pablo Riviere-Marichalar, Peter Woitke, Rowin Meijerink, Sean Brittain, Williams Dent, Wing-Fai Thi","submitted_at":"2013-09-19T20:46:29Z","abstract_excerpt":"At the distance of 99-116 pc, HD141569A is one of the nearest HerbigAe stars that is surrounded by a tenuous disk, probably in transition between a massive primordial disk and a debris disk. We observed the fine-structure lines of OI at 63 and 145 micron and the CII line at 157 micron with the PACS instrument onboard the Herschel Space Telescope as part of the open-time large programme GASPS. We complemented the atomic line observations with archival Spitzer spectroscopic and photometric continuum data, a ground-based VLT-VISIR image at 8.6 micron, and 12CO fundamental ro-vibrational and pure "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.5098","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":"1309.5098","created_at":"2026-05-18T01:47:35.308358+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.5098v1","created_at":"2026-05-18T01:47:35.308358+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.5098","created_at":"2026-05-18T01:47:35.308358+00:00"},{"alias_kind":"pith_short_12","alias_value":"XFMMEYZB3MCK","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_16","alias_value":"XFMMEYZB3MCK4E23","created_at":"2026-05-18T12:28:06.772260+00:00"},{"alias_kind":"pith_short_8","alias_value":"XFMMEYZB","created_at":"2026-05-18T12:28:06.772260+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/XFMMEYZB3MCK4E23LL2VYHALHZ","json":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ.json","graph_json":"https://pith.science/api/pith-number/XFMMEYZB3MCK4E23LL2VYHALHZ/graph.json","events_json":"https://pith.science/api/pith-number/XFMMEYZB3MCK4E23LL2VYHALHZ/events.json","paper":"https://pith.science/paper/XFMMEYZB"},"agent_actions":{"view_html":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ","download_json":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ.json","view_paper":"https://pith.science/paper/XFMMEYZB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.5098&json=true","fetch_graph":"https://pith.science/api/pith-number/XFMMEYZB3MCK4E23LL2VYHALHZ/graph.json","fetch_events":"https://pith.science/api/pith-number/XFMMEYZB3MCK4E23LL2VYHALHZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ/action/storage_attestation","attest_author":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ/action/author_attestation","sign_citation":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ/action/citation_signature","submit_replication":"https://pith.science/pith/XFMMEYZB3MCK4E23LL2VYHALHZ/action/replication_record"}},"created_at":"2026-05-18T01:47:35.308358+00:00","updated_at":"2026-05-18T01:47:35.308358+00:00"}