{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:MMMOZBEI6XFRALUO53WW33GCYL","short_pith_number":"pith:MMMOZBEI","schema_version":"1.0","canonical_sha256":"6318ec8488f5cb102e8eeeed6decc2c2f388d809f8cd3f57bfc502938ba2b205","source":{"kind":"arxiv","id":"0811.3903","version":3},"attestation_state":"computed","paper":{"title":"Evidence for Warped Disks of Young Stars in the Galactic Center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Sternberg, D. Rouan, F. Eisenhauer, F. Martins, G. Perrin, H. Bartko, H. B. Perets, K. Dodds-Eden, L. Mascetti, M. J. Reid, O. Gerhard, O. Pfuhl, R. Genzel, S. Gillessen, S. Nayakshin, S. Trippe, T. Alexander, T. K. Fritz, T. Ott, T. Paumard, Y. Levin","submitted_at":"2008-11-24T16:01:44Z","abstract_excerpt":"The central parsec around the super-massive black hole in the Galactic Center hosts more than 100 young and massive stars. Outside the central cusp (R~1\") the majority of these O and Wolf-Rayet (WR) stars reside in a main clockwise system, plus a second, less prominent disk or streamer system at large angles with respect to the main system. Here we present the results from new observations of the Galactic Center with the AO-assisted near-infrared imager NACO and the integral field spectrograph SINFONI on the ESO/VLT. These include the detection of 27 new reliably measured WR/O stars in the cen"},"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":"0811.3903","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-11-24T16:01:44Z","cross_cats_sorted":[],"title_canon_sha256":"65b6a690d35fa70226df4e5e714432588afa25230a2edb880992f9ab24ebd534","abstract_canon_sha256":"ce89b9ec00fc8d7bfd927e58b928baf4addea781ff6750c6652dd10478c4e0e5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:35:13.782045Z","signature_b64":"yY15CNDjNArp/nHsrzU31PH4uOh10NBSuR+GlYDR6nNV0MJM5QO6G1mXU2tNs1y6TNe2zzRlwicEWeO5U4fECg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6318ec8488f5cb102e8eeeed6decc2c2f388d809f8cd3f57bfc502938ba2b205","last_reissued_at":"2026-05-18T02:35:13.781660Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:35:13.781660Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evidence for Warped Disks of Young Stars in the Galactic Center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Sternberg, D. Rouan, F. Eisenhauer, F. Martins, G. Perrin, H. Bartko, H. B. Perets, K. Dodds-Eden, L. Mascetti, M. J. Reid, O. Gerhard, O. Pfuhl, R. Genzel, S. Gillessen, S. Nayakshin, S. Trippe, T. Alexander, T. K. Fritz, T. Ott, T. Paumard, Y. Levin","submitted_at":"2008-11-24T16:01:44Z","abstract_excerpt":"The central parsec around the super-massive black hole in the Galactic Center hosts more than 100 young and massive stars. Outside the central cusp (R~1\") the majority of these O and Wolf-Rayet (WR) stars reside in a main clockwise system, plus a second, less prominent disk or streamer system at large angles with respect to the main system. Here we present the results from new observations of the Galactic Center with the AO-assisted near-infrared imager NACO and the integral field spectrograph SINFONI on the ESO/VLT. These include the detection of 27 new reliably measured WR/O stars in the cen"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0811.3903","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":""},"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":"0811.3903","created_at":"2026-05-18T02:35:13.781721+00:00"},{"alias_kind":"arxiv_version","alias_value":"0811.3903v3","created_at":"2026-05-18T02:35:13.781721+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0811.3903","created_at":"2026-05-18T02:35:13.781721+00:00"},{"alias_kind":"pith_short_12","alias_value":"MMMOZBEI6XFR","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"MMMOZBEI6XFRALUO","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"MMMOZBEI","created_at":"2026-05-18T12:25:57.157939+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/MMMOZBEI6XFRALUO53WW33GCYL","json":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL.json","graph_json":"https://pith.science/api/pith-number/MMMOZBEI6XFRALUO53WW33GCYL/graph.json","events_json":"https://pith.science/api/pith-number/MMMOZBEI6XFRALUO53WW33GCYL/events.json","paper":"https://pith.science/paper/MMMOZBEI"},"agent_actions":{"view_html":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL","download_json":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL.json","view_paper":"https://pith.science/paper/MMMOZBEI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0811.3903&json=true","fetch_graph":"https://pith.science/api/pith-number/MMMOZBEI6XFRALUO53WW33GCYL/graph.json","fetch_events":"https://pith.science/api/pith-number/MMMOZBEI6XFRALUO53WW33GCYL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL/action/storage_attestation","attest_author":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL/action/author_attestation","sign_citation":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL/action/citation_signature","submit_replication":"https://pith.science/pith/MMMOZBEI6XFRALUO53WW33GCYL/action/replication_record"}},"created_at":"2026-05-18T02:35:13.781721+00:00","updated_at":"2026-05-18T02:35:13.781721+00:00"}