{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:4BZSAGM6FFKNNLVKCMSAZ5OMRE","short_pith_number":"pith:4BZSAGM6","canonical_record":{"source":{"id":"1803.10287","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-03-27T19:46:09Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"d27a007b7921fbd85a3e789635c4c4708000bc31cade18fdb713d0bcc9b71765","abstract_canon_sha256":"7e7c90f48de951bb6d9b74c584849b162e26a2f7199bd09eeed1323eecb04b3b"},"schema_version":"1.0"},"canonical_sha256":"e07320199e2954d6aeaa13240cf5cc891070e43bf69af11eb481567d40305285","source":{"kind":"arxiv","id":"1803.10287","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1803.10287","created_at":"2026-05-17T23:59:09Z"},{"alias_kind":"arxiv_version","alias_value":"1803.10287v2","created_at":"2026-05-17T23:59:09Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.10287","created_at":"2026-05-17T23:59:09Z"},{"alias_kind":"pith_short_12","alias_value":"4BZSAGM6FFKN","created_at":"2026-05-18T12:32:05Z"},{"alias_kind":"pith_short_16","alias_value":"4BZSAGM6FFKNNLVK","created_at":"2026-05-18T12:32:05Z"},{"alias_kind":"pith_short_8","alias_value":"4BZSAGM6","created_at":"2026-05-18T12:32:05Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:4BZSAGM6FFKNNLVKCMSAZ5OMRE","target":"record","payload":{"canonical_record":{"source":{"id":"1803.10287","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-03-27T19:46:09Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"d27a007b7921fbd85a3e789635c4c4708000bc31cade18fdb713d0bcc9b71765","abstract_canon_sha256":"7e7c90f48de951bb6d9b74c584849b162e26a2f7199bd09eeed1323eecb04b3b"},"schema_version":"1.0"},"canonical_sha256":"e07320199e2954d6aeaa13240cf5cc891070e43bf69af11eb481567d40305285","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:59:09.413380Z","signature_b64":"dirsAqaCwKecpi18Ljqb4ZPGXI7nO5KznVHFVi32VdGuiqmhaUEbOeDM9c3ijjPSjmLZAeoO+ggCekmS3lkpCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e07320199e2954d6aeaa13240cf5cc891070e43bf69af11eb481567d40305285","last_reissued_at":"2026-05-17T23:59:09.412899Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:59:09.412899Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1803.10287","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:59:09Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TYzZnpT7u/Jqo0pGYRYtYNk4V2xZGUH7cauxKPa4/XsDUuBZ4jPAI7HHjPHENF4L0jj2++GpTvF8DYpX1d/5Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-12T06:26:25.103138Z"},"content_sha256":"ac7141021413df7f7cc16e271e94789e01b0fb24aeed22907e9b8091e47620fb","schema_version":"1.0","event_id":"sha256:ac7141021413df7f7cc16e271e94789e01b0fb24aeed22907e9b8091e47620fb"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:4BZSAGM6FFKNNLVKCMSAZ5OMRE","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Ejection processes in the young open cluster NGC 2264. A study of the [OI]{\\lambda}6300 emission line","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"Catherine Dougados, J\\'er\\^ome Bouvier, Pauline McGinnis, Silvia H. P. Alencar, Sylvie Cabrit","submitted_at":"2018-03-27T19:46:09Z","abstract_excerpt":"We search for correlations between the [OI]6300 line, a well-known tracer of jets and winds in young stars, and stellar/disk/accretion properties in the young cluster NGC 2264, aiming to characterize the outflow phenomena that occur within the circumstellar environment. We analyzed FLAMES spectra of 184 stars, detecting the [OI]6300 line in 108 CTTSs and 2 Herbig AeBe stars. We identified the main features of this line: a high-velocity component (HVC), and a broad and narrow low-velocity components (BLVC and NLVC). We calculated their luminosities and kinematic properties, then compared with s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.10287","kind":"arxiv","version":2},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:59:09Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WoRIMKFGO258xpDaBsRcQfTwXie0qtv8cgKP70SWIcA5lp/5W/Ky1N4LHuVAfk+xPS1CcjvroEEvLTUupthaDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-12T06:26:25.103845Z"},"content_sha256":"5f71f5e884b114217bec6d64e6b7fd271f610dbd5ddb28792452e6a5b32bfca8","schema_version":"1.0","event_id":"sha256:5f71f5e884b114217bec6d64e6b7fd271f610dbd5ddb28792452e6a5b32bfca8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE/bundle.json","state_url":"https://pith.science/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-12T06:26:25Z","links":{"resolver":"https://pith.science/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE","bundle":"https://pith.science/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE/bundle.json","state":"https://pith.science/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/4BZSAGM6FFKNNLVKCMSAZ5OMRE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:4BZSAGM6FFKNNLVKCMSAZ5OMRE","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"7e7c90f48de951bb6d9b74c584849b162e26a2f7199bd09eeed1323eecb04b3b","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-03-27T19:46:09Z","title_canon_sha256":"d27a007b7921fbd85a3e789635c4c4708000bc31cade18fdb713d0bcc9b71765"},"schema_version":"1.0","source":{"id":"1803.10287","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1803.10287","created_at":"2026-05-17T23:59:09Z"},{"alias_kind":"arxiv_version","alias_value":"1803.10287v2","created_at":"2026-05-17T23:59:09Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1803.10287","created_at":"2026-05-17T23:59:09Z"},{"alias_kind":"pith_short_12","alias_value":"4BZSAGM6FFKN","created_at":"2026-05-18T12:32:05Z"},{"alias_kind":"pith_short_16","alias_value":"4BZSAGM6FFKNNLVK","created_at":"2026-05-18T12:32:05Z"},{"alias_kind":"pith_short_8","alias_value":"4BZSAGM6","created_at":"2026-05-18T12:32:05Z"}],"graph_snapshots":[{"event_id":"sha256:5f71f5e884b114217bec6d64e6b7fd271f610dbd5ddb28792452e6a5b32bfca8","target":"graph","created_at":"2026-05-17T23:59:09Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We search for correlations between the [OI]6300 line, a well-known tracer of jets and winds in young stars, and stellar/disk/accretion properties in the young cluster NGC 2264, aiming to characterize the outflow phenomena that occur within the circumstellar environment. We analyzed FLAMES spectra of 184 stars, detecting the [OI]6300 line in 108 CTTSs and 2 Herbig AeBe stars. We identified the main features of this line: a high-velocity component (HVC), and a broad and narrow low-velocity components (BLVC and NLVC). We calculated their luminosities and kinematic properties, then compared with s","authors_text":"Catherine Dougados, J\\'er\\^ome Bouvier, Pauline McGinnis, Silvia H. P. Alencar, Sylvie Cabrit","cross_cats":["astro-ph.GA"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-03-27T19:46:09Z","title":"Ejection processes in the young open cluster NGC 2264. A study of the [OI]{\\lambda}6300 emission line"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1803.10287","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:ac7141021413df7f7cc16e271e94789e01b0fb24aeed22907e9b8091e47620fb","target":"record","created_at":"2026-05-17T23:59:09Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"7e7c90f48de951bb6d9b74c584849b162e26a2f7199bd09eeed1323eecb04b3b","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-03-27T19:46:09Z","title_canon_sha256":"d27a007b7921fbd85a3e789635c4c4708000bc31cade18fdb713d0bcc9b71765"},"schema_version":"1.0","source":{"id":"1803.10287","kind":"arxiv","version":2}},"canonical_sha256":"e07320199e2954d6aeaa13240cf5cc891070e43bf69af11eb481567d40305285","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e07320199e2954d6aeaa13240cf5cc891070e43bf69af11eb481567d40305285","first_computed_at":"2026-05-17T23:59:09.412899Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:59:09.412899Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"dirsAqaCwKecpi18Ljqb4ZPGXI7nO5KznVHFVi32VdGuiqmhaUEbOeDM9c3ijjPSjmLZAeoO+ggCekmS3lkpCQ==","signature_status":"signed_v1","signed_at":"2026-05-17T23:59:09.413380Z","signed_message":"canonical_sha256_bytes"},"source_id":"1803.10287","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ac7141021413df7f7cc16e271e94789e01b0fb24aeed22907e9b8091e47620fb","sha256:5f71f5e884b114217bec6d64e6b7fd271f610dbd5ddb28792452e6a5b32bfca8"],"state_sha256":"9cc3117c1e43fcd600471f794975effa1bf624e1c272712a3c7506e146add203"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"4Q4dqYxogWsduvZNw9ikp/8Q5GcdxElv6eb4EvPR9UE/XkH6Al9fayNZGTYouRlsMSjfl8wa86J1qN5aUbFiBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-12T06:26:25.107500Z","bundle_sha256":"7fe1ffe917e3674cd357f47cfae10cacfce8cb0a29252d2f7bbb7cbc73514c5b"}}