{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:WVOZ7RHARWQWYMN7OS7RJWEEHY","short_pith_number":"pith:WVOZ7RHA","canonical_record":{"source":{"id":"1008.3728","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-22T23:06:28Z","cross_cats_sorted":[],"title_canon_sha256":"af687c2fcee6f3cdf72ce491f2fa066cf850ffac2ce2c6cc97bff20dcf512e1b","abstract_canon_sha256":"f77831dfd795643a6f6eda83d88698359148fb8b8f32435e70f2a0912b7650ba"},"schema_version":"1.0"},"canonical_sha256":"b55d9fc4e08da16c31bf74bf14d8843e3ce5c49842dfd9e09c034519afbd2bc3","source":{"kind":"arxiv","id":"1008.3728","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1008.3728","created_at":"2026-05-18T02:05:43Z"},{"alias_kind":"arxiv_version","alias_value":"1008.3728v2","created_at":"2026-05-18T02:05:43Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.3728","created_at":"2026-05-18T02:05:43Z"},{"alias_kind":"pith_short_12","alias_value":"WVOZ7RHARWQW","created_at":"2026-05-18T12:26:17Z"},{"alias_kind":"pith_short_16","alias_value":"WVOZ7RHARWQWYMN7","created_at":"2026-05-18T12:26:17Z"},{"alias_kind":"pith_short_8","alias_value":"WVOZ7RHA","created_at":"2026-05-18T12:26:17Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:WVOZ7RHARWQWYMN7OS7RJWEEHY","target":"record","payload":{"canonical_record":{"source":{"id":"1008.3728","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-22T23:06:28Z","cross_cats_sorted":[],"title_canon_sha256":"af687c2fcee6f3cdf72ce491f2fa066cf850ffac2ce2c6cc97bff20dcf512e1b","abstract_canon_sha256":"f77831dfd795643a6f6eda83d88698359148fb8b8f32435e70f2a0912b7650ba"},"schema_version":"1.0"},"canonical_sha256":"b55d9fc4e08da16c31bf74bf14d8843e3ce5c49842dfd9e09c034519afbd2bc3","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:43.954991Z","signature_b64":"F9qee1P7/8zDzM+8DdWi1wKgxE1G+dJo0khP69ms5JosbMduO1EWFkrJZe6WSdGSPIj++zDvKz5Ymy2YQKTkAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b55d9fc4e08da16c31bf74bf14d8843e3ce5c49842dfd9e09c034519afbd2bc3","last_reissued_at":"2026-05-18T02:05:43.954253Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:43.954253Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1008.3728","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":"2026-05-18T02:05:43Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EPxEwxFCGBAaJqa6+PFNJxkegDjBMzWSS6M1zlJyH8nY7HT1FI3pydJEwb6mfgIawfKbmYFtP0dvbJR6tVC8Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T20:07:45.583351Z"},"content_sha256":"8958032febad5cca47bc4f753d1c4d6fa073735ac984a33ac81e33d87afe23cf","schema_version":"1.0","event_id":"sha256:8958032febad5cca47bc4f753d1c4d6fa073735ac984a33ac81e33d87afe23cf"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:WVOZ7RHARWQWYMN7OS7RJWEEHY","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A High-Velocity Narrow Absorption Line Outflow in the Quasar J212329.46-005052.9","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. L. Malec, F. Hamann, J. X. Prochaska, M. T. Murphy, N. Kanekar, N. Milutinovic, S. Ellison, W. Ubachs","submitted_at":"2010-08-22T23:06:28Z","abstract_excerpt":"We report on a variable high-velocity narrow absorption line outflow in the redshift 2.3 quasar J2123-0050. Five distinct outflow systems are detected with velocity shifts from -9710 to -14,050 km/s and CIV 1548,1551 line widths of FWHM = 62-164 km/s. These data require five distinct outflow structures with similar kinematics, physical conditions and characteristic sizes of order 0.01-0.02 pc. The most likely location is ~5 pc from the quasar. The coordinated line variations in <0.63 yr (rest) are best explained by global changes in the outflow ionization caused by changes in the quasar's ioni"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.3728","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":"2026-05-18T02:05:43Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5ke0s47KbpfSCNecb+YCAnlGb2u9QPFpxlJYqCMTjfD1NA9QXfgzxi4d3oA3MxoU43AQ7GzvmxTHeNHtHOkNCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T20:07:45.584119Z"},"content_sha256":"7bf6b1617b6b5bf344fd417c140876314bd44d867621f60be49bde308adc7946","schema_version":"1.0","event_id":"sha256:7bf6b1617b6b5bf344fd417c140876314bd44d867621f60be49bde308adc7946"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY/bundle.json","state_url":"https://pith.science/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY/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":"2026-05-31T20:07:45Z","links":{"resolver":"https://pith.science/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY","bundle":"https://pith.science/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY/bundle.json","state":"https://pith.science/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY/state.json","well_known_bundle":"https://pith.science/.well-known/pith/WVOZ7RHARWQWYMN7OS7RJWEEHY/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:WVOZ7RHARWQWYMN7OS7RJWEEHY","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":"f77831dfd795643a6f6eda83d88698359148fb8b8f32435e70f2a0912b7650ba","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-22T23:06:28Z","title_canon_sha256":"af687c2fcee6f3cdf72ce491f2fa066cf850ffac2ce2c6cc97bff20dcf512e1b"},"schema_version":"1.0","source":{"id":"1008.3728","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1008.3728","created_at":"2026-05-18T02:05:43Z"},{"alias_kind":"arxiv_version","alias_value":"1008.3728v2","created_at":"2026-05-18T02:05:43Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.3728","created_at":"2026-05-18T02:05:43Z"},{"alias_kind":"pith_short_12","alias_value":"WVOZ7RHARWQW","created_at":"2026-05-18T12:26:17Z"},{"alias_kind":"pith_short_16","alias_value":"WVOZ7RHARWQWYMN7","created_at":"2026-05-18T12:26:17Z"},{"alias_kind":"pith_short_8","alias_value":"WVOZ7RHA","created_at":"2026-05-18T12:26:17Z"}],"graph_snapshots":[{"event_id":"sha256:7bf6b1617b6b5bf344fd417c140876314bd44d867621f60be49bde308adc7946","target":"graph","created_at":"2026-05-18T02:05:43Z","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 report on a variable high-velocity narrow absorption line outflow in the redshift 2.3 quasar J2123-0050. Five distinct outflow systems are detected with velocity shifts from -9710 to -14,050 km/s and CIV 1548,1551 line widths of FWHM = 62-164 km/s. These data require five distinct outflow structures with similar kinematics, physical conditions and characteristic sizes of order 0.01-0.02 pc. The most likely location is ~5 pc from the quasar. The coordinated line variations in <0.63 yr (rest) are best explained by global changes in the outflow ionization caused by changes in the quasar's ioni","authors_text":"A. L. Malec, F. Hamann, J. X. Prochaska, M. T. Murphy, N. Kanekar, N. Milutinovic, S. Ellison, W. Ubachs","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-22T23:06:28Z","title":"A High-Velocity Narrow Absorption Line Outflow in the Quasar J212329.46-005052.9"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.3728","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":"sha256:8958032febad5cca47bc4f753d1c4d6fa073735ac984a33ac81e33d87afe23cf","target":"record","created_at":"2026-05-18T02:05:43Z","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":"f77831dfd795643a6f6eda83d88698359148fb8b8f32435e70f2a0912b7650ba","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-08-22T23:06:28Z","title_canon_sha256":"af687c2fcee6f3cdf72ce491f2fa066cf850ffac2ce2c6cc97bff20dcf512e1b"},"schema_version":"1.0","source":{"id":"1008.3728","kind":"arxiv","version":2}},"canonical_sha256":"b55d9fc4e08da16c31bf74bf14d8843e3ce5c49842dfd9e09c034519afbd2bc3","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"b55d9fc4e08da16c31bf74bf14d8843e3ce5c49842dfd9e09c034519afbd2bc3","first_computed_at":"2026-05-18T02:05:43.954253Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:05:43.954253Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"F9qee1P7/8zDzM+8DdWi1wKgxE1G+dJo0khP69ms5JosbMduO1EWFkrJZe6WSdGSPIj++zDvKz5Ymy2YQKTkAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:05:43.954991Z","signed_message":"canonical_sha256_bytes"},"source_id":"1008.3728","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8958032febad5cca47bc4f753d1c4d6fa073735ac984a33ac81e33d87afe23cf","sha256:7bf6b1617b6b5bf344fd417c140876314bd44d867621f60be49bde308adc7946"],"state_sha256":"009526bfcc176cf8664f37b8b3b99275343ffebd3131b33ebe90d131e0148762"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Y2rR//DprBAIn2dCmUi2rO5toPBJH3xuZr7RrcQn979GzH/Fn330QPMkHaCn/tKKW4lVq8WrYpEfeJvtyajNCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T20:07:45.587955Z","bundle_sha256":"84e5eab3e4ff5da42ee360df0d02a6746f4f1212479b1c7add82927d3dba93a9"}}