{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:GIFVEZWLDCNKNJ3EDM3D4EUIP2","short_pith_number":"pith:GIFVEZWL","canonical_record":{"source":{"id":"1602.03181","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-09T21:00:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"700517f32d797d49077b5f5e6caa19f9b62c00a500700a18fc4924ee43170352","abstract_canon_sha256":"4635d6904c5d03debbba4f51dad6ada5992eaf0b2dd3526b5eae19cafb403914"},"schema_version":"1.0"},"canonical_sha256":"320b5266cb189aa6a7641b363e12887e8d7b58ad6165a1b3caf585c564943206","source":{"kind":"arxiv","id":"1602.03181","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1602.03181","created_at":"2026-05-18T01:18:29Z"},{"alias_kind":"arxiv_version","alias_value":"1602.03181v2","created_at":"2026-05-18T01:18:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.03181","created_at":"2026-05-18T01:18:29Z"},{"alias_kind":"pith_short_12","alias_value":"GIFVEZWLDCNK","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_16","alias_value":"GIFVEZWLDCNKNJ3E","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_8","alias_value":"GIFVEZWL","created_at":"2026-05-18T12:30:19Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:GIFVEZWLDCNKNJ3EDM3D4EUIP2","target":"record","payload":{"canonical_record":{"source":{"id":"1602.03181","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-09T21:00:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"700517f32d797d49077b5f5e6caa19f9b62c00a500700a18fc4924ee43170352","abstract_canon_sha256":"4635d6904c5d03debbba4f51dad6ada5992eaf0b2dd3526b5eae19cafb403914"},"schema_version":"1.0"},"canonical_sha256":"320b5266cb189aa6a7641b363e12887e8d7b58ad6165a1b3caf585c564943206","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:29.085965Z","signature_b64":"BPlqkpMcxW18h6shtvuobpAW96IILfctVJGlZAIF6cux+UJcraRE1qAnIgaPUqF0JIJYECT+5nYdomYMmIZDBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"320b5266cb189aa6a7641b363e12887e8d7b58ad6165a1b3caf585c564943206","last_reissued_at":"2026-05-18T01:18:29.085332Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:29.085332Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1602.03181","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":"2026-05-18T01:18:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dBs6s63qX25SPPB9pl+8LbPPlaR28oR+TnOSrfZw1OXewiNOUgHGaFeLMtmu+fFvQ1Reo1ugXRyhcgi/zxvFBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-21T09:44:09.342724Z"},"content_sha256":"8a7186ced3d356ebb63470082a07e78672ce1b57330842e4df87ae6f65f0f374","schema_version":"1.0","event_id":"sha256:8a7186ced3d356ebb63470082a07e78672ce1b57330842e4df87ae6f65f0f374"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:GIFVEZWLDCNKNJ3EDM3D4EUIP2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A fast ionised wind in a Star Forming-Quasar system at z~1.5 resolved through Adaptive Optics assisted near-infrared data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiorno, A. Comastri, A. Marconi, D. Kakkad, D. Rosario, F. Fiore, F. Lamareille, G. Cresci, G. Lanzuisi, G. Zamorani, I. Delvecchio, M. Brusa (DIFA & INAF-OABO), M. Mignoli, M. Perna, M. Schramm, S. Berta, T. Contini, V. Mainieri","submitted_at":"2016-02-09T21:00:02Z","abstract_excerpt":"Outflows are invoked in co-evolutionary models to link the growth of SMBH and galaxies through feedback phenomena, and from the analysis of both galaxies and Active Galactic Nuclei (AGN) samples at z$\\sim1-3$, it is becoming clear that powerful winds are quite common in AGN hosts. High-resolution and high S/N observations are needed in order to uncover the physical properties of the wind through kinematics analysis. We exploited VIMOS, SINFONI and Subaru/IRCS Adaptive Optics data to study the kinematics properties on the scale the host galaxy of XID5395, a luminous, X-ray obscured Starburst/Qu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.03181","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":"2026-05-18T01:18:29Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Kny5YyhFiddOUg3UkS+8QGlvkRP1C1MZKGpZ/s7jIpzjFjY811+rkfK3wGYNVREXQXcqFJgPziHMVeElthl0CQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-21T09:44:09.343084Z"},"content_sha256":"706ed95795bfced14fe8f9f99cc7e1627a178756d60f27ddf321c74e744122da","schema_version":"1.0","event_id":"sha256:706ed95795bfced14fe8f9f99cc7e1627a178756d60f27ddf321c74e744122da"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2/bundle.json","state_url":"https://pith.science/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2/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":"2026-05-21T09:44:09Z","links":{"resolver":"https://pith.science/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2","bundle":"https://pith.science/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2/bundle.json","state":"https://pith.science/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GIFVEZWLDCNKNJ3EDM3D4EUIP2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:GIFVEZWLDCNKNJ3EDM3D4EUIP2","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":"4635d6904c5d03debbba4f51dad6ada5992eaf0b2dd3526b5eae19cafb403914","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-09T21:00:02Z","title_canon_sha256":"700517f32d797d49077b5f5e6caa19f9b62c00a500700a18fc4924ee43170352"},"schema_version":"1.0","source":{"id":"1602.03181","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1602.03181","created_at":"2026-05-18T01:18:29Z"},{"alias_kind":"arxiv_version","alias_value":"1602.03181v2","created_at":"2026-05-18T01:18:29Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.03181","created_at":"2026-05-18T01:18:29Z"},{"alias_kind":"pith_short_12","alias_value":"GIFVEZWLDCNK","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_16","alias_value":"GIFVEZWLDCNKNJ3E","created_at":"2026-05-18T12:30:19Z"},{"alias_kind":"pith_short_8","alias_value":"GIFVEZWL","created_at":"2026-05-18T12:30:19Z"}],"graph_snapshots":[{"event_id":"sha256:706ed95795bfced14fe8f9f99cc7e1627a178756d60f27ddf321c74e744122da","target":"graph","created_at":"2026-05-18T01:18:29Z","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":"Outflows are invoked in co-evolutionary models to link the growth of SMBH and galaxies through feedback phenomena, and from the analysis of both galaxies and Active Galactic Nuclei (AGN) samples at z$\\sim1-3$, it is becoming clear that powerful winds are quite common in AGN hosts. High-resolution and high S/N observations are needed in order to uncover the physical properties of the wind through kinematics analysis. We exploited VIMOS, SINFONI and Subaru/IRCS Adaptive Optics data to study the kinematics properties on the scale the host galaxy of XID5395, a luminous, X-ray obscured Starburst/Qu","authors_text":"A. Bongiorno, A. Comastri, A. Marconi, D. Kakkad, D. Rosario, F. Fiore, F. Lamareille, G. Cresci, G. Lanzuisi, G. Zamorani, I. Delvecchio, M. Brusa (DIFA & INAF-OABO), M. Mignoli, M. Perna, M. Schramm, S. Berta, T. Contini, V. Mainieri","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-09T21:00:02Z","title":"A fast ionised wind in a Star Forming-Quasar system at z~1.5 resolved through Adaptive Optics assisted near-infrared data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.03181","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":"sha256:8a7186ced3d356ebb63470082a07e78672ce1b57330842e4df87ae6f65f0f374","target":"record","created_at":"2026-05-18T01:18:29Z","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":"4635d6904c5d03debbba4f51dad6ada5992eaf0b2dd3526b5eae19cafb403914","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-02-09T21:00:02Z","title_canon_sha256":"700517f32d797d49077b5f5e6caa19f9b62c00a500700a18fc4924ee43170352"},"schema_version":"1.0","source":{"id":"1602.03181","kind":"arxiv","version":2}},"canonical_sha256":"320b5266cb189aa6a7641b363e12887e8d7b58ad6165a1b3caf585c564943206","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"320b5266cb189aa6a7641b363e12887e8d7b58ad6165a1b3caf585c564943206","first_computed_at":"2026-05-18T01:18:29.085332Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:18:29.085332Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"BPlqkpMcxW18h6shtvuobpAW96IILfctVJGlZAIF6cux+UJcraRE1qAnIgaPUqF0JIJYECT+5nYdomYMmIZDBg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:18:29.085965Z","signed_message":"canonical_sha256_bytes"},"source_id":"1602.03181","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8a7186ced3d356ebb63470082a07e78672ce1b57330842e4df87ae6f65f0f374","sha256:706ed95795bfced14fe8f9f99cc7e1627a178756d60f27ddf321c74e744122da"],"state_sha256":"550794a03c18ff3c8f42778a98c3a60d0caf596d66433c24eab9ffe2d1c58e00"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"k1HkhFuoK4CHFjt7j+MmP6g+F7bIcvo+4NmCpKjs4RmGnvi7PqxVbf/P2rB47Pl2OWc/boMGsOKR8KxsA62eBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-21T09:44:09.346055Z","bundle_sha256":"ff1a9b4624de77b89e75c8e7bda7c3799fe76aa5e83c84219980a4ea65f2a528"}}