{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:PULBYF72CTQDEPE37GBVQ3RIVZ","short_pith_number":"pith:PULBYF72","canonical_record":{"source":{"id":"1606.06281","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-20T19:59:56Z","cross_cats_sorted":[],"title_canon_sha256":"9c16b5d2de9d5fa51f201c137b24d3033b5ebec4dc78cd425c9d50873a380781","abstract_canon_sha256":"ab64132ff6dfbcb8b3962ea03c31f6de4bc8a002ab13055e8e7a296181885003"},"schema_version":"1.0"},"canonical_sha256":"7d161c17fa14e0323c9bf983586e28ae490ebc5c74758635814d7cb8902fb7e0","source":{"kind":"arxiv","id":"1606.06281","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1606.06281","created_at":"2026-05-18T01:03:49Z"},{"alias_kind":"arxiv_version","alias_value":"1606.06281v1","created_at":"2026-05-18T01:03:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.06281","created_at":"2026-05-18T01:03:49Z"},{"alias_kind":"pith_short_12","alias_value":"PULBYF72CTQD","created_at":"2026-05-18T12:30:39Z"},{"alias_kind":"pith_short_16","alias_value":"PULBYF72CTQDEPE3","created_at":"2026-05-18T12:30:39Z"},{"alias_kind":"pith_short_8","alias_value":"PULBYF72","created_at":"2026-05-18T12:30:39Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:PULBYF72CTQDEPE37GBVQ3RIVZ","target":"record","payload":{"canonical_record":{"source":{"id":"1606.06281","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-20T19:59:56Z","cross_cats_sorted":[],"title_canon_sha256":"9c16b5d2de9d5fa51f201c137b24d3033b5ebec4dc78cd425c9d50873a380781","abstract_canon_sha256":"ab64132ff6dfbcb8b3962ea03c31f6de4bc8a002ab13055e8e7a296181885003"},"schema_version":"1.0"},"canonical_sha256":"7d161c17fa14e0323c9bf983586e28ae490ebc5c74758635814d7cb8902fb7e0","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:49.370852Z","signature_b64":"1M78TyJOd5NwblGj6yD0KisxMw2qiHPKzpYkPKgZ7TuemL1dgSh+I0PE3jQ+g/3X+BJ0WAEOQcma0zzFq34mDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7d161c17fa14e0323c9bf983586e28ae490ebc5c74758635814d7cb8902fb7e0","last_reissued_at":"2026-05-18T01:03:49.370199Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:49.370199Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1606.06281","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:03:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"rtOldR99WKxdY0sxLnYYwcIJCsxYfZakKViCqvRXg+mHPwgr5UM/5eR3Nx+OuzzIR3SgSG074oVJ1l4v4s3xCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T20:02:34.032038Z"},"content_sha256":"496e1886afd717ad3473ad67a1f8893f6c97c7b537b7e54725e4cc328a520a4a","schema_version":"1.0","event_id":"sha256:496e1886afd717ad3473ad67a1f8893f6c97c7b537b7e54725e4cc328a520a4a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:PULBYF72CTQDEPE37GBVQ3RIVZ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Alexander Y. Wagner, Gary A. Mamon, Joakim Rosdahl, Joseph Silk, Rebekka Bieri, Yohan Dubois","submitted_at":"2016-06-20T19:59:56Z","abstract_excerpt":"The quasar mode of Active Galactic Nuclei (AGN) in the high-redshift Universe is routinely observed in gas-rich galaxies together with large-scale AGN-driven winds. It is crucial to understand how photons emitted by the central AGN source couple to the ambient interstellar-medium to trigger large-scale outflows. By means of radiation-hydrodynamical simulations of idealised galactic discs, we study the coupling of photons with the multiphase galactic gas, and how it varies with gas cloud sizes, and the radiation bands included in the simulations, which are ultraviolet (UV), optical, and infrare"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.06281","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:03:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"sr+dRZhfFPieM4onBNYAFuq36VHvA9cbBPlg5uTsOv2WYMR1SIcEhCjgKMcFEubkoVjev43Guh4IMbBWDuorCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T20:02:34.032811Z"},"content_sha256":"b85a66fbaa1b656bd10899e1946f2355755fd207759ddd2d1118f59ecc93ba56","schema_version":"1.0","event_id":"sha256:b85a66fbaa1b656bd10899e1946f2355755fd207759ddd2d1118f59ecc93ba56"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PULBYF72CTQDEPE37GBVQ3RIVZ/bundle.json","state_url":"https://pith.science/pith/PULBYF72CTQDEPE37GBVQ3RIVZ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PULBYF72CTQDEPE37GBVQ3RIVZ/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":"2026-06-05T20:02:34Z","links":{"resolver":"https://pith.science/pith/PULBYF72CTQDEPE37GBVQ3RIVZ","bundle":"https://pith.science/pith/PULBYF72CTQDEPE37GBVQ3RIVZ/bundle.json","state":"https://pith.science/pith/PULBYF72CTQDEPE37GBVQ3RIVZ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PULBYF72CTQDEPE37GBVQ3RIVZ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:PULBYF72CTQDEPE37GBVQ3RIVZ","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":"ab64132ff6dfbcb8b3962ea03c31f6de4bc8a002ab13055e8e7a296181885003","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-20T19:59:56Z","title_canon_sha256":"9c16b5d2de9d5fa51f201c137b24d3033b5ebec4dc78cd425c9d50873a380781"},"schema_version":"1.0","source":{"id":"1606.06281","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1606.06281","created_at":"2026-05-18T01:03:49Z"},{"alias_kind":"arxiv_version","alias_value":"1606.06281v1","created_at":"2026-05-18T01:03:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1606.06281","created_at":"2026-05-18T01:03:49Z"},{"alias_kind":"pith_short_12","alias_value":"PULBYF72CTQD","created_at":"2026-05-18T12:30:39Z"},{"alias_kind":"pith_short_16","alias_value":"PULBYF72CTQDEPE3","created_at":"2026-05-18T12:30:39Z"},{"alias_kind":"pith_short_8","alias_value":"PULBYF72","created_at":"2026-05-18T12:30:39Z"}],"graph_snapshots":[{"event_id":"sha256:b85a66fbaa1b656bd10899e1946f2355755fd207759ddd2d1118f59ecc93ba56","target":"graph","created_at":"2026-05-18T01:03:49Z","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":"The quasar mode of Active Galactic Nuclei (AGN) in the high-redshift Universe is routinely observed in gas-rich galaxies together with large-scale AGN-driven winds. It is crucial to understand how photons emitted by the central AGN source couple to the ambient interstellar-medium to trigger large-scale outflows. By means of radiation-hydrodynamical simulations of idealised galactic discs, we study the coupling of photons with the multiphase galactic gas, and how it varies with gas cloud sizes, and the radiation bands included in the simulations, which are ultraviolet (UV), optical, and infrare","authors_text":"Alexander Y. Wagner, Gary A. Mamon, Joakim Rosdahl, Joseph Silk, Rebekka Bieri, Yohan Dubois","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-20T19:59:56Z","title":"Outflows Driven by Quasars in High-Redshift Galaxies with Radiation Hydrodynamics"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.06281","kind":"arxiv","version":1},"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":"sha256:496e1886afd717ad3473ad67a1f8893f6c97c7b537b7e54725e4cc328a520a4a","target":"record","created_at":"2026-05-18T01:03:49Z","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":"ab64132ff6dfbcb8b3962ea03c31f6de4bc8a002ab13055e8e7a296181885003","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-06-20T19:59:56Z","title_canon_sha256":"9c16b5d2de9d5fa51f201c137b24d3033b5ebec4dc78cd425c9d50873a380781"},"schema_version":"1.0","source":{"id":"1606.06281","kind":"arxiv","version":1}},"canonical_sha256":"7d161c17fa14e0323c9bf983586e28ae490ebc5c74758635814d7cb8902fb7e0","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"7d161c17fa14e0323c9bf983586e28ae490ebc5c74758635814d7cb8902fb7e0","first_computed_at":"2026-05-18T01:03:49.370199Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:03:49.370199Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"1M78TyJOd5NwblGj6yD0KisxMw2qiHPKzpYkPKgZ7TuemL1dgSh+I0PE3jQ+g/3X+BJ0WAEOQcma0zzFq34mDA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:03:49.370852Z","signed_message":"canonical_sha256_bytes"},"source_id":"1606.06281","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:496e1886afd717ad3473ad67a1f8893f6c97c7b537b7e54725e4cc328a520a4a","sha256:b85a66fbaa1b656bd10899e1946f2355755fd207759ddd2d1118f59ecc93ba56"],"state_sha256":"ea5b238c6a51975d60047271440b4a7ee52a8445697802b5fa9b74cf8d395e95"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"bEEqN7sBVVM/Otr6ummqZX451soUl9cVjxJzRski/oH2WAI12Q/Bj5ekLm9kVshCBi2oCuscb0w1gLPC+0VcAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T20:02:34.037597Z","bundle_sha256":"82373a7544baceb7aec97537646e2a7f0d05a6b0d3773447ed3a0faf107e39a5"}}