{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:XGTJKBR4R3HCRSEHJVKHQFY26P","short_pith_number":"pith:XGTJKBR4","canonical_record":{"source":{"id":"1512.05595","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-12-17T14:26:51Z","cross_cats_sorted":[],"title_canon_sha256":"c6e7ac8148ab79c44786c6d0ee9382b05254832033305f7d3ff1ea4605e0f403","abstract_canon_sha256":"f976b34d06879e2836deb96bc43d7fefd41540d56e5487107fc26fea4fb01dd0"},"schema_version":"1.0"},"canonical_sha256":"b9a695063c8ece28c8874d5478171af3fe43f4994a6e0966b0b3bb7e49539257","source":{"kind":"arxiv","id":"1512.05595","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1512.05595","created_at":"2026-05-18T01:02:45Z"},{"alias_kind":"arxiv_version","alias_value":"1512.05595v2","created_at":"2026-05-18T01:02:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.05595","created_at":"2026-05-18T01:02:45Z"},{"alias_kind":"pith_short_12","alias_value":"XGTJKBR4R3HC","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_16","alias_value":"XGTJKBR4R3HCRSEH","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_8","alias_value":"XGTJKBR4","created_at":"2026-05-18T12:29:50Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:XGTJKBR4R3HCRSEHJVKHQFY26P","target":"record","payload":{"canonical_record":{"source":{"id":"1512.05595","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-12-17T14:26:51Z","cross_cats_sorted":[],"title_canon_sha256":"c6e7ac8148ab79c44786c6d0ee9382b05254832033305f7d3ff1ea4605e0f403","abstract_canon_sha256":"f976b34d06879e2836deb96bc43d7fefd41540d56e5487107fc26fea4fb01dd0"},"schema_version":"1.0"},"canonical_sha256":"b9a695063c8ece28c8874d5478171af3fe43f4994a6e0966b0b3bb7e49539257","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:02:45.310720Z","signature_b64":"39DsjHtVf+uN4xSkfcN44awpwG7R6xtBurJIlYLhd4FdTnCg837RggnadHkzi8+NM9cSserjOIATYSGf1KywAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b9a695063c8ece28c8874d5478171af3fe43f4994a6e0966b0b3bb7e49539257","last_reissued_at":"2026-05-18T01:02:45.310234Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:02:45.310234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1512.05595","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":"2026-05-18T01:02:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WSZcfw+30cDJe6vUh7GKrs4OmJNWl4Xp1OCiomSC3uqiwguVhuHIVnSmtI1VxHHhnAIkXuEmWiDaZYwbAdKwDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T09:43:11.318170Z"},"content_sha256":"b322f121f010cefcaa91b62e61b5cb36b068a62f2471c5c242de92e25dee6275","schema_version":"1.0","event_id":"sha256:b322f121f010cefcaa91b62e61b5cb36b068a62f2471c5c242de92e25dee6275"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:XGTJKBR4R3HCRSEHJVKHQFY26P","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Large-scale outflows in luminous QSOs revisited: The impact of beam smearing on AGN feedback efficiencies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"(2) Observatoire de Paris, 3), (3) Gemini Observatory, (4) California Polytechnic State University, (5) Seoul National University), B. Husemann (1), D. Kakkad (1) ((1) European Southern Observatory, J.-H. Woo (5), J. Scharw\\\"achter (2, V. Mainieri (1), V. N. Bennert (4)","submitted_at":"2015-12-17T14:26:51Z","abstract_excerpt":"[Abridged] Enormous observational efforts have been made to constrain the energetics of AGN feedback by mapping the kinematics of the ionized gas on kpc scale. We study how the observed kinematics and inferred energetics are affected by beam smearing of a bright unresolved NLR due to seeing. We analyse IFU spectroscopy of a sample of twelve QSOs initially presented by Liu et al. (2014). The PSF for the observations is directly obtained from the light distribution of the broad Hb line component. We are able to compare the ionized gas kinematics and derived energetics of the total, spatially ext"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.05595","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":"2026-05-18T01:02:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"LjfWDa5JaVidEbqsmqtxCzMzXKWBl0rozLyxlShE7i/lQ6xpsPYmMVUKEZ6Yi0A0Hc2b9L/6pHcBlJVo3uAWAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T09:43:11.318547Z"},"content_sha256":"15e54d6fad62d561c0620fff678efb40f377c28fe5cb51bbac46d3e559b35d07","schema_version":"1.0","event_id":"sha256:15e54d6fad62d561c0620fff678efb40f377c28fe5cb51bbac46d3e559b35d07"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/XGTJKBR4R3HCRSEHJVKHQFY26P/bundle.json","state_url":"https://pith.science/pith/XGTJKBR4R3HCRSEHJVKHQFY26P/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/XGTJKBR4R3HCRSEHJVKHQFY26P/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":"2026-06-05T09:43:11Z","links":{"resolver":"https://pith.science/pith/XGTJKBR4R3HCRSEHJVKHQFY26P","bundle":"https://pith.science/pith/XGTJKBR4R3HCRSEHJVKHQFY26P/bundle.json","state":"https://pith.science/pith/XGTJKBR4R3HCRSEHJVKHQFY26P/state.json","well_known_bundle":"https://pith.science/.well-known/pith/XGTJKBR4R3HCRSEHJVKHQFY26P/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:XGTJKBR4R3HCRSEHJVKHQFY26P","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":"f976b34d06879e2836deb96bc43d7fefd41540d56e5487107fc26fea4fb01dd0","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-12-17T14:26:51Z","title_canon_sha256":"c6e7ac8148ab79c44786c6d0ee9382b05254832033305f7d3ff1ea4605e0f403"},"schema_version":"1.0","source":{"id":"1512.05595","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1512.05595","created_at":"2026-05-18T01:02:45Z"},{"alias_kind":"arxiv_version","alias_value":"1512.05595v2","created_at":"2026-05-18T01:02:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.05595","created_at":"2026-05-18T01:02:45Z"},{"alias_kind":"pith_short_12","alias_value":"XGTJKBR4R3HC","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_16","alias_value":"XGTJKBR4R3HCRSEH","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_8","alias_value":"XGTJKBR4","created_at":"2026-05-18T12:29:50Z"}],"graph_snapshots":[{"event_id":"sha256:15e54d6fad62d561c0620fff678efb40f377c28fe5cb51bbac46d3e559b35d07","target":"graph","created_at":"2026-05-18T01:02:45Z","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":"[Abridged] Enormous observational efforts have been made to constrain the energetics of AGN feedback by mapping the kinematics of the ionized gas on kpc scale. We study how the observed kinematics and inferred energetics are affected by beam smearing of a bright unresolved NLR due to seeing. We analyse IFU spectroscopy of a sample of twelve QSOs initially presented by Liu et al. (2014). The PSF for the observations is directly obtained from the light distribution of the broad Hb line component. We are able to compare the ionized gas kinematics and derived energetics of the total, spatially ext","authors_text":"(2) Observatoire de Paris, 3), (3) Gemini Observatory, (4) California Polytechnic State University, (5) Seoul National University), B. Husemann (1), D. Kakkad (1) ((1) European Southern Observatory, J.-H. Woo (5), J. Scharw\\\"achter (2, V. Mainieri (1), V. N. Bennert (4)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-12-17T14:26:51Z","title":"Large-scale outflows in luminous QSOs revisited: The impact of beam smearing on AGN feedback efficiencies"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.05595","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:b322f121f010cefcaa91b62e61b5cb36b068a62f2471c5c242de92e25dee6275","target":"record","created_at":"2026-05-18T01:02:45Z","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":"f976b34d06879e2836deb96bc43d7fefd41540d56e5487107fc26fea4fb01dd0","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-12-17T14:26:51Z","title_canon_sha256":"c6e7ac8148ab79c44786c6d0ee9382b05254832033305f7d3ff1ea4605e0f403"},"schema_version":"1.0","source":{"id":"1512.05595","kind":"arxiv","version":2}},"canonical_sha256":"b9a695063c8ece28c8874d5478171af3fe43f4994a6e0966b0b3bb7e49539257","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"b9a695063c8ece28c8874d5478171af3fe43f4994a6e0966b0b3bb7e49539257","first_computed_at":"2026-05-18T01:02:45.310234Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:02:45.310234Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"39DsjHtVf+uN4xSkfcN44awpwG7R6xtBurJIlYLhd4FdTnCg837RggnadHkzi8+NM9cSserjOIATYSGf1KywAA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:02:45.310720Z","signed_message":"canonical_sha256_bytes"},"source_id":"1512.05595","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b322f121f010cefcaa91b62e61b5cb36b068a62f2471c5c242de92e25dee6275","sha256:15e54d6fad62d561c0620fff678efb40f377c28fe5cb51bbac46d3e559b35d07"],"state_sha256":"f0ddb76776e735e0300dc828d1a58fd4e6cd2a9e1573fc09ccf4f93bba1b8568"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dzBddi1u00PrEGwVzhcvYxwtZ62MqbU2vzRoOE/bWUOgNTlh3D9Nmigdf0P9+d0f6/jTvPk4Egs5c23RbufXDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T09:43:11.320704Z","bundle_sha256":"846fc6610a7443a28241b2f383b0bf38c5fe337a204eb4b815d8779032b24d11"}}