{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:BFQPNNIWKZLZG7IR6QFNWYON5W","short_pith_number":"pith:BFQPNNIW","canonical_record":{"source":{"id":"1712.02708","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-07T16:45:46Z","cross_cats_sorted":[],"title_canon_sha256":"ef317fea494ff9439040ffe897b1638d7f268cc3310c63a4eaa7ba0fb8427229","abstract_canon_sha256":"2ea77c985363baf274ea41e08199a4aaf9eb1ddd3c276b30365ca671a2b1ed7f"},"schema_version":"1.0"},"canonical_sha256":"0960f6b5165657937d11f40adb61cded9efcbc4d4b5c9ce0d4b8cdbd60763284","source":{"kind":"arxiv","id":"1712.02708","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1712.02708","created_at":"2026-05-18T00:28:33Z"},{"alias_kind":"arxiv_version","alias_value":"1712.02708v1","created_at":"2026-05-18T00:28:33Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.02708","created_at":"2026-05-18T00:28:33Z"},{"alias_kind":"pith_short_12","alias_value":"BFQPNNIWKZLZ","created_at":"2026-05-18T12:31:08Z"},{"alias_kind":"pith_short_16","alias_value":"BFQPNNIWKZLZG7IR","created_at":"2026-05-18T12:31:08Z"},{"alias_kind":"pith_short_8","alias_value":"BFQPNNIW","created_at":"2026-05-18T12:31:08Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:BFQPNNIWKZLZG7IR6QFNWYON5W","target":"record","payload":{"canonical_record":{"source":{"id":"1712.02708","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-07T16:45:46Z","cross_cats_sorted":[],"title_canon_sha256":"ef317fea494ff9439040ffe897b1638d7f268cc3310c63a4eaa7ba0fb8427229","abstract_canon_sha256":"2ea77c985363baf274ea41e08199a4aaf9eb1ddd3c276b30365ca671a2b1ed7f"},"schema_version":"1.0"},"canonical_sha256":"0960f6b5165657937d11f40adb61cded9efcbc4d4b5c9ce0d4b8cdbd60763284","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:33.129095Z","signature_b64":"KhAP+T69p8TN3wcppvCDjTG7SNFzbMwBiEAcBE/CXmrAHKrbwm6D2uRNUUQWsCukQ28myBLgVLYVKBCAVGKtBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0960f6b5165657937d11f40adb61cded9efcbc4d4b5c9ce0d4b8cdbd60763284","last_reissued_at":"2026-05-18T00:28:33.128332Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:33.128332Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1712.02708","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":"2026-05-18T00:28:33Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"0VoRsqtr9ofjdYoNWqQmIgHAdRjAx2ocrVkZ9rb9rhORsGqE3sARKZ+kGBJkgnJ6cLWn0/ZyZfApWxJLVxJMBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T01:39:35.231688Z"},"content_sha256":"5c7363538098fe1d7e5df88943963e9237d9307ccac7915ec45ad3357439dbd6","schema_version":"1.0","event_id":"sha256:5c7363538098fe1d7e5df88943963e9237d9307ccac7915ec45ad3357439dbd6"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:BFQPNNIWKZLZG7IR6QFNWYON5W","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. M. Swinbank, C. M. Harrison, D. J. Rosario, D. M. Alexander, F. Stanley, J.R Mullaney, J. Scholtz (Durham), J. Simpson, P. Santini, R. C. Hickox, R. G. Bower, S. McAlpine, T. Theuns","submitted_at":"2017-12-07T16:45:46Z","abstract_excerpt":"We present sensitive 870$\\mu$m continuum measurements from our ALMA programmes of 114 X-ray selected AGN in the CDF-S and COSMOS fields. We use these observations in combination with data from Spitzer and Herschel to construct a sample of 86 X-ray selected AGN, 63 with ALMA constraints at $z=1.5-3.2$ with stellar mass $>2\\times10^{10}M_{\\odot}$. We constructed broad-band spectral energy distributions in the infrared band (8 - 1000$\\mu$m) and constrain star-formation rates (SFRs) uncontaminated by the AGN. Using a hierarchical Bayesian method that takes into account the information from upper l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.02708","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":"2026-05-18T00:28:33Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"LhYBZ5q465szDFYEWyN3urwPH0wNf+Fx+SSKL8Jms6cYYPNsE4d/B7P/cy9F6rPzMNh5KsgTSpj8TgdV5PV7Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T01:39:35.232038Z"},"content_sha256":"4c95b0539d695c7c63803b1bc35bdeb3566c4c09771f4db87da66b71384f9689","schema_version":"1.0","event_id":"sha256:4c95b0539d695c7c63803b1bc35bdeb3566c4c09771f4db87da66b71384f9689"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/BFQPNNIWKZLZG7IR6QFNWYON5W/bundle.json","state_url":"https://pith.science/pith/BFQPNNIWKZLZG7IR6QFNWYON5W/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/BFQPNNIWKZLZG7IR6QFNWYON5W/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":"2026-05-28T01:39:35Z","links":{"resolver":"https://pith.science/pith/BFQPNNIWKZLZG7IR6QFNWYON5W","bundle":"https://pith.science/pith/BFQPNNIWKZLZG7IR6QFNWYON5W/bundle.json","state":"https://pith.science/pith/BFQPNNIWKZLZG7IR6QFNWYON5W/state.json","well_known_bundle":"https://pith.science/.well-known/pith/BFQPNNIWKZLZG7IR6QFNWYON5W/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:BFQPNNIWKZLZG7IR6QFNWYON5W","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":"2ea77c985363baf274ea41e08199a4aaf9eb1ddd3c276b30365ca671a2b1ed7f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-07T16:45:46Z","title_canon_sha256":"ef317fea494ff9439040ffe897b1638d7f268cc3310c63a4eaa7ba0fb8427229"},"schema_version":"1.0","source":{"id":"1712.02708","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1712.02708","created_at":"2026-05-18T00:28:33Z"},{"alias_kind":"arxiv_version","alias_value":"1712.02708v1","created_at":"2026-05-18T00:28:33Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.02708","created_at":"2026-05-18T00:28:33Z"},{"alias_kind":"pith_short_12","alias_value":"BFQPNNIWKZLZ","created_at":"2026-05-18T12:31:08Z"},{"alias_kind":"pith_short_16","alias_value":"BFQPNNIWKZLZG7IR","created_at":"2026-05-18T12:31:08Z"},{"alias_kind":"pith_short_8","alias_value":"BFQPNNIW","created_at":"2026-05-18T12:31:08Z"}],"graph_snapshots":[{"event_id":"sha256:4c95b0539d695c7c63803b1bc35bdeb3566c4c09771f4db87da66b71384f9689","target":"graph","created_at":"2026-05-18T00:28:33Z","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 present sensitive 870$\\mu$m continuum measurements from our ALMA programmes of 114 X-ray selected AGN in the CDF-S and COSMOS fields. We use these observations in combination with data from Spitzer and Herschel to construct a sample of 86 X-ray selected AGN, 63 with ALMA constraints at $z=1.5-3.2$ with stellar mass $>2\\times10^{10}M_{\\odot}$. We constructed broad-band spectral energy distributions in the infrared band (8 - 1000$\\mu$m) and constrain star-formation rates (SFRs) uncontaminated by the AGN. Using a hierarchical Bayesian method that takes into account the information from upper l","authors_text":"A. M. Swinbank, C. M. Harrison, D. J. Rosario, D. M. Alexander, F. Stanley, J.R Mullaney, J. Scholtz (Durham), J. Simpson, P. Santini, R. C. Hickox, R. G. Bower, S. McAlpine, T. Theuns","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-07T16:45:46Z","title":"Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.02708","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":"sha256:5c7363538098fe1d7e5df88943963e9237d9307ccac7915ec45ad3357439dbd6","target":"record","created_at":"2026-05-18T00:28:33Z","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":"2ea77c985363baf274ea41e08199a4aaf9eb1ddd3c276b30365ca671a2b1ed7f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-07T16:45:46Z","title_canon_sha256":"ef317fea494ff9439040ffe897b1638d7f268cc3310c63a4eaa7ba0fb8427229"},"schema_version":"1.0","source":{"id":"1712.02708","kind":"arxiv","version":1}},"canonical_sha256":"0960f6b5165657937d11f40adb61cded9efcbc4d4b5c9ce0d4b8cdbd60763284","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"0960f6b5165657937d11f40adb61cded9efcbc4d4b5c9ce0d4b8cdbd60763284","first_computed_at":"2026-05-18T00:28:33.128332Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:28:33.128332Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"KhAP+T69p8TN3wcppvCDjTG7SNFzbMwBiEAcBE/CXmrAHKrbwm6D2uRNUUQWsCukQ28myBLgVLYVKBCAVGKtBg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:28:33.129095Z","signed_message":"canonical_sha256_bytes"},"source_id":"1712.02708","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:5c7363538098fe1d7e5df88943963e9237d9307ccac7915ec45ad3357439dbd6","sha256:4c95b0539d695c7c63803b1bc35bdeb3566c4c09771f4db87da66b71384f9689"],"state_sha256":"b58e682b714ab671a2ebdf0fd8d9ee9463bdc84ca38777770aa71a40cb8b2c42"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mSAwX+JV8ZIlr7A3oQeA1evCUr5BhQf/7T0ypHL+Tz495c50AtSpXX0bY4Fiwh2WkXcEeWEk7h6gtwVR5d48Bw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T01:39:35.233960Z","bundle_sha256":"5faf5238fb059392f9e18c898fc7ff68006294d171fe1c562ac76de0ad9a301e"}}