{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:CYD24A2GPCHUGYFPP5MUU5SYFQ","short_pith_number":"pith:CYD24A2G","canonical_record":{"source":{"id":"1403.0247","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-02T17:35:11Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"46725d5a9a93c32e77f32bba5546f2229e6ba4e432a7b0e7c4ad1f049109755e","abstract_canon_sha256":"261515704a9e9dc5c84dadf144bb9ab65478dd930303a51657efdf142ecd7bc0"},"schema_version":"1.0"},"canonical_sha256":"1607ae0346788f4360af7f594a76582c049d2c823d295d9fb99afa6630af69fb","source":{"kind":"arxiv","id":"1403.0247","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1403.0247","created_at":"2026-05-18T01:44:21Z"},{"alias_kind":"arxiv_version","alias_value":"1403.0247v2","created_at":"2026-05-18T01:44:21Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.0247","created_at":"2026-05-18T01:44:21Z"},{"alias_kind":"pith_short_12","alias_value":"CYD24A2GPCHU","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_16","alias_value":"CYD24A2GPCHUGYFP","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_8","alias_value":"CYD24A2G","created_at":"2026-05-18T12:28:25Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:CYD24A2GPCHUGYFPP5MUU5SYFQ","target":"record","payload":{"canonical_record":{"source":{"id":"1403.0247","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-02T17:35:11Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"46725d5a9a93c32e77f32bba5546f2229e6ba4e432a7b0e7c4ad1f049109755e","abstract_canon_sha256":"261515704a9e9dc5c84dadf144bb9ab65478dd930303a51657efdf142ecd7bc0"},"schema_version":"1.0"},"canonical_sha256":"1607ae0346788f4360af7f594a76582c049d2c823d295d9fb99afa6630af69fb","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:21.324252Z","signature_b64":"xTBNgWkprO2u9G+eT1gsJxraSooQFyEKSsUVsPebtS/684nvZA/AUo+XY3b71xJ01KXkb5kbFdYGiIBVlRvXBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1607ae0346788f4360af7f594a76582c049d2c823d295d9fb99afa6630af69fb","last_reissued_at":"2026-05-18T01:44:21.323609Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:21.323609Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1403.0247","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":"2026-05-18T01:44:21Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"90oPaolhm25s9SWOpp+tu3ipcE1C39Ah4LIv0M7q1+9Q9jK8liUGpYTIsENwOtzP2JLSezMleENZa/wHocEXDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T02:17:42.605122Z"},"content_sha256":"3cdca162ab262ef70ed337537243c47767b021550f0ae2532ae2a7aaba5145c3","schema_version":"1.0","event_id":"sha256:3cdca162ab262ef70ed337537243c47767b021550f0ae2532ae2a7aaba5145c3"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:CYD24A2GPCHUGYFPP5MUU5SYFQ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Imaging the environment of a z = 6.3 submillimeter galaxy with SCUBA-2","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"A. Conley, A. Cooray, A.G. Gibb, A.M. Swinbank, A. Omont, D. Bintley, D. Farrah, D.L. Clements, Douglas Scott, D. Riechers, E.I. Robson, E.L. Chapin, Hai Fu, Ian Smail, I. P\\'erez-Fournon, J. Bock, J.E. Geach, J.S. Dunlop, J. Wardlow, M. Fich, N. Laporte, P.A.R. Ade, R.J. Ivison, S.C. Chapman, S.J. Oliver, T. Jenness, W.S. Holland","submitted_at":"2014-03-02T17:35:11Z","abstract_excerpt":"We describe a search for submillimeter emission in the vicinity of one of the most distant, luminous galaxies known, HerMES FLS3 at z=6.34, exploiting it as a signpost to a potentially biased region of the early Universe, as might be expected in hierarchical structure formation models. Imaging to the confusion limit with the innovative, wide-field submillimeter bolometer camera, SCUBA-2, we are sensitive to colder and/or less luminous galaxies in the surroundings of HFLS3. We use the Millennium Simulation to illustrate that HFLS3 may be expected to have companions if it is as massive as claime"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.0247","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":"2026-05-18T01:44:21Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"xNMZlkKs09DIbn7QrrxqgVlVhRp5CEuz1JFLsQ7SlT1hi7+QXb6/KxeWh90+NXD9rScqt3jhH8xnec4J4vI7CA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T02:17:42.605489Z"},"content_sha256":"905d44e215b2b3ee2ade50d2b99469a22e29ec9492ad7dcde8006f9b0924b3d8","schema_version":"1.0","event_id":"sha256:905d44e215b2b3ee2ade50d2b99469a22e29ec9492ad7dcde8006f9b0924b3d8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ/bundle.json","state_url":"https://pith.science/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ/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":"2026-05-28T02:17:42Z","links":{"resolver":"https://pith.science/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ","bundle":"https://pith.science/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ/bundle.json","state":"https://pith.science/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CYD24A2GPCHUGYFPP5MUU5SYFQ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:CYD24A2GPCHUGYFPP5MUU5SYFQ","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":"261515704a9e9dc5c84dadf144bb9ab65478dd930303a51657efdf142ecd7bc0","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-02T17:35:11Z","title_canon_sha256":"46725d5a9a93c32e77f32bba5546f2229e6ba4e432a7b0e7c4ad1f049109755e"},"schema_version":"1.0","source":{"id":"1403.0247","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1403.0247","created_at":"2026-05-18T01:44:21Z"},{"alias_kind":"arxiv_version","alias_value":"1403.0247v2","created_at":"2026-05-18T01:44:21Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.0247","created_at":"2026-05-18T01:44:21Z"},{"alias_kind":"pith_short_12","alias_value":"CYD24A2GPCHU","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_16","alias_value":"CYD24A2GPCHUGYFP","created_at":"2026-05-18T12:28:25Z"},{"alias_kind":"pith_short_8","alias_value":"CYD24A2G","created_at":"2026-05-18T12:28:25Z"}],"graph_snapshots":[{"event_id":"sha256:905d44e215b2b3ee2ade50d2b99469a22e29ec9492ad7dcde8006f9b0924b3d8","target":"graph","created_at":"2026-05-18T01:44:21Z","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 describe a search for submillimeter emission in the vicinity of one of the most distant, luminous galaxies known, HerMES FLS3 at z=6.34, exploiting it as a signpost to a potentially biased region of the early Universe, as might be expected in hierarchical structure formation models. Imaging to the confusion limit with the innovative, wide-field submillimeter bolometer camera, SCUBA-2, we are sensitive to colder and/or less luminous galaxies in the surroundings of HFLS3. We use the Millennium Simulation to illustrate that HFLS3 may be expected to have companions if it is as massive as claime","authors_text":"A. Conley, A. Cooray, A.G. Gibb, A.M. Swinbank, A. Omont, D. Bintley, D. Farrah, D.L. Clements, Douglas Scott, D. Riechers, E.I. Robson, E.L. Chapin, Hai Fu, Ian Smail, I. P\\'erez-Fournon, J. Bock, J.E. Geach, J.S. Dunlop, J. Wardlow, M. Fich, N. Laporte, P.A.R. Ade, R.J. Ivison, S.C. Chapman, S.J. Oliver, T. Jenness, W.S. Holland","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-02T17:35:11Z","title":"Imaging the environment of a z = 6.3 submillimeter galaxy with SCUBA-2"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.0247","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":"sha256:3cdca162ab262ef70ed337537243c47767b021550f0ae2532ae2a7aaba5145c3","target":"record","created_at":"2026-05-18T01:44:21Z","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":"261515704a9e9dc5c84dadf144bb9ab65478dd930303a51657efdf142ecd7bc0","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-03-02T17:35:11Z","title_canon_sha256":"46725d5a9a93c32e77f32bba5546f2229e6ba4e432a7b0e7c4ad1f049109755e"},"schema_version":"1.0","source":{"id":"1403.0247","kind":"arxiv","version":2}},"canonical_sha256":"1607ae0346788f4360af7f594a76582c049d2c823d295d9fb99afa6630af69fb","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"1607ae0346788f4360af7f594a76582c049d2c823d295d9fb99afa6630af69fb","first_computed_at":"2026-05-18T01:44:21.323609Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:44:21.323609Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"xTBNgWkprO2u9G+eT1gsJxraSooQFyEKSsUVsPebtS/684nvZA/AUo+XY3b71xJ01KXkb5kbFdYGiIBVlRvXBw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:44:21.324252Z","signed_message":"canonical_sha256_bytes"},"source_id":"1403.0247","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3cdca162ab262ef70ed337537243c47767b021550f0ae2532ae2a7aaba5145c3","sha256:905d44e215b2b3ee2ade50d2b99469a22e29ec9492ad7dcde8006f9b0924b3d8"],"state_sha256":"099ca582e707756ac1876f4aeed23c2a244e60e63453d7b31ddf8ffc686bb800"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"NMout1hi3JMFk//8Dy1TB8Zi8di18KA1fS7hDYCrJSDV34EHro8WJ7+ZdmFhuSd6qvVccJokUE5E6LHW8GeAAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T02:17:42.607460Z","bundle_sha256":"8641beba9dd7af64c5d3dfef879311fb0f98dd3db82fcefc1abc46e82569042f"}}