{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:FALOWWSMSMIBF7FTFXFIXXHR3M","short_pith_number":"pith:FALOWWSM","canonical_record":{"source":{"id":"1709.04191","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-09-13T08:46:18Z","cross_cats_sorted":[],"title_canon_sha256":"1da714a5da9261edaf82d75dc0df69449e324c9835c590efcf4370bea53fc569","abstract_canon_sha256":"7401f0790c42d56a75e5182d96253f2883731e9d9742b1279895cc84d431413f"},"schema_version":"1.0"},"canonical_sha256":"2816eb5a4c931012fcb32dca8bdcf1db1b4b16913947f769fbcf7a568275b8d2","source":{"kind":"arxiv","id":"1709.04191","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1709.04191","created_at":"2026-05-18T00:35:15Z"},{"alias_kind":"arxiv_version","alias_value":"1709.04191v1","created_at":"2026-05-18T00:35:15Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.04191","created_at":"2026-05-18T00:35:15Z"},{"alias_kind":"pith_short_12","alias_value":"FALOWWSMSMIB","created_at":"2026-05-18T12:31:15Z"},{"alias_kind":"pith_short_16","alias_value":"FALOWWSMSMIBF7FT","created_at":"2026-05-18T12:31:15Z"},{"alias_kind":"pith_short_8","alias_value":"FALOWWSM","created_at":"2026-05-18T12:31:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:FALOWWSMSMIBF7FTFXFIXXHR3M","target":"record","payload":{"canonical_record":{"source":{"id":"1709.04191","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-09-13T08:46:18Z","cross_cats_sorted":[],"title_canon_sha256":"1da714a5da9261edaf82d75dc0df69449e324c9835c590efcf4370bea53fc569","abstract_canon_sha256":"7401f0790c42d56a75e5182d96253f2883731e9d9742b1279895cc84d431413f"},"schema_version":"1.0"},"canonical_sha256":"2816eb5a4c931012fcb32dca8bdcf1db1b4b16913947f769fbcf7a568275b8d2","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:15.150437Z","signature_b64":"yD+m+MIzDraHO/SzLB125xVyrwjuwh4MfCnvRL0qzDgWC0gT2hGkPGf32k7Ys3nSqpBMAtUjNbQ+KUOndnZPAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2816eb5a4c931012fcb32dca8bdcf1db1b4b16913947f769fbcf7a568275b8d2","last_reissued_at":"2026-05-18T00:35:15.149724Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:15.149724Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1709.04191","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":"2026-05-18T00:35:15Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5dhe1XUEb+Ur+V3VNoNZNHNCo8+e7j0dPYL5ehVs63Poqa3+pZ0U14KDWARFwVTZlbq4/7OJBvXvn+YM+xkuCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:58:44.993694Z"},"content_sha256":"6dd748d6606c613a392f47552344f760a4c06618edbcd3ad82653634f4b427bf","schema_version":"1.0","event_id":"sha256:6dd748d6606c613a392f47552344f760a4c06618edbcd3ad82653634f4b427bf"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:FALOWWSMSMIBF7FTFXFIXXHR3M","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Witnessing the birth of the red sequence: the physical scale and morphology of dust emission in hyper-luminous starbursts in the early Universe","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Cooray, A. J. R. Lewis, A. Omont, D. Farrah, D. L. Clements, D. Riechers, D. Scott, E. Ibar, G. de Zotti, H. Dannerbauer, I. Oteo, I. P\\'erez-Fournon, I. Smail, L. Dunne, M. Bremer, M. J. Micha{\\l}owski, M. Negrello, P. Mart\\'inez-Navajas, P. Temi, P. van der Werf, R. J. Ivison, R. Marques-Chaves, S. A. Eales, S. Duivenvoorden, S. Oliver","submitted_at":"2017-09-13T08:46:18Z","abstract_excerpt":"We present high-spatial-resolution ($\\sim 0.12''$ or $\\approx 800 \\, {\\rm pc}$ at $z = 4.5$) ALMA $870\\,\\mu$m dust continuum observations of a sample of 44 ultrared dusty star-forming galaxies (DSFGs) selected from the H-ATLAS and HerMES far-infrared surveys because of their red colors from 250 to 500 $\\mu$m: $S_{500} / S_{250} > 1.5$ and $S_{500} / S_{350} > 1.0$. With photometric redshifts in the range $z \\sim 4$-6, our sample includes the most luminous starbursting systems in the early Universe known so far, with total obscured star-formation rates (SFRs) of up to $\\sim 4,500 \\, M_\\odot \\, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.04191","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":"2026-05-18T00:35:15Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"kMwSL1DfE7izsVkccTfq7dIOYpCKTi6hV47E9fqKqXX12IuvnghZDtHGKLuyCjizeWo00VwiVrEco1MdiMObCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T17:58:44.994403Z"},"content_sha256":"77fca98b9837d49350ecb07a96c6c66ab65cf6e835cba3410fbbfe38f1eb7b8f","schema_version":"1.0","event_id":"sha256:77fca98b9837d49350ecb07a96c6c66ab65cf6e835cba3410fbbfe38f1eb7b8f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/FALOWWSMSMIBF7FTFXFIXXHR3M/bundle.json","state_url":"https://pith.science/pith/FALOWWSMSMIBF7FTFXFIXXHR3M/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/FALOWWSMSMIBF7FTFXFIXXHR3M/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":"2026-05-25T17:58:44Z","links":{"resolver":"https://pith.science/pith/FALOWWSMSMIBF7FTFXFIXXHR3M","bundle":"https://pith.science/pith/FALOWWSMSMIBF7FTFXFIXXHR3M/bundle.json","state":"https://pith.science/pith/FALOWWSMSMIBF7FTFXFIXXHR3M/state.json","well_known_bundle":"https://pith.science/.well-known/pith/FALOWWSMSMIBF7FTFXFIXXHR3M/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:FALOWWSMSMIBF7FTFXFIXXHR3M","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":"7401f0790c42d56a75e5182d96253f2883731e9d9742b1279895cc84d431413f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-09-13T08:46:18Z","title_canon_sha256":"1da714a5da9261edaf82d75dc0df69449e324c9835c590efcf4370bea53fc569"},"schema_version":"1.0","source":{"id":"1709.04191","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1709.04191","created_at":"2026-05-18T00:35:15Z"},{"alias_kind":"arxiv_version","alias_value":"1709.04191v1","created_at":"2026-05-18T00:35:15Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.04191","created_at":"2026-05-18T00:35:15Z"},{"alias_kind":"pith_short_12","alias_value":"FALOWWSMSMIB","created_at":"2026-05-18T12:31:15Z"},{"alias_kind":"pith_short_16","alias_value":"FALOWWSMSMIBF7FT","created_at":"2026-05-18T12:31:15Z"},{"alias_kind":"pith_short_8","alias_value":"FALOWWSM","created_at":"2026-05-18T12:31:15Z"}],"graph_snapshots":[{"event_id":"sha256:77fca98b9837d49350ecb07a96c6c66ab65cf6e835cba3410fbbfe38f1eb7b8f","target":"graph","created_at":"2026-05-18T00:35:15Z","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 high-spatial-resolution ($\\sim 0.12''$ or $\\approx 800 \\, {\\rm pc}$ at $z = 4.5$) ALMA $870\\,\\mu$m dust continuum observations of a sample of 44 ultrared dusty star-forming galaxies (DSFGs) selected from the H-ATLAS and HerMES far-infrared surveys because of their red colors from 250 to 500 $\\mu$m: $S_{500} / S_{250} > 1.5$ and $S_{500} / S_{350} > 1.0$. With photometric redshifts in the range $z \\sim 4$-6, our sample includes the most luminous starbursting systems in the early Universe known so far, with total obscured star-formation rates (SFRs) of up to $\\sim 4,500 \\, M_\\odot \\, ","authors_text":"A. Cooray, A. J. R. Lewis, A. Omont, D. Farrah, D. L. Clements, D. Riechers, D. Scott, E. Ibar, G. de Zotti, H. Dannerbauer, I. Oteo, I. P\\'erez-Fournon, I. Smail, L. Dunne, M. Bremer, M. J. Micha{\\l}owski, M. Negrello, P. Mart\\'inez-Navajas, P. Temi, P. van der Werf, R. J. Ivison, R. Marques-Chaves, S. A. Eales, S. Duivenvoorden, S. Oliver","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-09-13T08:46:18Z","title":"Witnessing the birth of the red sequence: the physical scale and morphology of dust emission in hyper-luminous starbursts in the early Universe"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.04191","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":"sha256:6dd748d6606c613a392f47552344f760a4c06618edbcd3ad82653634f4b427bf","target":"record","created_at":"2026-05-18T00:35:15Z","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":"7401f0790c42d56a75e5182d96253f2883731e9d9742b1279895cc84d431413f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-09-13T08:46:18Z","title_canon_sha256":"1da714a5da9261edaf82d75dc0df69449e324c9835c590efcf4370bea53fc569"},"schema_version":"1.0","source":{"id":"1709.04191","kind":"arxiv","version":1}},"canonical_sha256":"2816eb5a4c931012fcb32dca8bdcf1db1b4b16913947f769fbcf7a568275b8d2","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"2816eb5a4c931012fcb32dca8bdcf1db1b4b16913947f769fbcf7a568275b8d2","first_computed_at":"2026-05-18T00:35:15.149724Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:35:15.149724Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"yD+m+MIzDraHO/SzLB125xVyrwjuwh4MfCnvRL0qzDgWC0gT2hGkPGf32k7Ys3nSqpBMAtUjNbQ+KUOndnZPAg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:35:15.150437Z","signed_message":"canonical_sha256_bytes"},"source_id":"1709.04191","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:6dd748d6606c613a392f47552344f760a4c06618edbcd3ad82653634f4b427bf","sha256:77fca98b9837d49350ecb07a96c6c66ab65cf6e835cba3410fbbfe38f1eb7b8f"],"state_sha256":"ed1c4abb7374429d1f6857a945017dd3c2e74c6b74dd6a4c0927197f605a26ee"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dgw3eHWGyNk9wGOhNjOYaf7HXLgpTxIdmtLMF3oykj7X94sks5oZA7q5xCB8LLBp2VFZw8YYStrZH/yMIKbtCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T17:58:44.997934Z","bundle_sha256":"2909c27037b3ceb7d1d4bce967ba628e7cd8c302501e3d7232e085882df08359"}}