{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:6HQ37V6MJAOYOLT46FES5PKX2S","short_pith_number":"pith:6HQ37V6M","canonical_record":{"source":{"id":"1404.1378","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-04T20:00:38Z","cross_cats_sorted":[],"title_canon_sha256":"f040690dcdaa76c0709aaa08067414987ae3d6529587116dd456421274f4b82b","abstract_canon_sha256":"0da83135b98f53cc8b156f882807d21ddcf1b082c9c494c6be90ad6fe69160e6"},"schema_version":"1.0"},"canonical_sha256":"f1e1bfd7cc481d872e7cf1492ebd57d48e8ea2359fc17d4140d69b0b752946a6","source":{"kind":"arxiv","id":"1404.1378","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1404.1378","created_at":"2026-05-18T01:43:42Z"},{"alias_kind":"arxiv_version","alias_value":"1404.1378v1","created_at":"2026-05-18T01:43:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1378","created_at":"2026-05-18T01:43:42Z"},{"alias_kind":"pith_short_12","alias_value":"6HQ37V6MJAOY","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_16","alias_value":"6HQ37V6MJAOYOLT4","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_8","alias_value":"6HQ37V6M","created_at":"2026-05-18T12:28:16Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:6HQ37V6MJAOYOLT46FES5PKX2S","target":"record","payload":{"canonical_record":{"source":{"id":"1404.1378","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-04T20:00:38Z","cross_cats_sorted":[],"title_canon_sha256":"f040690dcdaa76c0709aaa08067414987ae3d6529587116dd456421274f4b82b","abstract_canon_sha256":"0da83135b98f53cc8b156f882807d21ddcf1b082c9c494c6be90ad6fe69160e6"},"schema_version":"1.0"},"canonical_sha256":"f1e1bfd7cc481d872e7cf1492ebd57d48e8ea2359fc17d4140d69b0b752946a6","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:42.058691Z","signature_b64":"/ThTuAYMElJ9cH2fxJNM7S+6x69gh6ttEs8Pmz0JD7hbQvFs+XXU5hJruRBYB8HOzVth3D72MX5D+HC761exBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1e1bfd7cc481d872e7cf1492ebd57d48e8ea2359fc17d4140d69b0b752946a6","last_reissued_at":"2026-05-18T01:43:42.058231Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:42.058231Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1404.1378","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":"2026-05-18T01:43:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7FwsyiIIStnSFzy2jWBZ+jreX6GJyOSrLXT5bJFe2H2DJ2zo7W53jWiluOE+zQfeu6o8X+DWVmMM7I/6DDUeDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T06:00:47.739114Z"},"content_sha256":"46c7f926f796a9b6f7fa578b42f4bf656bb9eff4b30a016ad2177263154f2202","schema_version":"1.0","event_id":"sha256:46c7f926f796a9b6f7fa578b42f4bf656bb9eff4b30a016ad2177263154f2202"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:6HQ37V6MJAOYOLT46FES5PKX2S","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"HerMES: The Rest-Frame UV Emission and A Lensing Model for the z=6.34 Luminous Dusty Starburst Galaxy HFLS3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Conley, Asantha Cooray, B. Lofaro, Brian Ma, C. Bridge, C.M. Casey, D. Burgarella, D. Clements, D. Farrah, D. Riechers, D. Rigopoulou, D. Scott, D. Watson, G. Magdis, H. Fu, I. Pe'rez-Fournon, Jae Calanog, J. Bock, Julie L. Wardlow, M. Viero, N. Laporte, R. Gavazzi, R.J. Ivison, R.S. Bussmann, S.J. Oliver, W.A. Osage","submitted_at":"2014-04-04T20:00:38Z","abstract_excerpt":"We discuss the restframe UV emission from the starbursting galaxy HFLS3 at z=6.34, discovered in Herschel/SPIRE data due to its red color in the submm wavelengths from 250-500 um. The apparent inst. SFR of HFLS3 inferred from the total FIR luminosity measured with over 15 photometric data points between 100 to 1000 um is 2900 Msun/yr. Keck/NIRC2 Ks band adaptive optics imaging data showed two potential NIR counterparts near HFLS3. Previously, the northern galaxy was taken to be in the foreground at z=2.1 while the southern galaxy was assumed to HFLS3's NIR counterpart. New HST/WFC3 and ACS ima"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1378","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":"2026-05-18T01:43:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"beldYXlWA+9zrIkqCA6kCCludyXTNIfqM7m+oBV5gGKFRPma9myGvZDez7tFox26n+ULkX1HjW0+n0Yt59AqBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T06:00:47.739628Z"},"content_sha256":"6e15faf98b94ea856fbf8d84e43d2fc1e3b2b6e289757fc71059ae98009fdbbd","schema_version":"1.0","event_id":"sha256:6e15faf98b94ea856fbf8d84e43d2fc1e3b2b6e289757fc71059ae98009fdbbd"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/6HQ37V6MJAOYOLT46FES5PKX2S/bundle.json","state_url":"https://pith.science/pith/6HQ37V6MJAOYOLT46FES5PKX2S/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/6HQ37V6MJAOYOLT46FES5PKX2S/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":"2026-05-26T06:00:47Z","links":{"resolver":"https://pith.science/pith/6HQ37V6MJAOYOLT46FES5PKX2S","bundle":"https://pith.science/pith/6HQ37V6MJAOYOLT46FES5PKX2S/bundle.json","state":"https://pith.science/pith/6HQ37V6MJAOYOLT46FES5PKX2S/state.json","well_known_bundle":"https://pith.science/.well-known/pith/6HQ37V6MJAOYOLT46FES5PKX2S/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:6HQ37V6MJAOYOLT46FES5PKX2S","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":"0da83135b98f53cc8b156f882807d21ddcf1b082c9c494c6be90ad6fe69160e6","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-04T20:00:38Z","title_canon_sha256":"f040690dcdaa76c0709aaa08067414987ae3d6529587116dd456421274f4b82b"},"schema_version":"1.0","source":{"id":"1404.1378","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1404.1378","created_at":"2026-05-18T01:43:42Z"},{"alias_kind":"arxiv_version","alias_value":"1404.1378v1","created_at":"2026-05-18T01:43:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.1378","created_at":"2026-05-18T01:43:42Z"},{"alias_kind":"pith_short_12","alias_value":"6HQ37V6MJAOY","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_16","alias_value":"6HQ37V6MJAOYOLT4","created_at":"2026-05-18T12:28:16Z"},{"alias_kind":"pith_short_8","alias_value":"6HQ37V6M","created_at":"2026-05-18T12:28:16Z"}],"graph_snapshots":[{"event_id":"sha256:6e15faf98b94ea856fbf8d84e43d2fc1e3b2b6e289757fc71059ae98009fdbbd","target":"graph","created_at":"2026-05-18T01:43:42Z","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 discuss the restframe UV emission from the starbursting galaxy HFLS3 at z=6.34, discovered in Herschel/SPIRE data due to its red color in the submm wavelengths from 250-500 um. The apparent inst. SFR of HFLS3 inferred from the total FIR luminosity measured with over 15 photometric data points between 100 to 1000 um is 2900 Msun/yr. Keck/NIRC2 Ks band adaptive optics imaging data showed two potential NIR counterparts near HFLS3. Previously, the northern galaxy was taken to be in the foreground at z=2.1 while the southern galaxy was assumed to HFLS3's NIR counterpart. New HST/WFC3 and ACS ima","authors_text":"A. Conley, Asantha Cooray, B. Lofaro, Brian Ma, C. Bridge, C.M. Casey, D. Burgarella, D. Clements, D. Farrah, D. Riechers, D. Rigopoulou, D. Scott, D. Watson, G. Magdis, H. Fu, I. Pe'rez-Fournon, Jae Calanog, J. Bock, Julie L. Wardlow, M. Viero, N. Laporte, R. Gavazzi, R.J. Ivison, R.S. Bussmann, S.J. Oliver, W.A. Osage","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-04T20:00:38Z","title":"HerMES: The Rest-Frame UV Emission and A Lensing Model for the z=6.34 Luminous Dusty Starburst Galaxy HFLS3"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.1378","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":"sha256:46c7f926f796a9b6f7fa578b42f4bf656bb9eff4b30a016ad2177263154f2202","target":"record","created_at":"2026-05-18T01:43:42Z","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":"0da83135b98f53cc8b156f882807d21ddcf1b082c9c494c6be90ad6fe69160e6","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-04-04T20:00:38Z","title_canon_sha256":"f040690dcdaa76c0709aaa08067414987ae3d6529587116dd456421274f4b82b"},"schema_version":"1.0","source":{"id":"1404.1378","kind":"arxiv","version":1}},"canonical_sha256":"f1e1bfd7cc481d872e7cf1492ebd57d48e8ea2359fc17d4140d69b0b752946a6","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"f1e1bfd7cc481d872e7cf1492ebd57d48e8ea2359fc17d4140d69b0b752946a6","first_computed_at":"2026-05-18T01:43:42.058231Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:43:42.058231Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"/ThTuAYMElJ9cH2fxJNM7S+6x69gh6ttEs8Pmz0JD7hbQvFs+XXU5hJruRBYB8HOzVth3D72MX5D+HC761exBw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:43:42.058691Z","signed_message":"canonical_sha256_bytes"},"source_id":"1404.1378","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:46c7f926f796a9b6f7fa578b42f4bf656bb9eff4b30a016ad2177263154f2202","sha256:6e15faf98b94ea856fbf8d84e43d2fc1e3b2b6e289757fc71059ae98009fdbbd"],"state_sha256":"8a3f02113f3e6f6233dde36ddb6d80bcac8145a69b326a332245c04bbf4a2b0c"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"34G3w8peal7xx8kvI4o9UFIdv/o2DzKRhqdLuSgzV9uH5HLKgFDn3LbdgPnKcgvA6fFsJB+z3WMJCxPshCpxBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T06:00:47.742604Z","bundle_sha256":"f757dd5b77a03fb19c9d236c712ec99f13fcd45559b7185be02aa92af54deb05"}}