{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:K3N3FOVEVUJYN3B4QJF5HDEVAQ","short_pith_number":"pith:K3N3FOVE","canonical_record":{"source":{"id":"1411.2870","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-11T16:19:48Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"bc2dd476a943c124b65abcd7687185f9235f02eb45e81598c58bb1be94c6df4b","abstract_canon_sha256":"1ebd105983945d913169ed105bb59d2f2c8116b039009d4e36f9251a71e9d8bf"},"schema_version":"1.0"},"canonical_sha256":"56dbb2baa4ad1386ec3c824bd38c95042be090447a43dc1d1653995a02230fc0","source":{"kind":"arxiv","id":"1411.2870","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.2870","created_at":"2026-05-18T01:18:10Z"},{"alias_kind":"arxiv_version","alias_value":"1411.2870v1","created_at":"2026-05-18T01:18:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.2870","created_at":"2026-05-18T01:18:10Z"},{"alias_kind":"pith_short_12","alias_value":"K3N3FOVEVUJY","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"K3N3FOVEVUJYN3B4","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"K3N3FOVE","created_at":"2026-05-18T12:28:35Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:K3N3FOVEVUJYN3B4QJF5HDEVAQ","target":"record","payload":{"canonical_record":{"source":{"id":"1411.2870","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-11T16:19:48Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"bc2dd476a943c124b65abcd7687185f9235f02eb45e81598c58bb1be94c6df4b","abstract_canon_sha256":"1ebd105983945d913169ed105bb59d2f2c8116b039009d4e36f9251a71e9d8bf"},"schema_version":"1.0"},"canonical_sha256":"56dbb2baa4ad1386ec3c824bd38c95042be090447a43dc1d1653995a02230fc0","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:18:10.190905Z","signature_b64":"cnaBHqdrt7OKHMfEV8+Y2IXlgUVhYD1Q40Uphyyz7mM8Ppz5pcg1laxmvZ70ClqVdf+XqHJdwlCujpgUWudvDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"56dbb2baa4ad1386ec3c824bd38c95042be090447a43dc1d1653995a02230fc0","last_reissued_at":"2026-05-18T01:18:10.190311Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:18:10.190311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1411.2870","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":"2026-05-18T01:18:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"+47CdQPpIRiFHEtk1kGnI52pOm7ceZ5pRZTCPTpaAGv2vnuA5NG+1CvPHXKsEIQq4KxrQNpd2vJlQ9WVJ0nWBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T13:27:07.891560Z"},"content_sha256":"28eb3b73eba9dd776ee0f5d9e1cc4c781862d79c2f3997276937387866c2026c","schema_version":"1.0","event_id":"sha256:28eb3b73eba9dd776ee0f5d9e1cc4c781862d79c2f3997276937387866c2026c"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:K3N3FOVEVUJYN3B4QJF5HDEVAQ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Confirming the Quiescent Galaxy Population out to $z=3$: A Stacking Analysis of Mid-, Far-Infrared and Radio Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Alexander Karim, Allison W. S. Man, Andrew W. Zirm, Benjamin Magnelli, Caitlin M. Casey, David B. Sanders, Emeric Le Floc'h, Eva Schinnerer, Felipe Navarrete, Frank Bertoldi, Kartik Sheth, Mara Salvato, Nicholas Lee, Olivier Ilbert, Sune Toft, Thomas R. Greve, Vernesa Smolcic, Yanxia Li","submitted_at":"2014-11-11T16:19:48Z","abstract_excerpt":"We present stringent constraints on the average mid-, far-infrared and radio emissions of $\\sim$14200 quiescent galaxies (QGs), identified out to $z=3$ in the COSMOS field via their rest-frame NUV$-$r and r$-$J colors, and with stellar masses $M_{\\star}=10^{9.8-12.2} \\,M_{\\odot} $. Stacking in deep Spitzer (MIPS $24\\,\\mu$m), Herschel (PACS and SPIRE), and VLA (1.4 GHz) maps reveals extremely low dust-obscured star formation rates for QGs (SFR $<0.1-3\\,M_{\\odot}$yr$^{-1}$ at $z \\leqslant 2$ and $<6-18\\,M_{\\odot}$yr$^{-1}$ at $z > 2$), consistent with the low unobscured SFRs ($<0.01-1.2\\,M_{\\odo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.2870","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":"2026-05-18T01:18:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"JnPqeLuryLpFnHQfsfioe2sDUGNl3KCYy/2LgzvV4BKPriq9NG4Pc+kXxs1yWykNEn/T9dpbrqBUff7cCzyXBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T13:27:07.891916Z"},"content_sha256":"5965b080bde114703d5ef66f7d306bf94cd5ad0788983b2da790a21e54b47511","schema_version":"1.0","event_id":"sha256:5965b080bde114703d5ef66f7d306bf94cd5ad0788983b2da790a21e54b47511"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ/bundle.json","state_url":"https://pith.science/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ/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":"2026-06-04T13:27:07Z","links":{"resolver":"https://pith.science/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ","bundle":"https://pith.science/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ/bundle.json","state":"https://pith.science/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/K3N3FOVEVUJYN3B4QJF5HDEVAQ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:K3N3FOVEVUJYN3B4QJF5HDEVAQ","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":"1ebd105983945d913169ed105bb59d2f2c8116b039009d4e36f9251a71e9d8bf","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-11T16:19:48Z","title_canon_sha256":"bc2dd476a943c124b65abcd7687185f9235f02eb45e81598c58bb1be94c6df4b"},"schema_version":"1.0","source":{"id":"1411.2870","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.2870","created_at":"2026-05-18T01:18:10Z"},{"alias_kind":"arxiv_version","alias_value":"1411.2870v1","created_at":"2026-05-18T01:18:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.2870","created_at":"2026-05-18T01:18:10Z"},{"alias_kind":"pith_short_12","alias_value":"K3N3FOVEVUJY","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"K3N3FOVEVUJYN3B4","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"K3N3FOVE","created_at":"2026-05-18T12:28:35Z"}],"graph_snapshots":[{"event_id":"sha256:5965b080bde114703d5ef66f7d306bf94cd5ad0788983b2da790a21e54b47511","target":"graph","created_at":"2026-05-18T01:18:10Z","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 stringent constraints on the average mid-, far-infrared and radio emissions of $\\sim$14200 quiescent galaxies (QGs), identified out to $z=3$ in the COSMOS field via their rest-frame NUV$-$r and r$-$J colors, and with stellar masses $M_{\\star}=10^{9.8-12.2} \\,M_{\\odot} $. Stacking in deep Spitzer (MIPS $24\\,\\mu$m), Herschel (PACS and SPIRE), and VLA (1.4 GHz) maps reveals extremely low dust-obscured star formation rates for QGs (SFR $<0.1-3\\,M_{\\odot}$yr$^{-1}$ at $z \\leqslant 2$ and $<6-18\\,M_{\\odot}$yr$^{-1}$ at $z > 2$), consistent with the low unobscured SFRs ($<0.01-1.2\\,M_{\\odo","authors_text":"Alexander Karim, Allison W. S. Man, Andrew W. Zirm, Benjamin Magnelli, Caitlin M. Casey, David B. Sanders, Emeric Le Floc'h, Eva Schinnerer, Felipe Navarrete, Frank Bertoldi, Kartik Sheth, Mara Salvato, Nicholas Lee, Olivier Ilbert, Sune Toft, Thomas R. Greve, Vernesa Smolcic, Yanxia Li","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-11T16:19:48Z","title":"Confirming the Quiescent Galaxy Population out to $z=3$: A Stacking Analysis of Mid-, Far-Infrared and Radio Data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.2870","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":"sha256:28eb3b73eba9dd776ee0f5d9e1cc4c781862d79c2f3997276937387866c2026c","target":"record","created_at":"2026-05-18T01:18:10Z","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":"1ebd105983945d913169ed105bb59d2f2c8116b039009d4e36f9251a71e9d8bf","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-11-11T16:19:48Z","title_canon_sha256":"bc2dd476a943c124b65abcd7687185f9235f02eb45e81598c58bb1be94c6df4b"},"schema_version":"1.0","source":{"id":"1411.2870","kind":"arxiv","version":1}},"canonical_sha256":"56dbb2baa4ad1386ec3c824bd38c95042be090447a43dc1d1653995a02230fc0","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"56dbb2baa4ad1386ec3c824bd38c95042be090447a43dc1d1653995a02230fc0","first_computed_at":"2026-05-18T01:18:10.190311Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:18:10.190311Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"cnaBHqdrt7OKHMfEV8+Y2IXlgUVhYD1Q40Uphyyz7mM8Ppz5pcg1laxmvZ70ClqVdf+XqHJdwlCujpgUWudvDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:18:10.190905Z","signed_message":"canonical_sha256_bytes"},"source_id":"1411.2870","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:28eb3b73eba9dd776ee0f5d9e1cc4c781862d79c2f3997276937387866c2026c","sha256:5965b080bde114703d5ef66f7d306bf94cd5ad0788983b2da790a21e54b47511"],"state_sha256":"386cc2174fd9dfc2dace189377e3771cab3bab1bbd5bf86c33d9b10d3acbe126"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7Yxcm4xRAhJead0VfF8q+Lh7nfpHadwgCg/vWDYFbyCr3SQYbla2nf22UDNda9UjwsCzGhjPfxUwD7IFbGmPAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T13:27:07.894033Z","bundle_sha256":"d32c0df743a280d4b9cd4dd50d71d133f8ba345e4ffefa5ea8325e9839666af0"}}