{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:3SDYNHTKHQPIIGYYVXJW43UMTR","short_pith_number":"pith:3SDYNHTK","canonical_record":{"source":{"id":"1506.05459","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-06-17T20:00:34Z","cross_cats_sorted":[],"title_canon_sha256":"84e724b103978167dc8a14f5da71da611722030640c5bd15ac2d95feab616034","abstract_canon_sha256":"c5ebac1b5ca02eed22c31f3d0cd1552befaddef8d62bcff319a19b27a3d77519"},"schema_version":"1.0"},"canonical_sha256":"dc87869e6a3c1e841b18add36e6e8c9c63afc0e1be2992bf9963aa82e4ece3b4","source":{"kind":"arxiv","id":"1506.05459","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1506.05459","created_at":"2026-05-18T01:33:42Z"},{"alias_kind":"arxiv_version","alias_value":"1506.05459v2","created_at":"2026-05-18T01:33:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.05459","created_at":"2026-05-18T01:33:42Z"},{"alias_kind":"pith_short_12","alias_value":"3SDYNHTKHQPI","created_at":"2026-05-18T12:29:02Z"},{"alias_kind":"pith_short_16","alias_value":"3SDYNHTKHQPIIGYY","created_at":"2026-05-18T12:29:02Z"},{"alias_kind":"pith_short_8","alias_value":"3SDYNHTK","created_at":"2026-05-18T12:29:02Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:3SDYNHTKHQPIIGYYVXJW43UMTR","target":"record","payload":{"canonical_record":{"source":{"id":"1506.05459","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-06-17T20:00:34Z","cross_cats_sorted":[],"title_canon_sha256":"84e724b103978167dc8a14f5da71da611722030640c5bd15ac2d95feab616034","abstract_canon_sha256":"c5ebac1b5ca02eed22c31f3d0cd1552befaddef8d62bcff319a19b27a3d77519"},"schema_version":"1.0"},"canonical_sha256":"dc87869e6a3c1e841b18add36e6e8c9c63afc0e1be2992bf9963aa82e4ece3b4","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:33:42.873738Z","signature_b64":"eocR+3qOcwK1LNqdJBuuPmTPy/6MEUqKzxH1titKphMPPbOw1aTrIBTTdn3lTN716MHpZJ7xV84FEr7FXOgWBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dc87869e6a3c1e841b18add36e6e8c9c63afc0e1be2992bf9963aa82e4ece3b4","last_reissued_at":"2026-05-18T01:33:42.873206Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:33:42.873206Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1506.05459","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":"2026-05-18T01:33:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Y3FTtcU26pjaFPZ37ESk9PxzvKkMO7HBeE5Oo/0OW3DVmenie4Rtl1v3j5/DmwoawXkOh2vrx9N32meJUmd5Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T14:49:25.052111Z"},"content_sha256":"1f0544a1ac0923bdfdd3ec364c998e764455a68fb7d57720725ae3194737cd49","schema_version":"1.0","event_id":"sha256:1f0544a1ac0923bdfdd3ec364c998e764455a68fb7d57720725ae3194737cd49"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:3SDYNHTKHQPIIGYYVXJW43UMTR","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"ALMA and Herschel reveal that X-ray selected AGN and main-sequence galaxies have different star formation rate distributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Del Moro, C. M. Harrison, C. Schreiber, D. Elbaz, D. Liu, D. M. Alexander, D. Rosario, E. Bernhard, E. Daddi, F. Stanley, J. Aird, J. R. Mullaney (Sheffield, J. Simpson, M. Dickinson, M. Pannella, M. Sargent, P. Santini, S. Juneau, UK)","submitted_at":"2015-06-17T20:00:34Z","abstract_excerpt":"Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray selected AGN host galaxies at 0.5<z<1.5 and 1.5<z<4, comparing them to that of normal, star-forming (i.e., \"main-sequence\", or MS) galaxies. We find 34--55 per cent of AGNs in our sample have SFRs at least a factor of two below that of the average MS galaxy, compared to ~15 per cent of all MS galaxies, suggesting significantly different SFR distributions. Indeed, when both are modelled as log-normal distributions, the mass and redshift-normalised SFR distributions of X-ray AGNs are ro"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.05459","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":"2026-05-18T01:33:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Y3GNUGxxfhv9wKLUaeTqpJzasCRZeSpF8qVovuolZsZf6X4fr2szrfgeqw3lkSww71JjWtrcslbLduBEcv4xAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T14:49:25.052837Z"},"content_sha256":"baecae86f79e7cd5c5438f49320415bb4adcbf9970e08e5b1bc9424762b4d2b8","schema_version":"1.0","event_id":"sha256:baecae86f79e7cd5c5438f49320415bb4adcbf9970e08e5b1bc9424762b4d2b8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/3SDYNHTKHQPIIGYYVXJW43UMTR/bundle.json","state_url":"https://pith.science/pith/3SDYNHTKHQPIIGYYVXJW43UMTR/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/3SDYNHTKHQPIIGYYVXJW43UMTR/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":"2026-06-06T14:49:25Z","links":{"resolver":"https://pith.science/pith/3SDYNHTKHQPIIGYYVXJW43UMTR","bundle":"https://pith.science/pith/3SDYNHTKHQPIIGYYVXJW43UMTR/bundle.json","state":"https://pith.science/pith/3SDYNHTKHQPIIGYYVXJW43UMTR/state.json","well_known_bundle":"https://pith.science/.well-known/pith/3SDYNHTKHQPIIGYYVXJW43UMTR/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:3SDYNHTKHQPIIGYYVXJW43UMTR","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":"c5ebac1b5ca02eed22c31f3d0cd1552befaddef8d62bcff319a19b27a3d77519","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-06-17T20:00:34Z","title_canon_sha256":"84e724b103978167dc8a14f5da71da611722030640c5bd15ac2d95feab616034"},"schema_version":"1.0","source":{"id":"1506.05459","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1506.05459","created_at":"2026-05-18T01:33:42Z"},{"alias_kind":"arxiv_version","alias_value":"1506.05459v2","created_at":"2026-05-18T01:33:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.05459","created_at":"2026-05-18T01:33:42Z"},{"alias_kind":"pith_short_12","alias_value":"3SDYNHTKHQPI","created_at":"2026-05-18T12:29:02Z"},{"alias_kind":"pith_short_16","alias_value":"3SDYNHTKHQPIIGYY","created_at":"2026-05-18T12:29:02Z"},{"alias_kind":"pith_short_8","alias_value":"3SDYNHTK","created_at":"2026-05-18T12:29:02Z"}],"graph_snapshots":[{"event_id":"sha256:baecae86f79e7cd5c5438f49320415bb4adcbf9970e08e5b1bc9424762b4d2b8","target":"graph","created_at":"2026-05-18T01:33:42Z","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":"Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray selected AGN host galaxies at 0.5<z<1.5 and 1.5<z<4, comparing them to that of normal, star-forming (i.e., \"main-sequence\", or MS) galaxies. We find 34--55 per cent of AGNs in our sample have SFRs at least a factor of two below that of the average MS galaxy, compared to ~15 per cent of all MS galaxies, suggesting significantly different SFR distributions. Indeed, when both are modelled as log-normal distributions, the mass and redshift-normalised SFR distributions of X-ray AGNs are ro","authors_text":"A. Del Moro, C. M. Harrison, C. Schreiber, D. Elbaz, D. Liu, D. M. Alexander, D. Rosario, E. Bernhard, E. Daddi, F. Stanley, J. Aird, J. R. Mullaney (Sheffield, J. Simpson, M. Dickinson, M. Pannella, M. Sargent, P. Santini, S. Juneau, UK)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-06-17T20:00:34Z","title":"ALMA and Herschel reveal that X-ray selected AGN and main-sequence galaxies have different star formation rate distributions"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.05459","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":"sha256:1f0544a1ac0923bdfdd3ec364c998e764455a68fb7d57720725ae3194737cd49","target":"record","created_at":"2026-05-18T01:33:42Z","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":"c5ebac1b5ca02eed22c31f3d0cd1552befaddef8d62bcff319a19b27a3d77519","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-06-17T20:00:34Z","title_canon_sha256":"84e724b103978167dc8a14f5da71da611722030640c5bd15ac2d95feab616034"},"schema_version":"1.0","source":{"id":"1506.05459","kind":"arxiv","version":2}},"canonical_sha256":"dc87869e6a3c1e841b18add36e6e8c9c63afc0e1be2992bf9963aa82e4ece3b4","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"dc87869e6a3c1e841b18add36e6e8c9c63afc0e1be2992bf9963aa82e4ece3b4","first_computed_at":"2026-05-18T01:33:42.873206Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:33:42.873206Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"eocR+3qOcwK1LNqdJBuuPmTPy/6MEUqKzxH1titKphMPPbOw1aTrIBTTdn3lTN716MHpZJ7xV84FEr7FXOgWBQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:33:42.873738Z","signed_message":"canonical_sha256_bytes"},"source_id":"1506.05459","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:1f0544a1ac0923bdfdd3ec364c998e764455a68fb7d57720725ae3194737cd49","sha256:baecae86f79e7cd5c5438f49320415bb4adcbf9970e08e5b1bc9424762b4d2b8"],"state_sha256":"0b37be336c9e91192f79e411e9c88218137b16f5ffba913569e6e02405abcb43"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"gIWQ+Z5M9JQmpooA5h1uLrkKrYOUEgET9gnYhdhsdb85IN9vD7ra+54dwBKxGvzxrbNNb0Hh7BgDnPFk2uLrBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-06T14:49:25.056468Z","bundle_sha256":"a2f0c301e6967ae05b176cf17da256912b02856755134cfabd0dfc900657d062"}}