{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:LGDE5QDUW5WVXT2L6VDH7437RV","short_pith_number":"pith:LGDE5QDU","canonical_record":{"source":{"id":"1001.1354","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-01-11T18:32:05Z","cross_cats_sorted":[],"title_canon_sha256":"38e77838213be9c5b39923fc487b240346ae6be6d23d770ef7bb104972afb6a7","abstract_canon_sha256":"7f39552bc38430f08adb1a58ab9bbcf10d71a417c8d03db96798427a9e75ef6a"},"schema_version":"1.0"},"canonical_sha256":"59864ec074b76d5bcf4bf5467ff37f8d4765f9a06490675e2813b24c5c3847fd","source":{"kind":"arxiv","id":"1001.1354","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1001.1354","created_at":"2026-05-18T02:10:03Z"},{"alias_kind":"arxiv_version","alias_value":"1001.1354v1","created_at":"2026-05-18T02:10:03Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1001.1354","created_at":"2026-05-18T02:10:03Z"},{"alias_kind":"pith_short_12","alias_value":"LGDE5QDUW5WV","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_16","alias_value":"LGDE5QDUW5WVXT2L","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_8","alias_value":"LGDE5QDU","created_at":"2026-05-18T12:26:10Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:LGDE5QDUW5WVXT2L6VDH7437RV","target":"record","payload":{"canonical_record":{"source":{"id":"1001.1354","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-01-11T18:32:05Z","cross_cats_sorted":[],"title_canon_sha256":"38e77838213be9c5b39923fc487b240346ae6be6d23d770ef7bb104972afb6a7","abstract_canon_sha256":"7f39552bc38430f08adb1a58ab9bbcf10d71a417c8d03db96798427a9e75ef6a"},"schema_version":"1.0"},"canonical_sha256":"59864ec074b76d5bcf4bf5467ff37f8d4765f9a06490675e2813b24c5c3847fd","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:10:03.600640Z","signature_b64":"WapEboJR4TkuWHCSKrBwXw+3AWSCSOSS56L/9Y6EqYqSvPoIYaN3qrpR9g4lZZu4I+lIxc39GmH/n4hpDp/GDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"59864ec074b76d5bcf4bf5467ff37f8d4765f9a06490675e2813b24c5c3847fd","last_reissued_at":"2026-05-18T02:10:03.600259Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:10:03.600259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1001.1354","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":"2026-05-18T02:10:03Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TY9e4+7Wzr33MQHIuyR3Y/CmcHyBs8tdytbhc4xlBubZYYJ1lzPTNG7ki40s0zs9DpgLvuhMH+U+kHQb/yIzDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T19:00:07.696732Z"},"content_sha256":"09eae1e337019586e4e042dfa619fd3c94020ff33d61f479c35e19b60e105b76","schema_version":"1.0","event_id":"sha256:09eae1e337019586e4e042dfa619fd3c94020ff33d61f479c35e19b60e105b76"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:LGDE5QDUW5WVXT2L6VDH7437RV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The VLA-COSMOS Perspective on the IR-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the IR/Radio Properties of Star Forming and AGN Galaxies at Intermediate and High Redshift","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Mart\\'inez-Sansigre, A. M. Koekemoer, C. M. Carollo, D. B. Sanders, D. T. Frayer, E. Le Floc'h, E. Murphy, E. Schinnerer, G. Zamorani, H. Aussel, J. Kartaltepe, Mark T. Sargent, M. Brusa, M. Salvato, N. Cappelluti, N. Z. Scoville, O. Ilbert, P. Oesch, S. J. Lilly, V. Smolcic","submitted_at":"2010-01-11T18:32:05Z","abstract_excerpt":"VLA 1.4 GHz (rms noise ~0.012 mJy) and MIPS 24 and 70 micron (rms noise ~0.02 and ~1.7 mJy, respectively) observations covering the 2 square degree COSMOS field are combined with an extensive multi-wavelength data set to study the evolution of the IR-radio relation at intermediate and high redshift. With ~4500 sources -- of which ~30% have spectroscopic redshifts -- the current sample is significantly larger than previous ones used for the same purpose. Both monochromatic IR/radio flux ratios (q24 & q70), as well as the ratio of the total IR and the 1.4 GHz luminosity (qTIR) are used as indica"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1001.1354","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":"2026-05-18T02:10:03Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iEsVtBbaLXNOkDWihY4C2OZ07toeTMdIHuskO+7PA79L93wIBHRhUdR2UGi5CF+EdtsN7KnFy7Bg6l6LR79PDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T19:00:07.697346Z"},"content_sha256":"d770085c08fa419ca35225d4f62c08dba7c9c3a5c7827b9f9a90ae5a097b5036","schema_version":"1.0","event_id":"sha256:d770085c08fa419ca35225d4f62c08dba7c9c3a5c7827b9f9a90ae5a097b5036"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/LGDE5QDUW5WVXT2L6VDH7437RV/bundle.json","state_url":"https://pith.science/pith/LGDE5QDUW5WVXT2L6VDH7437RV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/LGDE5QDUW5WVXT2L6VDH7437RV/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":"2026-05-27T19:00:07Z","links":{"resolver":"https://pith.science/pith/LGDE5QDUW5WVXT2L6VDH7437RV","bundle":"https://pith.science/pith/LGDE5QDUW5WVXT2L6VDH7437RV/bundle.json","state":"https://pith.science/pith/LGDE5QDUW5WVXT2L6VDH7437RV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/LGDE5QDUW5WVXT2L6VDH7437RV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:LGDE5QDUW5WVXT2L6VDH7437RV","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":"7f39552bc38430f08adb1a58ab9bbcf10d71a417c8d03db96798427a9e75ef6a","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-01-11T18:32:05Z","title_canon_sha256":"38e77838213be9c5b39923fc487b240346ae6be6d23d770ef7bb104972afb6a7"},"schema_version":"1.0","source":{"id":"1001.1354","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1001.1354","created_at":"2026-05-18T02:10:03Z"},{"alias_kind":"arxiv_version","alias_value":"1001.1354v1","created_at":"2026-05-18T02:10:03Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1001.1354","created_at":"2026-05-18T02:10:03Z"},{"alias_kind":"pith_short_12","alias_value":"LGDE5QDUW5WV","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_16","alias_value":"LGDE5QDUW5WVXT2L","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_8","alias_value":"LGDE5QDU","created_at":"2026-05-18T12:26:10Z"}],"graph_snapshots":[{"event_id":"sha256:d770085c08fa419ca35225d4f62c08dba7c9c3a5c7827b9f9a90ae5a097b5036","target":"graph","created_at":"2026-05-18T02:10:03Z","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":"VLA 1.4 GHz (rms noise ~0.012 mJy) and MIPS 24 and 70 micron (rms noise ~0.02 and ~1.7 mJy, respectively) observations covering the 2 square degree COSMOS field are combined with an extensive multi-wavelength data set to study the evolution of the IR-radio relation at intermediate and high redshift. With ~4500 sources -- of which ~30% have spectroscopic redshifts -- the current sample is significantly larger than previous ones used for the same purpose. Both monochromatic IR/radio flux ratios (q24 & q70), as well as the ratio of the total IR and the 1.4 GHz luminosity (qTIR) are used as indica","authors_text":"A. Mart\\'inez-Sansigre, A. M. Koekemoer, C. M. Carollo, D. B. Sanders, D. T. Frayer, E. Le Floc'h, E. Murphy, E. Schinnerer, G. Zamorani, H. Aussel, J. Kartaltepe, Mark T. Sargent, M. Brusa, M. Salvato, N. Cappelluti, N. Z. Scoville, O. Ilbert, P. Oesch, S. J. Lilly, V. Smolcic","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-01-11T18:32:05Z","title":"The VLA-COSMOS Perspective on the IR-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the IR/Radio Properties of Star Forming and AGN Galaxies at Intermediate and High Redshift"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1001.1354","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":"sha256:09eae1e337019586e4e042dfa619fd3c94020ff33d61f479c35e19b60e105b76","target":"record","created_at":"2026-05-18T02:10:03Z","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":"7f39552bc38430f08adb1a58ab9bbcf10d71a417c8d03db96798427a9e75ef6a","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-01-11T18:32:05Z","title_canon_sha256":"38e77838213be9c5b39923fc487b240346ae6be6d23d770ef7bb104972afb6a7"},"schema_version":"1.0","source":{"id":"1001.1354","kind":"arxiv","version":1}},"canonical_sha256":"59864ec074b76d5bcf4bf5467ff37f8d4765f9a06490675e2813b24c5c3847fd","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"59864ec074b76d5bcf4bf5467ff37f8d4765f9a06490675e2813b24c5c3847fd","first_computed_at":"2026-05-18T02:10:03.600259Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:10:03.600259Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"WapEboJR4TkuWHCSKrBwXw+3AWSCSOSS56L/9Y6EqYqSvPoIYaN3qrpR9g4lZZu4I+lIxc39GmH/n4hpDp/GDw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:10:03.600640Z","signed_message":"canonical_sha256_bytes"},"source_id":"1001.1354","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:09eae1e337019586e4e042dfa619fd3c94020ff33d61f479c35e19b60e105b76","sha256:d770085c08fa419ca35225d4f62c08dba7c9c3a5c7827b9f9a90ae5a097b5036"],"state_sha256":"5df24318129007ab3f5ce25211df251b0cd1f0d0702dde8d49caf11b47e8d110"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Fzf6QZ/y5V7G2/Pp7zj1b5BILerJlhKXtirzAhLCtLNJL1KAMLV9d+K6U7hb+bBikh98q2lNPcU68kxBVyG9CQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T19:00:07.700936Z","bundle_sha256":"82b463574b3f0b5fda66d711225d776a22795a29fad9aff602f93abea54f0d4f"}}