{"as_of":"2026-08-16T06:07:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fad568877f295e271b6df958b5e7288a42f4a893a976f629ff44cb99a3fb71b1","coverage":[{"denominator":66,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":66,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T00:51:23.241476Z","state":"measured"},{"denominator":66,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":66,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2505.02687/citation-record","integrity":"/paper/2505.02687/integrity","json":"/paper/2505.02687/citation-record.json","paper":"/paper/2505.02687"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.865215Z","title":"2016, ApJ, 825, 72","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.865215Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:785462a6f9a5ed947631c6e47caa28b943d80fbc92a2a356da2aba2b39144917","observation_id":"ac6b82d0-aea0-46ed-a7a0-e9c76f5216d6","resolution":{"observed_at":"2026-08-16T00:51:22.865215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.871575Z","title":"H., Jagannathan, P., & Nyland, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.871575Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:7769ee603159993dfe5e01f3d1df83f67add53223aaa772dbfe5221834b52b2e","observation_id":"0f10cbce-a10d-49e3-b638-d0c52e4ef5ee","resolution":{"observed_at":"2026-08-16T00:51:22.871575Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:24.212765Z","title":"& Owen, F","venue":null,"work_id":"7777d732-0ab3-44b9-b476-9801c4423af6","year":1995},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.876932Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:55157115df711d53dbcccbd7424cbd15d7a54a809dd504c6d78fd4a135dac715","observation_id":"021fbcd5-1660-4e70-9426-5cb59207b2ad","resolution":{"observed_at":"2026-08-16T00:51:24.217736Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.882300Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.882300Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:5e0046c2b3e947ec644f83d8916f40b12e28720a39f69c62fe744cd7d92dbbfb","observation_id":"c6b99fde-cef8-473c-9e6c-b872b7da28d4","resolution":{"observed_at":"2026-08-16T00:51:22.882300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.888415Z","title":"2024, A&A, 686, A82","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.888415Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:af25dd51d3d46ff44e89af87bfadc5b7333cdcfebdfaa8942cb5b3da63edb359","observation_id":"3e2691de-3aa3-4cb3-a0a1-1b3bc4dfd935","resolution":{"observed_at":"2026-08-16T00:51:22.888415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:24.171911Z","title":"2015, MNRAS, 453, 1079","venue":null,"work_id":"554c3288-5f6f-4193-b19d-cbeb35340f51","year":2015},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.893606Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:536d6c8a146f4a648c7336347d3a558f00832c476ef77588a5e9c6883005faa3","observation_id":"5c287739-0f44-4652-b559-6a4a7334af00","resolution":{"observed_at":"2026-08-16T00:51:24.177392Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.899830Z","title":"& Gavazzi, G","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.899830Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:635aadc3fd644aea95eaae80a991d2967dd2743295fb71c662fb81e60cb385a7","observation_id":"30643ced-9301-4339-8600-a25ad2642d42","resolution":{"observed_at":"2026-08-16T00:51:22.899830Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.905230Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.905230Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:fd71eb93db2627afbe1492ef5df18e26267cef521ef79fdcf3122e7f2c676548","observation_id":"59d2bc6b-37bf-4ea2-ab59-7d225b38f16d","resolution":{"observed_at":"2026-08-16T00:51:22.905230Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.910748Z","title":"H., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.910748Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:bd94b300485549cebe3a1ade15f08b5f43fc09826d4c846bb2227051d7243ae0","observation_id":"647849f0-901d-408e-a55c-4305f5873c0e","resolution":{"observed_at":"2026-08-16T00:51:22.910748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.915718Z","title":"A., Gonzalez, A","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.915718Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:890d189c626ebc37b24ef95d675443db584ce50497d83787f55234cc6a1f9019","observation_id":"016d1687-a3db-4292-ad67-51256b7633e2","resolution":{"observed_at":"2026-08-16T00:51:22.915718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:24.110873Z","title":"2011, ApJ, 732, 33 CASA Team, Bean, B., Bhatnagar, S., et al","venue":null,"work_id":"a94bd4f4-9c71-4e07-bbee-c39b2d7a33ee","year":2011},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.920939Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:0934d1b4ecfc719d6a5942c34138824bcad8df6876780705cc602a2a8726432e","observation_id":"c79848b0-1d58-4079-8fcf-90ff7e70c13c","resolution":{"observed_at":"2026-08-16T00:51:24.115805Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.925901Z","title":"C., Blain, A","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.925901Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:bc77a0de81f8de599734ba5832ff74156bb6bcebc5cc98d2c03537bd435cf8b5","observation_id":"da83df26-30a0-42f9-ace4-d1614ebe72bd","resolution":{"observed_at":"2026-08-16T00:51:22.925901Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.931983Z","title":"M., Kochanek, C","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.931983Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:9bd1dc4954cc8eb2ca688445046ce0efbfa79f190ae230141eb706cae9aa9138","observation_id":"73f7ba34-8f21-43e1-bbef-2bd976120497","resolution":{"observed_at":"2026-08-16T00:51:22.931983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.937503Z","title":null,"venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.937503Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:046e22af3ec7d47a570c9283a163bb4ddb596cc56c0047d4276aa54e1b60706d","observation_id":"5ad085b7-a763-41e3-b89b-a8ee19758385","resolution":{"observed_at":"2026-08-16T00:51:22.937503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.942839Z","title":"J., Anderson, M","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.942839Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:1a05af0c022dd05ce2e1c52f11f2abbab3ff5ef230049960162a8c64eacce1c8","observation_id":"8b2fdd53-43d4-44b0-8c7d-1b51227269c6","resolution":{"observed_at":"2026-08-16T00:51:22.942839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:24.044683Z","title":"C., Newman, J","venue":null,"work_id":"543790dd-3c93-43c3-afbf-d50131b339be","year":2008},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.948890Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:5ae906c7f823a1e892943aa81b5cce74bfbc9d3190b3c09aa769ceebc057b27d","observation_id":"fc0e8fec-5811-4575-b126-7644de63ab44","resolution":{"observed_at":"2026-08-16T00:51:24.049838Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:24.027294Z","title":"2007, ApJ, 670, 156 Del Moro, A., Alexander, D","venue":null,"work_id":"187bb3b0-3fc1-4ea7-8e82-dcab262d49fa","year":2007},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.954232Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:85a18d33acee72b4e5f405f0f9ee9e171510eb6630917d6234d4b66ebcbaae4b","observation_id":"453b6b3e-c6ae-4764-9601-dbd74b73cd01","resolution":{"observed_at":"2026-08-16T00:51:24.032695Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.959819Z","title":"T., et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.959819Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:3e561d8918860ab33430f8f775b84deb623306ab42cd72ca481d3e46febe24f5","observation_id":"d6c313c1-9430-4277-9c7b-e83606eec10f","resolution":{"observed_at":"2026-08-16T00:51:22.959819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.965424Z","title":"2017, A&A, 602, A3","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.965424Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:f12049036a55967956ce006bcfbe24d1b3f5a02509244dfbba7e22820b665e18","observation_id":"e01a2df2-9709-4ff5-b5c8-8b9fcad87976","resolution":{"observed_at":"2026-08-16T00:51:22.965424Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.977972Z","title":"& Prodanovi´c, T","venue":null,"work_id":"b16906a8-9f08-4816-a463-24ad8e2f90a7","year":2015},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.971658Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:0e00f702afbe1974f18ccd12e668ddee7c61685427f0674998713e1c7deb7e47","observation_id":"5709942b-a22f-4981-88b6-e71454caf7e1","resolution":{"observed_at":"2026-08-16T00:51:23.991061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.977427Z","title":"L., Koekemoer, A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.977427Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:3bf3e362d362ffc799f69ee9d7062e6a65ec680712c8b586d89155c5140275f8","observation_id":"ad5ad930-14d3-45fb-9c8c-9e6d90774a49","resolution":{"observed_at":"2026-08-16T00:51:22.977427Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.946466Z","title":"L., Rieke, G","venue":null,"work_id":"daaf7348-8529-4d0d-bda6-545e263be690","year":2005},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.983536Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:d0eb5fbd51ea91bc50f799b8f61f0d2c93f0a28adfb361aa82897b2544191186","observation_id":"1a8f28e8-a370-4c64-9c74-f2c535492c5d","resolution":{"observed_at":"2026-08-16T00:51:23.951786Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.926754Z","title":null,"venue":null,"work_id":"9978102e-9e9d-4b2d-a775-125acc634634","year":2008},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.988698Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:2bb1b8e20ccf1f58c53ddd1cf7776a6a32c86ffabb5cf533ed9fa6bcefc38a88","observation_id":"1d035c2d-e573-4cac-a261-3562ac31f5da","resolution":{"observed_at":"2026-08-16T00:51:23.932481Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.993734Z","title":"2007, A&A, 468, 33","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.993734Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:07c67d1f3c145cdcbe3c2efb750f3cfffdd94a25932193a6530f44396bb19f58","observation_id":"a246d069-efd0-44b7-9784-0755116d298a","resolution":{"observed_at":"2026-08-16T00:51:22.993734Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:22.998983Z","title":"S., et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:22.998983Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:209481c5d63e5daaf18afdfb37e8d36f3511fc4ff3227ebe82bce82a9c9d202b","observation_id":"a3f07a14-ad57-419d-89c5-a18ce56e167e","resolution":{"observed_at":"2026-08-16T00:51:22.998983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.887363Z","title":"2022, MNRAS, 511, 1408","venue":null,"work_id":"2c442013-b1dc-43ce-8fc7-0bcfa62bd88a","year":2022},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.004544Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:21bf243c5cf7269c7d1dcfd01bb72dd83e14cd9fb24dcab0b2dac95f27a0ec8a","observation_id":"da1a3acd-9426-49e2-aab9-2b6fcf196a6b","resolution":{"observed_at":"2026-08-16T00:51:23.892529Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.009482Z","title":"T., & Rowan-Robinson, M","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.009482Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:df5a6fba899a0488107f990dbd3f97edc1ecacdeda37fab57038987a969869d1","observation_id":"eaa62f58-fc43-46ad-851f-a4ed794b495f","resolution":{"observed_at":"2026-08-16T00:51:23.009482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.016520Z","title":"A., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.016520Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:f5e860679380dbc105870cd10e06a928ea931a317bf2fb861847ae7eb76d0201","observation_id":"408ee2ce-870e-4b97-a13d-88e4064d7727","resolution":{"observed_at":"2026-08-16T00:51:23.016520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.848734Z","title":"J., Magnelli, B., Ibar, E., et al","venue":null,"work_id":"c4ce0455-6268-4ac3-9dac-49bec0a27a02","year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.022156Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:cb9db9b661e867176a5fd3210b91c2394fb004dde9ac673fdcf3bcd5242d3862","observation_id":"c0aed53f-9a77-4db9-8769-32dc08e219f7","resolution":{"observed_at":"2026-08-16T00:51:23.853636Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.832749Z","title":"J., Smith, D","venue":null,"work_id":"4a86ef26-fa20-439d-9cde-f5ff31ad6089","year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.028016Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:09b98c472bfbd9a6b0bdb5fe9f2f03037476367a054c1b3199db8791e40d70b7","observation_id":"b5df710e-385b-4576-aa52-011c1852347c","resolution":{"observed_at":"2026-08-16T00:51:23.838112Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.033507Z","title":"J., Dawson, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.033507Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:76260a7303aa725a9894d30b8bc6980956e684c4a2d7ce6575f719b52dcb99b5","observation_id":"0b889c24-28b4-4843-b76e-74b256cdc45e","resolution":{"observed_at":"2026-08-16T00:51:23.033507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.805283Z","title":"S., Daddi, E., Coogan, R","venue":null,"work_id":"c9601826-0a04-416f-82e8-193857db9f76","year":2021},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.042717Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:a30871ec3bbf4cff31e97dc820084415a8160678767c9b607ba9e869f21a20c2","observation_id":"91b89821-0b99-42da-ac2b-d59acfcb1bc0","resolution":{"observed_at":"2026-08-16T00:51:23.810279Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.788080Z","title":"2013, ApJ, 763, 123","venue":null,"work_id":"1b9db034-e174-408b-935a-c47debe071b6","year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.048512Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:83cc7552bb65ef05260899077f2b397fd3e48fc5f4d76fae7f014404a8d77490","observation_id":"3c71224a-8ed3-4839-8391-8bda8959a287","resolution":{"observed_at":"2026-08-16T00:51:23.794129Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1308.6483","last_updated":"2013-08-29T14:34:43Z","snapshot_observed_at":"2026-08-15T00:05:02.399572Z","submitted_at":"2013-08-29T14:34:43Z","title":"Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies: Supplemental Material","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.6483","snapshot_observed_at":"2026-08-16T00:51:23.053691Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.053691Z"},"links":{"cited_paper":"/paper/1308.6483","citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:5c0f7ce96337f620f1b68dc6db6f1a517dd532e43fe594220e568f9bb4740178","observation_id":"5941aa8b-d9e9-4d27-8ea3-01184ac8ac6e","resolution":{"observed_at":"2026-08-16T00:51:23.053691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.060035Z","title":"2024, A&A, 686, A55","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.060035Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:cdf82720476320efcea2618a5fa6201c121527625de42d80873c20f2f177b0b1","observation_id":"b56f77e9-c0c2-4377-af87-319086260cae","resolution":{"observed_at":"2026-08-16T00:51:23.060035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.760634Z","title":"& Rieke, G","venue":null,"work_id":"f813b88b-337d-4335-b38b-2107e226bc6e","year":1972},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.068653Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:8307709ec94fb491be0956cd847f65bef682f87f81ebba3313ea0e5ba8dc0efa","observation_id":"30901829-6ae8-48e5-9cc0-4aa41fa8a6cd","resolution":{"observed_at":"2026-08-16T00:51:23.765600Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.743153Z","title":"H., & Rujopakarn, W","venue":null,"work_id":"c4943958-43bd-4ddc-a655-55eea40b607f","year":2022},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.074940Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:9bcda7d9d1e55a174d5b874486c322fb74ed9c626de67fa69f8073d3a136ecda","observation_id":"cdadb193-7d0f-4d49-92ac-d975fcd94478","resolution":{"observed_at":"2026-08-16T00:51:23.748921Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.080896Z","title":"J., Lutz, D., et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.080896Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:f2f07a75d0634cf0b9c1dc274f5a127a263264c30957900bb35e886bc8b8973b","observation_id":"4a09de9a-5171-48de-a6c6-ff9006d26870","resolution":{"observed_at":"2026-08-16T00:51:23.080896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.088988Z","title":"L., Gonzalez, A","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.088988Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:ac8c5930415867e5fc0a6196740f95f493ed7d5362945b918919812079d6dcf6","observation_id":"a151fa9d-33de-4639-930a-669d4a7b0b8b","resolution":{"observed_at":"2026-08-16T00:51:23.088988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.094195Z","title":"D., Brodwin, M., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.094195Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:ed492d4fdddf463bc8995f7bb3cc3421f293f8bd00b5e59cec96cafd97d689be","observation_id":"61e11295-818e-4fff-b149-630a07c3577b","resolution":{"observed_at":"2026-08-16T00:51:23.094195Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.686385Z","title":"C., Carroll, C","venue":null,"work_id":"b5720912-ffad-4fce-ad01-7c281a3cc3ab","year":2020},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.099557Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:791a6c2d63bd531c36ddd1c263c5e0f6b5ba23adfb5ff8cfd61617db193c442f","observation_id":"a6a34046-de93-4ff4-90b0-e904c8c1fdb7","resolution":{"observed_at":"2026-08-16T00:51:23.691757Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.104477Z","title":"P., Waters, B., Schiebel, D., Young, W., & Golap, K","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.104477Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:cdf3e8ac7e5a687e18028b0db4a7c6160ec23211d12db412ff4aaf8322bbd7fc","observation_id":"7f0de8ee-3cd7-4b08-85fb-d43f49188402","resolution":{"observed_at":"2026-08-16T00:51:23.104477Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.658019Z","title":null,"venue":null,"work_id":"7ebbca2c-2d5e-4ca8-adb8-822103d2fbfa","year":2001},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.109420Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:33b342083863f8c67df294609931af555c999553a2bbce1d0164eef0d62f150a","observation_id":"c52c3534-3a9d-4980-9427-7dbc37c7966a","resolution":{"observed_at":"2026-08-16T00:51:23.663247Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.641374Z","title":"& Ra fferty, D","venue":null,"work_id":"319eb542-08d4-4976-8113-cb3cad378f0a","year":2015},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.114678Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:278db59b995cce720a5b13175b84961487755e278bc9e6a7a8c6db5195c00c37","observation_id":"62676c95-624f-4b18-982e-37746aad2638","resolution":{"observed_at":"2026-08-16T00:51:23.646557Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.622556Z","title":"C., Sargent, M","venue":null,"work_id":"b7d0d55b-5504-4a62-b510-3ddd8098b140","year":2021},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.121229Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:0b17474502da4ce63a698cbf3714620c2a3f863cd69ef9b8c816f88a5bb4bb34","observation_id":"773fcf0b-caf8-4b35-8c10-14e309f823d8","resolution":{"observed_at":"2026-08-16T00:51:23.629546Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.126965Z","title":"2023, A&A, 672, A98","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.126965Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:5b31d40706ca29326e4be3cf9b7f625bd8560c62c083f8b6c585641e3cefbf96","observation_id":"15cedc46-7995-4a41-850e-0b0ff78abe66","resolution":{"observed_at":"2026-08-16T00:51:23.126965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.132814Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.132814Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:fbcf326ce5f9816d7b5cfbcfc372a92ad9c08659d062f3eb06325287a990ef91","observation_id":"93716bec-eb4a-4040-ae36-a869cd113d11","resolution":{"observed_at":"2026-08-16T00:51:23.132814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.138426Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.138426Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:828c87dd90974a7690d1a6f4d795b8415b726357b41a3b3b2bd7e741df4342e0","observation_id":"51241344-639b-45f1-9c5f-e74431b4827f","resolution":{"observed_at":"2026-08-16T00:51:23.138426Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.143639Z","title":"J., Bremseth, J., Mason, B","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.143639Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:ddaf8f4281860191757cc04790f4120d5b3e08c056c2329780c93aeaf5504888","observation_id":"c13a0b9c-0566-4270-a8ed-0dd3ccb0fd04","resolution":{"observed_at":"2026-08-16T00:51:23.143639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.149373Z","title":"J., Condon, J","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.149373Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:6946076f80fefe42a96321116bc6cb05d7c49eabb383e23d2083cec39f0cd41e","observation_id":"5c350aca-0a84-4916-a04e-fab6280f0fa6","resolution":{"observed_at":"2026-08-16T00:51:23.149373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.155394Z","title":"2020, MNRAS, 499, 3061","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.155394Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:d5f1cef7a73cfc85e4bc52415e13dd7785780a3fd37acf27a1cbba040a1df144","observation_id":"acaed3ce-cefc-4a82-b115-919f5fa6bdb4","resolution":{"observed_at":"2026-08-16T00:51:23.155394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.160406Z","title":"B., Muzzin, A., van der Burg, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.160406Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:63ebee49f05f94d87cc7ef3082a9628161b95ab56c326db17e0373b16047cfad","observation_id":"70a98d88-3e94-4a59-9185-9e249cdeda8c","resolution":{"observed_at":"2026-08-16T00:51:23.160406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.508308Z","title":"2017, Frontiers in Astronomy and Space Sciences, 4, 35 Pavlovi´c, , M., Prodanovi´c, & , T","venue":null,"work_id":"6e95ece1-ec02-4de8-8664-3c6c48d0fcd5","year":2017},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.165682Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:400ba755ab4c072a1dc177a168f55ea93fe0a52f93bf6441d7f28872ddc47773","observation_id":"de0cc89e-3d72-4b32-b155-ff47fa976dc6","resolution":{"observed_at":"2026-08-16T00:51:23.514323Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.490865Z","title":"B., Cochrane, R","venue":null,"work_id":"513524ce-e83c-42a4-b9cb-cff19191c348","year":2025},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.171990Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:2f323ab9803e001fddc680f267e90104091a1b5c05dca909ac856d7405687d73","observation_id":"a7d4dbce-8b50-4374-a37c-75fe7702990c","resolution":{"observed_at":"2026-08-16T00:51:23.496951Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.177952Z","title":"2011, A&A, 532, A145","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.177952Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:eac3b61f1f47f21afedafcc5187c541315d2907a480461620d9821cb51a4443c","observation_id":"17071284-35b8-4bf1-be7f-fab895dcc788","resolution":{"observed_at":"2026-08-16T00:51:23.177952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.461805Z","title":"M., Crawford, S","venue":null,"work_id":"695b12eb-cca8-41d1-a7a8-3c1852000fba","year":2015},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.183095Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:d5abb68493df78fbaa864ed7f00d52825e368d99df01ee4b85bd6c88e578b82f","observation_id":"28c0a07a-d03f-432a-b9a0-5968348b64fd","resolution":{"observed_at":"2026-08-16T00:51:23.466775Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.442223Z","title":null,"venue":null,"work_id":"8ace00eb-4959-44ad-ad3b-ebe8c63bd265","year":2004},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.188323Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:b395386540c93a0a7aafe53ba471ecdf7e42caeb212d4b4a31d602252bd762f6","observation_id":"833f9e03-b209-4f2e-bb0a-29a01811f3ac","resolution":{"observed_at":"2026-08-16T00:51:23.448208Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.195238Z","title":"H., Alonso-Herrero, A., Weiner, B","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.195238Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:b519d74e7ce9368c5351a90fd1bfa7a453dd3bac53da9ef3441fc7b04d6e4907","observation_id":"71d0c2bb-e42e-47c4-a4e7-27e245501f7f","resolution":{"observed_at":"2026-08-16T00:51:23.195238Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.200554Z","title":"2008, ApJ, 683, 659","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.200554Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:777d41763e2947b5ea285ff45b2e96cd702b01273b6b3d1b26eb260ee68d97fb","observation_id":"b6e44803-4c5f-45b6-a264-c218d1a0e9d5","resolution":{"observed_at":"2026-08-16T00:51:23.200554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.401052Z","title":"2010, A&A, 518, L154","venue":null,"work_id":"52027ee8-5421-493d-bc1e-dc6608ae470a","year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.206752Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:f35a537f694226e27372dfa6e8d6f7529ce8ce0feb9b4dc29e5888c820b48b45","observation_id":"8b313199-8f6f-4368-b088-43b9f53d9215","resolution":{"observed_at":"2026-08-16T00:51:23.405921Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.213089Z","title":"T., Schinnerer, E., Murphy, E., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.213089Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:e00b651c9bde4f9c89e6387f4c3037a651ebbd4b987ac1fdc06da2666103f89b","observation_id":"e8d6ca3c-61d2-41d1-8bd4-c29f55498685","resolution":{"observed_at":"2026-08-16T00:51:23.213089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.371414Z","title":"2013, ApJS, 206, 3 Smolˇci´c, V ., Karim, A., Miettinen, O., et al","venue":null,"work_id":"ef4659c0-d6c1-4069-886d-2414982f4e0e","year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.219494Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:a4270f8d483e550be52b07ec9c82c0baf8a5176fe47748a7e5116fc677d247b3","observation_id":"6fec50e1-545b-485a-9373-43a4fc373853","resolution":{"observed_at":"2026-08-16T00:51:23.376566Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.352893Z","title":"2005, A MIPS Study of Star Formation in a Protocluster at z=2.1, Spitzer Proposal ID 20593","venue":null,"work_id":"3b3322ef-dc31-40a9-b6f4-e05cfb728ac1","year":2005},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.225150Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:e652d56d9d0cd876f3e73023524205f8c7d7373860da78c2ad39a87372630342","observation_id":"d2a34f2d-4c91-49d8-95c5-606290834b9c","resolution":{"observed_at":"2026-08-16T00:51:23.359356Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.333672Z","title":"H., Papovich, C., Saintonge, A., et al","venue":null,"work_id":"15d85524-3c23-41a1-adaa-d8ec401725ba","year":2010},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.230219Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:09c596fd9af4b39c81fb94e742537facc6ed1b3eebda557bf3e37525676cdd49","observation_id":"f4527c00-464d-4ace-8c09-3d32055173f3","resolution":{"observed_at":"2026-08-16T00:51:23.340413Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.235806Z","title":"S., Reddy, N","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.235806Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:47997e5688061a9b100002a5f07fa1a33247ad9d03e3568951729ae3ed8dbf82","observation_id":"e3316244-e942-4b48-b44c-97ee3dbad583","resolution":{"observed_at":"2026-08-16T00:51:23.235806Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-16T00:51:23.303184Z","title":"R., Stanford, S","venue":null,"work_id":"7d1626da-03bf-44d7-85aa-95688d202b2a","year":2013},"citing_paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-16T00:51:23.241476Z"},"links":{"citing_paper":"/paper/2505.02687"},"observation_digest":"sha256:9d99105de17d73984dafd44ee01e1a0221b051bdb4e8df4f9378e263b1dc90e2","observation_id":"c1e7f8fe-b5e2-43f1-8da6-7be74be31c7d","resolution":{"observed_at":"2026-08-16T00:51:23.309593Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2505.02687","last_updated":"2025-05-05T14:35:40Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T00:41:37.306405Z","submitted_at":"2025-05-05T14:35:40Z","title":"Exploring the IR-radio correlation in massive galaxy clusters at the end of cosmic noon"},"reference_resolution":{"displayed":66,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":41,"verified_exact":0,"verified_fuzzy":25},"total_outbound_references":66},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 66 of 66 outbound references and 0 inbound Pith citation observations for arXiv:2505.02687."}