{"as_of":"2026-08-15T15:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:20166cb339577fa02ffc16a3b348dcb0235f46cab569ff0f040c261bede0c5d7","coverage":[{"denominator":62,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":62,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T06:50:28.521717Z","state":"measured"},{"denominator":62,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":62,"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/2511.10464/citation-record","integrity":"/paper/2511.10464/integrity","json":"/paper/2511.10464/citation-record.json","paper":"/paper/2511.10464"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T06:50:22.101932Z","title":"P., Tollerud, E","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:22.101932Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:95ff3b5cfe74d2c644558afb094b099ba9bbc1f4ff7c011b900191389310b65e","observation_id":"50a0d779-5066-42ac-9e97-4cf9df5af1ab","resolution":{"observed_at":"2026-08-04T06:50:22.101932Z","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":"10.1017/pasa.2024.129","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"J., et al","venue":"Publications of the Astronomical Society of Australia","work_id":"59e4c689-15a8-4b29-8374-436d1c1de96c","year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:22.199096Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:fc2de5566fa948744b6ab4de50793c78eb528df4bb8494747ec54f00055ae02f","observation_id":"b8453685-4c08-4a7a-94d9-bb41b31f4fc7","resolution":{"observed_at":"2026-08-04T06:53:26.336559Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-07-14T23:20:57.804025+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-14T23:20:57.804025+00:00","source":"openalex_status_cache"},{"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":"2026-08-04T06:50:22.371082Z","title":"R., Bershady, M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:22.371082Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:337b0ec51af4427c38fe32c3ad2c580f2eaef66e02bcd220ba038755901da07e","observation_id":"dc405ce7-7d77-4c83-9e11-57c358714356","resolution":{"observed_at":"2026-08-04T06:50:22.371082Z","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":"2026-08-04T06:50:22.492625Z","title":"A., Law, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:22.492625Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:bac7e550ee43a23f36b1112bdfadf87244232e00f7c387b06ab98f9084be59dd","observation_id":"33ee9e6c-b312-4c71-b198-30bf8dfe4dc6","resolution":{"observed_at":"2026-08-04T06:50:22.492625Z","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":"2026-08-04T06:50:22.664871Z","title":"2021, MNRAS, 500, 1261, doi: 10.1093/mnras/staa3288","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:22.664871Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:9961142e19c5f23c4705127443f4086b6bb7071e571f41a97740c7f2c604b8ab","observation_id":"ddd8d7ca-075f-4a8e-a1b4-00a7e2659ee3","resolution":{"observed_at":"2026-08-04T06:50:22.664871Z","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":"2026-08-04T06:50:22.844750Z","title":"K., Sandstrom, K., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:22.844750Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:6f5e107f7a4d39678a1a65969256d7b3fee70d2e7413d3ed76071b99162c7a9b","observation_id":"0c3aeefc-a9b3-417e-8b65-1b6605b3440a","resolution":{"observed_at":"2026-08-04T06:50:22.844750Z","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":"2026-08-04T06:50:23.020124Z","title":"2019, MNRAS, 482, 1618, doi: 10.1093/mnras/sty2777","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.020124Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:c0364ed75cd078f23e115d2c19ebad503b0b77752086995e120fc3907f2ac456","observation_id":"e920c61f-3858-4bbe-a044-3c28a61b42d1","resolution":{"observed_at":"2026-08-04T06:50:23.020124Z","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":"10.1086/184488","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"K., Tielens, A","venue":"The Astrophysical Journal","work_id":"e693fd1e-6aca-4c7a-9777-93b3822295c1","year":1985},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.191678Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:a1fbf2095f9063a386a292494855b099c23346cebaab8d3387fd5ab3012d5eca","observation_id":"5e22e635-0e83-4f8f-b562-667229889f56","resolution":{"observed_at":"2026-08-04T06:53:26.225743Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-04T06:50:23.295574Z","title":"2019, MNRAS, 486, 743, doi: 10.1093/mnras/stz805","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.295574Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:ed0ae3782cf91c27cb6725df709f4055d9837979e98b95459f17f40a7134de15","observation_id":"3effe802-cc83-431b-82fa-a91124ae12e9","resolution":{"observed_at":"2026-08-04T06:50:23.295574Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.8516","last_updated":"2015-04-10T12:27:56Z","snapshot_observed_at":"2026-08-12T12:07:47.951486Z","submitted_at":"2014-10-30T19:44:20Z","title":"NICE: Non-linear Independent Components Estimation","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.8516","snapshot_observed_at":"2026-08-04T06:50:23.397926Z","title":"2014, arXiv e-prints, arXiv:1410.8516, doi: 10.48550/arXiv.1410.8516","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.397926Z"},"links":{"cited_paper":"/paper/1410.8516","citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:34632ccd93a0190679cce7fcd1e5a123d693e1f83a21e50ef49a7cee65412ea0","observation_id":"85538aca-3464-4d54-a71b-688c587eb1fe","resolution":{"observed_at":"2026-08-04T06:50:23.397926Z","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":"2026-08-04T06:50:23.492824Z","title":"T., Li, A., Hensley, B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.492824Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:5e11c2eb498f87a8cf2ce97179046f39bf8c3220fdfb3c2eeedff9b0134c7f9f","observation_id":"2f4f74f7-9765-440d-a087-2c72baf55acf","resolution":{"observed_at":"2026-08-04T06:50:23.492824Z","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":"2026-08-04T06:50:23.595312Z","title":"2022, A&A, 659, A191, doi: 10.1051/0004-6361/202141727","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.595312Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:88b9f6fca7b0e7cbd7d8c7fbbed881d636d82e9d42fb8d6e5a9593f387aab673","observation_id":"20163da3-3eed-4903-a0d9-5434ec3fe9cd","resolution":{"observed_at":"2026-08-04T06:50:23.595312Z","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":"2026-08-04T06:50:23.711596Z","title":"1987, MNRAS, 225, 155, doi: 10.1093/mnras/225.1.155","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.711596Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:33f44a29a713b91d854c714266e0706a35f909b3c3e27f19715da5d0c6eef18d","observation_id":"afb3c9b0-d0db-473e-b753-72edb5b63ed5","resolution":{"observed_at":"2026-08-04T06:50:23.711596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2508.11044","last_updated":"2025-08-14T20:04:16Z","snapshot_observed_at":"2026-08-05T20:08:03.533606Z","submitted_at":"2025-08-14T20:04:16Z","title":"JWST NIRCam Imaging of NGC 4258: I. Observation Overview","version":1},"cited_work":{"arxiv_id":"2508.11044","doi":"10.48550/arxiv.2508.11044","metadata_source":"pith","pith_arxiv_id":"2508.11044","snapshot_observed_at":"2026-08-04T12:16:13.904932Z","title":"JWST NIRCam Imaging of NGC 4258: I. Observation Overview","venue":"astro-ph.GA","work_id":"cce7f6a5-3d05-4f3d-b8df-a414868fb54f","year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.779669Z"},"links":{"cited_paper":"/paper/2508.11044","citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:5f9f8bf5b2d2dca3c8036ddd2147bec430b34853fa443d86c34610ebdb4e9596","observation_id":"967efae3-2f80-46f0-8903-ae750eeac950","resolution":{"observed_at":"2026-08-04T06:53:26.062452Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2026-08-04T06:50:23.894187Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.894187Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:48e8e78524788cc7d6391a203e2345d4a0a9b2283eddd9ee39ff4302313f10ff","observation_id":"5f063e03-ce62-420f-8267-1a217485fd82","resolution":{"observed_at":"2026-08-04T06:50:23.894187Z","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":"2026-08-04T06:50:23.996798Z","title":"2022, ApJ, 940, 133, doi: 10.3847/1538-4357/ac9af1","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:23.996798Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:de2c5aa096d01b58c05ecde5a4568193ba8e1bbdd816e953ae748c3dc87f1fc2","observation_id":"ce4904ea-1c83-4332-b883-7e62ebe6e563","resolution":{"observed_at":"2026-08-04T06:50:23.996798Z","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":"2026-08-04T06:50:24.117242Z","title":"2019, ApJ, 887, 172, doi: 10.3847/1538-4357/ab557c","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.117242Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:8b67d3caad15e9af9cb9854a7bd9f31e0f89892390106a81677d3805877a3470","observation_id":"5c168149-7711-429d-b177-412aa92bcfab","resolution":{"observed_at":"2026-08-04T06:50:24.117242Z","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":"10.3847/1538-4357/ad9d0f","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, ApJ, 979, 105, doi: 10.3847/1538-4357/ad9d0f","venue":"The Astrophysical Journal","work_id":"7e74722c-46c5-4d6a-be0f-70b95cbdc3f2","year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.216912Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:2a4bead0428f28b24258ba8958247d14bdcd23e8b695b3119f4355bf5e17e42d","observation_id":"fd9a3e63-38d3-42ac-b08a-5fa5a8b0519b","resolution":{"observed_at":"2026-08-04T06:53:25.981563Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-04T06:50:24.363083Z","title":"P., Mather, J","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.363083Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:dd0b85c9e6d03fc40a9e80268a387aedd138f5d834c1dede2f48dd53afa603b5","observation_id":"73bea874-8f6a-48a7-95ae-da49d54d6af4","resolution":{"observed_at":"2026-08-04T06:50:24.363083Z","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":"2026-08-04T06:50:24.476139Z","title":"D., Fitzpatrick, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.476139Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:37a7d9973a57d355b5dcfd8c6157bad0c51f9f09e826d10b3191eac3c9eca797","observation_id":"5aa9e5f3-e13a-4f3c-b62f-33f84a974ec1","resolution":{"observed_at":"2026-08-04T06:50:24.476139Z","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":"2026-08-04T06:50:24.636160Z","title":"2025, Research in Astronomy and Astrophysics, 25, 065017, doi: 10.1088/1674-4527/add673","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.636160Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:5fff7c272d4381aa573c25b1af145400439749c57793009c2edffc98110e52cb","observation_id":"7f735864-d26e-4b3d-9f94-a18033196f2b","resolution":{"observed_at":"2026-08-04T06:50:24.636160Z","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":"2026-08-04T06:50:24.798308Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.798308Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:43b1b81c60dfa4bfa1b766642231099f1e246b4a507ecb98b65a0c1a979b7fe3","observation_id":"df86cc4d-0b73-4a36-8fd8-30305d5a7cb8","resolution":{"observed_at":"2026-08-04T06:50:24.798308Z","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":"2026-08-04T06:50:24.966263Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:24.966263Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:a3e92119f6af1bbab3815aa1eadab676a45aea916196e4bf2295a62a54fb1098","observation_id":"2bdcb58b-0d1e-4b2d-882c-12c0f683668e","resolution":{"observed_at":"2026-08-04T06:50:24.966263Z","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":"2026-08-04T06:50:25.074671Z","title":"2020, MNRAS, 499, 5749, doi: 10.1093/mnras/staa3259","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.074671Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:1f3f4535de94cedb5f1c49028debfd032e65ccc3c223fae1968252a03313fd4e","observation_id":"dd77370f-52b2-4fb3-b390-8ef21187f973","resolution":{"observed_at":"2026-08-04T06:50:25.074671Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.05770","last_updated":"2016-06-14T09:01:36Z","snapshot_observed_at":"2026-08-14T22:47:38.400768Z","submitted_at":"2015-05-21T15:36:37Z","title":"Variational Inference with Normalizing Flows","version":6},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.05770","snapshot_observed_at":"2026-08-04T06:50:25.192757Z","title":"2015, ApJ, 799, 92, doi: 10.1088/0004-637X/799/1/92 22Jing & Li Jimenez Rezende, D., & Mohamed, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.192757Z"},"links":{"cited_paper":"/paper/1505.05770","citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:5f5fae0119be9189b1d0e7d3465e2167c0583c1212b3aa17051782466f60e364","observation_id":"d7a5e089-543a-432f-9c0d-0e77c912f5a4","resolution":{"observed_at":"2026-08-04T06:50:25.192757Z","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":"10.3847/1538-3881/add891","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, AJ, 170, 45, doi: 10.3847/1538-3881/add891","venue":"The Astronomical Journal","work_id":"58299b09-6bf7-4ccf-b3be-09334a81ec30","year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.316851Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:a5d45f6ed8c38877451689b26cc25cb7498d51d6860c039a217a9b4b764b31cb","observation_id":"b58d8dfc-e9b5-485a-9c1f-a2db28355286","resolution":{"observed_at":"2026-08-04T06:53:25.889928Z","resolver_source":"doi","status":"verified_exact"},"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":"2510.03716","doi":"10.48550/arxiv.2510.03716","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv e-prints, arXiv:2510.03716, doi: 10.48550/arXiv.2510.03716","venue":"arXiv (Cornell University)","work_id":"09f9ae83-4dee-4c6c-9a15-87d14b9ba48a","year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.472806Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:b7242dad819165414752d9d969bf342b199ce9f46fa0ab8f09b4093f91efc2c7","observation_id":"66fbacca-a022-47c6-8faa-e3aaedba5700","resolution":{"observed_at":"2026-08-04T06:53:25.815856Z","resolver_source":"arxiv_id","status":"verified_exact"},"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":"2026-08-04T06:50:25.622949Z","title":"P., Marrone, D","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.622949Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:cae32c88f91aafe8f1eb6b8d67d7c5667d428618ef990e733898f9c7da99971a","observation_id":"dc37a231-3f8c-46dd-84e3-6a34af5a2e94","resolution":{"observed_at":"2026-08-04T06:50:25.622949Z","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":"2026-08-04T06:50:25.748099Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.748099Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:56bb99308acdd851fc2586f3932574f3cbf3ee4192ba6d28f832bb31fe99242b","observation_id":"9d4f1b6f-7bf5-4e8b-9dcc-816acd330d51","resolution":{"observed_at":"2026-08-04T06:50:25.748099Z","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":"10.3847/2515-5172/abe8df","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2021, Research Notes of the American Astronomical Society, 5, 39, doi: 10.3847/2515-5172/abe8df","venue":"Research Notes of the AAS","work_id":"d03dce96-948a-4f04-a37a-6c0e7c9d2372","year":2021},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.822821Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:62de6ace71d46177fe97b508bcbaa59799d968dfd1f91817d5687c40259e783a","observation_id":"82276a9a-6264-4ff2-9134-76e3e2f9bd52","resolution":{"observed_at":"2026-08-04T06:53:25.775803Z","resolver_source":"doi","status":"verified_exact"},"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":"2505.08876","last_updated":"2025-05-13T18:05:02Z","snapshot_observed_at":"2026-08-10T16:54:41.058808Z","submitted_at":"2025-05-13T18:05:02Z","title":"Dynamically-Driven Evolution of Molecular Gas in M83 Traced by CO 2-1/1-0 Line Ratio Variations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.08876","snapshot_observed_at":"2026-08-04T06:50:25.882045Z","title":"2025, arXiv e-prints, arXiv:2505.08876","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.882045Z"},"links":{"cited_paper":"/paper/2505.08876","citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:4dc6eb1f51b291827b93de89f4ddd6650c975e907cf01ad4170a7067e2652577","observation_id":"983f92d8-013e-4b57-8052-04c03222ee43","resolution":{"observed_at":"2026-08-04T06:50:25.882045Z","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":"2026-08-04T06:50:25.944237Z","title":"2025, ApJ, 980, 126, doi: 10.3847/1538-4357/ada6b5","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:25.944237Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:3824f5123f0c8a8c8213e16bf282b1b4fcc81d0e1e5e078210b2a9f877c9b5d1","observation_id":"df7a70ad-72da-451b-b73b-3ca745d40cb5","resolution":{"observed_at":"2026-08-04T06:50:25.944237Z","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":"2026-08-04T06:50:26.033868Z","title":"C., Sandstrom, K","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.033868Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:0ad533667d34b50f0a6bedd3a339132ac90222034db103414b1098c50c1c88a6","observation_id":"0b0bf30f-a7a4-4609-b53b-70580eb738f4","resolution":{"observed_at":"2026-08-04T06:50:26.033868Z","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":"2026-08-04T06:50:26.093953Z","title":"1985, A&A, 146, 81","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.093953Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:d66529ce7252d2d43e48b9e05fd8d02ad29ab34f92e99ebf1f00f2825ee52d18","observation_id":"37b5f112-e9c2-41e4-b59c-b3d6301b726b","resolution":{"observed_at":"2026-08-04T06:50:26.093953Z","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":"2026-08-04T06:50:26.148370Z","title":"K., Hughes, A., Liu, D., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.148370Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:f5a2f076ac57afcad44f2ffb6a9ff8b3ed262203c65ee7dd237d714045a810d6","observation_id":"4dbfbf3d-27c6-4035-8d42-046243411bf1","resolution":{"observed_at":"2026-08-04T06:50:26.148370Z","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":"2026-08-04T06:50:26.197818Z","title":"K., Schinnerer, E., Hughes, A., et al","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.197818Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:6c6c613fdb40839e8ee0eba97348cb4cfae6c687977b4f8660933c272ec9066b","observation_id":"6eb4345f-0dd0-4450-a7af-634d7fb71893","resolution":{"observed_at":"2026-08-04T06:50:26.197818Z","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":"2026-08-04T06:50:26.278636Z","title":"K., Bolatto, A","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.278636Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:caee5e25ce0abfe0d6eb90a924c288b4ed034615599d9b19b52b8bd31e1e8027","observation_id":"45af91e5-6c99-4650-86d7-83f5bd51a812","resolution":{"observed_at":"2026-08-04T06:50:26.278636Z","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":"2026-08-04T06:50:26.341940Z","title":"K., Sandstrom, K., Rosolowsky, E., et al","venue":null,"work_id":null,"year":2041},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.341940Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:73c11f82962e2fc6ddceb445043350fe5f347e2abbc0249ccee7801d0d1f5d43","observation_id":"19f17ef4-8a2f-4acc-95d8-781db15c94fb","resolution":{"observed_at":"2026-08-04T06:50:26.341940Z","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":"2026-08-04T06:50:26.383870Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.383870Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:4de4c066aeb881bcfd04ee6b3bae0e70b911f937adc55e883f858fb0f4fa045e","observation_id":"3be37f89-3200-4927-bd93-097b917bd75d","resolution":{"observed_at":"2026-08-04T06:50:26.383870Z","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":"2026-08-04T06:50:26.442328Z","title":"J., & Li, A","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.442328Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:9151ca0ba2eb2dcaa9ecf8967673d1c1eaa7c50ea1249944d3f52b97f04dec33","observation_id":"3d34b466-75bb-4284-b79e-7c3c933a835e","resolution":{"observed_at":"2026-08-04T06:50:26.442328Z","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":"10.3847/1538-4357/adc808","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal","work_id":"8ccae4b9-3cf8-4903-96f3-a3fdedcc3e01","year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.498849Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:30d0585f4ac19581cd6d4c791b69c81d79bd2f14ac04abc6e53a3da85c1ac4e6","observation_id":"9ae908ad-0c7d-496f-8cef-bfa9d65e715e","resolution":{"observed_at":"2026-08-04T06:53:25.628686Z","resolver_source":"doi","status":"verified_exact"},"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":"2505.09728","last_updated":"2025-07-24T18:08:57Z","snapshot_observed_at":"2026-08-07T15:45:19.242022Z","submitted_at":"2025-05-14T18:36:39Z","title":"A PAH deficit in the starburst core of a distant spiral galaxy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.09728","snapshot_observed_at":"2026-08-04T06:50:26.575403Z","title":"D., Daddi, E., et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.575403Z"},"links":{"cited_paper":"/paper/2505.09728","citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:92b887f6d1b2bfee0dfcdeeac4d97c987af1ba9e4dff5067d6a07f3e03273748","observation_id":"44ddf0e1-86c9-4344-80d4-b71fd19a4f5b","resolution":{"observed_at":"2026-08-04T06:50:26.575403Z","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":"2026-08-04T06:50:26.586010Z","title":"S., Tang, X","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.586010Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:764cbc2865213d70e3112a3e4f30d9d461857f6d36dbf07c0d5dbb72e24e77e0","observation_id":"6200d8d4-98c2-4e3c-81f9-cb349f3a831d","resolution":{"observed_at":"2026-08-04T06:50:26.586010Z","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":"2026-08-04T06:50:26.605237Z","title":"2022, ApJ, 926, 96, doi: 10.3847/1538-4357/ac4505","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.605237Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:7ad64af344c4ce48571cac067a3f485facd92ec263eb76ff32e7c004dded0335","observation_id":"f84cc4e3-a8ca-4a9d-851f-70fd00985c8b","resolution":{"observed_at":"2026-08-04T06:50:26.605237Z","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":"10.3847/1538-4357/ac3825","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"D., & Fitzpatrick, E","venue":"The Astrophysical Journal","work_id":"9eaf255c-8314-4ec2-9500-9dcf04f4df56","year":2022},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.745045Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:4e5b510fb87de8bdd539e43bde38164c03e2c944748bae241609446dca5d59a9","observation_id":"6a23091c-e788-43aa-a1a9-a0c28e7f63af","resolution":{"observed_at":"2026-08-04T06:53:25.485430Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-04T06:50:26.881320Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:26.881320Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:3ea594c49a35a4bb65783942034d724d53a2068c3f99a460c8832b97e8d4c633","observation_id":"cb30d4ef-b1ba-4c09-9b1a-e491f658886c","resolution":{"observed_at":"2026-08-04T06:50:26.881320Z","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":"2026-08-04T06:50:27.037050Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.037050Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:0c8babf80a38a6818fdc770ab517e55b485faad726f3c421ee88d02e3717b57c","observation_id":"d7a0a98d-e405-4ad5-8932-1380aaf89fe1","resolution":{"observed_at":"2026-08-04T06:50:27.037050Z","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":"2026-08-04T06:50:27.162400Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.162400Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:4dfcd05712d306a677e0703aba345cd86d2d97c719c855298d706b5a0e8c322f","observation_id":"933661cd-8b72-4cf4-889c-80b04211e275","resolution":{"observed_at":"2026-08-04T06:50:27.162400Z","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":"2026-08-04T06:50:27.269093Z","title":"M., & Hensley, B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.269093Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:4b2daab9a72e6cb4c0fd3c1cd31837bb41970764548825c7b56832477a8be876","observation_id":"e32c1dca-a9de-4b29-9e0a-6c8a81dc36e7","resolution":{"observed_at":"2026-08-04T06:50:27.269093Z","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":"2026-08-04T06:50:27.330520Z","title":"2024,, v0.13.1 Zenodo, doi: 10.5281/zenodo.10931886","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.330520Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:4405d38c7dd24be505145cec4992a2f8ee3e577b7dee9d0284cf870c4cd0f079","observation_id":"95f15a91-9fd2-4f30-b7b3-284a24e0822b","resolution":{"observed_at":"2026-08-04T06:50:27.330520Z","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":"10.1086/176844","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":null,"venue":"The Astrophysical Journal","work_id":"1e55fe9d-042b-4df2-82e9-57a0c7fd9cb2","year":1996},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.438559Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:826755d46989e3b79541b03103fb2e4ded0673435e7bcaa3e2a65da38b6ebc09","observation_id":"fc6270cc-fb7b-465a-ab7a-4ac6e2b5a003","resolution":{"observed_at":"2026-08-04T06:53:25.401322Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-04T06:50:27.544892Z","title":"2014, in IAU Symposium, Vol","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.544892Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:276b69abed88fa149a47df2f8e8aa21918ffaa22b3c5d28a8104528176108de0","observation_id":"7fd1a577-9e67-4ab8-bdb5-9c438a3a6699","resolution":{"observed_at":"2026-08-04T06:50:27.544892Z","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":"2026-08-04T06:50:27.629918Z","title":"A., Kre lowski, J., et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.629918Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:dcd56f9ce4ea15318b7c4850f73143157832befce95e1536a3cc8f2893ce6179","observation_id":"51d87a9d-b611-411c-8c01-7fa4885639ed","resolution":{"observed_at":"2026-08-04T06:50:27.629918Z","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":"2026-08-04T06:50:27.723018Z","title":"2022, MNRAS, 514, 1886, doi: 10.1093/mnras/stac1313","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.723018Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:89ff0f8bcfab09af802efd89968adfc424a6f22ca9c9bdc7078a3733c2dd7219","observation_id":"bc1a7423-43cc-4bfa-9c83-3b49d0bef91f","resolution":{"observed_at":"2026-08-04T06:50:27.723018Z","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":"2026-08-04T06:50:27.881796Z","title":"2025, arXiv e-prints, arXiv:2510.05214, doi: 10.48550/arXiv.2510.05214 van der Zwet, G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.881796Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:ad1bfb4ce2a24719ea976bc9f8f8241fc2a825a0c990dd7007921eec8275ca9a","observation_id":"cb6cac70-e662-48a0-ae8c-0cb191254b93","resolution":{"observed_at":"2026-08-04T06:50:27.881796Z","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":"2026-08-04T06:50:27.988376Z","title":"E., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:27.988376Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:ce45acdb234c085c32b6df7f3bd025429d4f7c5f2d14c48b97ede916cee48da0","observation_id":"55d6fda7-0de4-42d3-9b09-4bfb7b8f0dae","resolution":{"observed_at":"2026-08-04T06:50:27.988376Z","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":"2026-08-04T06:50:28.057275Z","title":"A., Bundy, K., Diamond-Stanic, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:28.057275Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:d9d3feac22e354bc1c634c94daafaead156c30f20da58a59c67a882e7b2e5f15","observation_id":"57e77d9b-e573-4aa6-a00b-46374a23baa1","resolution":{"observed_at":"2026-08-04T06:50:28.057275Z","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":"2026-08-04T06:50:28.156001Z","title":"W., Roellig, T","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:28.156001Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:904d17f248224fa47054c4b58c8f7d0fc418e432a792f8eb0134a858e6942343","observation_id":"0ea5975a-cf2d-487e-a768-ae59aaa9b4c8","resolution":{"observed_at":"2026-08-04T06:50:28.156001Z","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":"2026-08-04T06:50:28.238831Z","title":"M., Sandstrom, K., Leroy, A., & Smith, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:28.238831Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:dd973a5aacd32db4fb363d23e111508c5ab27f8f46b1290c964bebfed0aca616","observation_id":"e351a706-b5ae-48fc-9da6-358604658ae6","resolution":{"observed_at":"2026-08-04T06:50:28.238831Z","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":"2026-08-04T06:50:28.332031Z","title":"G., Lee, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:28.332031Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:273ebbfa2739adffdc74fa7f9fe87a7922f31e717cc24293d76e60291965f617","observation_id":"25163c55-209f-4a8a-a98a-2860c827f514","resolution":{"observed_at":"2026-08-04T06:50:28.332031Z","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":"2026-08-04T06:50:28.400966Z","title":"L., Eisenhardt, P","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:28.400966Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:ceea77abddec414f5e59d28e8496319c5d1c1101437651492aadddb788118572","observation_id":"95c18281-d722-4a27-aff0-b7501b68ee18","resolution":{"observed_at":"2026-08-04T06:50:28.400966Z","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":"2026-08-04T06:50:28.521717Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-04T06:50:28.521717Z"},"links":{"citing_paper":"/paper/2511.10464"},"observation_digest":"sha256:0de8078f41e791394d045863f6fe737b4bbef5a4c07fd089582b3a2e29d015f8","observation_id":"8489a9f1-683a-46d8-b115-7cbb33e54f31","resolution":{"observed_at":"2026-08-04T06:50:28.521717Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2511.10464","last_updated":"2026-08-01T03:27:31Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T00:49:38.055172Z","submitted_at":"2025-11-13T16:32:18Z","title":"Correlations of ALMA CO(2-1) with JWST mid-infrared fluxes down to scale of $\\lesssim$100 parsec in nearby star-forming galaxies from PHANGS"},"reference_resolution":{"displayed":62,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":52,"verified_exact":10,"verified_fuzzy":0},"total_outbound_references":62},"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 15 August 2026, this Paper Citation Record lists 62 of 62 outbound references and 0 inbound Pith citation observations for arXiv:2511.10464."}