{"as_of":"2026-08-20T01:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:383d23b93ddcecd67c9ecc15a5c2e45270604dca9fbdae9b0e8eed7ec66264a3","coverage":[{"denominator":110,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T22:01:22.291111Z","state":"measured"},{"denominator":108,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":108,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T17:35:29.254194Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-06T17:35:29.254194Z","title":"G., Breitman D., Qin Y., Trotta R., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2411.08134 , https://ui.adsabs.harvard.edu/abs/2024arXiv241108134C p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.10533","last_updated":"2025-08-25T11:39:48Z","snapshot_observed_at":"2026-08-13T02:41:42.103699Z","submitted_at":"2025-07-14T17:55:16Z","title":"Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-06T17:35:29.254194Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2507.10533"},"observation_digest":"sha256:cc327c299ccc19476ce3a66031a98e048e05296ee927b8d3d8136e9c33aa65e5","observation_id":"cc2002ec-56a6-4183-b3fe-a65b7ade8355","resolution":{"observed_at":"2026-08-06T17:35:29.254194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.00219","last_updated":"2026-05-29T18:00:05Z","snapshot_observed_at":"2026-07-06T23:40:56.510371Z","submitted_at":"2026-05-29T18:00:05Z","title":"21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables","version":1},"reference_index":274,"source":"arxiv_source","source_observed_at":"2026-06-28T20:53:04.280649Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.00219"},"observation_digest":"sha256:caff2b200663e845c54c084d34ac883ca8ff76f7d20602c3ad7766593b9d1753","observation_id":"0600397c-bc91-4c0d-a156-88dba1854215","resolution":{"observed_at":"2026-06-28T21:02:38.155266Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.26435","last_updated":"2026-06-26T01:20:06Z","snapshot_observed_at":"2026-07-07T00:00:46.505337Z","submitted_at":"2026-06-24T22:54:35Z","title":"Overview of 21cm Experiments at high redshift with SKAO","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-06-26T01:05:14.717641Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.26435"},"observation_digest":"sha256:259f322c4bf5e2b4405812b763e243c08b540548d72a799ef8eca42dd4995486","observation_id":"cee8cd12-8b8e-4b1e-939a-f08c3ca1f37a","resolution":{"observed_at":"2026-06-26T01:08:48.174418Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.26435","last_updated":"2026-06-26T01:20:06Z","snapshot_observed_at":"2026-07-07T00:00:46.505337Z","submitted_at":"2026-06-24T22:54:35Z","title":"Overview of 21cm Experiments at high redshift with SKAO","version":2},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-06-29T01:30:18.284179Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.26435"},"observation_digest":"sha256:e10c6a125158ddd653fc0cffb859598297fae8b4507fe2062a7e80a16ac97aa5","observation_id":"be43efc1-3988-4ba3-b110-4c7fadf00709","resolution":{"observed_at":"2026-06-29T01:32:59.114661Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.27858","last_updated":"2026-06-26T08:56:58Z","snapshot_observed_at":"2026-08-16T15:49:17.908865Z","submitted_at":"2026-06-26T08:56:58Z","title":"Inferring Cosmology and Astrophysics from the High-redshift 21cm Signal with SKA-Low","version":1},"reference_index":114,"source":"arxiv_source","source_observed_at":"2026-06-29T03:26:09.447942Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.27858"},"observation_digest":"sha256:0fcb446b2dcd73183bea9b0f9c0414e63727e577b426b871a53ed865b95bd202","observation_id":"cab5cacc-c52a-457e-87b7-e8f9c24feb8a","resolution":{"observed_at":"2026-06-29T03:43:05.047967Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.29903","last_updated":"2026-06-29T07:38:22Z","snapshot_observed_at":"2026-08-17T19:18:10.359154Z","submitted_at":"2026-06-29T07:38:22Z","title":"High-Redshift Signatures from the Cosmic Dawn and the Epoch of Reionization","version":1},"reference_index":120,"source":"arxiv_source","source_observed_at":"2026-06-30T05:35:40.361344Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.29903"},"observation_digest":"sha256:a2fd53e9fdc0ea7299d07e55d5f0f0acbadfaa05817987545528788bb6449584","observation_id":"ef03a783-592f-4879-abbf-d089b9575014","resolution":{"observed_at":"2026-06-30T05:44:18.375350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.30200","last_updated":"2026-06-29T12:16:29Z","snapshot_observed_at":"2026-07-31T16:51:53.334463Z","submitted_at":"2026-06-29T12:16:29Z","title":"Cosmology with Intensity Mapping via Statistics Beyond the Power Spectrum in the SKAO Era","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-06-30T05:15:12.358969Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.30200"},"observation_digest":"sha256:3511225fa9526560d6dfe3a0d35808a1a3089fc63cc4140f1505f1bbe71eaa09","observation_id":"a5b6a84c-bd5b-4b01-895c-7438d7590743","resolution":{"observed_at":"2026-06-30T05:24:17.655212Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"cited_work":{"arxiv_id":"2411.08134","doi":"10.48550/arxiv.2411.08134","metadata_source":"arxiv_reference","pith_arxiv_id":"2411.08134","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"3e507387-b456-4fca-b435-9e3a416928e1","year":null},"citing_paper":{"arxiv_id":"2606.30224","last_updated":"2026-06-29T12:38:59Z","snapshot_observed_at":"2026-08-14T03:29:15.888460Z","submitted_at":"2026-06-29T12:38:59Z","title":"Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-06-30T05:12:19.196876Z"},"links":{"cited_paper":"/paper/2411.08134","citing_paper":"/paper/2606.30224"},"observation_digest":"sha256:7f969ff57b7002b617fe5e507640ee2c2a9da301d73a8aba5c50b44453b6caaa","observation_id":"ccf47758-6040-496e-bfb2-ecc51237b323","resolution":{"observed_at":"2026-06-30T05:14:17.471231Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2411.08134/citation-record","integrity":"/paper/2411.08134/integrity","json":"/paper/2411.08134/citation-record.json","paper":"/paper/2411.08134"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T22:01:21.994537Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:21.994537Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:99f4bf17e27e739287e022175703cb7d1f6669e15a8a6f0881e1f11f3980225c","observation_id":"bc2a0c22-ecd7-4a56-8844-59b70b34fc47","resolution":{"observed_at":"2026-08-12T22:01:21.994537Z","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":"2026-08-12T22:01:21.998338Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:21.998338Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:a72cf983f400e683b4e7bc3f7a37e20785731f54adaf6addc72109d8395248ce","observation_id":"79014b05-7ccc-425b-b618-7a38a07b25bc","resolution":{"observed_at":"2026-08-12T22:01:21.998338Z","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":"2026-08-12T22:01:22.001935Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.001935Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:1dd4b07abc2c8c4d1837a04a31a0af4911278acb495031b7f661c8909d98961e","observation_id":"a07ccf5a-8397-4c9a-8278-131ee4bd3fb3","resolution":{"observed_at":"2026-08-12T22:01:22.001935Z","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":"2026-08-12T22:01:22.005496Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.005496Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:c89d6ef8790e97887c8037101a44f9ca38730665f7f18bbbb9c52a9557e1d17a","observation_id":"4c3b9a89-cdcd-4a13-8e25-561aaa670773","resolution":{"observed_at":"2026-08-12T22:01:22.005496Z","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":"2026-08-12T22:01:22.008939Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.008939Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:358d9c940aa1d0f71c9da3213e8f596b94fa251e8a7c619e31077585037ead4c","observation_id":"61db3a64-3e4f-475b-86c5-9098a0190c74","resolution":{"observed_at":"2026-08-12T22:01:22.008939Z","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":"2026-08-12T22:01:22.012170Z","title":"2018, Nature, 555, 71","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.012170Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:a33d42b182db92291b8740781b252f827409abc58bc24afeecec47107baf277e","observation_id":"7805cdb4-645a-48b7-bad1-ffb5fa4315b0","resolution":{"observed_at":"2026-08-12T22:01:22.012170Z","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":"2026-08-12T22:01:22.015366Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.015366Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:0e2596ef7b0afc0885ad611c29f93a03174cca4233c29ad96e6214778d5dc645","observation_id":"d9c75268-c9cc-45ad-803b-5e9e596c3958","resolution":{"observed_at":"2026-08-12T22:01:22.015366Z","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":"2026-08-12T22:01:22.018389Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.018389Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:03d92ffa2b338bf360ac5e1614919ddcb1d1d80b7030ad6f823e9c98a33e2c44","observation_id":"97927813-516e-4ef0-accf-10053d6163f0","resolution":{"observed_at":"2026-08-12T22:01:22.018389Z","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":"2026-08-12T22:01:22.021638Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.021638Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:378be44b059a3a34b2ac984ff32ea1bba84c045d60ca261d4abb662ec96355cd","observation_id":"f7f949c9-4151-459d-841e-4c4a009df929","resolution":{"observed_at":"2026-08-12T22:01:22.021638Z","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":"2026-08-12T22:01:22.024618Z","title":"J., Illingworth, G","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.024618Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:8e23647f3c9dcc1bd977318da000999c1396e13fcdfc3019bcd3f00ab561670a","observation_id":"958d1b6d-3feb-4e90-b775-b032f7b08c61","resolution":{"observed_at":"2026-08-12T22:01:22.024618Z","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":"2026-08-12T22:01:22.027796Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.027796Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:79b3388ae33fc67d0c7d0adf96a32fc03afff87217dfb81128914f1878979a51","observation_id":"02c5b27c-617a-4802-9242-3610144e2e7c","resolution":{"observed_at":"2026-08-12T22:01:22.027796Z","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":"2026-08-12T22:01:22.030737Z","title":"D., Rogers, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.030737Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:c7c3faa1fdd833e0f3350061fad28925bc5c258d2efb0826477c647a89f77efa","observation_id":"b037b745-e21c-4dab-8c60-7689e70af569","resolution":{"observed_at":"2026-08-12T22:01:22.030737Z","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":"2026-08-12T22:01:22.033710Z","title":"D., Rogers, A","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.033710Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:09241a8f8e3c53adfe0cbecaaa8e5df553448aac958af47f0c5afc622f6b1782","observation_id":"50039b12-06cf-408e-8c0f-f8aac81e92ea","resolution":{"observed_at":"2026-08-12T22:01:22.033710Z","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":"2026-08-12T22:01:22.036605Z","title":"G., et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.036605Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:3005f5cc061c886ff5831496765c3da1fa7b65a6b4844f7022af3b1ecb79d5c6","observation_id":"62017af0-233d-46dc-b7d4-18a2a6c797ab","resolution":{"observed_at":"2026-08-12T22:01:22.036605Z","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":"2026-08-12T22:01:22.039466Z","title":"2013, Rept","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.039466Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:eed0899537964b678ebab079a8b3fab0ce98f31849ff6a5594f08ad2c99f1221","observation_id":"71685eae-2b97-4f83-a42b-b40de4f3834d","resolution":{"observed_at":"2026-08-12T22:01:22.039466Z","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":"2026-08-12T22:01:22.042249Z","title":"& Larson, R","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.042249Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:e502e73267471d4c0badf17ce5f330bac7ca609db618fd933010e66c8d99dd45","observation_id":"65dd380f-0bda-464a-979c-db6851c5a060","resolution":{"observed_at":"2026-08-12T22:01:22.042249Z","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":"2026-08-12T22:01:22.045071Z","title":"2014, Astron","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.045071Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ab97f9cd6416818d3352f359ac5896a8e6683a9549af34260dfdbfe60cf434c4","observation_id":"292480a2-c105-4115-b54e-d8292c376fde","resolution":{"observed_at":"2026-08-12T22:01:22.045071Z","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":"2312.17499","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T22:01:22.439620Z","title":"2023 [ [arXiv] 2312.17499 ]","venue":null,"work_id":"73be389d-2217-483b-b2b0-bdc398481836","year":2023},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.047823Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:c6e140648b1ddaa8d3e92ab71217d69679c7d7f38d63c45137ee6f3f24fa0c3d","observation_id":"c4ac383f-fc24-4e03-84c1-a63b135f9323","resolution":{"observed_at":"2026-08-12T22:01:22.444829Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.050803Z","title":"2002, The Astronomical Journal, 124, 675","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.050803Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:78905b7ae8b9f86c3f507054de1343abd9579243e4bf8afbd59c65d1c8a87a3d","observation_id":"c7f6a4e3-455f-40a3-bd62-0997e4c57ad2","resolution":{"observed_at":"2026-08-12T22:01:22.050803Z","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":"2026-08-12T22:01:22.053764Z","title":"& Sheth, R","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.053764Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:a7836c4e6062add8087d71eb6e139de28e42ca6535320e6f23237eb8779b5c3e","observation_id":"a581a1f8-d614-4e57-a9e9-315260796965","resolution":{"observed_at":"2026-08-12T22:01:22.053764Z","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":"2026-08-12T22:01:22.056311Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.056311Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:65b8d3e94f0123545f49635bde99cdc2afe00f519c404d5ada3ad49eaf38496e","observation_id":"720ec956-6176-4fd7-88fd-743727127f51","resolution":{"observed_at":"2026-08-12T22:01:22.056311Z","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":"2026-08-12T22:01:22.059030Z","title":"O., et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.059030Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:f236910f7546471c814433836350bf941ed9ac503fa4d7dfcb6af9c50a75d8ed","observation_id":"34353801-6144-4b9a-ae97-c152e5f151ed","resolution":{"observed_at":"2026-08-12T22:01:22.059030Z","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":"2026-08-12T22:01:22.061882Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.061882Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:33631dcd52c87d04f3290ec94a20c0c04ee722dfe2ff5db5bf239d54a43007d7","observation_id":"203cd13a-54d2-4798-9de8-24ebdb222223","resolution":{"observed_at":"2026-08-12T22:01:22.061882Z","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":"2026-08-12T22:01:22.064529Z","title":"& Taylor, G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.064529Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:84ed0660f3f1200d7fa04ad363987e53cd28843dc952cebbcc2bdb1aab866ae4","observation_id":"e725a17d-ea44-4839-828b-ec7fa5142838","resolution":{"observed_at":"2026-08-12T22:01:22.064529Z","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":"2026-08-12T22:01:22.067718Z","title":"2014, JCAP, 11, 024","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.067718Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:6b7867345b180109df8c0416027c1ec7f15587d2fe602e97e0aee2be0e8af64f","observation_id":"cabd523c-6b2f-4315-9e67-27eef8f75fa3","resolution":{"observed_at":"2026-08-12T22:01:22.067718Z","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":"2026-08-12T22:01:22.070532Z","title":"2018, The Astrophysical Journal, 868, 63","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.070532Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:457c3b4114d5cdc6adb0be73d32c88b841cd19b228e541afa3cb3380d69dde8d","observation_id":"4e3c2b5e-3541-4acd-ab8f-13caaaae2dd7","resolution":{"observed_at":"2026-08-12T22:01:22.070532Z","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":"2026-08-12T22:01:22.073424Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.073424Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:bffe6b30ec54f2cf34ff4ce425088d8492596848583f7f4ea3cc88249c244b8e","observation_id":"c6c1a08b-7085-40fc-9e79-1c856d7f9a04","resolution":{"observed_at":"2026-08-12T22:01:22.073424Z","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":"2026-08-12T22:01:22.076124Z","title":"2024, JCAP, 01, 005","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.076124Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:2b48b664c84fce5fb5a38352d120ecaab691b307e49243fa46e0a9d3981ea6b7","observation_id":"69352376-e92c-45f8-9f86-33521e410e3f","resolution":{"observed_at":"2026-08-12T22:01:22.076124Z","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":"2026-08-12T22:01:22.078995Z","title":"& Holder, G","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.078995Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:e3b23347d9b28423c721e5acbb5691ab17981c8b415dc929ac69137b06f9bf02","observation_id":"6f45d4c6-5fec-43cf-b4a3-b995eb2f0aeb","resolution":{"observed_at":"2026-08-12T22:01:22.078995Z","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":"2026-08-12T22:01:22.081836Z","title":"P., & Bridges, M","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.081836Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:bc83c93918c4ed3889a30a79fa0fcfc631432b901c605b75542f2bf3201bab22","observation_id":"2a1bd84f-bb2d-41c5-8163-b4ae0ec49519","resolution":{"observed_at":"2026-08-12T22:01:22.081836Z","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":"2026-08-12T22:01:22.084826Z","title":"& Barkana, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.084826Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:b9f3720d441b00ea4f10cd4c0e1b4c31f9ba2c16375368d0029b8e3b3fadd1e6","observation_id":"33186f5c-c25a-4051-92c9-5c5ee2ac345c","resolution":{"observed_at":"2026-08-12T22:01:22.084826Z","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":"2026-08-12T22:01:23.073063Z","title":null,"venue":null,"work_id":"bbc69ab0-29d7-457e-a44c-f7b5aa6bd81b","year":2011},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.087713Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:828725c15ce9b3a47b40e31b4538f872b106fed212aace1393a2e776af8fe7fd","observation_id":"5b071930-8824-475e-98e3-5537b11461e8","resolution":{"observed_at":"2026-08-12T22:01:23.075982Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:23.064128Z","title":null,"venue":null,"work_id":"3e7431cd-4d3e-49eb-8dec-3c32de6d9fde","year":2013},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.090502Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:8cde8b3877a51728c1c64673d86a920733bfda4c0842df27968d693ff8d9e686","observation_id":"1a1f1f49-18b3-4a6a-be3a-7df41d874d26","resolution":{"observed_at":"2026-08-12T22:01:23.067425Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:23.054197Z","title":"& Briggs, F","venue":null,"work_id":"4dafd686-8b1f-4302-90d1-51a5a9923791","year":2004},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.093217Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:46afd43137992c28ad413584af21373305fbc8e93933965d8c0b0000ad2cacbc","observation_id":"e0f27711-1b1a-480b-92b8-9448147243a1","resolution":{"observed_at":"2026-08-12T22:01:23.057761Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:23.042736Z","title":"2004, Astrophys","venue":null,"work_id":"afba4e74-8260-40a8-9e8c-a949ff836d1c","year":2004},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.096210Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:dc4dc9597230151d522ef21e91166001fbb5b6b549fbcc10dc8355cdb5d07c20","observation_id":"00577cf0-2296-4b7b-9414-295673dce459","resolution":{"observed_at":"2026-08-12T22:01:23.047262Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:23.031238Z","title":null,"venue":null,"work_id":"ced9e124-3d81-4daa-939a-af7ef44daab0","year":2023},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.099190Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:fcdd6083bbd67accd552cee2e41fca13cb0eaf4d53f4bb7546ac04f78660aa78","observation_id":"39f74f6c-2f0b-42b5-993b-d02b4c73cf78","resolution":{"observed_at":"2026-08-12T22:01:23.034897Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.1700","last_updated":"2012-01-09T06:59:39Z","snapshot_observed_at":"2026-08-15T04:23:01.912363Z","submitted_at":"2012-01-09T06:59:39Z","title":"HI Epoch of Reionization Arrays","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.1700","snapshot_observed_at":"2026-08-12T22:01:22.102144Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.102144Z"},"links":{"cited_paper":"/paper/1201.1700","citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:2c808c3008baa6c851dd9c41331de160a97046ec0cf16711172f71ac96df24fb","observation_id":"d68f6e46-a78d-4f41-9dd2-02f574b4de5c","resolution":{"observed_at":"2026-08-12T22:01:22.102144Z","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":"2026-08-12T22:01:23.022199Z","title":"& Mesinger, A","venue":null,"work_id":"b8a69aa8-c0cc-4d3b-a7b5-1d48fc287cff","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.105528Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:11f61876c809136277ae42a55b9eab209f0ee6dd6f329f079b5a4a50a01235fa","observation_id":"ac63d650-df2a-46ad-b254-c82f70fa1114","resolution":{"observed_at":"2026-08-12T22:01:23.025326Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:23.013352Z","title":"J., Smith, D","venue":null,"work_id":"ebb3fb7e-7b58-482c-8886-89dca2139b19","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.109358Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ad300ee7c40c79a04c5aa983a07faf122c318ab99a8bbbb439366c70eecadae2","observation_id":"f541ccf7-f9d2-4af2-8012-407efa1c0e23","resolution":{"observed_at":"2026-08-12T22:01:23.016265Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:23.003854Z","title":"1981, Astronomy and Astrophysics, 100, 209","venue":null,"work_id":"ed719dda-fddb-48ed-b8e6-3ceb6b39239d","year":1981},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.112085Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:f64da3047df7db7588c1c3f82401b795154f89a52422df9287c890b1bd90ad7e","observation_id":"60a73c17-b02f-4f97-987d-472973714a7d","resolution":{"observed_at":"2026-08-12T22:01:23.006952Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.994059Z","title":"K., et al","venue":null,"work_id":"104fe157-6ee1-43be-8971-b014127e2f1f","year":2014},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.115124Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:3dd2ddc4485383629028c139cbbe4f1e54d5c910b19eedb46d066badb6aa0223","observation_id":"a44c296f-2381-418c-a6a6-8d1828fe3fb0","resolution":{"observed_at":"2026-08-12T22:01:22.998244Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.983532Z","title":"L., Woosley, S","venue":null,"work_id":"503ce005-845e-48d7-ac14-6c982862f70a","year":2003},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.118088Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:64a8d71143eff39e80409863b9a0d9b2a8935cda162412d13c59d631a29c0a49","observation_id":"1a710e7f-bcee-4d77-be3e-aaf0cf3ecac3","resolution":{"observed_at":"2026-08-12T22:01:22.987710Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.973597Z","title":"J., Rapetti, D., Burns, J","venue":null,"work_id":"d13df37f-f425-4265-af75-6b7442a6620d","year":2023},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.122167Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:faa83728bf10ead66701aa7615b7919e4104c47c61e20c2b36732bd8ae2f772f","observation_id":"04f11322-4aa3-4ccd-87a7-310c2b9288e4","resolution":{"observed_at":"2026-08-12T22:01:22.976907Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.963117Z","title":null,"venue":null,"work_id":"5f9ef45d-5791-46d0-81db-924659b38029","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.125021Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:f89c7a68a21c6e7a59e616cdb4ae9cda2be30e0c9ef66cb37cdc7c7f69f4d002","observation_id":"f79d6bec-491d-4752-be85-c8688fdc8311","resolution":{"observed_at":"2026-08-12T22:01:22.967089Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.128237Z","title":"D., & Puchwein, E","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.128237Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:5fbb45cdb3143d92dd638a9753968c913e275262714f9e850b9adc8e3f3124b7","observation_id":"baba08c3-4768-4a71-b850-ba92e71524d2","resolution":{"observed_at":"2026-08-12T22:01:22.128237Z","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":"2026-08-12T22:01:22.948186Z","title":null,"venue":null,"work_id":"722248f8-fc77-42a6-b2d2-da9ea66464a9","year":2006},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.131212Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:707a3e0bdb9fa02a3f5126cea8c5e69dbf3801b0021e91e54c9649ddf1ef98f2","observation_id":"e72597b4-a30e-4a9c-ac98-0368473d90b8","resolution":{"observed_at":"2026-08-12T22:01:22.951405Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.133954Z","title":null,"venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.133954Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:51c220679528748e5732c25f2ff28c255c85b2e2cd879d7bf37061a88301b92c","observation_id":"351e411b-3f07-4cc1-949d-41d152284227","resolution":{"observed_at":"2026-08-12T22:01:22.133954Z","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":"2026-08-12T22:01:22.933151Z","title":"A., Venumadhav, T., Dai, L., & Zaldarriaga, M","venue":null,"work_id":"270d8475-8bb3-44ad-b843-cfabde465f8a","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.136356Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:adf1e50ddd5de79820ed0ecdb502ecab89ade4b1b20257328758bebf6d071ae2","observation_id":"eeeb0cbe-4b2b-4489-8239-639a9c66254c","resolution":{"observed_at":"2026-08-12T22:01:22.936185Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.924184Z","title":null,"venue":null,"work_id":"94464d88-6d11-4fea-a109-4f65a26a3d0d","year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.139165Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:e6f70bc6c30c5b2813afc7af8e67793e47fc277627a8ea4d70ed20dc022c40ee","observation_id":"f0f2172a-6912-4b05-91a3-2a8aa3afaec2","resolution":{"observed_at":"2026-08-12T22:01:22.927339Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.914910Z","title":null,"venue":null,"work_id":"fd5f3588-b95a-4984-a366-beabc5e221f1","year":1993},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.141987Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:a9e0345c75194a5d576e904d06ffde0d4e8f383f0998ab6ca163f0bd73a09b58","observation_id":"a2287cbf-ffcc-484f-b2f7-af113b9a83ef","resolution":{"observed_at":"2026-08-12T22:01:22.918201Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.905160Z","title":"D., Eufrasio, R","venue":null,"work_id":"9c2e73b0-e354-43a8-a33b-7d9d0f404454","year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.145005Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:6a3e7c8ad436d568ae052b225d5945bb04c06b280a7a16c293040393c7bed2e0","observation_id":"9251c66f-e9c8-4c5e-872a-3825df583848","resolution":{"observed_at":"2026-08-12T22:01:22.909323Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.896953Z","title":"2017, Mon","venue":null,"work_id":"0d7702fd-b2f9-4340-a883-4ba48058491c","year":2017},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.147790Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ab0aeca82fd5b6cbfdee04bc2f494ae6441923d681cdc8bf2c35327266f55b8c","observation_id":"451d137d-f5c8-48b4-ab77-637b1d43ad18","resolution":{"observed_at":"2026-08-12T22:01:22.899506Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-08-12T19:40:10.586390Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-12T22:01:22.150587Z","title":"2019 [ [arXiv] 1910.13970 ]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.150587Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ff8ce9cd101f5449af52bc284e69d9f594f9528c0706766787c4774771b53ac3","observation_id":"a512a161-fb76-4204-b9e4-652cd9f29e8e","resolution":{"observed_at":"2026-08-12T22:01:22.150587Z","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":"2026-08-12T22:01:22.888550Z","title":null,"venue":null,"work_id":"bc0fda51-b090-4383-a027-4ff8c9adb5b1","year":2016},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.154931Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:7bd42ca2e7889953c2d5c791414ff323aa725f14dc51432d7c7d2b0d6f50865f","observation_id":"395b7d35-71cd-4067-ae54-fb13243b15d3","resolution":{"observed_at":"2026-08-12T22:01:22.891264Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.880086Z","title":"E., Bryan, G","venue":null,"work_id":"a5a2c500-457b-4abd-8cd2-8c108e8ed2fb","year":2001},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.157751Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:38061d0af8cc0ac54bec29cabe5c95c4ee27d79f817316eae93a31c4019b958a","observation_id":"69f6b0a6-5380-4f93-ae56-e961a0c5776e","resolution":{"observed_at":"2026-08-12T22:01:22.883068Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.871083Z","title":"1999, Astronomy and Astrophysics Supplement Series, 140, 145","venue":null,"work_id":"4da1d62e-3cb0-4d73-a3da-a7fb9ba2e746","year":1999},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.160310Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:590173def143e447c6adb30617f04a890532ccc5160577f4d976f5e65c236fcb","observation_id":"342081c8-e2e2-40f4-bdbd-3b1fc2e8faea","resolution":{"observed_at":"2026-08-12T22:01:22.874338Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.862398Z","title":"D., Mozdzen, T","venue":null,"work_id":"fbb0cb48-0dba-48c8-8768-a6ff9a6aefaa","year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.163172Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ba64fda70856ffe0ca5e4fde5e28ab77a9eaa3d9ccad686616bc71a4be76a071","observation_id":"0015785f-ffd9-47d1-8db7-68ce24022771","resolution":{"observed_at":"2026-08-12T22:01:22.865461Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.853485Z","title":"2015, Mon","venue":null,"work_id":"e84297d0-459e-4f89-9745-216d4a8d72f1","year":2015},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.165865Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:f96adfe2b995ae5d91e358630d163b3e78937b31538bd00fa1a1ce180da5762f","observation_id":"07967411-802d-4010-b5a2-301780637881","resolution":{"observed_at":"2026-08-12T22:01:22.856689Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.843250Z","title":null,"venue":null,"work_id":"028eae6c-ee2f-473b-ab90-c3dec6b07c90","year":2013},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.169318Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:c245793b8f3c5a4a992e4bab19362c93e09fbbddf32df214ff4fa8ee5c2567ca","observation_id":"7700c2ea-75d6-448c-80d1-3b6f1e0654e8","resolution":{"observed_at":"2026-08-12T22:01:22.847363Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.834371Z","title":"2014, Mon","venue":null,"work_id":"1e39bccc-cca2-4b0d-9ac8-eb3e125ef997","year":2014},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.171933Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:b34262327052c34445291ad1a72a9a4d52f6462dc56c77c56afae9aa38a62903","observation_id":"bc3c0a27-2d86-4891-a3f9-bdf7efd4b000","resolution":{"observed_at":"2026-08-12T22:01:22.837487Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.825027Z","title":"2011, Mon","venue":null,"work_id":"114b327f-4a51-4ed2-b2a1-336b6ceb8279","year":2011},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.175320Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:53a83f4fc1b0be94a97298391f509264e8d6d9177ba69c7f13e2653db91bda19","observation_id":"d81864d0-51ce-429d-9897-238aefe20dd6","resolution":{"observed_at":"2026-08-12T22:01:22.828776Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.815892Z","title":"2014, Mon","venue":null,"work_id":"54b7b592-33ca-4fd1-8869-2c70cdb41652","year":2014},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.178192Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:57299e6892632a5f58cbf1b3fac35533deba9a94cdea21ffc09aafbf816ee689","observation_id":"02be7e4a-82c9-4082-b321-cd3db4ffc678","resolution":{"observed_at":"2026-08-12T22:01:22.818975Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.806979Z","title":"& Furlanetto, S","venue":null,"work_id":"c6d61912-b071-42fb-866c-d9ca56330db2","year":2019},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.181172Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:5afc47b733f45226506644265b6b30cdb0ed7b04554de5af23440e0c8aaceef8","observation_id":"0c412225-4be8-4df7-869c-98c30927fd1b","resolution":{"observed_at":"2026-08-12T22:01:22.809589Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.798013Z","title":"A., Rogers, A","venue":null,"work_id":"7472baba-c3da-4a60-a366-f3e231d95fd8","year":2017},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.184143Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:57cbcd6bd6438cbfe145a173c018978286b55a90669d536c97c983e0207d2367","observation_id":"31afa28f-9edc-4095-be6d-8fd469311dfc","resolution":{"observed_at":"2026-08-12T22:01:22.801378Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.788821Z","title":null,"venue":null,"work_id":"b6ec9f0e-d859-477e-9f23-00485cdffb0b","year":2024},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.187230Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:c20e476f57d00dc3da14079e52bde6f805292f77b5d0d3122ecafe1ea1db7d88","observation_id":"16c6606f-a92c-43fe-be3c-72902b05d6d4","resolution":{"observed_at":"2026-08-12T22:01:22.791669Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.780573Z","title":null,"venue":null,"work_id":"b4c49a9f-670e-4da2-8588-6b5bb3385ab5","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.190149Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:91a22be81042eb6f342f4f26be0de37a8e7f193a8d1518177ee2746f3d57f362","observation_id":"797f235f-cbd5-499e-9134-8b10fdeaffe9","resolution":{"observed_at":"2026-08-12T22:01:22.783504Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.771822Z","title":"B., Qin, Y., Mesinger, A., et al","venue":null,"work_id":"691817e7-edeb-41d2-8182-0b5b17f12d3d","year":2022},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.193147Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:4a16f5f04ed6f9a645d67c1a9c217168204f265528dca7978af72df7d54020ae","observation_id":"3b89f603-9913-4122-894c-ec46b9d0807c","resolution":{"observed_at":"2026-08-12T22:01:22.775111Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.763476Z","title":null,"venue":null,"work_id":"e448e4d8-b10e-4927-9627-e6416e1948dd","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.196226Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ed1856dc869f958f05a8932052e22b37cd3f43831ce0301628d4280f662deee6","observation_id":"d11afbef-7717-4281-8227-8a438f4f58b3","resolution":{"observed_at":"2026-08-12T22:01:22.766331Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.754539Z","title":"G., Bowman, J","venue":null,"work_id":"060698d2-c194-491b-9082-0d2f709523c0","year":2022},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.199263Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:583c511081af3eff0d8cc399378f44de587894677e00514e795bf3b9249b3281","observation_id":"25129cfd-d3a8-4501-9aba-e28917395853","resolution":{"observed_at":"2026-08-12T22:01:22.758152Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.746760Z","title":"G., Greig, B., Mesinger, A., et al","venue":null,"work_id":"2ab55a87-5a70-439e-bd0c-311bdb90ed5c","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.202432Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:b2ab91ce86984033bd437683d8991cbf91d14f4223d8cf9ff06adb8e997ce848","observation_id":"0af16d67-a71d-46a1-a686-e50aae0c89fc","resolution":{"observed_at":"2026-08-12T22:01:22.749654Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.08552","last_updated":"2020-03-19T03:27:20Z","snapshot_observed_at":"2026-08-16T21:38:51.880468Z","submitted_at":"2020-03-19T03:27:20Z","title":"The Impact of Realistic Foreground and Instrument Models on 21cm Epoch of Reionization Experiments","version":1},"cited_work":{"arxiv_id":"2003.08552","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.08552","snapshot_observed_at":"2026-08-12T22:01:22.363552Z","title":"The Impact of Realistic Foreground and Instrument Models on 21cm Epoch of Reionization Experiments","venue":"astro-ph.CO","work_id":"f4925768-6c5f-4257-a74c-c00a104e166b","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.205159Z"},"links":{"cited_paper":"/paper/2003.08552","citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:fd2ad261f97078974a545f23274c60bf08fc0e64c5f39aa89c44bb0c315a8a97","observation_id":"81ca54bc-f537-4c83-89dc-4c688783e840","resolution":{"observed_at":"2026-08-12T22:01:22.369075Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.738648Z","title":"A., Bouwens, R","venue":null,"work_id":"9a9a54f1-a243-49e2-ab1b-eeafc94b59e6","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.208273Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:5418a9d453a8e0b66c132f498b7936a024723b62ef9e863a9ad9e1d2a4edd4af","observation_id":"90254f7a-fa21-4ca2-8677-4fc3da5c3a71","resolution":{"observed_at":"2026-08-12T22:01:22.741599Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.730566Z","title":"2019, Mon","venue":null,"work_id":"ef522cd5-f63d-4486-a7d5-9c7c9cc3a91a","year":2019},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.211049Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:202616eac00cc5de8438b5c55bb43b2f229d749af6f868c3496f0f301f205da9","observation_id":"616a9817-2cca-492c-a111-c1d7ae3cad2c","resolution":{"observed_at":"2026-08-12T22:01:22.733465Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.01703","last_updated":"2019-12-03T22:06:05Z","snapshot_observed_at":"2026-07-06T08:41:49.632205Z","submitted_at":"2019-12-03T22:06:05Z","title":"PyTorch: An Imperative Style, High-Performance Deep Learning Library","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.01703","snapshot_observed_at":"2026-08-12T22:01:22.213972Z","title":"2019, arXiv e-prints, arXiv:1912.01703","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.213972Z"},"links":{"cited_paper":"/paper/1912.01703","citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:1e5b45a4de7535f481b602a3fdc9cc842d53d4076465a91812d7e482ca252e79","observation_id":"518ab70b-c0cd-4ae2-889f-fcb668893477","resolution":{"observed_at":"2026-08-12T22:01:22.213972Z","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":"2026-08-12T22:01:22.722072Z","title":null,"venue":null,"work_id":"a9157309-6c90-4a5e-8da6-f6673a147ef6","year":2007},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.217280Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:e5d1d6efdab5946ec033f66b8ce8932aa8c74f294f76c341defa39a891641148","observation_id":"69d853fa-b98a-45bb-a01a-7b097744e781","resolution":{"observed_at":"2026-08-12T22:01:22.725020Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.713219Z","title":null,"venue":null,"work_id":"f3143027-d63f-4030-a14e-57e5c7490ec5","year":2012},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.220251Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:e0c12f093a141a90877c7be75cb6642a514ac067e670d33fde3c8165187cf538","observation_id":"c3a997f2-906b-4190-83f9-fe002e325523","resolution":{"observed_at":"2026-08-12T22:01:22.716743Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.704541Z","title":"2021, Mon","venue":null,"work_id":"6d458594-8c6d-493a-a7bd-52915d6d88f9","year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.223042Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:2d8deddeb1f20f543c601cf116ed9cd96b832f8d206115e945699e76da686d13","observation_id":"9b21de98-91a3-4b44-bdb4-f81ba3e6432c","resolution":{"observed_at":"2026-08-12T22:01:22.708232Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.695870Z","title":null,"venue":null,"work_id":"143cdd9a-171b-45af-aafc-4b233021a19e","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.225884Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:9c1089884f8cf72a99867eac0050146854c0503bb387eed51cd3122930b8fc87","observation_id":"4279bfe7-8dc0-49f4-b807-299d0030e1d1","resolution":{"observed_at":"2026-08-12T22:01:22.699171Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.687520Z","title":"2020 b , Mon","venue":null,"work_id":"06b9f2ac-b570-423c-afca-ecd1166aa08e","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.229019Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:38f52b9a0d7d9c485d5b3380a91b3c98f4accfa91ce477f68a1a436c68c6d8f6","observation_id":"09abcd37-ad7d-438d-bf7c-d651e81852d1","resolution":{"observed_at":"2026-08-12T22:01:22.690491Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.680109Z","title":"& Reich, W","venue":null,"work_id":"cb5a02d6-9486-4251-9b6a-a0bff6dc23d8","year":1986},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.231590Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:7dd2c26f89b0568b22c17f69dcfa5c46b7866fee83a4f8e5e9039f1b217115e9","observation_id":"f7463654-6af4-47e0-bc64-22c10f503ee6","resolution":{"observed_at":"2026-08-12T22:01:22.682695Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.671556Z","title":"2020, Mon","venue":null,"work_id":"324fdf9e-9cd9-4ea6-be16-bf41167701cd","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.234088Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ba4268547890ba518c8a156f3fb5f325882e6a3332ab93c04f442b2361497ada","observation_id":"27a356b3-050e-48d7-96ec-4376dfd26ed3","resolution":{"observed_at":"2026-08-12T22:01:22.675131Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.663487Z","title":"S., Costain, C","venue":null,"work_id":"7ecb6ad0-a4e3-4816-afed-122e30d064b2","year":1999},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.237182Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:844b72627c0f9be96b8a00a821131b2540cdbd5896cd969292ccbaa87ded1c69","observation_id":"32d2c34b-19f5-4d8e-a501-809a8a855b24","resolution":{"observed_at":"2026-08-12T22:01:22.666208Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.654472Z","title":"2006, JHEP, 05, 002","venue":null,"work_id":"ec466412-4206-4511-b4fe-f999ec90ad1e","year":2006},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.239994Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:7bc83cffc5979ae4801c64e6a999b19dd315f7c34aa985a9edf820918c5ee334","observation_id":"8da4c34e-e6d1-42e1-9461-2f3ff6424590","resolution":{"observed_at":"2026-08-12T22:01:22.657795Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.646061Z","title":"2011, Mon","venue":null,"work_id":"f4138c7b-10ab-437c-8ed3-d4464487b570","year":2011},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.242467Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:7604a9cbe2436adbbb9c82c5608e2396bd8cf6024c53d8d046fbc5a6999c69e6","observation_id":"81e7228b-36e3-4104-aece-53afc29701d6","resolution":{"observed_at":"2026-08-12T22:01:22.649004Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.638269Z","title":null,"venue":null,"work_id":"22975bd1-a107-4bd4-b226-c764113508b0","year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.245345Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:59275a1f280147823c0912d689adbbc3d2cb03cd26b4acad443f3b0fb48df102","observation_id":"bbf98538-8074-4675-ba0c-4d3aa167fae0","resolution":{"observed_at":"2026-08-12T22:01:22.640933Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.631069Z","title":"2018, Mon","venue":null,"work_id":"ee89579a-7e0c-4e99-9167-69f52197b690","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.248710Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:00ae625f3130d3890ca16408d1e161883b8303acd543e45e63ee1ac1e4d7c471","observation_id":"fa120e89-1656-47ee-b4eb-da92614a04d7","resolution":{"observed_at":"2026-08-12T22:01:22.633651Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.622714Z","title":"2021, Mon","venue":null,"work_id":"182747d8-e422-4778-9a99-c273c220810e","year":2021},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.251028Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:2e4c37ae689913b47dc2ac7bfb36f89246c3577074210c44daa51d36d7482487","observation_id":"c1124ddc-bbd7-4ca9-8d13-c0320657c359","resolution":{"observed_at":"2026-08-12T22:01:22.625762Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.614294Z","title":"2024, Astrophys","venue":null,"work_id":"15150849-ba93-498b-a261-7e22c1897e55","year":2024},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.254104Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:ac41dfb2543e15df4bbae9b01ca7d0cea8000adf24e258cc4ef0231cd5a80b4b","observation_id":"6a094c54-d314-4662-ad15-1bf30f427afa","resolution":{"observed_at":"2026-08-12T22:01:22.617585Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.604925Z","title":"2023, Mon","venue":null,"work_id":"7348e337-3683-44c5-80a3-1b357626da24","year":2023},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.256891Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:548f065f1bc56926158dd4753e19502b16b72d55e0cffa31dcf13cc65ed4d999","observation_id":"fb8fd020-f18a-4d9e-aa9c-83972733c25e","resolution":{"observed_at":"2026-08-12T22:01:22.608671Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.595658Z","title":"H., Bowman, J","venue":null,"work_id":"df27c479-8eb9-4480-a3c0-80bbd9f4d628","year":2023},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.260043Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:9e5ef5643b1332329cb866960968a411591a72f06dfe57df516649fc0d4ecddc","observation_id":"3e44d046-4962-49a3-a70d-624910753984","resolution":{"observed_at":"2026-08-12T22:01:22.599501Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.587194Z","title":null,"venue":null,"work_id":"1dc52dca-4878-4814-a6e9-b8e46a11579e","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.263369Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:a1928efedfe75ee485d662306a61385415f5b87f69442714cebaae2dd7c70fb7","observation_id":"59aab737-9727-4f65-a7c3-32e2beadc870","resolution":{"observed_at":"2026-08-12T22:01:22.590229Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.579015Z","title":"2022, Nature Astron., 6, 607","venue":null,"work_id":"3b532e7d-09e0-480c-b429-e1b80e4d78ac","year":2022},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.266416Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:4c90dbd892efc67724dec6b140f3b029d5aa17a76f9e26a2d0ab8e3631d073f4","observation_id":"6a6de969-cca7-4df6-9875-3c0526318534","resolution":{"observed_at":"2026-08-12T22:01:22.581996Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04540","last_updated":"2019-06-06T15:36:35Z","snapshot_observed_at":"2026-08-15T20:19:19.111642Z","submitted_at":"2019-03-11T18:53:27Z","title":"The redshifted 21-cm signal in the EDGES low-band spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.04540","snapshot_observed_at":"2026-08-12T22:01:22.269659Z","title":"& Subrahmanyan, R","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.269659Z"},"links":{"cited_paper":"/paper/1903.04540","citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:2b5ff2db1909675c646df7a273df4aa3a0a0676ff3cb65fbead9b7bbc94dcd9b","observation_id":"030126c1-b55e-4cfc-8749-34a8a3d3be10","resolution":{"observed_at":"2026-08-12T22:01:22.269659Z","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":"2026-08-12T22:01:22.569997Z","title":"U., et al","venue":null,"work_id":"f47da1c5-bdb5-4cb4-81e0-cdf45cfc0152","year":2018},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.273217Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:f8973bf7c5343f31046117764e13f89eeea2b49a762983077c276c6f66d67521","observation_id":"2b2984d1-8c87-4578-9ea1-b1cad1d2a13e","resolution":{"observed_at":"2026-08-12T22:01:22.572710Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.561876Z","title":"2004, AIP Conf","venue":null,"work_id":"6bac2646-dcc9-4992-a236-393b55776f15","year":2004},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.276369Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:4e3c1e5e6cdb0f38b9a8ae87270ca4b0d053ae3b844dd13cffbe4376e31fd14a","observation_id":"9fd05720-46a6-4fdc-bde1-b549ca538d5b","resolution":{"observed_at":"2026-08-12T22:01:22.564752Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.553641Z","title":"& Mesinger, A","venue":null,"work_id":"b9891e2f-72e9-4024-98e4-9a5fd3758049","year":2013},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.279353Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:336ccfa0f7a7e4eb1a577c2f1a61b964549e2c8abe276885378d7491b38a0ea1","observation_id":"60258f56-d1a8-4b8a-a6a7-3a607235ba43","resolution":{"observed_at":"2026-08-12T22:01:22.556616Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.544852Z","title":"& Mesinger, A","venue":null,"work_id":"43bc434e-ff94-4679-9471-0fa0fff2a286","year":2014},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.282393Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:3fbc2128bf018b6b53acbce7342ccf59909079d285a07d7a14ed7960ad3e7a44","observation_id":"0cbcacda-044d-4685-9b01-728a39e55a2e","resolution":{"observed_at":"2026-08-12T22:01:22.547944Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+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":"2026-08-12T22:01:22.536224Z","title":null,"venue":null,"work_id":"c78d07c4-0794-4949-b060-28b78942aff4","year":1999},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.285156Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:36163fbd7b1972e601c4fd1eef0412fcb52efb0c17ec7a7253e105bb658b0350","observation_id":"5d2392ef-02ee-4d7f-8f0f-91ee88410edd","resolution":{"observed_at":"2026-08-12T22:01:22.539178Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.11608","last_updated":"2023-12-18T19:00:00Z","snapshot_observed_at":"2026-08-16T14:33:39.013813Z","submitted_at":"2023-12-18T19:00:00Z","title":"Inhomogeneous Energy Injection in the 21-cm Power Spectrum: Sensitivity to Dark Matter Decay","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.11608","snapshot_observed_at":"2026-08-12T22:01:22.288182Z","title":"W., Liu, H., Mu\\ noz, J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.288182Z"},"links":{"cited_paper":"/paper/2312.11608","citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:8bb4e55ae8a02e24fe5ea9fc82bfa55ccf551914a4e34b47411de468eb26ba90","observation_id":"6f7c194d-c85a-4269-b0c2-6fa775b173c9","resolution":{"observed_at":"2026-08-12T22:01:22.288182Z","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":"2026-08-12T22:01:22.527994Z","title":null,"venue":null,"work_id":"edc12b67-37e9-4899-a38d-55a6949de12b","year":2020},"citing_paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-12T22:01:22.291111Z"},"links":{"citing_paper":"/paper/2411.08134"},"observation_digest":"sha256:65e184813787372ec1a8fc9a8fd0685ad2bc0fedc49d72a0bb691b07d9dd7855","observation_id":"7d6864a7-be53-41e7-994e-4ad0d08347b8","resolution":{"observed_at":"2026-08-12T22:01:22.530799Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.08134","last_updated":"2024-11-12T19:26:34Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-19T07:44:17.689964Z","submitted_at":"2024-11-12T19:26:34Z","title":"The EDGES measurement disfavors an excess radio background during the cosmic dawn"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":56,"verified_exact":1,"verified_fuzzy":42},"total_outbound_references":110},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 100 of 110 outbound references and 8 inbound Pith citation observations for arXiv:2411.08134."}