{"as_of":"2026-08-13T17:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c94bf5be30de750a453e5ad4896c3be3ab14470ceab08f7d25536317dce1b419","coverage":[{"denominator":71,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":71,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-08T19:14:15.479515Z","state":"measured"},{"denominator":73,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":73,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T21:39:28.419506Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-06-30T14:04:45.181032Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"cited_work":{"arxiv_id":"2605.01990","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.01990","snapshot_observed_at":"2026-06-30T14:04:45.181032Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","venue":"astro-ph.CO","work_id":"ac6266f6-4d28-4952-bbcc-354d0c6f185d","year":2026},"citing_paper":{"arxiv_id":"2606.29761","last_updated":"2026-06-29T04:12:51Z","snapshot_observed_at":"2026-08-09T07:44:14.344274Z","submitted_at":"2026-06-29T04:12:51Z","title":"Estimating Cosmological Parameters from Localized Fast Radio Bursts: A Method for Removing Milky Way Dispersion-Measure Contributions","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-06-30T05:38:11.796883Z"},"links":{"cited_paper":"/paper/2605.01990","citing_paper":"/paper/2606.29761"},"observation_digest":"sha256:f6be7b1ba9e20a7a6b4282aba1586e3d2218d21b2c5066d9b7d300e75c6246bd","observation_id":"96c9f538-1d05-41aa-b033-b0e7df061c19","resolution":{"observed_at":"2026-06-30T14:04:45.182366Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2605.01990","snapshot_observed_at":"2026-07-11T21:39:28.419506Z","title":"L., de Farias, K","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.04106","last_updated":"2026-07-05T04:04:05Z","snapshot_observed_at":"2026-08-07T13:53:36.853851Z","submitted_at":"2026-07-05T04:04:05Z","title":"Measuring the Angular Auto-power Spectrum of Fast Radio Burst Dispersion Measures as a Robust Cosmological Probe and Baryon Tracer","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-11T21:39:28.419506Z"},"links":{"cited_paper":"/paper/2605.01990","citing_paper":"/paper/2607.04106"},"observation_digest":"sha256:cac58b293d93d63d3b5cf8590e59a067cb7bf6b5b0c8beccc1ecc3504dcdc75d","observation_id":"6f036c9c-b34e-40af-8345-d41130e2a43e","resolution":{"observed_at":"2026-07-11T21:39:28.419506Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2605.01990/citation-record","integrity":"/paper/2605.01990/integrity","json":"/paper/2605.01990/citation-record.json","paper":"/paper/2605.01990"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"0709.4301","last_updated":"2007-09-27T02:56:15Z","snapshot_observed_at":"2026-08-13T03:46:03.377177Z","submitted_at":"2007-09-27T02:56:15Z","title":"A bright millisecond radio burst of extragalactic origin","version":1},"cited_work":{"arxiv_id":"0709.4301","doi":null,"metadata_source":"pith","pith_arxiv_id":"0709.4301","snapshot_observed_at":"2026-07-04T05:29:35.280847Z","title":"A bright millisecond radio burst of extragalactic origin","venue":"astro-ph","work_id":"a75d14b0-e704-49e8-afe5-abb95d60773e","year":2007},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/0709.4301","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:7e2ce592151a33fbc0b77b78cf577787059debf0701176dfb6ae2a8da36372eb","observation_id":"c47082cb-2ca3-46b6-8c54-c6a2630225f0","resolution":{"observed_at":"2026-05-09T06:00:35.622297Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.00609","last_updated":"2021-08-31T06:51:56Z","snapshot_observed_at":"2026-07-06T11:34:38.097152Z","submitted_at":"2021-08-02T02:59:55Z","title":"81 New Candidate Fast Radio Bursts in Parkes Archive","version":2},"cited_work":{"arxiv_id":"2108.00609","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.00609","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Yang et al.,81 New candidate fast radio bursts in Parkes archive,Mon","venue":null,"work_id":"18b87585-5076-4a5f-97e3-a912f8fa8431","year":2021},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2108.00609","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:327caefcd689b3c83e4ba51b9d817bb09b06296e158726277f25553391d4aa31","observation_id":"3bd1229d-badb-4b83-b9a3-1b6e5eed9ace","resolution":{"observed_at":"2026-05-09T06:00:35.395030Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.00753","last_updated":"2015-11-12T20:48:25Z","snapshot_observed_at":"2026-07-06T04:05:17.521328Z","submitted_at":"2015-01-05T03:10:11Z","title":"Supergiant Pulses from Extragalactic Neutron Stars","version":2},"cited_work":{"arxiv_id":"1501.00753","doi":null,"metadata_source":"pith","pith_arxiv_id":"1501.00753","snapshot_observed_at":"2026-06-26T03:18:57.626311Z","title":"Supergiant Pulses from Extragalactic Neutron Stars","venue":"astro-ph.HE","work_id":"9100de51-f602-4424-9cc5-cb0ac9663441","year":2015},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1501.00753","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:eb989c94431dfe74b051b7206fca3727a54049759e0eb02aedaef7c29c0cc8b0","observation_id":"7f1b37f0-ab02-4623-a6db-33042ff82916","resolution":{"observed_at":"2026-05-09T06:00:35.625741Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.2006","last_updated":"2007-11-28T16:19:17Z","snapshot_observed_at":"2026-07-06T01:30:38.641244Z","submitted_at":"2007-10-10T13:25:13Z","title":"Hyperflares of SGRs as an engine for millisecond extragalactic radio bursts","version":2},"cited_work":{"arxiv_id":"0710.2006","doi":"10.48550/arxiv.0710.2006","metadata_source":"pith","pith_arxiv_id":"0710.2006","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Hyperflares of SGRs as an engine for millisecond extragalactic radio bursts","venue":"astro-ph","work_id":"1641c874-4af9-4623-9569-1e3f3e75bc66","year":2007},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/0710.2006","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:f16bcc5386046a516e485e8a9bed041e72ea9a3d6e5cabc248c8ff8b4881cd20","observation_id":"dd35ded7-d4a3-4311-8022-89657fdfb66e","resolution":{"observed_at":"2026-05-09T06:00:35.756540Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-07-12T17:50:14.953705+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T17:50:14.953705+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01341","last_updated":"2015-05-20T21:58:27Z","snapshot_observed_at":"2026-08-10T09:39:42.163856Z","submitted_at":"2015-01-07T00:55:41Z","title":"Local Circumnuclear Magnetar Solution to Extragalactic Fast Radio Bursts","version":4},"cited_work":{"arxiv_id":"1501.01341","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1501.01341","snapshot_observed_at":"2026-07-04T20:28:32.687110Z","title":"Pen and L","venue":null,"work_id":"171d0742-9425-43f2-b175-041d337783cc","year":2015},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1501.01341","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:fd8787ad0da5652ffea2ad349ad558af0827f9aa5ccfe1e622eb52a706df71c2","observation_id":"bc909226-3f13-470e-8b7e-bc0e72af7beb","resolution":{"observed_at":"2026-07-04T20:28:32.687110Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2005.13161","last_updated":"2020-05-27T04:58:52Z","snapshot_observed_at":"2026-08-11T03:42:42.243173Z","submitted_at":"2020-05-27T04:58:52Z","title":"A census of baryons in the Universe from localized fast radio bursts","version":1},"cited_work":{"arxiv_id":"2005.13161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2005.13161","snapshot_observed_at":"2026-07-04T05:29:35.354941Z","title":"Macquart et","venue":null,"work_id":"6dfe3867-9a0e-41f2-ac4a-966dba174a80","year":2020},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2005.13161","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:6ea670a7b9b27074a552c020a4a37488901fd4056d7d69379420713462798cb1","observation_id":"216d9b10-59c8-41e0-b993-cdc0f6baf4d2","resolution":{"observed_at":"2026-05-09T06:00:35.397846Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.16952","last_updated":"2025-06-24T23:58:30Z","snapshot_observed_at":"2026-08-12T22:37:44.755734Z","submitted_at":"2024-09-25T14:07:23Z","title":"A gas-rich cosmic web revealed by the partitioning of the missing baryons","version":2},"cited_work":{"arxiv_id":"2409.16952","doi":"10.48550/arxiv.2409.16952","metadata_source":"arxiv_reference","pith_arxiv_id":"2409.16952","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Connor et al","venue":"arXiv (Cornell University)","work_id":"9f597119-ef4e-4409-aba8-399c0c8d7099","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2409.16952","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:58fc49d3d4387a531a625c76661acb7026708482bb5d191b2e340ea6a2bc8879","observation_id":"8ed99459-f261-463b-a645-b8a689d3dddb","resolution":{"observed_at":"2026-05-09T06:00:35.740058Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Wang, S.-J","venue":null,"work_id":"e142f426-61ad-44bd-b20a-e470bd9d955a","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e65fd10b8623f314ebd2ddbe26ecf0de35db767aa0d7bed2d14dc2a849334f45","observation_id":"144abe31-d675-422f-949f-29857f0b2cb4","resolution":{"observed_at":"2026-05-26T03:11:37.678340Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Wu, S.-B","venue":null,"work_id":"c704cf0e-a961-4c42-ac6e-9d34a738499d","year":2016},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e17fa24c39390d35c2b17e1fed4a95d8bd0e56e82ea36e7585f29d57ee721c20","observation_id":"061438f3-a268-472c-a218-eb5c0637d637","resolution":{"observed_at":"2026-05-26T03:11:37.681882Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.06975","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-04T05:29:35.256827Z","title":"Sales, K.E.L","venue":null,"work_id":"0fdba392-487e-484a-a34b-ca9d21ab26b2","year":2026},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e7e8489fe19eaf5e23ca53032dbd702438b898542f24d1497e7be6358338030a","observation_id":"c249f1f9-4a34-4157-a76d-50843b9dd43f","resolution":{"observed_at":"2026-05-09T06:00:35.584680Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"15229f20-f6a9-431e-948a-a4eb9b4ed718","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:98bb82d460b5915f2000b71a29c42a29b8702e7fffda5d0c794bf50c55283f52","observation_id":"6e531c51-fe3d-494c-932e-115e90746776","resolution":{"observed_at":"2026-05-26T03:11:37.685329Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"G´ omez-Vargas, R","venue":null,"work_id":"e63458e2-54d3-43db-a3f6-939eb340c84a","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:4b5110811c776095402e41a19262822fc81eca2e6dbbbeb05a9de1c9499548bc","observation_id":"059cef5a-2328-4567-877d-5853e6e238bf","resolution":{"observed_at":"2026-05-26T03:11:37.654501Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Lemos, R.S","venue":null,"work_id":"56434a59-6642-4454-bd34-5b1f1a69fe6d","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:671d1b59b4aa31fbd5a68b0606bb2d16d95c0d42778a1e0e201ef0d384bc6f21","observation_id":"d887f4df-2586-4aee-a342-a1d35f7d1acf","resolution":{"observed_at":"2026-05-26T03:11:37.649136Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.03636","last_updated":"2022-08-24T20:54:25Z","snapshot_observed_at":"2026-08-08T13:09:33.951599Z","submitted_at":"2019-10-08T18:40:29Z","title":"Reconstructing Functions and Estimating Parameters with Artificial Neural Networks: A Test with the Hubble Parameter and SNe Ia","version":5},"cited_work":{"arxiv_id":"1910.03636","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.03636","snapshot_observed_at":"2026-07-10T20:07:33.185268Z","title":"Wang, X.-J","venue":"astro-ph.CO","work_id":"9b214378-b016-4f90-b23a-54ff64693ca1","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1910.03636","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:04a69501d9c34bd13d87f8181ab243bf65acb0ef3503e6aa1267f51beb90258f","observation_id":"fe90cd39-21b6-4889-ba63-1d24a171bca0","resolution":{"observed_at":"2026-05-09T06:00:35.778723Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Aghanim, Y","venue":null,"work_id":"4bafaa25-0318-463f-a42e-17da3b991e2d","year":2018},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:94f04c19cc78ce7909272035abdcadab6ff0f74630a771f26e42199feb1bf215","observation_id":"3e666ed1-4092-4b39-8f3c-231bcbbd11ea","resolution":{"observed_at":"2026-05-26T03:11:37.651737Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Cooke, M","venue":null,"work_id":"cb07fdb3-295e-40a9-bda3-fcd4de6dffd5","year":2018},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:219b734632f36601d958ad0280903583db041a1ef861d5c4c20a33e24a596fac","observation_id":"a48f6db1-938f-4b10-99df-198e4d5ad9b9","resolution":{"observed_at":"2026-05-26T03:11:37.646501Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Petroff, J","venue":null,"work_id":"27adfa34-2f4f-4087-b598-813b5e9414cc","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:6d712ad31f10b636b88dc184b438178d618114ef0dccf9310e6ec5f3fe266bc3","observation_id":"e1995c62-491a-4b1d-bcfe-c309f12b3df8","resolution":{"observed_at":"2026-05-26T03:11:37.640722Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Cordes and S","venue":null,"work_id":"d2007ede-1380-4a91-a03a-e02f6be577c6","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:51201fe5f327f2b95466dd3d97794167f9d08ab8c0a1ead85d5cfdee30d5906e","observation_id":"ff0dfbc5-845e-4b10-9e35-a7b04a42f191","resolution":{"observed_at":"2026-05-26T03:11:37.675102Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1412.0342","last_updated":"2014-12-01T04:09:48Z","snapshot_observed_at":"2026-08-10T06:35:55.433022Z","submitted_at":"2014-12-01T04:09:48Z","title":"A real-time fast radio burst: polarization detection and multiwavelength follow-up","version":1},"cited_work":{"arxiv_id":"1412.0342","doi":null,"metadata_source":"pith","pith_arxiv_id":"1412.0342","snapshot_observed_at":"2026-07-04T05:29:35.296077Z","title":"Petroff et al., Mon","venue":"astro-ph.HE","work_id":"aac85a04-1cd4-4228-8f50-eafb16c88800","year":2014},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1412.0342","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:b719cb365a9f59d8e5fd1599235941f6e3635bd0fb5bf4c0ba72347fa899d4c6","observation_id":"ec794948-b27e-4300-a540-0b9cbc8178f9","resolution":{"observed_at":"2026-05-09T06:00:35.590697Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.07947","last_updated":"2019-04-16T19:54:57Z","snapshot_observed_at":"2026-07-06T07:46:37.610002Z","submitted_at":"2019-04-16T19:54:57Z","title":"Fast Radio Bursts","version":1},"cited_work":{"arxiv_id":"1904.07947","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.07947","snapshot_observed_at":"2026-07-03T08:27:48.071378Z","title":"Fast Radio Bursts","venue":"astro-ph.HE","work_id":"ac992982-af48-4bba-9827-a24dfccdb6c1","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1904.07947","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:9b01858251269f1d83cf0e90e21ee90b8f0113b156c813c7d3d1b27619f662f3","observation_id":"c794f8fd-d539-4b12-8ee8-c15d1adb1ad5","resolution":{"observed_at":"2026-05-09T06:00:35.389794Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Shull, B.D","venue":null,"work_id":"a9063a7c-2627-441b-9dd5-ec0c61f3a130","year":2012},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:17d2e2f49e0bce1f6ba433128a324e89bbb2844eb0776585eb09dd1109bebe4d","observation_id":"93aab518-eee3-4189-beca-2cf1dab1eedb","resolution":{"observed_at":"2026-05-26T03:11:37.668555Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0711.3358","last_updated":"2008-12-15T12:13:53Z","snapshot_observed_at":"2026-07-06T01:32:56.328535Z","submitted_at":"2007-11-21T12:10:28Z","title":"The Physics of the Intergalactic Medium","version":3},"cited_work":{"arxiv_id":"0711.3358","doi":null,"metadata_source":"pith","pith_arxiv_id":"0711.3358","snapshot_observed_at":"2026-07-04T15:29:55.099000Z","title":"The Physics of the Intergalactic Medium","venue":"astro-ph","work_id":"bad8bdd3-f380-4da0-964e-b58cad174b59","year":2007},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/0711.3358","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:d31995376726c9f9c241864c246af6e5896704c19770382ff901e017d87bf5b7","observation_id":"40269cdf-3889-475c-81bf-134e4b4512d1","resolution":{"observed_at":"2026-05-09T06:00:35.305103Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Becker, J.S","venue":null,"work_id":"f23befab-dd4a-4067-91c0-276e4a54e987","year":2011},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e16a7dde4d4a7110f948cb5b28dea0e46c56687929221559169341a4ab96f453","observation_id":"027ecdd5-75db-4a76-a98b-149fc67eec72","resolution":{"observed_at":"2026-05-26T03:11:37.657784Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Zhang, H","venue":null,"work_id":"7f419834-326b-4fe1-8df1-766bf9633064","year":2020},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:2626a8875bc9a801623b125444f29f68f6d6cc4388d6e5c65ba19c83acd061ff","observation_id":"e11f8866-1cf2-422d-8330-82ee6d951d24","resolution":{"observed_at":"2026-05-26T03:11:37.637707Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1511.07289","last_updated":"2016-02-22T07:02:58Z","snapshot_observed_at":"2026-08-12T19:49:02.032824Z","submitted_at":"2015-11-23T15:58:05Z","title":"Fast and Accurate Deep Network Learning by Exponential Linear Units (ELUs)","version":5},"cited_work":{"arxiv_id":"1511.07289","doi":"10.48550/arxiv.1511.07289","metadata_source":"pith","pith_arxiv_id":"1511.07289","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Fast and Accurate Deep Network Learning by Exponential Linear Units (ELUs)","venue":"cs.LG","work_id":"619b409a-ddb8-4401-b55e-d8ca367322ce","year":2015},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1511.07289","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:85349e354b0647900ecea77aa4f25981f43700a1b70feb9db1291b5c42892419","observation_id":"978f5e19-822f-434b-8fe5-c621fbc6e25d","resolution":{"observed_at":"2026-05-09T06:00:35.725202Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.15499","last_updated":"2023-10-29T04:27:53Z","snapshot_observed_at":"2026-08-13T11:34:06.669819Z","submitted_at":"2023-05-24T18:42:21Z","title":"Neural network reconstruction of cosmology using the Pantheon compilation","version":2},"cited_work":{"arxiv_id":"2305.15499","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2305.15499","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Dialektopoulos, P","venue":null,"work_id":"0d90c27b-f3d3-405f-9fcf-6f1b925c1f64","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2305.15499","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:ad1553913fd21dddb7c7507c03cb7c93a782c8dcc22573db9cdc266163da06e1","observation_id":"e2404038-a632-4de8-a11d-3e394fd51473","resolution":{"observed_at":"2026-05-09T06:00:35.702702Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.06450","last_updated":"2024-10-09T01:13:58Z","snapshot_observed_at":"2026-08-12T22:27:43.626239Z","submitted_at":"2024-10-09T01:13:58Z","title":"Hints of new physics for the Hubble tension: violation of cosmological principle","version":1},"cited_work":{"arxiv_id":"2410.06450","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.06450","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"25c41db9-2c08-4cc9-bc51-10dbfd6dfb89","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2410.06450","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:ae01e3536b8f09e7adc7acc6238ee6497aef850bce2b7562716a46718bd65922","observation_id":"0e3e7536-1c31-444d-b0c0-97cc330f3fa8","resolution":{"observed_at":"2026-05-09T06:00:35.400433Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2510.09463","last_updated":"2026-05-01T12:31:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-10T15:15:00Z","title":"Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology","version":3},"cited_work":{"arxiv_id":"2510.09463","doi":null,"metadata_source":"pith","pith_arxiv_id":"2510.09463","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology","venue":"astro-ph.CO","work_id":"1b5adf34-1522-4af1-a131-5f43df544885","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2510.09463","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:1c68edd78ebcab6569cadd1e1c1c07ef3af5ad491b7267e4d7afba6adc8aadc0","observation_id":"01c0823d-eb2b-4e1b-9665-61aec7508131","resolution":{"observed_at":"2026-05-09T06:00:35.249480Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2604.16154","last_updated":"2026-06-10T16:34:42Z","snapshot_observed_at":"2026-07-12T19:25:28.019823Z","submitted_at":"2026-04-17T15:24:35Z","title":"Probing Primordial Black Holes with upcoming Radio Telescopes: a case study for LOFAR2.0, FAST Core Array and BINGO","version":3},"cited_work":{"arxiv_id":"2604.16154","doi":null,"metadata_source":"pith","pith_arxiv_id":"2604.16154","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Probing Primordial Black Holes with upcoming Radio Telescopes: a case study for LOFAR2.0, FAST Core Array and BINGO","venue":"astro-ph.CO","work_id":"07441b50-3d8f-43e2-8a05-bb38f970d100","year":2026},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2604.16154","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:67632ad8be1b3cdf8b5494bfa3c617a031c75b9568234b381d596e75066bb159","observation_id":"07611c7e-2b09-4689-9bfb-adbaf0f2bfcc","resolution":{"observed_at":"2026-05-09T06:00:35.743165Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207156","last_updated":"2003-01-28T16:07:00Z","snapshot_observed_at":"2026-07-07T00:27:17.742565Z","submitted_at":"2002-07-08T08:32:31Z","title":"NE2001.I. A New Model for the Galactic Distribution of Free Electrons and its Fluctuations","version":3},"cited_work":{"arxiv_id":"astro-ph/0207156","doi":"10.48550/arxiv.astro-ph/0207156","metadata_source":"pith","pith_arxiv_id":"astro-ph/0207156","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"NE2001.I. A New Model for the Galactic Distribution of Free Electrons and its Fluctuations","venue":"astro-ph","work_id":"68414f2c-2cc8-4708-b999-0d98f6ee7aac","year":2002},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/astro-ph/0207156","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:8b19251f8d3197bcccff27b54a6910b9915c7d90f8bb27c433ce55c4189a89d3","observation_id":"dd5dc4e8-86b3-4bcf-9187-7fda0aa9f18e","resolution":{"observed_at":"2026-05-09T06:00:35.735699Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-03T21:38:30.240113+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T21:38:30.240113+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2504.06845","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zhang, Y","venue":null,"work_id":"8006df7e-3df2-4306-b801-d013b7d2cac6","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:852546aceedc410c640b9bd6b1b88c8d3161e9936b493400e57f0b599c3ffbac","observation_id":"39bf160c-cd80-4b10-aaf2-871bb72aa094","resolution":{"observed_at":"2026-05-09T06:00:35.768765Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Buchner,A statistical test for nested sampling algorithms,Statistics and Computing26 (2016) 383","venue":null,"work_id":"c418eb61-ff34-4666-8c56-2495c89cc6da","year":2016},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:9053426fb918fdcd7c8a1f23f6b9366bf736c1f74a6a81adcb62c059d0a436cd","observation_id":"722bce91-89df-439a-8f2e-8b83d0a885de","resolution":{"observed_at":"2026-05-26T03:11:37.643929Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Buchner,Collaborative nested sampling: Big data versus complex physical models, Publications of the Astronomical Society of the Pacific131(2019) 108005","venue":null,"work_id":"8c5e268f-ddbd-48ce-8dde-b206a64a1027","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:51db8c5dab177b8ff27061e84647c1b925b3552ddeffafad945c4dbc55ef0331","observation_id":"8d1b7ab8-7e7c-4d39-949f-b92609410226","resolution":{"observed_at":"2026-05-26T03:11:37.634448Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.09604","last_updated":"2021-04-07T13:27:40Z","snapshot_observed_at":"2026-08-05T15:12:13.168556Z","submitted_at":"2021-01-23T23:32:43Z","title":"UltraNest -- a robust, general purpose Bayesian inference engine","version":2},"cited_work":{"arxiv_id":"2101.09604","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.09604","snapshot_observed_at":"2026-07-08T13:54:58.353112Z","title":"2021, UltraNest – a robust, general purpose Bayesian inference engine","venue":"stat.CO","work_id":"091f7954-87f0-4dbd-8b57-6bf91374b5f6","year":2021},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2101.09604","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e03e722a2b2f5c92afa9651825a516a35aa8df85c60f174e6dcedbc327d400ec","observation_id":"464ef27b-3e59-4604-8b08-7d79aa73d06d","resolution":{"observed_at":"2026-05-09T06:00:35.762797Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Lewis,Getdist: a python package for analysing monte carlo samples,Journal of Cosmology and Astroparticle Physics2025(2025) 025","venue":null,"work_id":"754767ee-e1aa-4dae-925c-7b86ce02007a","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:a119fa367649572d1d468e801a1765f07988f115f4d6c5f1daa180b4725f0d03","observation_id":"08272f1f-dc90-42f7-85af-efadcd79b4f1","resolution":{"observed_at":"2026-05-26T03:11:37.661555Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"b06837ca-8fc9-428f-bc6d-c91d5a6ab39b","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:67da8d31b45e4089d1ddd5a9c076ee89716cba001fa394e73775460709422692","observation_id":"dab192a4-69a6-437e-b700-6f1ebaeb1120","resolution":{"observed_at":"2026-05-26T03:11:37.665236Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Zhang, Z","venue":null,"work_id":"568e7f4e-4e3c-4882-bbc9-663505dbdb41","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:99f6ef4682bff531a587bbefe7933359d1af6a6de03e84f749d9f7a746c3333d","observation_id":"2db4a1ea-e4bd-4883-a145-d8fc737d8b43","resolution":{"observed_at":"2026-05-26T03:11:37.627204Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"de2473e8-737d-4d6c-9928-5ec1ee0b4e36","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:1bfd992072d2bfdc7d89cdacabe635f7a5749d9976fcf2f6e46f5d59b652dfa7","observation_id":"28768c46-f44e-41fc-a05b-c1747cd11e0a","resolution":{"observed_at":"2026-05-26T03:11:37.630440Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"James, E","venue":null,"work_id":"160a2789-42fc-446b-8b5f-e62e6aaca79b","year":2022},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:3148198b070390b7893aa3ccecd2bd0db62f3316647d260d8ca582d928ab4874","observation_id":"41a4f229-c9c8-44ee-922f-61190d42f2ed","resolution":{"observed_at":"2026-05-26T03:11:37.621324Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01295","last_updated":"2021-04-07T16:38:31Z","snapshot_observed_at":"2026-07-06T10:45:48.672430Z","submitted_at":"2021-03-01T20:35:48Z","title":"A nearby repeating fast radio burst in the direction of M81","version":2},"cited_work":{"arxiv_id":"2103.01295","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2103.01295","snapshot_observed_at":"2026-07-04T05:29:35.345181Z","title":"Bhardwaj et al","venue":null,"work_id":"73b99e3e-3180-41bc-b830-57f49f25bb7d","year":2021},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2103.01295","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:83c6f777006671ee5ce26b2e24a5a2abf265c55bab4d649cc8ae10c619c994e3","observation_id":"043979ab-20d1-423f-baaf-aafad0940e10","resolution":{"observed_at":"2026-05-09T06:00:35.556678Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.12122","last_updated":"2021-08-27T05:24:05Z","snapshot_observed_at":"2026-08-05T23:26:46.341475Z","submitted_at":"2021-08-27T05:24:05Z","title":"A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A","version":1},"cited_work":{"arxiv_id":"2108.12122","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.12122","snapshot_observed_at":"2026-07-04T05:29:35.257600Z","title":"Bhardwaj et al","venue":null,"work_id":"ac8a1b4d-3273-4c6d-832e-d4e2408877db","year":2021},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2108.12122","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:2352673b39e375f940a59032d1ff2a341102e91a12c6681596e10853ec250ba6","observation_id":"f4c50b2d-68d0-47e6-9faa-3a086f399eb7","resolution":{"observed_at":"2026-05-09T06:00:35.568410Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.04354","last_updated":"2018-10-10T04:00:35Z","snapshot_observed_at":"2026-08-04T02:23:15.290218Z","submitted_at":"2018-10-10T04:00:35Z","title":"A search for the host galaxy of FRB171020","version":1},"cited_work":{"arxiv_id":"1810.04354","doi":null,"metadata_source":"pith","pith_arxiv_id":"1810.04354","snapshot_observed_at":"2026-07-04T05:29:35.320032Z","title":"A search for the host galaxy of FRB171020","venue":"astro-ph.HE","work_id":"14bfb51f-3fd9-48e4-ac8e-bf5864de9d52","year":2018},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1810.04354","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:5ffc02a252ecb651208ab23132ee3783135c3ecbcdeabd7cff8f2b2ce535424e","observation_id":"27f9beb0-1b9d-4cfc-82e6-6aec082c5d77","resolution":{"observed_at":"2026-05-09T06:00:35.759683Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.02083","last_updated":"2025-01-22T05:00:48Z","snapshot_observed_at":"2026-08-12T23:08:52.186656Z","submitted_at":"2024-08-04T16:36:50Z","title":"The Commensal Real-time ASKAP Fast Transient incoherent-sum survey","version":2},"cited_work":{"arxiv_id":"2408.02083","doi":"10.48550/arxiv.2408.02083","metadata_source":"arxiv_reference","pith_arxiv_id":"2408.02083","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"434420ff-6160-4a17-8459-9dea6fe5cc70","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2408.02083","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:6e79a3039d2c44d49dc466c67669c8669b2ff0eedd55335f1e0a1650781dd9bc","observation_id":"0d1f8e42-ae38-4cb8-a6bd-4e037326a234","resolution":{"observed_at":"2026-05-09T06:00:35.436849Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.10018","last_updated":"2023-10-16T02:37:58Z","snapshot_observed_at":"2026-08-13T05:48:54.001173Z","submitted_at":"2023-10-16T02:37:58Z","title":"Host Galaxies for Four Nearby CHIME/FRB Sources and the Local Universe FRB Host Galaxy Population","version":1},"cited_work":{"arxiv_id":"2310.10018","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.10018","snapshot_observed_at":"2026-07-04T05:29:35.318698Z","title":"Bhardwaj et al","venue":null,"work_id":"603eadae-8640-4502-ab21-658a70be9435","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2310.10018","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:c6d7e5292c165e4cb9c8394b5d0cfa8a5d17cd4abec5cea53879624daee230c1","observation_id":"0038c33d-0f08-4aa6-a5c7-776b17daa789","resolution":{"observed_at":"2026-05-09T06:00:35.655729Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Gordon, W.-f","venue":null,"work_id":"af53dbd1-feed-4b61-81e3-5f60d56ec1c8","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:2dcc6a37d2c737c14757201ff36f276f97d040caadb8f659f824fb2db109da2d","observation_id":"dea89988-3720-4d5d-8ed8-fbd4c995e621","resolution":{"observed_at":"2026-05-26T03:11:37.624020Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":"Glowacki, A","venue":null,"work_id":"05ace890-0d8f-4734-bd11-1748b6c6c5d3","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:57a947089e5fb725156c8d506a99c85ddadb067e57b51f571e478805d21c23fe","observation_id":"cccc3607-126b-4661-ba6b-a22337369177","resolution":{"observed_at":"2026-05-26T03:11:37.671674Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.03344","last_updated":"2024-01-24T20:19:49Z","snapshot_observed_at":"2026-08-13T11:00:33.624747Z","submitted_at":"2023-07-07T01:19:46Z","title":"Deep Synoptic Array Science: First FRB and Host Galaxy Catalog","version":2},"cited_work":{"arxiv_id":"2307.03344","doi":"10.48550/arxiv.2307.03344","metadata_source":"arxiv_reference","pith_arxiv_id":"2307.03344","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Deep Synoptic Array Science: First FRB and Host Galaxy Catalog","venue":"arXiv (Cornell University)","work_id":"95397e95-b3af-4f5b-a607-bd0e4902b429","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2307.03344","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:8b7c98df6b2205138192afd814f5b2be1335126f1ca9867ffd9ab5c8d87f6cbe","observation_id":"4eb2bdff-421f-419d-bb8d-4adff9742f43","resolution":{"observed_at":"2026-05-09T06:00:35.572202Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.14600","last_updated":"2022-05-29T08:42:18Z","snapshot_observed_at":"2026-08-13T15:34:39.936625Z","submitted_at":"2022-05-29T08:42:18Z","title":"First discoveries and localisations of Fast Radio Bursts with MeerTRAP: a real-time, commensal MeerKAT survey","version":1},"cited_work":{"arxiv_id":"2205.14600","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2205.14600","snapshot_observed_at":"2026-07-04T05:29:35.307281Z","title":"Rajwade et al.,First discoveries and localizations of Fast Radio Bursts with MeerTRAP: real-time, commensal MeerKAT survey,Mon","venue":null,"work_id":"46767a1b-ac0b-4462-90b5-65601ea99a37","year":2022},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2205.14600","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:fab3cc97755967be5ae74d0ae6394255ff38c1fd22c1a57bf0580d459b967d65","observation_id":"c44b8acf-d98b-49dd-bff8-288643ac0bbd","resolution":{"observed_at":"2026-05-09T06:00:35.231265Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.02638","last_updated":"2023-10-02T21:58:20Z","snapshot_observed_at":"2026-08-13T12:08:33.634464Z","submitted_at":"2023-04-05T17:58:18Z","title":"Proposed host galaxies of repeating fast radio burst sources detected by CHIME/FRB","version":2},"cited_work":{"arxiv_id":"2304.02638","doi":"10.48550/arxiv.2304.02638","metadata_source":"arxiv_reference","pith_arxiv_id":"2304.02638","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Ibik et al.,Proposed Host Galaxies of Repeating Fast Radio Burst Sources Detected by CHIME/FRB,Astrophys","venue":"arXiv (Cornell University)","work_id":"296d3115-2c04-41b1-bdbf-505d6da5daf9","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2304.02638","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:3db280e7f4851e0211c2760259c76aa5cad941686c4669c32f8b83c65eef24ad","observation_id":"8c49b3e1-e156-458b-9356-f82c9032e7fe","resolution":{"observed_at":"2026-05-09T06:00:35.716682Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2212.11941","last_updated":"2022-12-22T18:21:58Z","snapshot_observed_at":"2026-08-13T13:15:39.324305Z","submitted_at":"2022-12-22T18:21:58Z","title":"Sub-arcminute localization of 13 repeating fast radio bursts detected by CHIME/FRB","version":1},"cited_work":{"arxiv_id":"2212.11941","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2212.11941","snapshot_observed_at":"2026-07-04T05:29:35.312629Z","title":"Michilli et al","venue":null,"work_id":"461731b2-517b-482a-8b8e-3c4ccad9731d","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2212.11941","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:96a56c3fcaaefba70f660b67a86c2705dca417dfc7db49ade7c3508e6c908fd9","observation_id":"76fdb15e-d311-4125-93e9-3874950d6dbe","resolution":{"observed_at":"2026-05-09T06:00:35.619105Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09787","last_updated":"2023-10-30T02:08:13Z","snapshot_observed_at":"2026-08-13T12:41:45.522758Z","submitted_at":"2023-02-20T06:24:50Z","title":"FRB 20210405I: a nearby Fast Radio Burst localised to sub-arcsecond precision with MeerKAT","version":2},"cited_work":{"arxiv_id":"2302.09787","doi":"10.48550/arxiv.2302.09787","metadata_source":"arxiv_reference","pith_arxiv_id":"2302.09787","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"2a697945-6d0f-4700-a059-1e798527bd3a","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2302.09787","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:87e7f84bff8489d5e6d122d43796f2b2bc9704287b6fe708d73cda74201c0353","observation_id":"a35c224a-c0b7-4f13-befb-bd6cc69431c9","resolution":{"observed_at":"2026-05-09T06:00:35.765896Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.16964","last_updated":"2024-09-25T14:23:42Z","snapshot_observed_at":"2026-08-12T22:37:44.637240Z","submitted_at":"2024-09-25T14:23:42Z","title":"Preferential Occurrence of Fast Radio Bursts in Massive Star-Forming Galaxies","version":1},"cited_work":{"arxiv_id":"2409.16964","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2409.16964","snapshot_observed_at":"2026-06-30T02:54:11.267039Z","title":"Sharma et al","venue":null,"work_id":"dbda2f56-0859-4b01-a4cb-34c4d5f6ac27","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2409.16964","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:ae4227102c4a7bd9bb2539ffa1e6bca0d8917d26d536e5defe3ed97a8dab7cac","observation_id":"fca38a50-2d8d-4fa2-9533-726266bdd278","resolution":{"observed_at":"2026-05-09T06:00:35.746011Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.14665","last_updated":"2023-04-28T07:52:25Z","snapshot_observed_at":"2026-08-13T11:53:28.969336Z","submitted_at":"2023-04-28T07:52:25Z","title":"FAST Observations of FRB 20220912A: Burst Properties and Polarization Characteristics","version":1},"cited_work":{"arxiv_id":"2304.14665","doi":"10.48550/arxiv.2304.14665","metadata_source":"arxiv_reference","pith_arxiv_id":"2304.14665","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Zhang et al., Astrophys","venue":"arXiv (Cornell University)","work_id":"9b41d465-53fa-49c2-9f03-71c46552f0db","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2304.14665","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:43035f3770945b443c63d09c8b542fc3f2676a14901038ad6ab129fda68f7bcc","observation_id":"514c3dba-5182-4738-8c44-b152b328553a","resolution":{"observed_at":"2026-05-09T06:00:35.237350Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.09254","last_updated":"2021-12-12T21:29:01Z","snapshot_observed_at":"2026-07-06T11:49:21.110199Z","submitted_at":"2021-09-20T00:42:01Z","title":"A sudden period of high activity from repeating Fast Radio Burst 20201124A","version":3},"cited_work":{"arxiv_id":"2109.09254","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2109.09254","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lanman et al.,A Sudden Period of High Activity from Repeating Fast Radio Burst 20201124A,Astrophys","venue":null,"work_id":"b455d8fb-810e-4be5-80af-4c728f466431","year":2022},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2109.09254","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:3cbfac48112cd93270f03c3f08f4ed66721567964c8364f6328b73900e96a7c4","observation_id":"75219090-7ed2-4421-8e0e-89ed5a6bbb94","resolution":{"observed_at":"2026-05-09T06:00:35.576283Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.03974","last_updated":"2023-05-06T20:10:47Z","snapshot_observed_at":"2026-08-13T13:47:44.177021Z","submitted_at":"2022-11-08T03:02:56Z","title":"Limits on Simultaneous and Delayed Optical Emission from Well-localized Fast Radio Bursts","version":2},"cited_work":{"arxiv_id":"2211.03974","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.03974","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Hiramatsu et al","venue":null,"work_id":"238697e1-a75f-4a3b-b7a4-d696115835e0","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2211.03974","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e557d8ea90e35650133be5d0106dcc672e18d2c67824d501fe67298c8bb38df6","observation_id":"e7b1cd27-8daf-495a-bbe1-9ca06220d6f4","resolution":{"observed_at":"2026-05-09T06:00:35.732227Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.12804","last_updated":"2024-10-09T19:46:42Z","snapshot_observed_at":"2026-08-12T23:39:52.169921Z","submitted_at":"2024-06-18T17:20:25Z","title":"Varying activity and the burst properties of FRB 20240114A probed with GMRT down to 300 MHz","version":2},"cited_work":{"arxiv_id":"2406.12804","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.12804","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Kumar, Y","venue":null,"work_id":"1af340d8-16ea-4c08-8245-5998a8fa4e11","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2406.12804","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:9954805704c0c203fa4c5e42d8e8c3dfe9c450257eba7bb30bfc633284532f85","observation_id":"d6d688d9-46c2-411b-9567-f008feb2a226","resolution":{"observed_at":"2026-05-09T06:00:35.408474Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.23374","last_updated":"2024-10-30T18:18:55Z","snapshot_observed_at":"2026-08-12T22:11:28.293549Z","submitted_at":"2024-10-30T18:18:55Z","title":"A repeating fast radio burst source in the outskirts of a quiescent galaxy","version":1},"cited_work":{"arxiv_id":"2410.23374","doi":"10.48550/arxiv.2410.23374","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.23374","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Shah et al., Astrophys","venue":"arXiv (Cornell University)","work_id":"6b14ce43-0acd-410e-8e45-f9ce818ee1fe","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2410.23374","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:314481d5776c7b57b5e151d045a9c517709e4c5b7e6b90dbc56438331b8358f0","observation_id":"7bdddbff-9d53-4908-9c21-9fea0913e7a9","resolution":{"observed_at":"2026-05-09T06:00:35.344576Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2302.09754","last_updated":"2023-06-13T18:49:25Z","snapshot_observed_at":"2026-08-13T12:41:47.944771Z","submitted_at":"2023-02-20T04:22:51Z","title":"A sub-arcsec localised fast radio burst with a significant host galaxy dispersion measure contribution","version":2},"cited_work":{"arxiv_id":"2302.09754","doi":"10.48550/arxiv.2302.09754","metadata_source":"arxiv_reference","pith_arxiv_id":"2302.09754","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Caleb et al","venue":"arXiv (Cornell University)","work_id":"d66730c3-e9d5-4000-82d6-818ad3a7219b","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2302.09754","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:0e48893153421e7f8a56e824fc4fc7d0a539d74d384b07ec01112f1d976849dc","observation_id":"57666d67-020c-4850-bba0-7026df1c3bc7","resolution":{"observed_at":"2026-05-09T06:00:35.404329Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2307.09502","last_updated":"2024-11-04T19:03:28Z","snapshot_observed_at":"2026-08-13T10:53:07.512888Z","submitted_at":"2023-07-18T18:00:00Z","title":"A fast radio burst localized at detection to an edge-on galaxy using very-long-baseline interferometry","version":4},"cited_work":{"arxiv_id":"2307.09502","doi":"10.48550/arxiv.2307.09502","metadata_source":"arxiv_reference","pith_arxiv_id":"2307.09502","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"b82749b2-0e7e-4cfb-9e22-578d97204171","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2307.09502","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:c74d24b8ef24dde01abb7e8da0dac9e418b530fb4b05178cd58e3f140460abcf","observation_id":"e2a71899-e339-47b6-ab93-a732b03cc751","resolution":{"observed_at":"2026-05-09T06:00:35.699928Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-05-21T04:52:57.809703+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-21T04:52:57.809703+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"99ab6a76-3aaa-444e-abce-4cb159384e83","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:5a48c9945ce4aabddde3166193e9d20086b58f2a5f0b686f961badbc06732c24","observation_id":"c700e73f-0d80-4988-af76-620533072ba9","resolution":{"observed_at":"2026-05-26T03:11:37.618145Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.16790","last_updated":"2023-06-05T06:59:16Z","snapshot_observed_at":"2026-08-13T13:31:53.379735Z","submitted_at":"2022-11-30T07:07:17Z","title":"A non-repeating fast radio burst in a dwarf host galaxy","version":2},"cited_work":{"arxiv_id":"2211.16790","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.16790","snapshot_observed_at":"2026-07-04T05:29:35.223467Z","title":"Bhandari et al","venue":null,"work_id":"c4f9672f-fbb7-4963-9c5d-0f5669d5c829","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2211.16790","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:65f5b61b5d32d5c50e12595755f1cd356a5da45097ac48c9d4ccad2f392b0584","observation_id":"058a1cdd-135b-40c8-ac32-5519806f2104","resolution":{"observed_at":"2026-05-09T06:00:35.719436Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.12488","last_updated":"2020-10-12T02:50:27Z","snapshot_observed_at":"2026-08-03T17:46:01.326441Z","submitted_at":"2020-08-28T06:01:38Z","title":"Limits on precursor and afterglow radio emission from a fast radio burst in a star-forming galaxy","version":3},"cited_work":{"arxiv_id":"2008.12488","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2008.12488","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bhandari et al","venue":null,"work_id":"7a6648a3-5248-470f-90ea-336dea15cc7b","year":2020},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2008.12488","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:e64068c3f38bf3ad95e5865ceadf244321b29ea2abe8f3aaa965455fa29b885b","observation_id":"e0ab0551-a890-4fb9-a0dd-8d695f963164","resolution":{"observed_at":"2026-05-09T06:00:35.771440Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2003.10889","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Guidorzi et al","venue":null,"work_id":"439f9e73-6da4-4305-96d3-bb17df596211","year":2020},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:d7c3bdef15d2637cc2d10190a7e439f644f5147ef6f824538d6133953457f1bb","observation_id":"04a9e39b-3c2a-4f30-974f-f8062fa28953","resolution":{"observed_at":"2026-05-09T06:00:35.234206Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2108.01282","last_updated":"2021-11-16T13:08:08Z","snapshot_observed_at":"2026-08-11T01:35:42.556021Z","submitted_at":"2021-08-03T04:09:35Z","title":"Characterizing the FRB host galaxy population and its connection to transients in the local and extragalactic Universe","version":2},"cited_work":{"arxiv_id":"2108.01282","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2108.01282","snapshot_observed_at":"2026-07-04T05:29:35.303522Z","title":"Bhandari et al","venue":null,"work_id":"dfa26e6b-bca6-4d97-8ced-670cd8c28a87","year":2022},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2108.01282","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:aed00c62081ab658a3f798aa5ded067e39e667e39d075346c4abe866dfb637ea","observation_id":"ee87e915-23af-4864-9b9f-2c2468770fe8","resolution":{"observed_at":"2026-05-09T06:00:35.242975Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.05982","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T00:52:55.690820Z","title":"Pastor-Marazuela et al","venue":null,"work_id":"f773851a-dde7-4598-bb9b-62dd20858885","year":2026},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:ad6dfefd5e9d79b055cbaf7cfc942c74d4c9e0ce658e2de78dd83a970fd3bc99","observation_id":"01144cd2-197c-4b49-a508-b75c0ee2b0fa","resolution":{"observed_at":"2026-05-09T06:00:35.711200Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.07412","last_updated":"2019-01-22T15:27:37Z","snapshot_observed_at":"2026-07-06T07:28:14.627901Z","submitted_at":"2019-01-22T15:27:37Z","title":"A Fast Radio Burst with frequency-dependent polarization detected during Breakthrough Listen observations","version":1},"cited_work":{"arxiv_id":"1901.07412","doi":null,"metadata_source":"pith","pith_arxiv_id":"1901.07412","snapshot_observed_at":"2026-07-01T05:35:26.029263Z","title":"A Fast Radio Burst with frequency-dependent polarization detected during Breakthrough Listen observations","venue":"astro-ph.HE","work_id":"b83f88a4-8201-4ef6-922e-7b8bb995c832","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1901.07412","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:4319709dc5cca78b440a71a270961a7da2d76db5c67ada2ac4896a6e3361eccc","observation_id":"77ccadcd-73bd-487d-8d53-9d0566325d2c","resolution":{"observed_at":"2026-05-09T06:00:35.386356Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.02173","last_updated":"2024-07-02T11:27:05Z","snapshot_observed_at":"2026-08-12T23:30:30.748208Z","submitted_at":"2024-07-02T11:27:05Z","title":"A study of two FRBs with low polarization fractions localized with the MeerTRAP transient buffer system","version":1},"cited_work":{"arxiv_id":"2407.02173","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.02173","snapshot_observed_at":"2026-07-04T05:29:35.298360Z","title":"Rajwade et al.,A study of two FRBs with low polarization fractions localized with the MeerTRAP transient buffer system,Mon","venue":null,"work_id":"0a8b5ccf-e9d5-44b4-87b1-8403c0cdf570","year":2024},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2407.02173","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:f8aa3c9caf1f37cd7d10737c47d5f49a13f34538edf1a3ff905888cb0434dde1","observation_id":"f37373f2-b480-42ed-91f7-a4205d0866f6","resolution":{"observed_at":"2026-05-09T06:00:35.264598Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.02155","last_updated":"2020-07-04T18:19:05Z","snapshot_observed_at":"2026-07-06T09:35:23.261370Z","submitted_at":"2020-07-04T18:19:05Z","title":"A Distant Fast Radio Burst Associated to its Host Galaxy with the Very Large Array","version":1},"cited_work":{"arxiv_id":"2007.02155","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.02155","snapshot_observed_at":"2026-07-04T05:29:35.260026Z","title":"Law et al.,A Distant Fast Radio Burst Associated with Its Host Galaxy by the Very Large Array,Astrophys","venue":null,"work_id":"32b27937-2fb9-48db-9bde-6a8c651b8717","year":2020},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2007.02155","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:c45fa71fc60fc335680eaaca6ee412cb7f6023b57e74f29567c79dd461b61b69","observation_id":"2381e285-483b-4ebc-a3a1-3207d507f044","resolution":{"observed_at":"2026-05-09T06:00:35.208950Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.01542","last_updated":"2019-07-02T17:50:28Z","snapshot_observed_at":"2026-08-12T21:50:09.134907Z","submitted_at":"2019-07-02T17:50:28Z","title":"A fast radio burst localised to a massive galaxy","version":1},"cited_work":{"arxiv_id":"1907.01542","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.01542","snapshot_observed_at":"2026-07-01T05:35:25.928072Z","title":"A fast radio burst localised to a massive galaxy","venue":"astro-ph.HE","work_id":"472df467-46ad-46fc-a95e-f7a81ad04d97","year":2019},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/1907.01542","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:055f2286bbcdf02d17dda5e65937d2f5ec5c7e41a133d0e23b64918ea3526c1d","observation_id":"4957cf0f-0d7e-4cbf-81f0-36b5b265b11c","resolution":{"observed_at":"2026-05-09T06:00:35.222663Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.04680","last_updated":"2023-10-25T00:39:00Z","snapshot_observed_at":"2026-08-13T14:09:16.136204Z","submitted_at":"2022-10-10T13:31:24Z","title":"A luminous fast radio burst that probes the Universe at redshift 1","version":2},"cited_work":{"arxiv_id":"2210.04680","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.04680","snapshot_observed_at":"2026-07-04T05:29:35.259404Z","title":"Ryder et al.,A luminous fast radio burst that probes the Universe at redshift 1,Science 392(2023) 294 [2210.04680]","venue":null,"work_id":"e95461f3-4b9e-4041-9086-dde1c93d54dd","year":2023},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2210.04680","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:a4585a7235e42f96033fcc6d7bf5c61dcf22992d3973d35b6888708df5af36ad","observation_id":"4b38de2c-a687-4d04-a1a4-1ddee6168c49","resolution":{"observed_at":"2026-05-09T06:00:35.213233Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2508.01648","last_updated":"2025-08-03T08:13:30Z","snapshot_observed_at":"2026-08-10T16:16:41.911482Z","submitted_at":"2025-08-03T08:13:30Z","title":"A fast radio burst from the first 3 billion years of the Universe","version":1},"cited_work":{"arxiv_id":"2508.01648","doi":"10.48550/arxiv.2508.01648","metadata_source":"arxiv_reference","pith_arxiv_id":"2508.01648","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv","venue":"ArXiv.org","work_id":"c2b51f36-6079-489c-82af-cca68de3fddf","year":2025},"citing_paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-08T19:14:15.479515Z"},"links":{"cited_paper":"/paper/2508.01648","citing_paper":"/paper/2605.01990"},"observation_digest":"sha256:d1fd26c32e1d064bd853d5098c553bf3f0f83532ca3f940d4628549f72989eda","observation_id":"c30c3ccb-d0af-43f4-ae04-81612a74a08c","resolution":{"observed_at":"2026-05-09T06:00:35.228380Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-05-21T22:52:29.862555+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-21T22:52:29.862555+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.01990","last_updated":"2026-05-03T17:48:16Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-03T17:48:16Z","title":"Constraints on the baryon density from fast radio bursts using a non-parametric reconstruction of the Hubble parameter"},"reference_resolution":{"displayed":71,"state_counts":{"malformed_identifier":0,"metadata_mismatch":18,"parse_uncertain":0,"unresolved":4,"verified_exact":31,"verified_fuzzy":18},"total_outbound_references":71},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 71 of 71 outbound references and 2 inbound Pith citation observations for arXiv:2605.01990."}