{"as_of":"2026-08-13T14:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2ea3e58f68c35dc25b9b18612ce6195b91ab3037d32a43b30a23836ad4ed3379","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":15,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":15,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":15,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":15,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T22:02:04.232307Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-06-29T05:43:08.027409Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-12T22:02:04.232307Z","title":"title On the detection of a cosmic dawn signal in the radio background","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08113","last_updated":"2024-11-12T19:00:05Z","snapshot_observed_at":"2026-08-12T21:54:52.381701Z","submitted_at":"2024-11-12T19:00:05Z","title":"Cosmology with HI","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-12T22:02:04.232307Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2411.08113"},"observation_digest":"sha256:d1621f364637cc85c1ebc18a2d1f0f13b9b17b56dca504071e335e6526d118d7","observation_id":"fadd365b-e6c3-4c01-8c5a-25d265dfb90d","resolution":{"observed_at":"2026-08-12T22:02:04.232307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-12T21:23:26.345345Z","title":"Singh, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09042","last_updated":"2025-08-27T14:06:34Z","snapshot_observed_at":"2026-08-13T14:42:57.022999Z","submitted_at":"2024-11-13T21:49:55Z","title":"Excess Radiation from Axion-Photon Conversion","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T21:23:26.345345Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2411.09042"},"observation_digest":"sha256:232f992e989d3cabce7095d0da3e48065ff0e5b89b33c522a2825ef437decd53","observation_id":"f8815ef2-5b5d-4def-aae4-2baa056b2fb5","resolution":{"observed_at":"2026-08-12T21:23:26.345345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-04T20:07:40.919486Z","title":"Singh, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.08886","last_updated":"2026-06-04T09:17:16Z","snapshot_observed_at":"2026-08-05T23:46:33.451796Z","submitted_at":"2025-09-10T18:00:03Z","title":"A New Boundary Condition on Reionization","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-04T20:07:40.919486Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2509.08886"},"observation_digest":"sha256:45df5d6403e1d36111b1c7dd618e30d53ae5e0537b9ad80c6ed741da20d875d3","observation_id":"8953e128-8c26-478b-bdd9-710cd174b217","resolution":{"observed_at":"2026-08-04T20:07:40.919486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-04T19:14:21.307457Z","title":"Singh, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.09472","last_updated":"2025-09-11T13:54:20Z","snapshot_observed_at":"2026-08-13T14:33:28.179369Z","submitted_at":"2025-09-11T13:54:20Z","title":"Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-04T19:14:21.307457Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2509.09472"},"observation_digest":"sha256:745d04fca1c39e5233f365b36b03cdd3eccb7b39ca988900373ff2593468837b","observation_id":"b3ee3411-8465-44f4-a577-44b34d56a350","resolution":{"observed_at":"2026-08-04T19:14:21.307457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-04T08:41:23.730867Z","title":"Singh, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2510.19647","last_updated":"2026-06-01T19:20:15Z","snapshot_observed_at":"2026-08-08T08:56:02.579588Z","submitted_at":"2025-10-22T14:53:10Z","title":"The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T08:41:23.730867Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2510.19647"},"observation_digest":"sha256:660ef8b987a8e7adc7dc7e578944f40798b1cf8a62471d9dc981dfed84907966","observation_id":"1a7c96f1-cbc1-49a4-8da1-8450953ecfb8","resolution":{"observed_at":"2026-08-04T08:41:23.730867Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":"2112.06778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-06-29T05:43:08.027409Z","title":"Singh, N.T","venue":null,"work_id":"f02629b0-d866-44ef-9cc3-f3e26944a443","year":2022},"citing_paper":{"arxiv_id":"2510.25886","last_updated":"2026-03-29T08:40:10Z","snapshot_observed_at":"2026-07-06T22:34:23.736456Z","submitted_at":"2025-10-29T18:33:39Z","title":"Mitigating gain calibration errors from EoR observations with SKA1-Low AA*","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-22T12:15:58.895991Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2510.25886"},"observation_digest":"sha256:cc4712b5ac1a87557ba0c749db99e570b6f37981049a7b87e7926a6deb96dabf","observation_id":"cf9aa6cf-c049-48b1-afbc-f6a57f0d25af","resolution":{"observed_at":"2026-05-22T12:16:31.593452Z","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":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-03T23:49:30.640932Z","title":"Singh, J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.04210","last_updated":"2026-06-14T01:23:31Z","snapshot_observed_at":"2026-08-11T02:20:28.834835Z","submitted_at":"2025-11-06T09:15:20Z","title":"NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes, and implications for the origins of Little Red Dots","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-03T23:49:30.640932Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2511.04210"},"observation_digest":"sha256:7d342aa56a306ee8d70f4967d9100ae85d729bb424b2f891376fbcfc601d89e1","observation_id":"ab75f6f4-1031-4fc4-b6bc-62ea0b85038c","resolution":{"observed_at":"2026-08-03T23:49:30.640932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":"2112.06778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-06-29T05:43:08.027409Z","title":"Singh, N.T","venue":null,"work_id":"f02629b0-d866-44ef-9cc3-f3e26944a443","year":2022},"citing_paper":{"arxiv_id":"2604.17083","last_updated":"2026-04-18T17:42:06Z","snapshot_observed_at":"2026-07-06T23:04:14.688737Z","submitted_at":"2026-04-18T17:42:06Z","title":"Dark ages bounds on non-accreting massive compact halo objects","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-10T06:27:01.390276Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2604.17083"},"observation_digest":"sha256:f8585a2465f35447f7401482606fd2b8ab77716620ccb7d4bd250ec5f875ecb8","observation_id":"cd325561-649d-48e8-b4b8-7e574b55cc0d","resolution":{"observed_at":"2026-05-10T06:31:30.991242Z","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":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":"2112.06778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-06-29T05:43:08.027409Z","title":"Singh, N.T","venue":null,"work_id":"f02629b0-d866-44ef-9cc3-f3e26944a443","year":2022},"citing_paper":{"arxiv_id":"2604.19198","last_updated":"2026-07-30T08:09:15Z","snapshot_observed_at":"2026-08-02T23:16:52.903876Z","submitted_at":"2026-04-21T08:07:34Z","title":"Cosmological constraints on TeV-scale dark matter subcomponents decaying between recombination and reionisation","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-10T01:53:10.188601Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2604.19198"},"observation_digest":"sha256:c106d4f9b5fe275519bd8632e334cdbb54a6ac4403878cbb094df91371ed5c33","observation_id":"3e85bf04-a946-4a1d-b1ff-9e27506f5e29","resolution":{"observed_at":"2026-05-11T13:21:05.797495Z","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":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-02T15:54:09.713241Z","title":"5 607–617, [arXiv:2112.06778]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2604.19198","last_updated":"2026-07-30T08:09:15Z","snapshot_observed_at":"2026-08-02T23:16:52.903876Z","submitted_at":"2026-04-21T08:07:34Z","title":"Cosmological constraints on TeV-scale dark matter subcomponents decaying between recombination and reionisation","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-02T15:54:09.713241Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2604.19198"},"observation_digest":"sha256:4a393dc1951bc740604906f15f4a0ada5887b5ac3f2bf679e1cb256468708cdb","observation_id":"9505a0f9-7730-4422-9161-48e332856b4a","resolution":{"observed_at":"2026-08-02T15:54:09.713241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":"2112.06778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-06-29T05:43:08.027409Z","title":"Singh, N.T","venue":null,"work_id":"f02629b0-d866-44ef-9cc3-f3e26944a443","year":2022},"citing_paper":{"arxiv_id":"2605.02547","last_updated":"2026-05-04T12:51:03Z","snapshot_observed_at":"2026-08-11T03:51:53.683949Z","submitted_at":"2026-05-04T12:51:03Z","title":"How neutrinos could help solving cosmological anomalies and tensions","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-08T18:37:06.126807Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2605.02547"},"observation_digest":"sha256:52bdf932fa827f8b78969750caac6393330503aaea505d6170c2adbf80bc3851","observation_id":"a6396e3c-4b73-4cf1-9dee-8fb9c9fb0224","resolution":{"observed_at":"2026-05-09T06:20:40.808710Z","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":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":"2112.06778","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-06-29T05:43:08.027409Z","title":"Singh, N.T","venue":null,"work_id":"f02629b0-d866-44ef-9cc3-f3e26944a443","year":2022},"citing_paper":{"arxiv_id":"2605.30259","last_updated":"2026-05-28T17:22:19Z","snapshot_observed_at":"2026-07-06T23:39:34.232661Z","submitted_at":"2026-05-28T17:22:19Z","title":"Late-time Quantum Vacuum Decay and its Cosmological Implications","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-06-29T05:39:36.647189Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2605.30259"},"observation_digest":"sha256:cfeddb7802e55da71d27eba9434696c60173fcb0b3075c8832242dfb8aef02d8","observation_id":"f5d1a059-cc98-4222-849a-4663208bdeac","resolution":{"observed_at":"2026-06-29T05:43:08.029064Z","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":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-01T09:49:25.514618Z","title":"On the detection of a cosmic dawn signal in the radio back- ground,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.20651","last_updated":"2026-07-22T18:24:26Z","snapshot_observed_at":"2026-08-06T11:42:58.436065Z","submitted_at":"2026-07-22T18:24:26Z","title":"When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-01T09:49:25.514618Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2607.20651"},"observation_digest":"sha256:2739e2b305c03d8f76d01ac2633b3a8cb5c2bfa7f6e3b78e57c226eaafc11842","observation_id":"c5ea860f-b6ae-4410-b408-e1ac45ef7284","resolution":{"observed_at":"2026-08-01T09:49:25.514618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-07-30T17:19:19.254121Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.26911","last_updated":"2026-07-29T13:42:14Z","snapshot_observed_at":"2026-08-04T03:20:04.709827Z","submitted_at":"2026-07-29T13:42:14Z","title":"Impact of numerical stability in Bayesian noise wave calibration on global 21-cm experiments","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-30T17:19:19.254121Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2607.26911"},"observation_digest":"sha256:347d5c829f172c95fa64be2c60a4824e45475cca420f252ba7927ca752141e40","observation_id":"97cd5f24-7d2f-4c7d-9848-c4b965995a7f","resolution":{"observed_at":"2026-07-30T17:19:19.254121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.06778","snapshot_observed_at":"2026-08-03T17:20:51.415944Z","title":"Singh et al.,On the detection of a cosmic dawn signal in the radio background,Nature Astronomy6(2022) 607 [2112.06778]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28918","last_updated":"2026-07-31T00:34:31Z","snapshot_observed_at":"2026-08-12T13:30:48.544731Z","submitted_at":"2026-07-31T00:34:31Z","title":"A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T17:20:51.415944Z"},"links":{"cited_paper":"/paper/2112.06778","citing_paper":"/paper/2607.28918"},"observation_digest":"sha256:87189f8f7d38c0b4c2cab04198550dcd53df1bef34609fd0cec72cd7aaabdab8","observation_id":"ecd34898-b3c0-4846-87c8-1bc99b453e82","resolution":{"observed_at":"2026-08-03T17:20:51.415944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2112.06778/citation-record","integrity":"/paper/2112.06778/integrity","json":"/paper/2112.06778/citation-record.json","paper":"/paper/2112.06778"},"outbound":[],"paper":{"arxiv_id":"2112.06778","last_updated":"2021-12-13T16:42:48Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T12:18:11.444272Z","submitted_at":"2021-12-13T16:42:48Z","title":"On the detection of a cosmic dawn signal in the radio background"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:2112.06778."}