{"as_of":"2026-08-09T15:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:53a269f1056b082980e3ea4de9d9d28a18e0c5e7ca2961c6a26d6a481066afae","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":20,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":20,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":20,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":20,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T00:02:53.672719Z","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":"2026-07-03T07:07:44.885497Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-08T00:02:53.672719Z","title":"Stress testing ΛCDM with high-redshift galaxy candidates,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.08701","last_updated":"2025-02-12T19:00:00Z","snapshot_observed_at":"2026-08-07T23:52:24.926526Z","submitted_at":"2025-02-12T19:00:00Z","title":"Early Galaxies from Rare Inflationary Processes and JWST Observations","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-08T00:02:53.672719Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2502.08701"},"observation_digest":"sha256:3cc8b7a2dbeceeda410d5a3197ea0589c16f7d5991cdfc657d127922a6ea08a1","observation_id":"cccdb316-1710-495c-8c7d-58d5225d47f3","resolution":{"observed_at":"2026-08-08T00:02:53.672719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2506.12131","last_updated":"2025-06-13T18:00:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-06-13T18:00:01Z","title":"Early Growth of Structure in Warm Wave Dark Matter","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-19T09:22:41.197004Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2506.12131"},"observation_digest":"sha256:c72424191d6f183dd23a60dcccae47dc6e3ed8c7332bd0b3a90cd127050c39e5","observation_id":"fef2fec7-6ecd-429e-9be7-5d16e1c728ac","resolution":{"observed_at":"2026-05-19T09:23:03.141665Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-06T23:21:50.153407Z","title":"Boylan-Kolchin, Nature Astronomy7, 731 (2023), 2208.01611","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.153407Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:6867d91d4617a4fc4bf2bc1c0b971666501573c09b4d702efa5a845b35b6edbe","observation_id":"58a802d0-5fee-4f0a-a13c-574387650f3a","resolution":{"observed_at":"2026-08-06T23:21:50.153407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-05T20:39:29.805488Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high- redshift galaxy candidates, Nature Astronomy 7, 731 (2023), arXiv:2208.01611 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.10183","last_updated":"2025-08-13T20:36:14Z","snapshot_observed_at":"2026-08-07T04:51:36.014165Z","submitted_at":"2025-08-13T20:36:14Z","title":"Risk-based framework to determine climate-informed design storms for road drainage infrastructure","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-05T20:39:29.805488Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2508.10183"},"observation_digest":"sha256:b0eddfa1089a7c67953bc4aa728fbc359c924c4a9b5928b574fcb6527d4bda10","observation_id":"14d4db20-13ad-4663-bbd9-78c0e7fee39a","resolution":{"observed_at":"2026-08-05T20:39:29.805488Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2510.15046","last_updated":"2026-05-15T21:17:07Z","snapshot_observed_at":"2026-07-31T16:02:14.376653Z","submitted_at":"2025-10-16T18:03:25Z","title":"Multi-species Dark Matter with Warmth and Randomness","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-21T21:01:12.105296Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2510.15046"},"observation_digest":"sha256:0883c89f52cecde49e27a31b615f184f120c2343b56c3a775d1e09d5b81309d1","observation_id":"0689af54-eef4-4b99-9b3f-30fd98edd263","resolution":{"observed_at":"2026-05-21T21:04:21.799936Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2510.17977","last_updated":"2026-05-19T19:21:08Z","snapshot_observed_at":"2026-08-02T00:00:36.112013Z","submitted_at":"2025-10-20T18:00:10Z","title":"Growth of Structure in Multi-species Wave Dark Matter","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-21T20:59:52.011652Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2510.17977"},"observation_digest":"sha256:de49c377600ee220d66b61e66da23d03622654fcac8c29bd26a7f6b586c00b84","observation_id":"33d4e40e-a73a-49d5-b7b1-0719a8daa171","resolution":{"observed_at":"2026-05-21T21:00:38.039252Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-04T00:10:16.736816Z","title":"Boylan-Kolchin,Stress testingΛCDM with high-redshift galaxy candidates,Nature Astron.7 (2023) 731–735, [2208.01611]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.02906","last_updated":"2026-07-13T21:59:28Z","snapshot_observed_at":"2026-08-06T14:11:33.684472Z","submitted_at":"2025-11-04T19:00:01Z","title":"Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-04T00:10:16.736816Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2511.02906"},"observation_digest":"sha256:153fe87d9c9cb5476f318f451bc446997e1c4f56c8971be5c2e16dc6d02a0b11","observation_id":"d89055b7-35a2-4227-bcc5-cc9b2f5e66fd","resolution":{"observed_at":"2026-08-04T00:10:16.736816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2511.13708","last_updated":"2026-04-25T19:06:14Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-11-17T18:55:24Z","title":"Statistics Meet Systematics: Resolution of the Massive Early JWST Galaxy Tension","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-17T21:42:40.737453Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2511.13708"},"observation_digest":"sha256:cf3eb33fd2e679788da5ae240e03942695da5b66ffa5d68e3ce7a25533c6640a","observation_id":"74352149-ed79-4adb-9af6-0e4e92cac6f6","resolution":{"observed_at":"2026-05-17T21:45:18.357995Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2601.14664","last_updated":"2026-05-12T17:07:08Z","snapshot_observed_at":"2026-07-06T22:42:26.083572Z","submitted_at":"2026-01-21T05:21:40Z","title":"Covariant interpretation of proper infall times in Kerr spacetime","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-16T12:47:20.491829Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2601.14664"},"observation_digest":"sha256:5af124c542ff5a15e73b09453da225ebb812970dbd91837167f69eb72b8d72c3","observation_id":"ba32598b-9ca5-41d0-98c6-c3364cb7ba12","resolution":{"observed_at":"2026-05-16T12:47:54.027938Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-02T20:12:34.523133Z","title":"Stress testingΛCDM with high-redshift galaxy candidates","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2602.23913","last_updated":"2026-06-01T10:10:58Z","snapshot_observed_at":"2026-08-02T20:12:33.769011Z","submitted_at":"2026-02-27T11:02:50Z","title":"Probing inflationary features with galaxy ultraviolet luminosity function observables","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-02T20:12:34.523133Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2602.23913"},"observation_digest":"sha256:4ffe2a12e93bc69b344106813e484d1d16a4ee838cfa163a27afb75a16fadcc7","observation_id":"a8e3e090-7ca2-4416-8d5c-075846053429","resolution":{"observed_at":"2026-08-02T20:12:34.523133Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2605.22161","last_updated":"2026-06-01T08:46:45Z","snapshot_observed_at":"2026-08-01T14:47:05.448656Z","submitted_at":"2026-05-21T08:30:11Z","title":"Blue-tilted Runnings and the JWST Early Galaxy Tension","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-22T04:42:34.379268Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2605.22161"},"observation_digest":"sha256:de9eca4840f7ee75966d1d99d1ba814eb5b8b2419daf147a6a1819b31d52a70e","observation_id":"c4c2cb23-1ac4-4ab3-a5e9-b105fdc76748","resolution":{"observed_at":"2026-05-22T04:44:35.588734Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2605.22161","last_updated":"2026-06-01T08:46:45Z","snapshot_observed_at":"2026-08-01T14:47:05.448656Z","submitted_at":"2026-05-21T08:30:11Z","title":"Blue-tilted Runnings and the JWST Early Galaxy Tension","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-30T16:25:37.707011Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2605.22161"},"observation_digest":"sha256:9d0854e5c8cc6dd215edc9e62b1924032111835c03883ab685fa97cc4503ca99","observation_id":"a584d0de-59db-4d98-924a-c5a26e6c63e4","resolution":{"observed_at":"2026-06-30T16:35:13.062029Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2606.02097","last_updated":"2026-06-01T11:28:21Z","snapshot_observed_at":"2026-08-06T05:31:00.560567Z","submitted_at":"2026-06-01T11:28:21Z","title":"Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-06-28T13:17:56.799399Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2606.02097"},"observation_digest":"sha256:f1e5de5f7ef8b15a447ad0cef245e233e2fb97b81b7a764a0f13053a554225b5","observation_id":"55f82df5-b189-487c-8f05-e4373f5950e2","resolution":{"observed_at":"2026-07-02T00:46:23.785804Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-12T14:25:03.782538Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates.Nature Astronomy7, 731 (2023), arXiv:2208.01611 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2606.11061","last_updated":"2026-07-06T04:28:26Z","snapshot_observed_at":"2026-07-12T14:25:03.436159Z","submitted_at":"2026-06-09T16:22:18Z","title":"Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-12T14:25:03.782538Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2606.11061"},"observation_digest":"sha256:4fd22302a5f21064bdcebe269000e33ed10da542ceac9f9f152a9119536031c9","observation_id":"17d5ac12-06d2-4166-9485-e8a2e62f1fae","resolution":{"observed_at":"2026-07-12T14:25:03.782538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2606.11062","last_updated":"2026-06-09T16:23:08Z","snapshot_observed_at":"2026-08-01T22:02:37.358175Z","submitted_at":"2026-06-09T16:23:08Z","title":"A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-27T12:16:15.909335Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2606.11062"},"observation_digest":"sha256:f2071c77f77ecc91c3e27468c740bc3a998de3617e5397a05b237e3b543942aa","observation_id":"d2ce24e3-24cf-41d8-a3d4-46ae7eb64032","resolution":{"observed_at":"2026-07-03T07:07:44.887064Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":"2208.01611","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-07-03T07:07:44.885497Z","title":"Boylan-Kolchin, Stress testing ΛCDM with high-redshift galaxy candidates, Nature Astron","venue":null,"work_id":"ba0ed85d-3448-4444-9ec1-5020cbe75649","year":2023},"citing_paper":{"arxiv_id":"2606.28246","last_updated":"2026-06-26T16:32:52Z","snapshot_observed_at":"2026-08-02T12:29:30.797723Z","submitted_at":"2026-06-26T16:32:52Z","title":"The cosmology of long range Yukawa interactions in general backgrounds","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-06-29T03:02:39.937426Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2606.28246"},"observation_digest":"sha256:1bfdee87b1dbb4a58b7cba9a92b9410ed44118c05b0d45d5e32e73b7e796a808","observation_id":"063498b6-ac26-48ce-a3fb-98ce2f944678","resolution":{"observed_at":"2026-07-01T17:45:52.499295Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-01T21:18:56.647955Z","title":"Boylan-Kolchin,Stress testingΛCDM with high-redshift galaxy candidates,Nature Astron.7 (2023), no","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.16152","last_updated":"2026-07-17T17:34:18Z","snapshot_observed_at":"2026-08-08T19:37:45.375959Z","submitted_at":"2026-07-17T17:34:18Z","title":"Large deviations for halos and voids: beyond perturbative non-gaussianities","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-01T21:18:56.647955Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2607.16152"},"observation_digest":"sha256:cb39d1c9fa3045e01333b9ea100eefb7189ea94ae37d74015b42d548f1470f59","observation_id":"ba7fac9e-2378-4ab1-b342-2904115c54fc","resolution":{"observed_at":"2026-08-01T21:18:56.647955Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-01T14:10:56.448838Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.18868","last_updated":"2026-07-21T08:59:21Z","snapshot_observed_at":"2026-08-06T05:25:42.394772Z","submitted_at":"2026-07-21T08:59:21Z","title":"Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-01T14:10:56.448838Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2607.18868"},"observation_digest":"sha256:164624fdb7a0355ce565d39123ba0f657e27c4c3d98331d05b576e3b50097358","observation_id":"a1db14a0-9a7a-4940-ae73-486490882e8d","resolution":{"observed_at":"2026-08-01T14:10:56.448838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-03T00:28:21.786160Z","title":"Boylan-Kolchin, Nature Astron.7, 731 (2023), arXiv:2208.01611 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28800","last_updated":"2026-07-30T19:48:33Z","snapshot_observed_at":"2026-08-09T04:37:43.207204Z","submitted_at":"2026-07-30T19:48:33Z","title":"Ab Initio Cosmological Simulations: From Inflation to Present-Day Structure Formation","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-03T00:28:21.786160Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2607.28800"},"observation_digest":"sha256:8f7bb1c1e563d1fc8aeb8145d6be6244886df2624197c79cbec78e977af2481a","observation_id":"8a395c21-1c64-4941-b3a4-a015b230f65b","resolution":{"observed_at":"2026-08-03T00:28:21.786160Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-04T19:55:29.009731Z","title":"Boylan-Kolchin, Nature Astron.7, 731 (2023), arXiv:2208.01611 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.01844","last_updated":"2026-08-03T07:52:17Z","snapshot_observed_at":"2026-08-08T19:41:52.136413Z","submitted_at":"2026-08-03T07:52:17Z","title":"Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T19:55:29.009731Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2608.01844"},"observation_digest":"sha256:f92f5c23f5bb75a7dcbcc0a40b364571881bb6c87c9e4bd4047055e694e9d1c4","observation_id":"d0f431f5-c965-4813-91d6-9f981bf1cba1","resolution":{"observed_at":"2026-08-04T19:55:29.009731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2208.01611/citation-record","integrity":"/paper/2208.01611/integrity","json":"/paper/2208.01611/citation-record.json","paper":"/paper/2208.01611"},"outbound":[],"paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 20 inbound Pith citation observations for arXiv:2208.01611."}