{"as_of":"2026-08-23T17:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8bb266459c487fa05c6ebd976d8a105296116bd5c6938342624dfe6b61c8ec3e","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:26:09.581628Z","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":"2026-07-10T02:16:42.378967Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-08T00:02:53.696390Z","title":"The im- pact of UV variability on the abundance of bright galax- ies at z ≥ 9,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.08701","last_updated":"2025-02-12T19:00:00Z","snapshot_observed_at":"2026-08-15T06:27:32.442563Z","submitted_at":"2025-02-12T19:00:00Z","title":"Early Galaxies from Rare Inflationary Processes and JWST Observations","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T00:02:53.696390Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2502.08701"},"observation_digest":"sha256:8db77962443d026d57d1827c2736e7c79af4ead4c195330c3e09ca69e213e2a9","observation_id":"d425ec61-329b-4e1e-a7bd-fd2d8cd97f29","resolution":{"observed_at":"2026-08-08T00:02:53.696390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-15T21:11:35.517387Z","title":"2023, arXiv e-prints, arXiv:2305.05679, doi: 10.48550/arXiv.2305.05679","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.10619","last_updated":"2025-08-22T15:02:45Z","snapshot_observed_at":"2026-08-16T05:28:09.492745Z","submitted_at":"2025-05-15T18:00:02Z","title":"Redshift evolution of Lyman continuum escape fraction after JWST","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-15T21:11:35.517387Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2505.10619"},"observation_digest":"sha256:679cc90ef75d8ac3cdfe551e93108054d1142dbf91dae76e111a0e739050b4c5","observation_id":"9c513b40-addc-48e8-9c45-b307329cace8","resolution":{"observed_at":"2026-08-15T21:11:35.517387Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-06T12:54:07.953556Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.21409","last_updated":"2025-07-29T00:33:44Z","snapshot_observed_at":"2026-08-16T16:36:07.997157Z","submitted_at":"2025-07-29T00:33:44Z","title":"Explaining the \"too massive\" high-redshift galaxies in JWST data: numerical study of three effects and a simple relation","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-06T12:54:07.953556Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2507.21409"},"observation_digest":"sha256:8f71d01483cfe13bcd9c4f0cf8cb0f8e60b75d2eb9486fa114c3c6911cfe4fcb","observation_id":"66380ae9-8328-4cc7-88b9-63ee35ebf90b","resolution":{"observed_at":"2026-08-06T12:54:07.953556Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-04T00:10:33.532429Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.02906","last_updated":"2026-07-13T21:59:28Z","snapshot_observed_at":"2026-08-16T10:51:02.401539Z","submitted_at":"2025-11-04T19:00:01Z","title":"Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST","version":2},"reference_index":188,"source":"pdf_text","source_observed_at":"2026-08-04T00:10:33.532429Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2511.02906"},"observation_digest":"sha256:3c22b3d0b4a0c8b9026f86a9de2005d73cd79f8445ee54c4a8849ab51d7f6796","observation_id":"3f2bb947-d920-45f5-a62e-c241a1dc3a51","resolution":{"observed_at":"2026-08-04T00:10:33.532429Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-02T20:12:34.558456Z","title":"The impact of UV variability on the abundance of bright galaxies at z≥9","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2602.23913","last_updated":"2026-06-01T10:10:58Z","snapshot_observed_at":"2026-08-12T17:35:21.459357Z","submitted_at":"2026-02-27T11:02:50Z","title":"Probing inflationary features with galaxy ultraviolet luminosity function observables","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-02T20:12:34.558456Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2602.23913"},"observation_digest":"sha256:a5e658d235ea048a38222ad10da10dcd4050a2191ec4ab8bdb1483fb355a40bb","observation_id":"7a312f4f-2ecf-4e8e-a8c1-adc887efd099","resolution":{"observed_at":"2026-08-02T20:12:34.558456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":"2305.05679","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-07-10T02:16:42.378967Z","title":"author Vogelsberger, M","venue":"astro-ph.GA","work_id":"c9c171b8-b00d-4adc-937c-727a8cd53a1a","year":2023},"citing_paper":{"arxiv_id":"2604.13866","last_updated":"2026-04-29T11:42:23Z","snapshot_observed_at":"2026-08-21T11:23:59.007821Z","submitted_at":"2026-04-15T13:29:50Z","title":"Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies","version":2},"reference_index":134,"source":"arxiv_source","source_observed_at":"2026-05-10T12:34:33.213779Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2604.13866"},"observation_digest":"sha256:07ca7b32e2cff6598852411f06f6d0fdd12271cf1055412d1290380beb59e0b9","observation_id":"e15e6dda-7d6f-4363-81bf-f42711f5227f","resolution":{"observed_at":"2026-05-11T11:46:34.624585Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":"2305.05679","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-07-10T02:16:42.378967Z","title":"author Vogelsberger, M","venue":"astro-ph.GA","work_id":"c9c171b8-b00d-4adc-937c-727a8cd53a1a","year":2023},"citing_paper":{"arxiv_id":"2605.01023","last_updated":"2026-05-01T18:35:29Z","snapshot_observed_at":"2026-08-13T11:56:28.629068Z","submitted_at":"2026-05-01T18:35:29Z","title":"Formation and Redshift Evolution of Dark Matter Spikes","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-05-09T18:22:03.254023Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2605.01023"},"observation_digest":"sha256:3cba520f5a7e636043047624743fc0daf6e4645c07ef3c59d8daaa8e140b6279","observation_id":"620fd34d-7522-4117-9d15-407cf200e099","resolution":{"observed_at":"2026-05-11T16:16:07.961818Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":"2305.05679","doi":null,"metadata_source":"pith","pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-07-10T02:16:42.378967Z","title":"author Vogelsberger, M","venue":"astro-ph.GA","work_id":"c9c171b8-b00d-4adc-937c-727a8cd53a1a","year":2023},"citing_paper":{"arxiv_id":"2607.08749","last_updated":"2026-07-09T17:49:55Z","snapshot_observed_at":"2026-08-20T12:43:23.973909Z","submitted_at":"2026-07-09T17:49:55Z","title":"Deep Spectroscopic Follow-Up of Maisie's Galaxy -- A Typical Galaxy in the Early Universe","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2607.08749"},"observation_digest":"sha256:c45b8a5dc052958dc2272f0211ac673a0ce1141f041cc2b508128a81015beec9","observation_id":"d485a873-19db-4b8a-9ec8-09b19004e917","resolution":{"observed_at":"2026-07-10T02:16:42.380235Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-07-13T06:20:04.707661Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.08846","last_updated":"2026-07-09T18:11:36Z","snapshot_observed_at":"2026-08-17T04:17:42.426140Z","submitted_at":"2026-07-09T18:11:36Z","title":"mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy","version":1},"reference_index":171,"source":"arxiv_source","source_observed_at":"2026-07-13T06:20:04.707661Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2607.08846"},"observation_digest":"sha256:256d116a758b30410899e68ff38c285fb8ba69ab28cdb40d2d5f04b055fb33b5","observation_id":"18fa1267-74b0-4757-8eb3-73d78a70bf39","resolution":{"observed_at":"2026-07-13T06:20:04.707661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-07-14T15:06:13.177523Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.09846","last_updated":"2026-07-10T18:00:00Z","snapshot_observed_at":"2026-08-18T15:45:57.409852Z","submitted_at":"2026-07-10T18:00:00Z","title":"The Rise and Fall of Acoustic Oscillations at Cosmic Dawn","version":1},"reference_index":104,"source":"pdf_text","source_observed_at":"2026-07-14T15:06:13.177523Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2607.09846"},"observation_digest":"sha256:23ca19c1482d682683cb49354eaccb769bc33e1e5aff3355b8c570b64170e81d","observation_id":"2bfed309-14f9-45ef-910c-b46b4b6ae2e8","resolution":{"observed_at":"2026-07-14T15:06:13.177523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-01T14:10:56.793582Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.18868","last_updated":"2026-07-21T08:59:21Z","snapshot_observed_at":"2026-08-15T22:55:44.404302Z","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":179,"source":"arxiv_source","source_observed_at":"2026-08-01T14:10:56.793582Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2607.18868"},"observation_digest":"sha256:615e416a09615284d649454b34821ce141b83e9e7d9e2139df32e2c78112535c","observation_id":"d84049c7-81bf-422c-b7ab-7e9607bd32bd","resolution":{"observed_at":"2026-08-01T14:10:56.793582Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-15T14:54:41.542726Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.03441","last_updated":"2026-08-04T10:36:35Z","snapshot_observed_at":"2026-08-18T09:22:32.553111Z","submitted_at":"2026-08-04T10:36:35Z","title":"SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-15T14:54:41.542726Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2608.03441"},"observation_digest":"sha256:5b57f4b2d532403d41a6a8587f7058d624a850e98f866b0a6c87adf71e91b4f9","observation_id":"ecd330b1-3299-4f54-957b-1eb8f9eae0f4","resolution":{"observed_at":"2026-08-15T14:54:41.542726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05679","snapshot_observed_at":"2026-08-16T04:26:09.581628Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.12699","last_updated":"2026-08-19T15:39:04Z","snapshot_observed_at":"2026-08-22T23:11:56.541729Z","submitted_at":"2026-08-13T01:22:49Z","title":"SPURS: Massive Stars, Dense Gas, and Ly$\\alpha$ Escape in GN-z11 at $z = 10.6$","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-16T04:26:09.581628Z"},"links":{"cited_paper":"/paper/2305.05679","citing_paper":"/paper/2608.12699"},"observation_digest":"sha256:08bc1013c872cc6492b17ed83967cbc23c00051863a4006f41bf805d2a511b40","observation_id":"b098cb15-24cb-42e9-aa76-f51d6dbb7fb2","resolution":{"observed_at":"2026-08-16T04:26:09.581628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2305.05679/citation-record","integrity":"/paper/2305.05679/integrity","json":"/paper/2305.05679/citation-record.json","paper":"/paper/2305.05679"},"outbound":[],"paper":{"arxiv_id":"2305.05679","last_updated":"2023-08-29T09:19:12Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-18T07:37:27.376826Z","submitted_at":"2023-05-09T18:00:00Z","title":"The impact of UV variability on the abundance of bright galaxies at $z \\geq 9$"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2305.05679."}