{"as_of":"2026-08-12T18:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2f575cb6f0b04f22443ad414b1122f6664b4c802e992cf28bb0f4bf92b1b881c","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T05:47:34.275546Z","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":"2026-07-02T19:57:19.911219Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-08-12T05:47:34.275546Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.19911","last_updated":"2025-03-10T19:59:49Z","snapshot_observed_at":"2026-08-12T06:21:04.814417Z","submitted_at":"2024-11-29T18:17:14Z","title":"Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T05:47:34.275546Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2411.19911"},"observation_digest":"sha256:5fe7cef81f7b9da72d7289e522a035fe3de5dfe65dbd03912f42b39fd0128764","observation_id":"4046c37d-6827-45e3-866c-17867abf1a18","resolution":{"observed_at":"2026-08-12T05:47:34.275546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-08-11T16:14:56.576486Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.10310","last_updated":"2024-12-13T17:49:04Z","snapshot_observed_at":"2026-08-11T15:55:52.869361Z","submitted_at":"2024-12-13T17:49:04Z","title":"Simulation-based inference on warm dark matter from HERA forecasts","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T16:14:56.576486Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2412.10310"},"observation_digest":"sha256:72b2c3f89efc05e0e7268a9adf095a8fb1559466cb87490a16bf9c51608eebcf","observation_id":"2a6bec31-ecc7-498c-86d2-b0db086c9af6","resolution":{"observed_at":"2026-08-11T16:14:56.576486Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-08-04T00:26:09.846512Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.01612","last_updated":"2026-06-18T21:25:41Z","snapshot_observed_at":"2026-08-05T17:56:23.069298Z","submitted_at":"2025-11-03T14:19:16Z","title":"Running of the spectral index: Reconciling the CMB with the Lyman-$\\alpha$ Forest","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T00:26:09.846512Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2511.01612"},"observation_digest":"sha256:6296a8d64c9017572cfa9b0fb35dc03c9a9b7b553f16c5c3e99b72c430931572","observation_id":"350a15f5-6e73-4323-a5ed-38f710c45b53","resolution":{"observed_at":"2026-08-04T00:26:09.846512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-08-04T00:10:30.848205Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.02906","last_updated":"2026-07-13T21:59:28Z","snapshot_observed_at":"2026-08-10T13:18:25.502116Z","submitted_at":"2025-11-04T19:00:01Z","title":"Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST","version":2},"reference_index":165,"source":"pdf_text","source_observed_at":"2026-08-04T00:10:30.848205Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2511.02906"},"observation_digest":"sha256:f94b54adb8a0bdb31e894bdc30e96aacdff34291699329a8751d7e6e99e8af89","observation_id":"9ee97e05-0e90-4d20-b659-2c8eb1f4fd4f","resolution":{"observed_at":"2026-08-04T00:10:30.848205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":"2206.08188","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-07-02T19:57:19.911219Z","title":"Hooper, N","venue":null,"work_id":"b815479f-9398-4f80-aa45-34a67e4ab9ef","year":2022},"citing_paper":{"arxiv_id":"2605.22489","last_updated":"2026-05-21T13:43:46Z","snapshot_observed_at":"2026-08-02T05:18:16.583127Z","submitted_at":"2026-05-21T13:43:46Z","title":"Machine Learning Techniques for Astrophysics and Cosmology: Lyman-$\\alpha$ forest","version":1},"reference_index":270,"source":"pdf_text","source_observed_at":"2026-05-22T04:03:53.162706Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2605.22489"},"observation_digest":"sha256:f105f5ea24a7b2dd6884ad4793f74376c7c2151a6561e7b3e8f9e37bedbb715c","observation_id":"a298283c-2578-41a9-b124-7e387826a46a","resolution":{"observed_at":"2026-05-22T04:06:01.890519Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":"2206.08188","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-07-02T19:57:19.911219Z","title":"Hooper, N","venue":null,"work_id":"b815479f-9398-4f80-aa45-34a67e4ab9ef","year":2022},"citing_paper":{"arxiv_id":"2606.06969","last_updated":"2026-08-05T14:05:21Z","snapshot_observed_at":"2026-08-09T14:59:29.083072Z","submitted_at":"2026-06-05T06:57:12Z","title":"Lyman-$\\alpha$ forest constraints on pure and mixed fuzzy dark matter","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-06-27T21:11:32.865715Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2606.06969"},"observation_digest":"sha256:bc3a579f744ff82ea862ab4df269c44a15556fa40a17eccccdcf86737dc1e414","observation_id":"39a668cd-79b2-4b53-8ae5-3c667033ed3c","resolution":{"observed_at":"2026-07-02T19:57:19.912531Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":"2206.08188","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-07-02T19:57:19.911219Z","title":"Hooper, N","venue":null,"work_id":"b815479f-9398-4f80-aa45-34a67e4ab9ef","year":2022},"citing_paper":{"arxiv_id":"2606.28482","last_updated":"2026-06-26T18:00:00Z","snapshot_observed_at":"2026-08-01T23:39:07.858768Z","submitted_at":"2026-06-26T18:00:00Z","title":"Strongest constraints on dark acoustic oscillations from the Lyman-alpha forest","version":1},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-06-30T01:34:51.681907Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2606.28482"},"observation_digest":"sha256:39b0f0593fa2b389837aed32136e5e213eb2b646c3a196439b2274790b0d0ad4","observation_id":"373b5f23-12e4-4f6d-a1a6-1c9955b08c04","resolution":{"observed_at":"2026-07-01T15:25:47.806339Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.08188","snapshot_observed_at":"2026-08-02T00:29:48.536993Z","title":"Hooper, Nils Sch¨ oneberg, Riccardo Murgia, et al.,One likelihood to bind them all: Lyman-αconstraints on non-standard dark matter,JCAP10(2022) 032, [arXiv:2206.08188]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.15020","last_updated":"2026-07-16T14:05:52Z","snapshot_observed_at":"2026-08-09T01:03:03.719877Z","submitted_at":"2026-07-16T14:05:52Z","title":"High resolution Lyman-{\\alpha} forest constraints on dark matter-neutrino scattering","version":1},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-02T00:29:48.536993Z"},"links":{"cited_paper":"/paper/2206.08188","citing_paper":"/paper/2607.15020"},"observation_digest":"sha256:40edc3050f555464ab481139937cc6f4bc150eff013539d4ee6907b6528a213f","observation_id":"9ad8ee59-55d1-4793-a26e-97aa95955522","resolution":{"observed_at":"2026-08-02T00:29:48.536993Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2206.08188/citation-record","integrity":"/paper/2206.08188/integrity","json":"/paper/2206.08188/citation-record.json","paper":"/paper/2206.08188"},"outbound":[],"paper":{"arxiv_id":"2206.08188","last_updated":"2022-06-16T14:01:28Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T21:14:18.818230Z","submitted_at":"2022-06-16T14:01:28Z","title":"One likelihood to bind them all: Lyman-$\\alpha$ constraints on non-standard dark matter"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2206.08188."}