{"as_of":"2026-08-07T11:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:306f3e850ed1d05eff07a41118934f411edc57164c7372e66356eb51c30473a0","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":25,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":25,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":25,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":25,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T18:36:06.097868Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":169,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-06T18:36:06.097868Z","title":"Chisari, A.J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.07991","last_updated":"2025-07-10T17:59:06Z","snapshot_observed_at":"2026-08-07T06:12:38.992728Z","submitted_at":"2025-07-10T17:59:06Z","title":"Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T18:36:06.097868Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2507.07991"},"observation_digest":"sha256:b9f5a53bb29cb2639b886c85bc170d96fd945b2e145ce2444cda648991f22c6b","observation_id":"af57cec6-a746-44cb-aa9e-521b4ecb820d","resolution":{"observed_at":"2026-08-06T18:36:06.097868Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-06T16:15:51.710262Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.14136","last_updated":"2025-07-18T17:59:24Z","snapshot_observed_at":"2026-08-06T19:41:48.838383Z","submitted_at":"2025-07-18T17:59:24Z","title":"Missing baryons recovered: a measurement of the gas fraction in galaxies and groups with the kinematic Sunyaev-Zel'dovich effect and CMB lensing","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T16:15:51.710262Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2507.14136"},"observation_digest":"sha256:350de0e6734b9a264f0156d68f88aed50030bb47c487edaf0563a9acea3acd98","observation_id":"413394bf-89af-4a66-983a-192dc25bbd87","resolution":{"observed_at":"2026-08-06T16:15:51.710262Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2603.13053","last_updated":"2026-04-16T17:34:24Z","snapshot_observed_at":"2026-07-06T22:48:57.474272Z","submitted_at":"2026-03-13T15:03:05Z","title":"A unified harmonic framework for dark siren cosmology","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-05-15T11:29:59.268052Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2603.13053"},"observation_digest":"sha256:f28f795318c539b07f6cbd3a078622f65f36f0c7b59b91838e6abccc72b6f578","observation_id":"6b8bfdde-675e-4bd2-af7f-03be3afd8424","resolution":{"observed_at":"2026-05-15T11:30:31.164279Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2604.15797","last_updated":"2026-04-17T07:55:57Z","snapshot_observed_at":"2026-07-06T23:03:16.345488Z","submitted_at":"2026-04-17T07:55:57Z","title":"Inverting Fisher biases for fast systematics exploration","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-10T09:08:46.802880Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2604.15797"},"observation_digest":"sha256:22e3b0633e4b8993e8ad82cb7584df4895c074f7621a9b606dd5b7ccbdfd0b09","observation_id":"2462c94b-ae9f-4cfb-a9c9-51e075cc9922","resolution":{"observed_at":"2026-05-10T09:13:28.932046Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2604.17162","last_updated":"2026-04-18T22:37:05Z","snapshot_observed_at":"2026-08-02T20:43:04.061854Z","submitted_at":"2026-04-18T22:37:05Z","title":"Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-10T05:45:46.799115Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2604.17162"},"observation_digest":"sha256:f1c9eefab8a439b21caf39367e9ae2a7d35bf47dcdfda5aa9d524b5db3d4d471","observation_id":"5be2f06c-6f05-4db6-bc22-906dfe773089","resolution":{"observed_at":"2026-05-10T05:46:09.168137Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2604.22105","last_updated":"2026-04-23T22:27:47Z","snapshot_observed_at":"2026-07-06T23:08:33.204647Z","submitted_at":"2026-04-23T22:27:47Z","title":"Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-08T13:59:58.241577Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2604.22105"},"observation_digest":"sha256:426fc32a16edcad556d5da0c96bc1d92327ec0b7d33a8817a283335a32b023b1","observation_id":"c2aef8fa-dea1-4e36-bebb-7a6dc3c6db6f","resolution":{"observed_at":"2026-05-08T21:19:13.480148Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2604.26022","last_updated":"2026-04-30T00:23:11Z","snapshot_observed_at":"2026-07-06T23:11:48.524898Z","submitted_at":"2026-04-28T18:05:05Z","title":"Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-07T14:53:02.246257Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2604.26022"},"observation_digest":"sha256:debb9c6119d92f54bdb5873d36bfe3f65578967a2b246c94726ed933d53202b5","observation_id":"86d76176-385c-45e0-8791-85aa8d496170","resolution":{"observed_at":"2026-05-12T00:36:17.374990Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2605.00818","last_updated":"2026-05-01T17:57:07Z","snapshot_observed_at":"2026-07-06T23:14:11.211164Z","submitted_at":"2026-05-01T17:57:07Z","title":"$4\\times3$ Point Correlation Functions in Galaxy Surveys: Impact of Baryonic Feedback","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-09T18:38:12.253954Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2605.00818"},"observation_digest":"sha256:9212327729ec4bfd06bd6d04d9d49f27eca1a5ec428088b0b3d1be8b4f751001","observation_id":"2fa0da27-2d48-4f6b-be34-c4bea45f4000","resolution":{"observed_at":"2026-05-11T16:11:07.752354Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2605.01963","last_updated":"2026-05-03T16:50:00Z","snapshot_observed_at":"2026-07-31T21:42:31.294100Z","submitted_at":"2026-05-03T16:50:00Z","title":"Constraints on Halo Gas Profiles from Joint kSZ and Galaxy Clustering Analysis of ACT DR6 and CMASS","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-08T19:30:05.210473Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2605.01963"},"observation_digest":"sha256:17a8c6f80c137544b70a6d47537f7931e4488cb5e483d9de2339cb6847734455","observation_id":"f7e5c37b-46a9-4b33-9f9f-be1fac7e8d52","resolution":{"observed_at":"2026-05-09T05:50:26.602351Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2605.02723","last_updated":"2026-05-04T15:22:39Z","snapshot_observed_at":"2026-07-06T23:15:46.390406Z","submitted_at":"2026-05-04T15:22:39Z","title":"Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-05-08T18:17:47.203929Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2605.02723"},"observation_digest":"sha256:08bcb318b6b5d206f6334079f9caae2454f5df4cde5f6a718dba91d89aff6678","observation_id":"d181cda1-3b52-464c-9f3b-c0dfc70ca8a6","resolution":{"observed_at":"2026-05-08T18:18:55.164139Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2605.12877","last_updated":"2026-05-13T01:45:54Z","snapshot_observed_at":"2026-08-03T06:28:58.100231Z","submitted_at":"2026-05-13T01:45:54Z","title":"Machine-learning applications for weak-lensing cosmology","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2605.12877"},"observation_digest":"sha256:4d9f5242859ed25ba5bd9da8033660787cb2d6da5676c3a4e5459d5659315593","observation_id":"09723970-f641-4315-8d26-edc4e2930113","resolution":{"observed_at":"2026-05-14T19:07:49.624673Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2605.21483","last_updated":"2026-05-20T17:59:05Z","snapshot_observed_at":"2026-08-02T20:49:07.449881Z","submitted_at":"2026-05-20T17:59:05Z","title":"Velocityformer: Broken-Symmetry-Matched Equivariant Graph Transformers for Cosmological Velocity Reconstruction","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-21T02:53:29.870619Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2605.21483"},"observation_digest":"sha256:0e2c0dd7d6470b6ad135cd81f7cb9f50692ba05d956c2708c98db8b0c640e0c6","observation_id":"690a5ceb-c950-4c6c-a074-dd5dc6654e36","resolution":{"observed_at":"2026-05-21T02:53:55.252187Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.03753","last_updated":"2026-06-02T15:03:13Z","snapshot_observed_at":"2026-08-02T00:40:03.579480Z","submitted_at":"2026-06-02T15:03:13Z","title":"The impact of source and survey modelling on the connection between [O III] emitters and Ly $\\alpha$ forest transmission at z ~ 6","version":1},"reference_index":114,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.03753"},"observation_digest":"sha256:901a5413182ff2fe119762cd4d0733b83170b72aec251ea4e6956d334e70bce9","observation_id":"3dfa4bd5-5940-4af9-be89-c057c384c01d","resolution":{"observed_at":"2026-06-28T08:31:48.572203Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.24061","last_updated":"2026-06-23T02:10:14Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-23T02:10:14Z","title":"Probing Baryonic Feedback Effect with CSST Weak Lensing and Future FRB Measurements","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.24061"},"observation_digest":"sha256:54439da2f903979d39a235b9fa6a918f5e6f2215b27aef75e89d105acfbaf8dc","observation_id":"eaddb00c-c441-4f8f-92da-94260a3e7ffc","resolution":{"observed_at":"2026-06-25T23:58:42.221754Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.24159","last_updated":"2026-06-23T05:27:38Z","snapshot_observed_at":"2026-07-06T23:58:49.574536Z","submitted_at":"2026-06-23T05:27:38Z","title":"A First Measurement of Circumgalactic Dust Reddening from Only 4.6 deg$^2$ of the Rubin Observatory's DP1","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.24159"},"observation_digest":"sha256:44121f6b189a13fbf4eda1527778d3b55b091fec42ede55408b69637ef3773db","observation_id":"eea1361f-c97c-48fe-ab09-917d48ef680e","resolution":{"observed_at":"2026-06-26T00:18:43.056964Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.26223","last_updated":"2026-07-02T17:54:11Z","snapshot_observed_at":"2026-08-04T21:43:23.762833Z","submitted_at":"2026-06-24T18:00:01Z","title":"Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing","version":1},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.26223"},"observation_digest":"sha256:7f3f5e0ce9e20fb988feae02e18fc2122a1d9622472cc68b95e24a3ab028e106","observation_id":"9f743476-c568-4586-8e79-979f1657b05d","resolution":{"observed_at":"2026-06-26T01:48:54.479977Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.26223","last_updated":"2026-07-02T17:54:11Z","snapshot_observed_at":"2026-08-04T21:43:23.762833Z","submitted_at":"2026-06-24T18:00:01Z","title":"Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing","version":2},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.26223"},"observation_digest":"sha256:560b6f0b54fcd58d57acb147c6a6fa7818aa70903c4eb0eece07f42960c6416e","observation_id":"ae29a25c-9b64-4518-bd56-489c9af1977c","resolution":{"observed_at":"2026-07-03T23:09:00.616255Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.27714","last_updated":"2026-06-26T04:44:56Z","snapshot_observed_at":"2026-08-01T17:32:21.309572Z","submitted_at":"2026-06-26T04:44:56Z","title":"Fast Radio Bursts as Cosmological Probes","version":1},"reference_index":121,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.27714"},"observation_digest":"sha256:c07724e4399f00aae97b7be8323e6bb4b1b2ca49e9363b12679746f60383ae41","observation_id":"344f7935-c73b-4b40-bd54-8b37af7689e0","resolution":{"observed_at":"2026-06-29T03:53:04.832616Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":"1905.06082","doi":"10.21105/astro.1905.06082","metadata_source":"pith","pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Modelling baryonic feedback for survey cosmology","venue":"astro-ph.CO","work_id":"944ba138-aa94-4532-9fea-9933e1acd8a5","year":2019},"citing_paper":{"arxiv_id":"2606.29388","last_updated":"2026-07-13T15:48:00Z","snapshot_observed_at":"2026-07-16T23:19:38.624707Z","submitted_at":"2026-06-28T13:26:01Z","title":"Probing the Baryon Distribution with Fast Radio Bursts","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.29388"},"observation_digest":"sha256:f6f275abf31a632f965504daf98f18b499aa3806eee3f1972c15874fe2e1eb34","observation_id":"cb0af7a0-d88c-4704-98e7-5941628bfe72","resolution":{"observed_at":"2026-06-30T02:24:12.611025Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-07-14T17:05:40.776219Z","title":null,"venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"2606.29388","last_updated":"2026-07-13T15:48:00Z","snapshot_observed_at":"2026-07-16T23:19:38.624707Z","submitted_at":"2026-06-28T13:26:01Z","title":"Probing the Baryon Distribution with Fast Radio Bursts","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-14T17:05:40.776219Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2606.29388"},"observation_digest":"sha256:8d05e491456f8f36cd6daebb8908c27709f87d75fc8b1744f68c9ee817acbf2f","observation_id":"e810ab68-0d04-4d34-95ca-6942dd17d1ea","resolution":{"observed_at":"2026-07-14T17:05:40.776219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-01T23:42:37.848723Z","title":"E., Mead, A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.15344","last_updated":"2026-07-16T18:00:29Z","snapshot_observed_at":"2026-08-06T19:09:37.043711Z","submitted_at":"2026-07-16T18:00:29Z","title":"The Azahar Project: Non-Thermal Physics Drives Star Formation Burstiness and the Evolution of the UV Luminosity Density at Cosmic Dawn","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-01T23:42:37.848723Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2607.15344"},"observation_digest":"sha256:4a5e0140c9644e3feef4db4bcff6d687a485991c7e9de40f196f60278b251d49","observation_id":"39f72c38-bdc1-4a6d-af47-652b20b49a85","resolution":{"observed_at":"2026-08-01T23:42:37.848723Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-07-31T23:49:33.012236Z","title":"The Open Journal of Astrophysics , keywords =","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"2607.23339","last_updated":"2026-07-25T19:35:29Z","snapshot_observed_at":"2026-08-02T05:19:25.373749Z","submitted_at":"2026-07-25T19:35:29Z","title":"Interpreting the stacked kinetic SZ effect I: velocity reconstruction and non-linear velocity effects","version":1},"reference_index":177,"source":"arxiv_source","source_observed_at":"2026-07-31T23:49:33.012236Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2607.23339"},"observation_digest":"sha256:80f52e676391fe435c765b93df95b0618bdabc7b5d88bdf61df77ed10faba59e","observation_id":"56560de8-ed8b-4f12-bed8-ab363171d1f1","resolution":{"observed_at":"2026-07-31T23:49:33.012236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-07-30T11:19:08.083079Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.27149","last_updated":"2026-07-29T17:23:42Z","snapshot_observed_at":"2026-08-03T08:27:44.569841Z","submitted_at":"2026-07-29T17:23:42Z","title":"Shear-kSZ: A New Estimator for the Matter-Electron Power Spectrum from kSZ Tomography and Weak Lensing","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-30T11:19:08.083079Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2607.27149"},"observation_digest":"sha256:5efc4f1b3cc38c1b4954a2f7efbdc65e8b5dc98c947612c48a3c0d814ed70756","observation_id":"910bd1d8-5e59-4155-810a-a79bb69c69c8","resolution":{"observed_at":"2026-07-30T11:19:08.083079Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-03T13:53:46.223632Z","title":"Mead, Shahab Joudaki, Pedro G","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.29091","last_updated":"2026-07-31T07:17:11Z","snapshot_observed_at":"2026-08-05T23:12:35.807552Z","submitted_at":"2026-07-31T07:17:11Z","title":"Direct shear $\\times$ kSZ correlation: controlling baryons without modeling galaxies","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T13:53:46.223632Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2607.29091"},"observation_digest":"sha256:6f45fd21e4f891735bbe03414687107a7d46743e2b604f76d76615a02a176d35","observation_id":"3e3e40d5-1c1d-403f-87c2-bf0e14ad2e46","resolution":{"observed_at":"2026-08-03T13:53:46.223632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.06082","snapshot_observed_at":"2026-08-05T10:39:42.873039Z","title":"CAMB: Code for Anisotropies in the Microwave Background,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"2608.03876","last_updated":"2026-08-04T16:15:51Z","snapshot_observed_at":"2026-08-07T10:21:53.008629Z","submitted_at":"2026-08-04T16:15:51Z","title":"Fisher Forecasting for the DESC with $\\texttt{Augur}$","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-05T10:39:42.873039Z"},"links":{"cited_paper":"/paper/1905.06082","citing_paper":"/paper/2608.03876"},"observation_digest":"sha256:6d94d5efdf96785d472a1ac4387d8cb2e10a4aa78a389635bb0bab0dbf81b142","observation_id":"e1bc12b5-abb9-4194-b00c-f637b7368fae","resolution":{"observed_at":"2026-08-05T10:39:42.873039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1905.06082/citation-record","integrity":"/paper/1905.06082/integrity","json":"/paper/1905.06082/citation-record.json","paper":"/paper/1905.06082"},"outbound":[],"paper":{"arxiv_id":"1905.06082","last_updated":"2019-06-25T11:10:58Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T07:53:09.636582Z","submitted_at":"2019-05-15T10:54:01Z","title":"Modelling baryonic feedback for survey cosmology"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 25 inbound Pith citation observations for arXiv:1905.06082."}