{"as_of":"2026-08-07T08:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c54c1c6236ef57ee165d448ede5b465ffa14a00d9c6d71851792463b57b4eeda","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":15,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":15,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":15,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":15,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T04:21:37.231600Z","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":"2026-07-01T20:36:11.497231Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-07T04:21:37.231600Z","title":"Sales, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.11201","last_updated":"2026-06-16T19:38:57Z","snapshot_observed_at":"2026-08-07T04:10:09.882539Z","submitted_at":"2025-06-12T18:00:40Z","title":"Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-07T04:21:37.231600Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2506.11201"},"observation_digest":"sha256:a86d5bc2f2fb523fb207ed40dcee0e55a6031c566d1f16de915e6a67cb16463b","observation_id":"e7309f2d-27bd-4df7-917f-037f30930170","resolution":{"observed_at":"2026-08-07T04:21:37.231600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-06T18:16:16.478741Z","title":"V., Wetzel A., Fattahi A., 2022, @doi [Nature Astronomy] 10.1038/s41550-022-01689-w , https://ui.adsabs.harvard.edu/abs/2022NatAs...6..897S 6, 897 ( @eprint arXiv 2206.05295 )","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.08925","last_updated":"2025-07-11T18:00:00Z","snapshot_observed_at":"2026-08-06T21:48:06.406035Z","submitted_at":"2025-07-11T18:00:00Z","title":"Cosmological Simulations of Galaxies","version":1},"reference_index":257,"source":"arxiv_source","source_observed_at":"2026-08-06T18:16:16.478741Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2507.08925"},"observation_digest":"sha256:31e2d2a5b876f63eb4526e3efcde5d3e542829f6c5d7fceb962ad1e146427bd7","observation_id":"1164598d-a6ab-4790-b737-90fac8589a4a","resolution":{"observed_at":"2026-08-06T18:16:16.478741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":"2206.05295","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-01T20:36:11.497231Z","title":null,"venue":null,"work_id":"d833408f-98ce-4605-b055-c2d791435a70","year":2022},"citing_paper":{"arxiv_id":"2511.09306","last_updated":"2026-05-20T08:58:17Z","snapshot_observed_at":"2026-07-06T22:35:37.039024Z","submitted_at":"2025-11-12T13:17:24Z","title":"Self-Interaction of Super-Resonant Dark Matter","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-21T19:49:36.832677Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2511.09306"},"observation_digest":"sha256:25937d0887d61c99d81f307840da93b70d393c2134d25a651bd92679f00c6b4d","observation_id":"50780981-5530-4eea-8f7e-c4b7ceff6fe0","resolution":{"observed_at":"2026-05-21T19:50:33.517762Z","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":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":"2206.05295","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-01T20:36:11.497231Z","title":null,"venue":null,"work_id":"d833408f-98ce-4605-b055-c2d791435a70","year":2022},"citing_paper":{"arxiv_id":"2601.17117","last_updated":"2026-04-25T12:29:32Z","snapshot_observed_at":"2026-07-06T22:42:52.947644Z","submitted_at":"2026-01-23T19:00:02Z","title":"Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-16T11:34:12.521105Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2601.17117"},"observation_digest":"sha256:baeeac0ee4d78ac7293f6a700fff805df3e95700a100fdaaace8cac7e9ecba89","observation_id":"37b22142-7141-4852-ac48-417a72c72b2b","resolution":{"observed_at":"2026-05-16T11:37:48.948680Z","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":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":"2206.05295","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-01T20:36:11.497231Z","title":null,"venue":null,"work_id":"d833408f-98ce-4605-b055-c2d791435a70","year":2022},"citing_paper":{"arxiv_id":"2605.12589","last_updated":"2026-05-12T18:00:00Z","snapshot_observed_at":"2026-07-06T23:24:18.302402Z","submitted_at":"2026-05-12T18:00:00Z","title":"Tunneling and tidal stripping in multifield ultralight dark matter halos","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-14T21:07:24.717478Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2605.12589"},"observation_digest":"sha256:d83c47bbdf8add2cc41ed98874842233233da78480c6c1966d2216e194f66baf","observation_id":"0da4f39a-c191-45d5-a4fd-e1a08fdc73c0","resolution":{"observed_at":"2026-05-14T21:09:28.935126Z","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":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":"2206.05295","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-01T20:36:11.497231Z","title":null,"venue":null,"work_id":"d833408f-98ce-4605-b055-c2d791435a70","year":2022},"citing_paper":{"arxiv_id":"2605.31335","last_updated":"2026-05-29T14:16:44Z","snapshot_observed_at":"2026-08-02T13:53:50.544392Z","submitted_at":"2026-05-29T14:16:44Z","title":"Gravothermal Collapse: Robust Against Baryonic Feedback","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-28T20:58:05.796638Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2605.31335"},"observation_digest":"sha256:97d46ccc2b65d91129dc76e84770418d61e5cb98b46dbc3947a657262545e2a0","observation_id":"508886b9-ee6e-40f9-a0c0-7d232a8a2303","resolution":{"observed_at":"2026-07-01T20:36:11.498591Z","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":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-11T11:50:44.784525Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.04893","last_updated":"2026-07-06T10:22:37Z","snapshot_observed_at":"2026-08-07T01:31:17.403632Z","submitted_at":"2026-07-06T10:22:37Z","title":"Collisionless damping of the gravitational instability in fuzzy dark matter: spectral shape and quantum-to-thermal crossover","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:44.784525Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.04893"},"observation_digest":"sha256:1c92772efe431e3e7fd3c8de2a36c159dc1c7395ca23fef906a2ce12c031617e","observation_id":"afe0279b-2b20-4937-8394-5731b50424e3","resolution":{"observed_at":"2026-07-11T11:50:44.784525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-02T06:19:13.974120Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.13141","last_updated":"2026-07-14T18:00:04Z","snapshot_observed_at":"2026-08-05T07:27:31.199936Z","submitted_at":"2026-07-14T18:00:04Z","title":"S-matrix bootstrap bounds on self-interacting dark matter","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-02T06:19:13.974120Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.13141"},"observation_digest":"sha256:6a34c136db97327ce518ae0659b65a7ef03b31d6f5c8f301717a7a49b7718c51","observation_id":"f164d47e-7674-44a8-98f5-3a2a8870e178","resolution":{"observed_at":"2026-08-02T06:19:13.974120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-01T08:43:56.076049Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.21034","last_updated":"2026-07-23T08:16:48Z","snapshot_observed_at":"2026-08-06T04:48:53.870171Z","submitted_at":"2026-07-23T08:16:48Z","title":"A RELHIC twin candidate near the galaxy M51","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-01T08:43:56.076049Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.21034"},"observation_digest":"sha256:3e1bb63b0d35d3c376dacd3f1ad7155bc944e4b010a7b0d6bb7d6b392ed67113","observation_id":"7adec086-c9f7-442d-8a9c-5464d6d178f5","resolution":{"observed_at":"2026-08-01T08:43:56.076049Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-01T06:39:31.972071Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.21834","last_updated":"2026-07-23T21:52:06Z","snapshot_observed_at":"2026-08-06T07:45:56.126782Z","submitted_at":"2026-07-23T21:52:06Z","title":"The diffraction-lensing interpretation of GW231123 with astrophysical priors","version":1},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-01T06:39:31.972071Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.21834"},"observation_digest":"sha256:e0ed17b01e1d6bd1997ae39108ee8fd23d5ece57e811f2ef59e5bd9c25a6dcae","observation_id":"cda041f2-70bf-42ae-8fdf-7075a79536ce","resolution":{"observed_at":"2026-08-01T06:39:31.972071Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-01T03:02:58.672457Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.25261","last_updated":"2026-07-28T04:03:37Z","snapshot_observed_at":"2026-08-01T03:02:56.762810Z","submitted_at":"2026-07-28T04:03:37Z","title":"Tightening Bounds on Warm Dark Matter with High-Redshift Gamma-Ray Bursts","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-01T03:02:58.672457Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.25261"},"observation_digest":"sha256:e8a8e35549226580c0820151433ede275a4cef676856804de4c843858f8fad86","observation_id":"0d5e8b35-63f2-421b-9ef8-1c65662ec339","resolution":{"observed_at":"2026-08-01T03:02:58.672457Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-01T09:45:37.424761Z","title":"and Wetzel, Andrew and Fattahi, Azadeh","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.27312","last_updated":"2026-07-29T18:00:00Z","snapshot_observed_at":"2026-08-05T16:49:23.261541Z","submitted_at":"2026-07-29T18:00:00Z","title":"Non-linear Evolution of Dark Plasma Subhalos","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-01T09:45:37.424761Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.27312"},"observation_digest":"sha256:9d89cd3094f838feb1b8b27318f4249719b891e7ebaa8672e1458af7e678958d","observation_id":"527cdf29-9c41-402f-bff6-cf7faa139d5a","resolution":{"observed_at":"2026-08-01T09:45:37.424761Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-31T04:54:06.697017Z","title":"Sales, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.28517","last_updated":"2026-07-30T16:55:29Z","snapshot_observed_at":"2026-08-06T02:08:11.250516Z","submitted_at":"2026-07-30T16:55:29Z","title":"Dynamical flattening of halo density cusps by Q-ball dark matter","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-31T04:54:06.697017Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.28517"},"observation_digest":"sha256:490eab03e40f770d9e8bd011320173f84044cf0113586416a29d177166844593","observation_id":"2fd02cf5-ef53-4ae9-bc4d-ee74725d2555","resolution":{"observed_at":"2026-07-31T04:54:06.697017Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-07-31T02:27:16.865975Z","title":"Nature Astronomy , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28604","last_updated":"2026-07-30T17:54:43Z","snapshot_observed_at":"2026-08-06T11:18:05.221988Z","submitted_at":"2026-07-30T17:54:43Z","title":"Cosmo-SPINN: Fuzzy Dark Matter Simulations with Physics-Informed Generative Networks","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-31T02:27:16.865975Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2607.28604"},"observation_digest":"sha256:c45b054f858d81e5553babaad3485b427fe317bb11ec0ea70b47dd1ef52ecb13","observation_id":"460976e7-5617-47ae-9161-2035f9b64de9","resolution":{"observed_at":"2026-07-31T02:27:16.865975Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.05295","snapshot_observed_at":"2026-08-04T01:15:10.606860Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2608.00161","last_updated":"2026-07-31T18:00:00Z","snapshot_observed_at":"2026-08-06T23:11:58.995583Z","submitted_at":"2026-07-31T18:00:00Z","title":"Ubiquitous Corotation of Dark Matter Halos: Implications for Direct Detection","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T01:15:10.606860Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2608.00161"},"observation_digest":"sha256:d69743df656379800ba88fc85f20bf01c8073fd263855828316c18d4b5c09d36","observation_id":"27d97d41-317f-4998-a0fc-f72a71ee8acb","resolution":{"observed_at":"2026-08-04T01:15:10.606860Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2206.05295/citation-record","integrity":"/paper/2206.05295/integrity","json":"/paper/2206.05295/citation-record.json","paper":"/paper/2206.05295"},"outbound":[],"paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-04T13:37:37.114737Z","submitted_at":"2022-06-10T18:00:01Z","title":"Baryonic solutions and challenges for cosmological models of dwarf galaxies"},"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 15 inbound Pith citation observations for arXiv:2206.05295."}