{"as_of":"2026-08-21T02:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a9b6763cd23d249ef506234fee5d026f7939073af5ab75915409aecd5baf9527","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":17,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":17,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":17,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":17,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T18:12:01.422667Z","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-12T18:12:01.422667Z","title":"Sales, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.11965","last_updated":"2025-04-23T00:28:50Z","snapshot_observed_at":"2026-08-16T18:28:13.065323Z","submitted_at":"2024-11-18T19:00:14Z","title":"The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T18:12:01.422667Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2411.11965"},"observation_digest":"sha256:ef8382d4914e7b6442401c273495f64f14fa7fc2a982c4ee8652f55a8c754b40","observation_id":"7fe0c90f-62f0-480a-b162-7796d75515ce","resolution":{"observed_at":"2026-08-12T18:12:01.422667Z","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-08T14:18:32.731850Z","title":"title Baryonic solutions and challenges for cosmological models of dwarf galaxies","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.06948","last_updated":"2025-02-10T19:00:03Z","snapshot_observed_at":"2026-08-18T12:41:37.939828Z","submitted_at":"2025-02-10T19:00:03Z","title":"The satellite galaxies of the Milky Way and Andromeda","version":1},"reference_index":211,"source":"arxiv_source","source_observed_at":"2026-08-08T14:18:32.731850Z"},"links":{"cited_paper":"/paper/2206.05295","citing_paper":"/paper/2502.06948"},"observation_digest":"sha256:3e27d751388edcce1df56d4667e99a4ffb8cc13bcaffd02cd2cb72f4421d74c1","observation_id":"9253c9b9-dafd-45d8-91d0-ff4906a0dc8f","resolution":{"observed_at":"2026-08-08T14:18:32.731850Z","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-09T12:26:56.470583Z","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":"sha256:749f9103be76d0d742fd97d87611b13efeddd483845c115710a8986cf3868eb8","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-20T20:23:57.494247Z","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":"sha256:7339c06e94b6e37f6d53bec00116705c1df1020e069eaf75b576631b13c8d3fa","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-16T05:29:29.191783Z","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":"sha256:3cc76e8d73ababdace17f945acc8a3d23fe50b8a509660b66c6d9704840b369e","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 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-18T09:54:33.764955Z","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":"2026-08-16T07:15:03.867617Z","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:ce3dbfccead144b345ce2350717645baf08e90dfb1f33ccdbf08be38be6ea944","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 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-18T09:54:33.764955Z","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":"sha256:5836b07817d49af341de40771ddfe3cc26c60d3b4199358d7a35e9d2fda01afd","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 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-18T09:54:33.764955Z","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":"2026-08-14T20:10:37.718399Z","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":"sha256:4281e480bc4cde84d5f435809ec8214e692b7f37e8aa681d58268e05290b900c","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 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.05295","last_updated":"2022-06-10T18:00:01Z","snapshot_observed_at":"2026-08-18T09:54:33.764955Z","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":"2026-08-14T18:39:59.999538Z","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":"sha256:030e4c93d03788ece00fd0b05c7e02061db277a50f4f64c371d1fd8b15498dd4","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-14T23:21:37.112631Z","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:ff7ff4695159e7e018b6afccfbe9091709800a1ce1dff5358ee2984df84a703f","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-14T19:42:36.044174Z","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":"sha256:9927cf5ec0b2c20b3f98daf482eb71892a523dec22cb989c09e998c7c1ae8951","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-18T09:43:43.238120Z","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:ec4295aea2867c704d33d82912836a15be043360256f64864b6924eb5db2b031","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-14T18:25:13.141066Z","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:da3cb4b1322e6ee47c506d5148164f36b2457c534800614f103dd264ed77f5de","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-19T04:10:56.947783Z","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:fbd8f8ec4c6b87a5fcda746454788b3aaf5f236794d60ac80b3f750b62e7cf17","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-15T23:24:16.872609Z","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":"sha256:90c554b422769bbf033f332ea6c4054845f61267e0bd57a18357d95000ca436a","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":"2026-08-18T09:54:33.764955Z","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:f4fe9c9d24dbfdd9795b4ea46a889a1905bf15b362f5986fee646a467ee47685","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-15T12:44:46.267860Z","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:da2a835cdef2cf7979316140374232f5014f39e4adcab6e55f8c45ad9226d0e1","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":"2026-08-18T09:54:33.764955Z","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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2206.05295."}