{"as_of":"2026-08-14T19:21:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:764f5ff25cabf034cf306c8c3e56c3e780c41a3e65de9fcd08bb401450158675","coverage":[{"denominator":28,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":28,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:26:00.536690Z","state":"measured"},{"denominator":29,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":29,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:26:00.394741Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-06T21:26:01.059838Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"cited_work":{"arxiv_id":"2507.00410","doi":null,"metadata_source":"pith","pith_arxiv_id":"2507.00410","snapshot_observed_at":"2026-08-06T21:26:01.059838Z","title":"The Density Profile of Dynamical Halos","venue":"astro-ph.CO","work_id":"100d2771-f0cc-49ff-9766-71fd0a1fb3aa","year":2025},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.394741Z"},"links":{"cited_paper":"/paper/2507.00410","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:0dfc83cfe7cc801b75f49ca204b3b4a1ea29305d7752d65cc1f28c775d62f567","observation_id":"90cbff43-bfcf-47a1-85f9-ae360f31a6e8","resolution":{"observed_at":"2026-08-06T21:26:01.064856Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2507.00410/citation-record","integrity":"/paper/2507.00410/integrity","json":"/paper/2507.00410/citation-record.json","paper":"/paper/2507.00410"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.172171Z","title":null,"venue":null,"work_id":"d2dcd011-56be-4caf-a88c-24d4b153d295","year":null},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.407501Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:0a323df3c8bec56ccbd43251f873825860d97dd8e4592fc84a6133e22d052712","observation_id":"4db73bd0-cbe0-4552-9c30-efb648bb2ddc","resolution":{"observed_at":"2026-08-06T21:26:01.177586Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.188164Z","title":"Salazar et al","venue":null,"work_id":"39322cd3-92e5-442e-ab3b-7452e439b4e2","year":2025},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.401125Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:1cbcb7bca39a5dcade60861c85435bc44f312085aec0651e53642be8d4e9a25b","observation_id":"6e1babc8-01b4-4084-9a09-0141254ea1be","resolution":{"observed_at":"2026-08-06T21:26:01.193448Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.124227Z","title":null,"venue":null,"work_id":"e1b065bb-af99-4a04-8447-04c8c326daaf","year":1965},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.433088Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:71f1f58dca13318741d34075eabe4294af5a159d62bc7f1de6045a0a508c828c","observation_id":"b3405a34-f03f-42e3-9c9a-430029bcc716","resolution":{"observed_at":"2026-08-06T21:26:01.128942Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.156299Z","title":"This reduces the number of degrees of freedom in the individual fits to two, the same number of degrees of freedom in the Salazar et al","venue":null,"work_id":"ed7a52c2-172c-41ce-8796-0e01a8de0b5e","year":null},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.412541Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:2e4ca4cd16fc894011931de12a3f9108ed4c8f1690dabf684b9d58fa38211c0b","observation_id":"3268af59-ec39-431b-a5c9-a5aeea9cedb1","resolution":{"observed_at":"2026-08-06T21:26:01.161423Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1504.05591","last_updated":"2015-04-21T20:01:40Z","snapshot_observed_at":"2026-08-14T17:16:15.488484Z","submitted_at":"2015-04-21T20:01:40Z","title":"The splashback radius as a physical halo boundary and the growth of halo mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1504.05591","snapshot_observed_at":"2026-08-06T21:26:00.444390Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.444390Z"},"links":{"cited_paper":"/paper/1504.05591","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:5611f77d1c989eeb3c9b58802b4646c669b6ce9e4cd2d5e28ef4df64ff97a966","observation_id":"010ad846-ca0c-47f6-a836-e743beaecff0","resolution":{"observed_at":"2026-08-06T21:26:00.444390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2207.11827","last_updated":"2022-07-24T22:02:25Z","snapshot_observed_at":"2026-08-14T16:14:41.579216Z","submitted_at":"2022-07-24T22:02:25Z","title":"A Better Way to Define Dark Matter Haloes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2207.11827","snapshot_observed_at":"2026-08-06T21:26:00.422941Z","title":"Garc ´ ıa, E","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.422941Z"},"links":{"cited_paper":"/paper/2207.11827","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:bf48823f216b8e3160a3e50689ea02317245ea3070aa034e00b0d9bcc3560e5a","observation_id":"de6f7702-f139-4f47-899f-90ba0966edc6","resolution":{"observed_at":"2026-08-06T21:26:00.422941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611107","last_updated":"1997-10-21T23:14:37Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-13T22:59:55Z","title":"A Universal Density Profile from Hierarchical Clustering","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611107","snapshot_observed_at":"2026-08-06T21:26:00.428087Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.428087Z"},"links":{"cited_paper":"/paper/astro-ph/9611107","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:ec306872e97a616f4098921834c5c6b5c1a59ff0476974825ede068457822d4b","observation_id":"f63e9d50-5e78-45f9-b458-6ce67769c70e","resolution":{"observed_at":"2026-08-06T21:26:00.428087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.03477","last_updated":"2021-01-27T11:37:06Z","snapshot_observed_at":"2026-08-12T17:35:41.891738Z","submitted_at":"2020-08-08T08:50:21Z","title":"A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations","version":2},"cited_work":{"arxiv_id":"2008.03477","doi":null,"metadata_source":"pith","pith_arxiv_id":"2008.03477","snapshot_observed_at":"2026-08-06T21:26:00.931620Z","title":"A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations","venue":"astro-ph.CO","work_id":"bf85c1af-6cbe-4c89-a91d-2a6307cc484b","year":2020},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.461195Z"},"links":{"cited_paper":"/paper/2008.03477","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:2cfbf7cdf4ce0f95277592117edd003fc1c7c4e6977425e71958409993f557f3","observation_id":"c930ecf2-565f-41ca-a92b-43584a47430f","resolution":{"observed_at":"2026-08-06T21:26:00.936993Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"cited_work":{"arxiv_id":"2507.00410","doi":null,"metadata_source":"pith","pith_arxiv_id":"2507.00410","snapshot_observed_at":"2026-08-06T21:26:01.059838Z","title":"The Density Profile of Dynamical Halos","venue":"astro-ph.CO","work_id":"100d2771-f0cc-49ff-9766-71fd0a1fb3aa","year":2025},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.394741Z"},"links":{"cited_paper":"/paper/2507.00410","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:0dfc83cfe7cc801b75f49ca204b3b4a1ea29305d7752d65cc1f28c775d62f567","observation_id":"90cbff43-bfcf-47a1-85f9-ae360f31a6e8","resolution":{"observed_at":"2026-08-06T21:26:01.064856Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1401.1216","last_updated":"2014-06-10T02:18:11Z","snapshot_observed_at":"2026-07-06T03:32:35.866926Z","submitted_at":"2014-01-06T21:00:06Z","title":"Dependence of the outer density profiles of halos on their mass accretion rate","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.1216","snapshot_observed_at":"2026-08-06T21:26:00.438150Z","title":"Diemer and A","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.438150Z"},"links":{"cited_paper":"/paper/1401.1216","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:f907bdc3678971691444fa1af7ccb6d371bd13a358a681ed03df481af7b37f11","observation_id":"3d1e9580-2ceb-4a81-84e5-ce1a2a14478e","resolution":{"observed_at":"2026-08-06T21:26:00.438150Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1612.01531","last_updated":"2017-05-08T14:39:52Z","snapshot_observed_at":"2026-07-06T05:21:26.600622Z","submitted_at":"2016-12-05T21:00:03Z","title":"Splashback Shells of Cold Dark Matter Halos","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1612.01531","snapshot_observed_at":"2026-08-06T21:26:00.450520Z","title":"Mansfield, A","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.450520Z"},"links":{"cited_paper":"/paper/1612.01531","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:ef1a8322b2dc7fb2fdafc830599c5b003a5271410288cf3fa0f182e69a8c3002","observation_id":"c0db2737-24bf-434a-bc32-8fd656205328","resolution":{"observed_at":"2026-08-06T21:26:00.450520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.12751","last_updated":"2020-06-23T04:32:54Z","snapshot_observed_at":"2026-08-14T05:22:13.101379Z","submitted_at":"2020-06-23T04:32:54Z","title":"A Redefinition of the Halo Boundary Leads to a Simple yet Accurate Halo Model of Large Scale Structure","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.12751","snapshot_observed_at":"2026-08-06T21:26:00.455654Z","title":"Garc ´ ıa, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.455654Z"},"links":{"cited_paper":"/paper/2006.12751","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:6ffe89ff583c556976db57dfc2d5f6529b9408c1cf5e8583e9019dc7f10a58a5","observation_id":"fcb107cd-7691-410e-8d51-45b6bda09d64","resolution":{"observed_at":"2026-08-06T21:26:00.455654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:00.487702Z","title":"Springel, The cosmological simulation code GADGET-2, MNRAS 364, 1105 (2005), arXiv:astro- ph/0505010 [astro-ph]","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.487702Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:ddecb7a060253ddaf8b85f528a506366a2b04e27de7d83c8dbff3022c54d09b0","observation_id":"0933e9fd-c7bd-4bfd-8767-ffda67369cc3","resolution":{"observed_at":"2026-08-06T21:26:00.487702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.04054","last_updated":"2024-09-09T18:48:58Z","snapshot_observed_at":"2026-08-12T23:48:47.358147Z","submitted_at":"2024-06-06T13:20:54Z","title":"Dynamics-based halo model for large scale structure","version":2},"cited_work":{"arxiv_id":"2406.04054","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.04054","snapshot_observed_at":"2026-08-06T21:26:00.908096Z","title":"Dynamics-based halo model for large scale structure","venue":"astro-ph.CO","work_id":"8b88afb9-4c6a-43b1-8e45-21e76861bdaa","year":2024},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.466783Z"},"links":{"cited_paper":"/paper/2406.04054","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:9920507104966f79e5dc21adfa07da46482be8eb408b379286c6145bc8838aca","observation_id":"1b9773ea-a2e9-43f5-ae6f-1cfb146ba86c","resolution":{"observed_at":"2026-08-06T21:26:00.913835Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03921","last_updated":"2022-04-28T14:34:47Z","snapshot_observed_at":"2026-08-12T18:07:38.503357Z","submitted_at":"2021-12-07T19:00:00Z","title":"A dynamics-based density profile for dark haloes. I. Algorithm and basic results","version":2},"cited_work":{"arxiv_id":"2112.03921","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.03921","snapshot_observed_at":"2026-08-06T21:26:00.883029Z","title":"A dynamics-based density profile for dark haloes. I. Algorithm and basic results","venue":"astro-ph.CO","work_id":"b9880ab6-bfdd-42cd-9111-8c9983bf5726","year":2021},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.472440Z"},"links":{"cited_paper":"/paper/2112.03921","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:c179178cd04e337ea85ed5ba4bd55747e9e52702e4693d56ec0e24eee9d20cae","observation_id":"b5e2c8c7-b349-42fc-ba6e-a152e452ab9c","resolution":{"observed_at":"2026-08-06T21:26:00.889465Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.03420","last_updated":"2023-01-09T16:20:32Z","snapshot_observed_at":"2026-08-13T15:48:44.834988Z","submitted_at":"2022-05-06T18:00:01Z","title":"A dynamics-based density profile for dark haloes -- II. Fitting function","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.03420","snapshot_observed_at":"2026-08-06T21:26:00.477686Z","title":"Diemer, A dynamics-based density profile for dark haloes - II","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.477686Z"},"links":{"cited_paper":"/paper/2205.03420","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:97579a3a710ec6795a46355d7d1c52325be768cfe6ed62d573322b7153aff8dd","observation_id":"d6eabf66-9996-413c-a705-37ee0e043c80","resolution":{"observed_at":"2026-08-06T21:26:00.477686Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.139862Z","title":"read off","venue":null,"work_id":"595f0f1e-3201-4722-9658-20c29c6cfe74","year":null},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.418067Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:5e122d95c2fb631ce3abb148f07311e4e29b05c5068b7e28136be0ccaa93fd49","observation_id":"3ec9cda6-8f58-4cb1-a2bd-d60a38d8cdca","resolution":{"observed_at":"2026-08-06T21:26:01.144762Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05273","last_updated":"2021-08-16T01:22:46Z","snapshot_observed_at":"2026-08-13T05:50:31.580181Z","submitted_at":"2019-09-11T18:01:04Z","title":"The Quijote simulations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05273","snapshot_observed_at":"2026-08-06T21:26:00.482546Z","title":"Villaescusa-Navarro, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.482546Z"},"links":{"cited_paper":"/paper/1909.05273","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:2d045b3a1fc5f097a618514c8172176daa3f96e3ae1e09f150f297e685360f30","observation_id":"b694a51d-999d-4b21-8ee9-3e7ec67fc097","resolution":{"observed_at":"2026-08-06T21:26:00.482546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.108163Z","title":"Springel, N-GenIC: Cosmological structure initial conditions, Astrophysics Source Code Library, record ascl:1502.003 (2015)","venue":null,"work_id":"892ccf38-a753-4150-a093-f51c2aee14d6","year":2015},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.493031Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:86b1bdbceed618fb61b104e9f350e948418333cb4da9edf1d988cd9a99317dfb","observation_id":"a32c5db6-9a37-405a-a0c6-c685fc2d41f5","resolution":{"observed_at":"2026-08-06T21:26:01.113204Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.4372","last_updated":"2013-01-12T02:16:53Z","snapshot_observed_at":"2026-07-06T02:36:06.035370Z","submitted_at":"2011-10-19T20:00:04Z","title":"The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.4372","snapshot_observed_at":"2026-08-06T21:26:00.498376Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.498376Z"},"links":{"cited_paper":"/paper/1110.4372","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:04b08be10051b9aeecfbe826e6d9f04b4ab5ed5b17b72d83ed79cb188130cda4","observation_id":"106ee624-9fd2-4d04-a13d-43f73f33b237","resolution":{"observed_at":"2026-08-06T21:26:00.498376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0108151","last_updated":"2001-11-05T00:26:57Z","snapshot_observed_at":"2026-07-07T00:20:25.571880Z","submitted_at":"2001-08-09T21:27:45Z","title":"Concentrations of Dark Halos from their Assembly Histories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0108151","snapshot_observed_at":"2026-08-06T21:26:00.503695Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.503695Z"},"links":{"cited_paper":"/paper/astro-ph/0108151","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:861874bde3d4afaa9a0b253856d5a50739cb903123ec7d16db45eb8c790a2c01","observation_id":"13992247-8bb7-477c-9504-8f7b5731be80","resolution":{"observed_at":"2026-08-06T21:26:00.503695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.17324","last_updated":"2024-10-22T18:00:08Z","snapshot_observed_at":"2026-08-12T22:17:18.745417Z","submitted_at":"2024-10-22T18:00:08Z","title":"A dynamics-based density profile for dark haloes -- III. Parameter space","version":1},"cited_work":{"arxiv_id":"2410.17324","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.17324","snapshot_observed_at":"2026-08-06T21:26:00.723414Z","title":"A dynamics-based density profile for dark haloes -- III. Parameter space","venue":"astro-ph.CO","work_id":"fe91d99e-43ad-4061-8f17-191ed5d95640","year":2024},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.508590Z"},"links":{"cited_paper":"/paper/2410.17324","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:fcb75ccd69de42236ead338b591378c1e180212363685fba9a81de50b7904407","observation_id":"0e45456a-6b21-463f-95d6-75bde81298b9","resolution":{"observed_at":"2026-08-06T21:26:00.731245Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:00.513619Z","title":"Vladimir, C","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.513619Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:54a957c14d9dc6c5f7da99b17c6649a902d6de18f958857483c09b9c5b8aab92","observation_id":"018b5de4-f179-430c-9564-d84adb50175f","resolution":{"observed_at":"2026-08-06T21:26:00.513619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.091380Z","title":"Bertschinger, Self-similar secondary infall and ac- cretion in an Einstein-de Sitter universe, ApJS 58, 39 (1985)","venue":null,"work_id":"f71fda6e-fb3f-4169-854e-454179c32a9f","year":1985},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.517822Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:3023d50cece5909d9f1ca42429e8d75169385bc60e4913e13ce07825bdad2b2a","observation_id":"79176c18-fb65-4bc3-ac33-10b4e595ee14","resolution":{"observed_at":"2026-08-06T21:26:01.096637Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T21:26:01.075998Z","title":null,"venue":null,"work_id":"aa4a8d0f-1cd3-4fba-b7d3-ba4382d77b92","year":1984},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.522255Z"},"links":{"citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:f8b3a665b37c76b5cbf6fa5f5ce5a3b94f4d8cfd0f79fbe3dc2335d0c32e2705","observation_id":"1aef62de-7724-4fe2-97ff-48bfcbbc0726","resolution":{"observed_at":"2026-08-06T21:26:01.080733Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.01742","last_updated":"2016-06-13T19:19:35Z","snapshot_observed_at":"2026-07-06T04:48:27.018540Z","submitted_at":"2016-03-05T17:13:42Z","title":"The outer profile of dark matter halos: an analytical approach","version":2},"cited_work":{"arxiv_id":"1603.01742","doi":null,"metadata_source":"pith","pith_arxiv_id":"1603.01742","snapshot_observed_at":"2026-08-06T21:26:00.618519Z","title":"The outer profile of dark matter halos: an analytical approach","venue":"astro-ph.CO","work_id":"1c4d1209-6f7d-4ba5-ae9c-45c4c62e4ad0","year":2016},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.526770Z"},"links":{"cited_paper":"/paper/1603.01742","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:21a9992966a2d662202dd49e644576e82b8410ba82b8d5961e385fbf08b52de3","observation_id":"b72744d1-cd65-404b-931f-bc052512c74b","resolution":{"observed_at":"2026-08-06T21:26:00.623434Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.14262","last_updated":"2022-10-25T18:32:07Z","snapshot_observed_at":"2026-08-13T13:57:12.467470Z","submitted_at":"2022-10-25T18:32:07Z","title":"What sets the splashback radius of dark matter haloes: accretion history or other properties?","version":1},"cited_work":{"arxiv_id":"2210.14262","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.14262","snapshot_observed_at":"2026-08-06T21:26:00.592469Z","title":"What sets the splashback radius of dark matter haloes: accretion history or other properties?","venue":"astro-ph.CO","work_id":"b8cb3fb1-b3bf-439b-8151-de2003b5f02c","year":2022},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.531904Z"},"links":{"cited_paper":"/paper/2210.14262","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:2e2df8b75d418243a99999fb5b6ab31ccc89aa6baf9f5cd5d4bf3e7c21f35d2a","observation_id":"23d71a06-8503-46ca-a70c-57e70b462327","resolution":{"observed_at":"2026-08-06T21:26:00.600501Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1110.4370","last_updated":"2013-01-12T02:46:43Z","snapshot_observed_at":"2026-08-13T11:33:38.523205Z","submitted_at":"2011-10-19T20:00:03Z","title":"Gravitationally Consistent Halo Catalogs and Merger Trees for Precision Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.4370","snapshot_observed_at":"2026-08-06T21:26:00.536690Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T21:26:00.536690Z"},"links":{"cited_paper":"/paper/1110.4370","citing_paper":"/paper/2507.00410"},"observation_digest":"sha256:20f61bcce65354953491c60647c0e83d38f5e06fee15d6f8bf0bc16e01c1aa5c","observation_id":"5d4f7979-603d-4d09-b5f0-f12a9d11c222","resolution":{"observed_at":"2026-08-06T21:26:00.536690Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.00410","last_updated":"2026-07-09T17:36:47Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T21:27:51.048423Z","submitted_at":"2025-07-01T03:53:32Z","title":"The Density Profile of Dynamical Halos"},"reference_resolution":{"displayed":28,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":16,"verified_exact":7,"verified_fuzzy":5},"total_outbound_references":28},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 28 of 28 outbound references and 1 inbound Pith citation observation for arXiv:2507.00410."}