{"as_of":"2026-08-15T23:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b9c8a9e39fbd66d74a1274f37dc4d72762c5d646ff77672f6e0907e568f05074","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T21:20:27.325562Z","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":"2026-07-03T06:57:42.804809Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-11T13:33:27.440803Z","title":"G., Kaplinghat , M., Valli , M., & Yu , H.-B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.13065","last_updated":"2025-06-14T15:47:10Z","snapshot_observed_at":"2026-08-14T13:03:28.626913Z","submitted_at":"2024-12-17T16:29:37Z","title":"COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions","version":2},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-11T13:33:27.440803Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2412.13065"},"observation_digest":"sha256:6054a546edb669d484c232e8b79b8fb6a9b3e2d1045daf6ef0941db1cbbdda37","observation_id":"eb91efc2-3649-402b-b3b6-92a163e4424b","resolution":{"observed_at":"2026-08-11T13:33:27.440803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":"2407.15005","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-07-03T06:57:42.804809Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","venue":null,"work_id":"422fd0c5-9118-4dcc-8751-10bf13bd64ea","year":2025},"citing_paper":{"arxiv_id":"2504.13004","last_updated":"2025-08-27T17:25:36Z","snapshot_observed_at":"2026-07-06T21:11:00.903522Z","submitted_at":"2025-04-17T15:14:35Z","title":"Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-22T19:28:30.312766Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2504.13004"},"observation_digest":"sha256:121d60840ab89ec6f7b1396a4a1b18253810923d9a5585b00ac10cd9fb2fdfbd","observation_id":"570f1282-0152-4436-886d-59284cd296f1","resolution":{"observed_at":"2026-05-22T19:32:00.842999Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-15T21:20:27.325562Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.10451","last_updated":"2025-05-15T16:08:57Z","snapshot_observed_at":"2026-08-15T21:06:34.417349Z","submitted_at":"2025-05-15T16:08:57Z","title":"Constraints on dark matter self-interaction from velocity distribution function in isolated halos","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-15T21:20:27.325562Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2505.10451"},"observation_digest":"sha256:9c80cd5da47daf6db1221dcca196a52047ce5b31c8687b00706283898b5b80ae","observation_id":"930f3517-a249-4a35-96cc-b431ab2dd3bd","resolution":{"observed_at":"2026-08-15T21:20:27.325562Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-07T13:11:59.168710Z","title":"G., Kaplinghat , M., Valli , M., & Yu , H.-B","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.22727","last_updated":"2025-06-17T18:38:05Z","snapshot_observed_at":"2026-08-14T16:57:42.082118Z","submitted_at":"2025-05-28T18:00:02Z","title":"The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass","version":3},"reference_index":202,"source":"arxiv_source","source_observed_at":"2026-08-07T13:11:59.168710Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2505.22727"},"observation_digest":"sha256:3e77518a3d3db4206dd2f0b85aa4d5b6b29bdacfd55b7d1244adeefa96d83300","observation_id":"305d3778-9c0c-4ee5-8628-048bc01dca3b","resolution":{"observed_at":"2026-08-07T13:11:59.168710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-05T14:45:20.943607Z","title":"Roberts, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.21121","last_updated":"2025-08-28T18:00:05Z","snapshot_observed_at":"2026-08-13T21:29:13.105232Z","submitted_at":"2025-08-28T18:00:05Z","title":"Pion dark matter in a $\\theta$ vacuum: a thermal relic with sharp velocity-dependent self-interactions","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-05T14:45:20.943607Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2508.21121"},"observation_digest":"sha256:038cea01655a4104ae6c37b76178a8eff0cf085f273ad58432bec95479608b2b","observation_id":"3fe548c2-ef0d-4e4c-b0fd-ebbe91f32ed8","resolution":{"observed_at":"2026-08-05T14:45:20.943607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-04T16:47:01.002112Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.11896","last_updated":"2025-09-15T13:12:07Z","snapshot_observed_at":"2026-08-07T22:36:48.250749Z","submitted_at":"2025-09-15T13:12:07Z","title":"Testing CCC+TL Cosmology with Galaxy Rotation Curves","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T16:47:01.002112Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2509.11896"},"observation_digest":"sha256:ced9face6ddbec59bd506717d7186c73fdc9a5e39ca6689ca2fb27fa52ed1f98","observation_id":"6415bedc-7876-46ac-bedb-b2dda20b4e0d","resolution":{"observed_at":"2026-08-04T16:47:01.002112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-04T12:56:22.582390Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.01491","last_updated":"2026-07-15T03:08:10Z","snapshot_observed_at":"2026-08-14T07:41:39.595176Z","submitted_at":"2025-10-01T22:06:50Z","title":"Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T12:56:22.582390Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2510.01491"},"observation_digest":"sha256:2cc498313b3c31a4170db484e1e83e9fa868619aac36b7c42674f60098a4ffa4","observation_id":"35d1fb10-365b-48a2-9917-403a0cd93a2f","resolution":{"observed_at":"2026-08-04T12:56:22.582390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":"2407.15005","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-07-03T06:57:42.804809Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","venue":null,"work_id":"422fd0c5-9118-4dcc-8751-10bf13bd64ea","year":2025},"citing_paper":{"arxiv_id":"2604.21168","last_updated":"2026-04-23T00:23:02Z","snapshot_observed_at":"2026-08-14T00:00:28.904755Z","submitted_at":"2026-04-23T00:23:02Z","title":"Neutron Portal and Dark Matter-Baryon Coincidence: from UV Completion to Phenomenology","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-09T22:12:43.021872Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2604.21168"},"observation_digest":"sha256:a1d6afb5e6a990cbab550cff98d82c983244b4ae63e128b58e2b16394f86bdc8","observation_id":"5ed9e0aa-2511-4f04-a319-b60ddfcfae31","resolution":{"observed_at":"2026-05-09T22:49:16.349032Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":"2407.15005","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-07-03T06:57:42.804809Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","venue":null,"work_id":"422fd0c5-9118-4dcc-8751-10bf13bd64ea","year":2025},"citing_paper":{"arxiv_id":"2605.24174","last_updated":"2026-05-22T19:48:35Z","snapshot_observed_at":"2026-08-12T21:20:37.102718Z","submitted_at":"2026-05-22T19:48:35Z","title":"The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-30T14:07:25.688498Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2605.24174"},"observation_digest":"sha256:c96468e14413d31e58b2e81d845954de646833277b22b6c40eaeaef6e405395e","observation_id":"253eac59-8949-4d4c-8da4-b5141e71d15b","resolution":{"observed_at":"2026-06-30T14:14:45.676351Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":"2407.15005","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-07-03T06:57:42.804809Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","venue":null,"work_id":"422fd0c5-9118-4dcc-8751-10bf13bd64ea","year":2025},"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":60,"source":"pdf_text","source_observed_at":"2026-06-28T20:58:05.796638Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2605.31335"},"observation_digest":"sha256:1db79d844a29d2e6be2de9ad1785585c838316f2dbb8b4c2a76df9f2f8e97dc9","observation_id":"ff0a03b0-86f9-4cbe-a831-fee91d04a5d2","resolution":{"observed_at":"2026-07-01T20:36:11.488131Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":"2407.15005","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-07-03T06:57:42.804809Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","venue":null,"work_id":"422fd0c5-9118-4dcc-8751-10bf13bd64ea","year":2025},"citing_paper":{"arxiv_id":"2607.02151","last_updated":"2026-07-02T13:26:31Z","snapshot_observed_at":"2026-08-06T16:24:28.071885Z","submitted_at":"2026-07-02T13:26:31Z","title":"Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-03T06:49:14.051341Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2607.02151"},"observation_digest":"sha256:ff2f7b2b15afe0e5fd93b288a210f124326bd5ef41dc72743e31c5b4b5ac1152","observation_id":"5fa0e2ae-8dca-4761-b01b-8f0c23732983","resolution":{"observed_at":"2026-07-03T06:57:42.806241Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-07-31T04:54:06.810000Z","title":"Roberts, M","venue":null,"work_id":null,"year":2025},"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":25,"source":"pdf_text","source_observed_at":"2026-07-31T04:54:06.810000Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2607.28517"},"observation_digest":"sha256:99f8f156987fd2edb2adc852f833339d54205ea92df69e13b56f6e455ef1cd02","observation_id":"fbfd7e58-de6a-4179-82cf-665618ec575b","resolution":{"observed_at":"2026-07-31T04:54:06.810000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15005","snapshot_observed_at":"2026-08-08T19:05:21.351271Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04362","last_updated":"2026-08-05T02:07:51Z","snapshot_observed_at":"2026-08-15T22:01:03.944492Z","submitted_at":"2026-08-05T02:07:51Z","title":"Cold Dark Matter and Self-Interacting Dark Matter Interpretations of Cloud-9","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-08T19:05:21.351271Z"},"links":{"cited_paper":"/paper/2407.15005","citing_paper":"/paper/2608.04362"},"observation_digest":"sha256:a5727605a6036a54e03e23f2d98de5c7ef5c70518b59ff8b0e50b82b117cf32c","observation_id":"edddeb75-b6a0-4828-9f72-4f5b53713357","resolution":{"observed_at":"2026-08-08T19:05:21.351271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.15005/citation-record","integrity":"/paper/2407.15005/integrity","json":"/paper/2407.15005/citation-record.json","paper":"/paper/2407.15005"},"outbound":[],"paper":{"arxiv_id":"2407.15005","last_updated":"2025-05-08T01:04:30Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-14T16:57:21.329651Z","submitted_at":"2024-07-20T23:19:16Z","title":"Gravothermal collapse and the diversity of galactic rotation curves"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2407.15005."}