{"as_of":"2026-08-19T03:52:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bcf2d3484f97ef9bb29ce9a7d0aa9d2d1b345f46bf6f7022eafabbe7f88b47a7","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:27:08.459192Z","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":"2026-07-01T11:05:42.053052Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"0707.0737","last_updated":"2008-06-13T01:18:29Z","snapshot_observed_at":"2026-08-16T22:51:15.887701Z","submitted_at":"2007-07-05T08:53:22Z","title":"The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.0737","snapshot_observed_at":"2026-08-11T04:27:08.459192Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.18880","last_updated":"2025-07-28T13:23:47Z","snapshot_observed_at":"2026-08-18T08:50:14.263060Z","submitted_at":"2024-12-25T11:39:21Z","title":"Variable gravitational potential of Milky Way analogues in HESTIA suite","version":2},"reference_index":1088,"source":"pdf_text","source_observed_at":"2026-08-11T04:27:08.459192Z"},"links":{"cited_paper":"/paper/0707.0737","citing_paper":"/paper/2412.18880"},"observation_digest":"sha256:63410eb37dbce756b08b1c9e84d74adc7c8647dd87cc3eff6a859f2ef0d2b7f8","observation_id":"d98edaf0-d8dc-4a65-b4a4-0022bad59ae5","resolution":{"observed_at":"2026-08-11T04:27:08.459192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0707.0737","last_updated":"2008-06-13T01:18:29Z","snapshot_observed_at":"2026-08-16T22:51:15.887701Z","submitted_at":"2007-07-05T08:53:22Z","title":"The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures","version":2},"cited_work":{"arxiv_id":"0707.0737","doi":null,"metadata_source":"pith","pith_arxiv_id":"0707.0737","snapshot_observed_at":"2026-07-01T11:05:42.053052Z","title":"The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures","venue":"astro-ph","work_id":"566e4c1d-e7d6-4071-8436-c9f9c317a5f3","year":2007},"citing_paper":{"arxiv_id":"2606.31434","last_updated":"2026-06-30T10:03:04Z","snapshot_observed_at":"2026-08-15T04:35:13.248103Z","submitted_at":"2026-06-30T10:03:04Z","title":"Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-07-01T04:45:13.319437Z"},"links":{"cited_paper":"/paper/0707.0737","citing_paper":"/paper/2606.31434"},"observation_digest":"sha256:207eed60c9fec9dc1561819a6bfe968fe26606bcfe3ba67f9bdc6b417dd1e2d9","observation_id":"d0a66191-ddaf-4043-8b4a-699513f01c22","resolution":{"observed_at":"2026-07-01T11:05:42.054465Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0707.0737","last_updated":"2008-06-13T01:18:29Z","snapshot_observed_at":"2026-08-16T22:51:15.887701Z","submitted_at":"2007-07-05T08:53:22Z","title":"The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0707.0737","snapshot_observed_at":"2026-07-11T06:35:48.157333Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05510","last_updated":"2026-07-06T18:00:04Z","snapshot_observed_at":"2026-08-06T10:32:42.332283Z","submitted_at":"2026-07-06T18:00:04Z","title":"Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams","version":1},"reference_index":161,"source":"arxiv_source","source_observed_at":"2026-07-11T06:35:48.157333Z"},"links":{"cited_paper":"/paper/0707.0737","citing_paper":"/paper/2607.05510"},"observation_digest":"sha256:0c57122908a06ce787cee91541ecb1b6462d9ce3fda8945cc032df7666099306","observation_id":"c4d07668-ef99-4ae9-96f8-6b0c9ea22c60","resolution":{"observed_at":"2026-07-11T06:35:48.157333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/0707.0737/citation-record","integrity":"/paper/0707.0737/integrity","json":"/paper/0707.0737/citation-record.json","paper":"/paper/0707.0737"},"outbound":[],"paper":{"arxiv_id":"0707.0737","last_updated":"2008-06-13T01:18:29Z","latest_version":2,"primary_category":"astro-ph","snapshot_observed_at":"2026-08-16T22:51:15.887701Z","submitted_at":"2007-07-05T08:53:22Z","title":"The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0707.0737."}