{"as_of":"2026-08-19T12:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:562dee39cbddc5933436fece677caebe5c5eaeb5ebaaef388168f065a649d166","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T10:52:33.766032Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2504.07187","last_updated":"2025-04-09T18:08:06Z","snapshot_observed_at":"2026-08-16T12:42:36.320510Z","submitted_at":"2025-04-09T18:08:06Z","title":"Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo","version":1},"cited_work":{"arxiv_id":"2504.07187","doi":"10.48550/arxiv.2504.07187","metadata_source":"arxiv_reference","pith_arxiv_id":"2504.07187","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2025, arXiv e-prints, arXiv:2504.07187, doi: 10.48550/arXiv.2504.07187","venue":"arXiv (Cornell University)","work_id":"81332cff-0129-47aa-b739-9b4f5d4e00f1","year":2025},"citing_paper":{"arxiv_id":"2508.02666","last_updated":"2026-04-07T16:46:22Z","snapshot_observed_at":"2026-08-11T11:44:20.490350Z","submitted_at":"2025-08-04T17:55:49Z","title":"Testing Dark Matter with Generative Models for Extragalactic Stellar Streams","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-19T00:32:58.118498Z"},"links":{"cited_paper":"/paper/2504.07187","citing_paper":"/paper/2508.02666"},"observation_digest":"sha256:27ec98557841195e3904712ac9b9b8f8be425a8ee9ae7392855e97e28404b0a2","observation_id":"af177216-ca32-434b-9cd4-0b9ac7785225","resolution":{"observed_at":"2026-05-19T00:36:56.079271Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07187","last_updated":"2025-04-09T18:08:06Z","snapshot_observed_at":"2026-08-16T12:42:36.320510Z","submitted_at":"2025-04-09T18:08:06Z","title":"Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07187","snapshot_observed_at":"2026-08-05T10:52:33.766032Z","title":"2025, arXiv e-prints, arXiv:2504.07187, doi: 10.48550/arXiv.2504.07187","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03599","last_updated":"2025-09-03T18:01:20Z","snapshot_observed_at":"2026-08-10T03:42:19.469435Z","submitted_at":"2025-09-03T18:01:20Z","title":"Breaking Down the $\\textsf{CosmoGEMS}$: Toward Modeling and Understanding Globular Cluster Stellar Streams in a Fully Cosmological Context","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-05T10:52:33.766032Z"},"links":{"cited_paper":"/paper/2504.07187","citing_paper":"/paper/2509.03599"},"observation_digest":"sha256:599bca05f1796611f4b4ce7e9800ae0072d7894e826211570437f1cddf258179","observation_id":"10db989b-684b-41cc-b158-ac38813a0e74","resolution":{"observed_at":"2026-08-05T10:52:33.766032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07187","last_updated":"2025-04-09T18:08:06Z","snapshot_observed_at":"2026-08-16T12:42:36.320510Z","submitted_at":"2025-04-09T18:08:06Z","title":"Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07187","snapshot_observed_at":"2026-08-02T21:27:58.359367Z","title":"Nibauer and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.20252","last_updated":"2026-07-13T09:34:03Z","snapshot_observed_at":"2026-08-07T18:44:54.025175Z","submitted_at":"2026-02-23T19:00:02Z","title":"Galactic Center gamma-ray excess from a generic triaxial halo","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-02T21:27:58.359367Z"},"links":{"cited_paper":"/paper/2504.07187","citing_paper":"/paper/2602.20252"},"observation_digest":"sha256:13ac12637a9d47558caf4d8ee82bc0ee765f39fc285edcd3d38525cfb0b15262","observation_id":"aac3dace-4efa-4f4d-980c-11bdff2f0ee1","resolution":{"observed_at":"2026-08-02T21:27:58.359367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07187","last_updated":"2025-04-09T18:08:06Z","snapshot_observed_at":"2026-08-16T12:42:36.320510Z","submitted_at":"2025-04-09T18:08:06Z","title":"Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07187","snapshot_observed_at":"2026-07-11T06:35:48.157333Z","title":", keywords =","venue":null,"work_id":null,"year":2041},"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":20,"source":"arxiv_source","source_observed_at":"2026-07-11T06:35:48.157333Z"},"links":{"cited_paper":"/paper/2504.07187","citing_paper":"/paper/2607.05510"},"observation_digest":"sha256:5aa77e59522dfb41023aef37851e6d0a41d69bc0280e927eaf01096ac80ac13e","observation_id":"0df6e24d-4a47-4f13-b4af-8226779f7add","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/2504.07187/citation-record","integrity":"/paper/2504.07187/integrity","json":"/paper/2504.07187/citation-record.json","paper":"/paper/2504.07187"},"outbound":[],"paper":{"arxiv_id":"2504.07187","last_updated":"2025-04-09T18:08:06Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T12:42:36.320510Z","submitted_at":"2025-04-09T18:08:06Z","title":"Galactic Accelerations from the GD-1 Stream Suggest a Tilted Dark Matter Halo"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2504.07187."}