{"as_of":"2026-08-15T09:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:68e4334975de00cf264a35d500841a9c56774488abc663278d0b60f914c1d53f","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":"2026-08-15T06:32:42.880941+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":"2026-08-11T10:53:42.106829Z","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":"2026-08-05T11:31:04.180846Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.04198","last_updated":"2025-02-28T10:56:59Z","snapshot_observed_at":"2026-08-13T09:31:08.257373Z","submitted_at":"2024-07-05T00:53:12Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04198","snapshot_observed_at":"2026-08-11T10:53:42.106829Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.16072","last_updated":"2026-07-11T06:25:29Z","snapshot_observed_at":"2026-08-14T12:04:23.846374Z","submitted_at":"2024-12-20T17:16:05Z","title":"Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T10:53:42.106829Z"},"links":{"cited_paper":"/paper/2407.04198","citing_paper":"/paper/2412.16072"},"observation_digest":"sha256:fb7931cc22f7ebc827eb6a31e5b11edf5697e884713701b3ad076515345ca529","observation_id":"ac8fb276-4eb9-4134-ad53-bffaf9a84009","resolution":{"observed_at":"2026-08-11T10:53:42.106829Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04198","last_updated":"2025-02-28T10:56:59Z","snapshot_observed_at":"2026-08-13T09:31:08.257373Z","submitted_at":"2024-07-05T00:53:12Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties","version":2},"cited_work":{"arxiv_id":"2407.04198","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.04198","snapshot_observed_at":"2026-08-05T11:31:04.180846Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties","venue":"astro-ph.CO","work_id":"b511c777-d046-4d2d-b5e4-79e3e111afac","year":2024},"citing_paper":{"arxiv_id":"2509.02781","last_updated":"2025-09-02T19:35:25Z","snapshot_observed_at":"2026-08-15T02:54:56.855076Z","submitted_at":"2025-09-02T19:35:25Z","title":"Updated bounds on ultra-light dark matter from the tiniest galaxies","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-05T11:31:04.023670Z"},"links":{"cited_paper":"/paper/2407.04198","citing_paper":"/paper/2509.02781"},"observation_digest":"sha256:abf5e6455ae61291457d97f7cb4afb73389ce6f1a6b00747ce803d049dc8a3b3","observation_id":"b93f648e-54c7-4335-93c3-f9f99c535467","resolution":{"observed_at":"2026-08-05T11:31:04.184136Z","resolver_source":"local_arxiv","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":"2407.04198","last_updated":"2025-02-28T10:56:59Z","snapshot_observed_at":"2026-08-13T09:31:08.257373Z","submitted_at":"2024-07-05T00:53:12Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04198","snapshot_observed_at":"2026-08-04T00:10:24.739538Z","title":"Dekker and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.02906","last_updated":"2026-07-13T21:59:28Z","snapshot_observed_at":"2026-08-10T13:18:25.502116Z","submitted_at":"2025-11-04T19:00:01Z","title":"Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-04T00:10:24.739538Z"},"links":{"cited_paper":"/paper/2407.04198","citing_paper":"/paper/2511.02906"},"observation_digest":"sha256:3ae7c5465a4f998fc41c7529fe71778e6e76a2a86b40bd5ebae94d6b77013d5b","observation_id":"f0b08ee0-9a6e-4e47-9256-518cab77ab21","resolution":{"observed_at":"2026-08-04T00:10:24.739538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04198","last_updated":"2025-02-28T10:56:59Z","snapshot_observed_at":"2026-08-13T09:31:08.257373Z","submitted_at":"2024-07-05T00:53:12Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04198","snapshot_observed_at":"2026-08-03T23:07:54.683329Z","title":"Dekker and A","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.07513","last_updated":"2026-07-01T19:58:59Z","snapshot_observed_at":"2026-08-14T04:46:41.279967Z","submitted_at":"2025-11-10T19:00:00Z","title":"JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios","version":5},"reference_index":158,"source":"pdf_text","source_observed_at":"2026-08-03T23:07:54.683329Z"},"links":{"cited_paper":"/paper/2407.04198","citing_paper":"/paper/2511.07513"},"observation_digest":"sha256:25e0bd0fdd35cbf82e900dbb3467782775f81cbb9e7d7921291ffc4856d77ac0","observation_id":"f483f93c-153f-42e2-ba8a-76647c38b72e","resolution":{"observed_at":"2026-08-03T23:07:54.683329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2407.04198/citation-record","integrity":"/paper/2407.04198/integrity","json":"/paper/2407.04198/citation-record.json","paper":"/paper/2407.04198"},"outbound":[],"paper":{"arxiv_id":"2407.04198","last_updated":"2025-02-28T10:56:59Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T09:31:08.257373Z","submitted_at":"2024-07-05T00:53:12Z","title":"Constraints on blue and red tilted primordial power spectra using dwarf galaxy properties"},"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 4 inbound Pith citation observations for arXiv:2407.04198."}