{"as_of":"2026-08-06T01:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:72cb26a396afc1d2933a7c2e87f21d8e1944cb2b9dfaf4e1c5e97914e6cb4fef","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-27T08:24:36.251007Z","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":"2026-07-03T13:08:08.951722Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.12157","last_updated":"2024-04-18T13:05:17Z","snapshot_observed_at":"2026-07-06T18:02:10.806722Z","submitted_at":"2024-04-18T13:05:17Z","title":"Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples","version":1},"cited_work":{"arxiv_id":"2404.12157","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.12157","snapshot_observed_at":"2026-07-03T13:08:08.951722Z","title":"Dournacet al.(Euclid), Astron","venue":null,"work_id":"bc107334-39d1-4916-bfda-004d9ab435db","year":2024},"citing_paper":{"arxiv_id":"2508.19106","last_updated":"2026-05-05T13:24:19Z","snapshot_observed_at":"2026-07-31T18:56:03.457219Z","submitted_at":"2025-08-26T15:10:00Z","title":"Tracing Signatures of Modified Gravity in Redshift-Space Galaxy Bispectrum Multipoles: Prospects for Euclid","version":3},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-05-18T21:27:09.201445Z"},"links":{"cited_paper":"/paper/2404.12157","citing_paper":"/paper/2508.19106"},"observation_digest":"sha256:31f6ba81c61c5b772d218b64ff09660e9fc5f62be9e00028bb158bf77b7f0da5","observation_id":"f42997d8-3f20-4127-ae00-6a63994757f6","resolution":{"observed_at":"2026-05-18T21:31:52.124282Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.12157","last_updated":"2024-04-18T13:05:17Z","snapshot_observed_at":"2026-07-06T18:02:10.806722Z","submitted_at":"2024-04-18T13:05:17Z","title":"Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples","version":1},"cited_work":{"arxiv_id":"2404.12157","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.12157","snapshot_observed_at":"2026-07-03T13:08:08.951722Z","title":"Dournacet al.(Euclid), Astron","venue":null,"work_id":"bc107334-39d1-4916-bfda-004d9ab435db","year":2024},"citing_paper":{"arxiv_id":"2606.12551","last_updated":"2026-06-10T18:02:40Z","snapshot_observed_at":"2026-07-06T23:51:27.152983Z","submitted_at":"2026-06-10T18:02:40Z","title":"Complex yet Hermitian: Gaussian covariance of cross-correlation and multi-tracer power spectra","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-06-27T08:24:36.251007Z"},"links":{"cited_paper":"/paper/2404.12157","citing_paper":"/paper/2606.12551"},"observation_digest":"sha256:d96e895ed8aedd0a343a6115b0c6aabdd7f8c58fdb0f641ee3602f2ae5449ac4","observation_id":"3998bbaa-9c90-4ede-8d6c-ad3ab267b1fd","resolution":{"observed_at":"2026-07-03T13:08:08.953431Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2404.12157/citation-record","integrity":"/paper/2404.12157/integrity","json":"/paper/2404.12157/citation-record.json","paper":"/paper/2404.12157"},"outbound":[],"paper":{"arxiv_id":"2404.12157","last_updated":"2024-04-18T13:05:17Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T18:02:10.806722Z","submitted_at":"2024-04-18T13:05:17Z","title":"Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2404.12157."}