{"as_of":"2026-08-22T00:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0aee78410b6383db4bc79847f75c99f69766bc71e5fe4efe62f4bf4dd00248c0","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:40:25.939906Z","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":"2026-05-12T08:06:30.307127Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.13114","last_updated":"2024-04-19T18:01:36Z","snapshot_observed_at":"2026-08-18T00:13:29.388520Z","submitted_at":"2024-04-19T18:01:36Z","title":"Cosmic-Ray Propagation Models Elucidate the Prospects for Antinuclei Detection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.13114","snapshot_observed_at":"2026-08-16T12:40:25.939906Z","title":"Cosmic-ray propagation models elucidate the prospects for antinuclei detection,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.12372","last_updated":"2025-04-16T18:00:00Z","snapshot_observed_at":"2026-08-19T19:36:24.103047Z","submitted_at":"2025-04-16T18:00:00Z","title":"dSphobic Dark Matter","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T12:40:25.939906Z"},"links":{"cited_paper":"/paper/2404.13114","citing_paper":"/paper/2504.12372"},"observation_digest":"sha256:bca0ce7c963785764a06ceb95eddf20081254f404b5a7dd614286c7c0cd43bb9","observation_id":"0facdd3e-badb-4205-8c3a-690b96d05627","resolution":{"observed_at":"2026-08-16T12:40:25.939906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.13114","last_updated":"2024-04-19T18:01:36Z","snapshot_observed_at":"2026-08-18T00:13:29.388520Z","submitted_at":"2024-04-19T18:01:36Z","title":"Cosmic-Ray Propagation Models Elucidate the Prospects for Antinuclei Detection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.13114","snapshot_observed_at":"2026-08-16T05:22:15.480365Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.20920","last_updated":"2025-04-29T16:37:08Z","snapshot_observed_at":"2026-08-20T13:45:08.955487Z","submitted_at":"2025-04-29T16:37:08Z","title":"Inelastic Antideutron Interaction with Nuclei","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-16T05:22:15.480365Z"},"links":{"cited_paper":"/paper/2404.13114","citing_paper":"/paper/2504.20920"},"observation_digest":"sha256:15e51ad7fabd9bd920c75066352d03a9d3d21d1164084bd84fbb3c2481c6753d","observation_id":"3817e097-ee82-4369-adee-7e0fc4995814","resolution":{"observed_at":"2026-08-16T05:22:15.480365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.13114","last_updated":"2024-04-19T18:01:36Z","snapshot_observed_at":"2026-08-18T00:13:29.388520Z","submitted_at":"2024-04-19T18:01:36Z","title":"Cosmic-Ray Propagation Models Elucidate the Prospects for Antinuclei Detection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.13114","snapshot_observed_at":"2026-08-15T22:42:56.710060Z","title":"De La Torre Luque, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.06734","last_updated":"2025-08-19T16:13:25Z","snapshot_observed_at":"2026-08-16T01:02:48.101430Z","submitted_at":"2025-05-10T18:57:37Z","title":"Searching for dark matter annihilation in the Sun with the IceCube Upgrade","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-15T22:42:56.710060Z"},"links":{"cited_paper":"/paper/2404.13114","citing_paper":"/paper/2505.06734"},"observation_digest":"sha256:83c9ac24bf8411d350d776a52e942b1e9802efb8728e8060742cf264e1485c1d","observation_id":"dd00364a-60df-4496-9971-7177a8904eb7","resolution":{"observed_at":"2026-08-15T22:42:56.710060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.13114","last_updated":"2024-04-19T18:01:36Z","snapshot_observed_at":"2026-08-18T00:13:29.388520Z","submitted_at":"2024-04-19T18:01:36Z","title":"Cosmic-Ray Propagation Models Elucidate the Prospects for Antinuclei Detection","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.13114","snapshot_observed_at":"2026-07-13T22:06:10.004220Z","title":"De La Torre Luque, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.19352","last_updated":"2026-06-03T13:05:18Z","snapshot_observed_at":"2026-08-14T10:45:18.296870Z","submitted_at":"2026-03-19T18:00:00Z","title":"Toward universal coalescence models for antideuteron production","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-13T22:06:10.004220Z"},"links":{"cited_paper":"/paper/2404.13114","citing_paper":"/paper/2603.19352"},"observation_digest":"sha256:f5397e5dad9dd5fda263e48cc92ddd6897bbfcb230c141bd6598000b39b6add5","observation_id":"893ec5a5-9865-4d2c-bfe9-eb4c788a5b0e","resolution":{"observed_at":"2026-07-13T22:06:10.004220Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.13114","last_updated":"2024-04-19T18:01:36Z","snapshot_observed_at":"2026-08-18T00:13:29.388520Z","submitted_at":"2024-04-19T18:01:36Z","title":"Cosmic-Ray Propagation Models Elucidate the Prospects for Antinuclei Detection","version":1},"cited_work":{"arxiv_id":"2404.13114","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.13114","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"De La Torre Luque, M","venue":null,"work_id":"43641df3-94f1-4439-aa79-3e6941e9ab94","year":2024},"citing_paper":{"arxiv_id":"2605.08338","last_updated":"2026-05-08T18:00:01Z","snapshot_observed_at":"2026-08-15T02:28:47.587284Z","submitted_at":"2026-05-08T18:00:01Z","title":"Revisiting predictions for cosmic-ray antinucleon fluxes from Galactic Dark Matter","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-12T01:17:32.186211Z"},"links":{"cited_paper":"/paper/2404.13114","citing_paper":"/paper/2605.08338"},"observation_digest":"sha256:c038234d00c3b531cd9568849e2af004470296c81534bd11695cafcbfaa1e4bc","observation_id":"72ab465d-a624-4776-8198-a20732d1567a","resolution":{"observed_at":"2026-05-12T08:06:30.310504Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2404.13114/citation-record","integrity":"/paper/2404.13114/integrity","json":"/paper/2404.13114/citation-record.json","paper":"/paper/2404.13114"},"outbound":[],"paper":{"arxiv_id":"2404.13114","last_updated":"2024-04-19T18:01:36Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-18T00:13:29.388520Z","submitted_at":"2024-04-19T18:01:36Z","title":"Cosmic-Ray Propagation Models Elucidate the Prospects for Antinuclei Detection"},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2404.13114."}