{"as_of":"2026-08-19T05:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ddf373694a4271ee2c91f45fcafbcf1c364d10fe8be9b15c74e87d5164f7e5df","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":"2026-08-18T06:34:40.430872+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":"2026-08-15T16:39:05.493535Z","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":"2026-07-03T08:07:45.184892Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2002.10481","last_updated":"2020-07-08T06:41:27Z","snapshot_observed_at":"2026-08-18T22:25:35.625914Z","submitted_at":"2020-02-24T19:06:36Z","title":"Revisiting cosmic ray antinuclei fluxes with a new coalescence model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.10481","snapshot_observed_at":"2026-08-15T16:39:05.493535Z","title":"Kachelrieß, S","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2509.03195","last_updated":"2025-10-03T13:38:22Z","snapshot_observed_at":"2026-08-17T16:32:54.209646Z","submitted_at":"2025-09-03T10:28:47Z","title":"Confronting the production mechanisms of nuclei with deuteron and proton-triggered balance functions","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T16:39:05.493535Z"},"links":{"cited_paper":"/paper/2002.10481","citing_paper":"/paper/2509.03195"},"observation_digest":"sha256:af36dc61e4487c1050a20db8929f1576a9b43cfa2634ac296ecc1c4ba5057f2e","observation_id":"303055b6-ba48-474c-aba4-7e6515ad25d5","resolution":{"observed_at":"2026-08-15T16:39:05.493535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.10481","last_updated":"2020-07-08T06:41:27Z","snapshot_observed_at":"2026-08-18T22:25:35.625914Z","submitted_at":"2020-02-24T19:06:36Z","title":"Revisiting cosmic ray antinuclei fluxes with a new coalescence model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.10481","snapshot_observed_at":"2026-07-13T22:06:10.004220Z","title":"Kachelrieß, S","venue":null,"work_id":null,"year":2020},"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":9,"source":"pdf_text","source_observed_at":"2026-07-13T22:06:10.004220Z"},"links":{"cited_paper":"/paper/2002.10481","citing_paper":"/paper/2603.19352"},"observation_digest":"sha256:07b609d7dc369d864eafdcae40b7093ea70df55c37fd388e8d4f47842844bab3","observation_id":"7472f5ca-97c5-4bb8-b334-ae21cd5f8af8","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":"2002.10481","last_updated":"2020-07-08T06:41:27Z","snapshot_observed_at":"2026-08-18T22:25:35.625914Z","submitted_at":"2020-02-24T19:06:36Z","title":"Revisiting cosmic ray antinuclei fluxes with a new coalescence model","version":2},"cited_work":{"arxiv_id":"2002.10481","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.10481","snapshot_observed_at":"2026-07-03T08:07:45.184892Z","title":"Kachelrieß, S","venue":null,"work_id":"fcc70d20-91aa-4656-9ce1-c3c7f18ba090","year":2002},"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":27,"source":"pdf_text","source_observed_at":"2026-05-12T01:17:32.186211Z"},"links":{"cited_paper":"/paper/2002.10481","citing_paper":"/paper/2605.08338"},"observation_digest":"sha256:382e385fda72276092cb4201a2ff9930032b0768ea799a8edc1a13d49ac8ca85","observation_id":"86da03ef-0b53-4e73-9a4b-c087c17ec669","resolution":{"observed_at":"2026-05-12T08:06:29.778864Z","resolver_source":"arxiv_id","status":"verified_exact"},"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":"2002.10481","last_updated":"2020-07-08T06:41:27Z","snapshot_observed_at":"2026-08-18T22:25:35.625914Z","submitted_at":"2020-02-24T19:06:36Z","title":"Revisiting cosmic ray antinuclei fluxes with a new coalescence model","version":2},"cited_work":{"arxiv_id":"2002.10481","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.10481","snapshot_observed_at":"2026-07-03T08:07:45.184892Z","title":"Kachelrieß, S","venue":null,"work_id":"fcc70d20-91aa-4656-9ce1-c3c7f18ba090","year":2002},"citing_paper":{"arxiv_id":"2606.10668","last_updated":"2026-06-09T10:19:24Z","snapshot_observed_at":"2026-08-14T10:12:31.388721Z","submitted_at":"2026-06-09T10:19:24Z","title":"$\\Lambda$(1520) as a probe of resonance-driven deuteron formation at the LHC","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-27T11:09:03.376163Z"},"links":{"cited_paper":"/paper/2002.10481","citing_paper":"/paper/2606.10668"},"observation_digest":"sha256:a082c44c5f2efb3a962e8ef8e1d2401b1d3c51a5f6a87b1bbc48228365112dfd","observation_id":"dfa4ad25-0f33-4a9b-a58e-78a7d40ef13e","resolution":{"observed_at":"2026-07-03T08:07:45.186512Z","resolver_source":"arxiv_id","status":"verified_exact"},"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"}}],"links":{"evidence":"/evidence","html":"/paper/2002.10481/citation-record","integrity":"/paper/2002.10481/integrity","json":"/paper/2002.10481/citation-record.json","paper":"/paper/2002.10481"},"outbound":[],"paper":{"arxiv_id":"2002.10481","last_updated":"2020-07-08T06:41:27Z","latest_version":2,"primary_category":"hep-ph","snapshot_observed_at":"2026-08-18T22:25:35.625914Z","submitted_at":"2020-02-24T19:06:36Z","title":"Revisiting cosmic ray antinuclei fluxes with a new coalescence model"},"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 4 inbound Pith citation observations for arXiv:2002.10481."}