{"as_of":"2026-07-14T13:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:725734ed8de6983e0d9677229f6f0045f9917eb86b86e3077108b5a8504b2279","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":null,"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":"2026-07-02T10:01:27.867493Z","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":"2026-07-02T10:06:51.472603Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.00007","last_updated":"2019-07-31T18:00:00Z","snapshot_observed_at":"2026-07-05T01:14:27.025544Z","submitted_at":"2019-07-31T18:00:00Z","title":"Implications of BBN Bounds for Cosmic Ray Upscattered Dark Matter","version":1},"cited_work":{"arxiv_id":"1908.00007","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00007","snapshot_observed_at":"2026-07-02T10:06:51.472603Z","title":"Krnjaic and S","venue":null,"work_id":"006cbfe0-c37e-4521-a2a7-a291e890bca6","year":2020},"citing_paper":{"arxiv_id":"2602.04858","last_updated":"2026-06-23T09:20:24Z","snapshot_observed_at":"2026-06-26T23:13:37.264594Z","submitted_at":"2026-02-04T18:43:59Z","title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","version":2},"reference_index":107,"source":"pdf_text","source_observed_at":"2026-05-16T06:48:35.787193Z"},"links":{"cited_paper":"/paper/1908.00007","citing_paper":"/paper/2602.04858"},"observation_digest":"sha256:64f0e3f2ee94ed9db918e06c9b29f9db1e50419070c9b9fcc8dd579f0b6c96b6","observation_id":"07729248-950d-4931-8c4c-4d510c1f65e9","resolution":{"observed_at":"2026-05-16T06:50:42.592426Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"reason":"named_source_frontier_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00007","last_updated":"2019-07-31T18:00:00Z","snapshot_observed_at":"2026-07-05T01:14:27.025544Z","submitted_at":"2019-07-31T18:00:00Z","title":"Implications of BBN Bounds for Cosmic Ray Upscattered Dark Matter","version":1},"cited_work":{"arxiv_id":"1908.00007","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.00007","snapshot_observed_at":"2026-07-02T10:06:51.472603Z","title":"Krnjaic and S","venue":null,"work_id":"006cbfe0-c37e-4521-a2a7-a291e890bca6","year":2020},"citing_paper":{"arxiv_id":"2607.00840","last_updated":"2026-07-01T12:06:57Z","snapshot_observed_at":"2026-07-04T23:16:33.514596Z","submitted_at":"2026-07-01T12:06:57Z","title":"Dark matter energy exchange in stars orbiting supermassive black holes","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-02T10:01:27.867493Z"},"links":{"cited_paper":"/paper/1908.00007","citing_paper":"/paper/2607.00840"},"observation_digest":"sha256:5761e7bb2976794d11fd7415f64d01b5f74bff310dfec29ca2177a5e40f8b0c4","observation_id":"e7965915-8b39-440c-a0be-336e2686ec0b","resolution":{"observed_at":"2026-07-02T10:06:51.473960Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"reason":"named_source_frontier_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1908.00007/citation-record","integrity":"/paper/1908.00007/integrity","json":"/paper/1908.00007/citation-record.json","paper":"/paper/1908.00007"},"outbound":[],"paper":{"arxiv_id":"1908.00007","last_updated":"2019-07-31T18:00:00Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-07-05T01:14:27.025544Z","submitted_at":"2019-07-31T18:00:00Z","title":"Implications of BBN Bounds for Cosmic Ray Upscattered Dark Matter"},"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":[],"thesis":"As of 14 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1908.00007."}