{"as_of":"2026-08-18T21:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6401f201c940df58f7719b7fa64b5679e66e0fbd90ef1ddb6809e3c75ba854da","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":"2026-08-18T06:34:40.430872+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":"2026-08-11T14:22:05.116118Z","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":"2026-08-07T18:16:16.850658Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.06601","last_updated":"2021-02-24T09:53:32Z","snapshot_observed_at":"2026-08-07T00:15:20.667844Z","submitted_at":"2020-04-14T15:30:53Z","title":"Technical comment on the paper of Dessert et al. \"The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations\"","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.06601","snapshot_observed_at":"2026-08-11T14:22:05.116118Z","title":"Boyarsky, D","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12084","last_updated":"2024-12-16T18:55:12Z","snapshot_observed_at":"2026-08-18T12:54:46.001077Z","submitted_at":"2024-12-16T18:55:12Z","title":"DarkNESS: developing a skipper-CCD instrument to search for Dark Matter from Low Earth Orbit","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T14:22:05.116118Z"},"links":{"cited_paper":"/paper/2004.06601","citing_paper":"/paper/2412.12084"},"observation_digest":"sha256:439c3b6d7eb062ffc089b24bafe7f29cbd4a6741d27b665c348d4c1a3c065edf","observation_id":"8ed96dc9-b176-46d9-a443-f527f139316a","resolution":{"observed_at":"2026-08-11T14:22:05.116118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.06601","last_updated":"2021-02-24T09:53:32Z","snapshot_observed_at":"2026-08-07T00:15:20.667844Z","submitted_at":"2020-04-14T15:30:53Z","title":"Technical comment on the paper of Dessert et al. \"The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations\"","version":2},"cited_work":{"arxiv_id":"2004.06601","doi":"10.48550/arxiv.2004.06601","metadata_source":"pith","pith_arxiv_id":"2004.06601","snapshot_observed_at":"2026-08-07T18:16:16.850658Z","title":"Technical comment on the paper of Dessert et al. \"The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations\"","venue":"astro-ph.CO","work_id":"726263f0-a696-4fb8-99b9-c6f98e80e394","year":2020},"citing_paper":{"arxiv_id":"2505.16981","last_updated":"2025-05-22T17:52:52Z","snapshot_observed_at":"2026-08-18T12:54:41.309442Z","submitted_at":"2025-05-22T17:52:52Z","title":"DarkNESS: A skipper-CCD NanoSatellite for Dark Matter Searches","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T14:55:25.991607Z"},"links":{"cited_paper":"/paper/2004.06601","citing_paper":"/paper/2505.16981"},"observation_digest":"sha256:40923fe36bc62ae1b4f92e609041bb8fb574be6c1f7745e20219abdc3f85ff14","observation_id":"f4c93721-6a07-4bba-88fc-875d71223f60","resolution":{"observed_at":"2026-08-07T14:55:30.148365Z","resolver_source":"local_arxiv","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/2004.06601/citation-record","integrity":"/paper/2004.06601/integrity","json":"/paper/2004.06601/citation-record.json","paper":"/paper/2004.06601"},"outbound":[],"paper":{"arxiv_id":"2004.06601","last_updated":"2021-02-24T09:53:32Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T00:15:20.667844Z","submitted_at":"2020-04-14T15:30:53Z","title":"Technical comment on the paper of Dessert et al. \"The dark matter interpretation of the 3.5 keV line is inconsistent with blank-sky observations\""},"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 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2004.06601."}