{"as_of":"2026-08-24T01:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9720640f6ed14e42d6f1167022f4a5ee1efe4b62e2c19d54d693577034e1af60","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":"2026-08-23T06:30:58.430688+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":"2026-08-11T18:29:44.567837Z","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":"2026-07-01T14:35:47.781909Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2312.13979","last_updated":"2023-12-21T16:10:01Z","snapshot_observed_at":"2026-08-16T14:32:32.444869Z","submitted_at":"2023-12-21T16:10:01Z","title":"The effectiveness of exoplanets and Brown Dwarfs as sub-GeV Dark Matter detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.13979","snapshot_observed_at":"2026-08-11T18:29:44.567837Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.07953","last_updated":"2025-09-09T21:31:18Z","snapshot_observed_at":"2026-08-18T21:00:19.622423Z","submitted_at":"2024-12-10T22:40:32Z","title":"Constraining Asymmetric DM Properties by Black Hole Formation in Neutron Stars and Population III Stars","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T18:29:44.567837Z"},"links":{"cited_paper":"/paper/2312.13979","citing_paper":"/paper/2412.07953"},"observation_digest":"sha256:11b963bd9b5e9c23d6605907b5c6f143c3d3edca48ca5ff7cfdfcd89e41d7481","observation_id":"4428f774-ce35-4415-9988-61f4549ba7e5","resolution":{"observed_at":"2026-08-11T18:29:44.567837Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.13979","last_updated":"2023-12-21T16:10:01Z","snapshot_observed_at":"2026-08-16T14:32:32.444869Z","submitted_at":"2023-12-21T16:10:01Z","title":"The effectiveness of exoplanets and Brown Dwarfs as sub-GeV Dark Matter detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.13979","snapshot_observed_at":"2026-08-06T06:07:21.754531Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2508.00980","last_updated":"2026-06-25T17:23:36Z","snapshot_observed_at":"2026-08-13T17:02:58.785596Z","submitted_at":"2025-08-01T18:00:00Z","title":"Complementary Planetary Spectroscopy Probes of Dark Matter","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-06T06:07:21.754531Z"},"links":{"cited_paper":"/paper/2312.13979","citing_paper":"/paper/2508.00980"},"observation_digest":"sha256:e437a244a948259bfd4f1439790d6f05cfb24e2ec2921068521d0f6bdfb1b21f","observation_id":"215697a8-431a-4e76-8e0a-eaea9f0c864e","resolution":{"observed_at":"2026-08-06T06:07:21.754531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.13979","last_updated":"2023-12-21T16:10:01Z","snapshot_observed_at":"2026-08-16T14:32:32.444869Z","submitted_at":"2023-12-21T16:10:01Z","title":"The effectiveness of exoplanets and Brown Dwarfs as sub-GeV Dark Matter detectors","version":1},"cited_work":{"arxiv_id":"2312.13979","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.13979","snapshot_observed_at":"2026-07-01T14:35:47.781909Z","title":null,"venue":null,"work_id":"be72eb77-1ad0-4a38-bae8-cb04fdeb4d3e","year":2024},"citing_paper":{"arxiv_id":"2605.14887","last_updated":"2026-05-14T14:32:09Z","snapshot_observed_at":"2026-08-17T06:54:16.059031Z","submitted_at":"2026-05-14T14:32:09Z","title":"Self-Interacting Dark Matter in Brown Dwarfs","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-30T20:16:26.088576Z"},"links":{"cited_paper":"/paper/2312.13979","citing_paper":"/paper/2605.14887"},"observation_digest":"sha256:9d4bf847ac7346eeaaf1d944f6e4d5bf7b9f5ebf3d8fd77cbe1e9c755b30acd1","observation_id":"421d91e6-153e-4ed7-b631-42b271cf932b","resolution":{"observed_at":"2026-07-01T14:35:47.783555Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.13979","last_updated":"2023-12-21T16:10:01Z","snapshot_observed_at":"2026-08-16T14:32:32.444869Z","submitted_at":"2023-12-21T16:10:01Z","title":"The effectiveness of exoplanets and Brown Dwarfs as sub-GeV Dark Matter detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.13979","snapshot_observed_at":"2026-07-12T14:05:11.011544Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.14827","last_updated":"2026-07-09T09:33:51Z","snapshot_observed_at":"2026-08-22T14:42:20.516212Z","submitted_at":"2026-06-12T14:29:14Z","title":"Probing the fate of large primordial perturbations with exoplanets","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-12T14:05:11.011544Z"},"links":{"cited_paper":"/paper/2312.13979","citing_paper":"/paper/2606.14827"},"observation_digest":"sha256:c10e8d90e0098d6726bf34bafbd9b5b27d692f22751370504cc7d75a286690dc","observation_id":"e213cd31-6ff3-4bb6-8ed2-6a0473f4ca34","resolution":{"observed_at":"2026-07-12T14:05:11.011544Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2312.13979/citation-record","integrity":"/paper/2312.13979/integrity","json":"/paper/2312.13979/citation-record.json","paper":"/paper/2312.13979"},"outbound":[],"paper":{"arxiv_id":"2312.13979","last_updated":"2023-12-21T16:10:01Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T14:32:32.444869Z","submitted_at":"2023-12-21T16:10:01Z","title":"The effectiveness of exoplanets and Brown Dwarfs as sub-GeV Dark Matter detectors"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 24 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2312.13979."}