{"as_of":"2026-08-12T10:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3e83bde6b52642a945455c69fab5060775ba435864e4f6f2b18aec8b817d3cdc","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":"2026-08-12T06:34:41.77262+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":"2026-08-11T14:28:26.447738Z","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":"2026-05-14T21:04:03.422085Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1703.10180","last_updated":"2017-10-02T01:15:04Z","snapshot_observed_at":"2026-07-06T05:35:45.732137Z","submitted_at":"2017-03-29T18:07:43Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10180","snapshot_observed_at":"2026-08-11T14:28:26.447738Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.12012","last_updated":"2024-12-16T17:37:49Z","snapshot_observed_at":"2026-08-11T20:25:12.223316Z","submitted_at":"2024-12-16T17:37:49Z","title":"Fuzzy Axions and Associated Relics","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T14:28:26.447738Z"},"links":{"cited_paper":"/paper/1703.10180","citing_paper":"/paper/2412.12012"},"observation_digest":"sha256:8b2e2b40e9b6186b8b0299672a561949b2e29803ee73a543a8369ecd24c73d68","observation_id":"0d8b4061-b91d-4fc2-980a-640e1337248b","resolution":{"observed_at":"2026-08-11T14:28:26.447738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10180","last_updated":"2017-10-02T01:15:04Z","snapshot_observed_at":"2026-07-06T05:35:45.732137Z","submitted_at":"2017-03-29T18:07:43Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.10180","snapshot_observed_at":"2026-08-11T11:38:58.908107Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.15192","last_updated":"2026-07-24T03:29:13Z","snapshot_observed_at":"2026-08-11T11:31:00.867228Z","submitted_at":"2024-12-19T18:57:34Z","title":"Accurate method for ultralight axion CMB and matter power spectra","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T11:38:58.908107Z"},"links":{"cited_paper":"/paper/1703.10180","citing_paper":"/paper/2412.15192"},"observation_digest":"sha256:cc7c8385e7d965537fa35a4e66b9eb9bf5e8d1bf01039df066177b280dfea3a3","observation_id":"57ff70be-7406-4e01-8167-077a0f4a13eb","resolution":{"observed_at":"2026-08-11T11:38:58.908107Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10180","last_updated":"2017-10-02T01:15:04Z","snapshot_observed_at":"2026-07-06T05:35:45.732137Z","submitted_at":"2017-03-29T18:07:43Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential","version":3},"cited_work":{"arxiv_id":"1703.10180","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.10180","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential","venue":"gr-qc","work_id":"8df3d98b-25da-425c-bef3-06c310af7bfd","year":2017},"citing_paper":{"arxiv_id":"2503.14743","last_updated":"2025-04-03T13:50:59Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:17Z","title":"Extended Dark Energy analysis using DESI DR2 BAO measurements","version":2},"reference_index":231,"source":"pdf_text","source_observed_at":"2026-05-14T21:04:02.994288Z"},"links":{"cited_paper":"/paper/1703.10180","citing_paper":"/paper/2503.14743"},"observation_digest":"sha256:1ec7f015e2a88244a1d30d4308a0e908d7b08fdd683095ce9d7851544e6d8516","observation_id":"7dc2d567-ba0f-4d98-94df-df99e2fd3f66","resolution":{"observed_at":"2026-05-14T21:04:03.423943Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.10180","last_updated":"2017-10-02T01:15:04Z","snapshot_observed_at":"2026-07-06T05:35:45.732137Z","submitted_at":"2017-03-29T18:07:43Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential","version":3},"cited_work":{"arxiv_id":"1703.10180","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.10180","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential","venue":"gr-qc","work_id":"8df3d98b-25da-425c-bef3-06c310af7bfd","year":2017},"citing_paper":{"arxiv_id":"2604.09141","last_updated":"2026-04-10T09:20:28Z","snapshot_observed_at":"2026-07-06T22:58:04.106299Z","submitted_at":"2026-04-10T09:20:28Z","title":"Bounding axion dark energy","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-05-10T17:16:44.930430Z"},"links":{"cited_paper":"/paper/1703.10180","citing_paper":"/paper/2604.09141"},"observation_digest":"sha256:50396205ecf827bd0452ba4e6f1835cb8a16d3033b1a42cffd1e1d4ecb78ea44","observation_id":"451f21f4-00f6-4ed0-897c-eeed5e479c60","resolution":{"observed_at":"2026-05-11T07:10:58.453137Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1703.10180/citation-record","integrity":"/paper/1703.10180/integrity","json":"/paper/1703.10180/citation-record.json","paper":"/paper/1703.10180"},"outbound":[],"paper":{"arxiv_id":"1703.10180","last_updated":"2017-10-02T01:15:04Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T05:35:45.732137Z","submitted_at":"2017-03-29T18:07:43Z","title":"Cosmological signatures of ultralight dark matter with an axionlike potential"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1703.10180."}