{"as_of":"2026-08-08T21:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0d653371c795b70fb72d5c681f63db25e6c3f18886fdec4ada98bee8bc0c98da","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T10:51:09.576227Z","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":"2026-07-10T18:27:31.497997Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","snapshot_observed_at":"2026-08-07T04:19:36.513613Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.06434","snapshot_observed_at":"2026-08-07T10:51:09.576227Z","title":"Tutusaus, C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.04387","last_updated":"2025-06-04T19:07:40Z","snapshot_observed_at":"2026-08-08T20:39:30.594065Z","submitted_at":"2025-06-04T19:07:40Z","title":"A novel test of gravity: Does spacetime geometry track matter density?","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T10:51:09.576227Z"},"links":{"cited_paper":"/paper/2312.06434","citing_paper":"/paper/2506.04387"},"observation_digest":"sha256:683c49b8876ef948349f85a008f275fb0b701c74f1513033214e5927776df6ef","observation_id":"32ba5cc5-e529-4f1a-912b-fb163e241753","resolution":{"observed_at":"2026-08-07T10:51:09.576227Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","snapshot_observed_at":"2026-08-07T04:19:36.513613Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.06434","snapshot_observed_at":"2026-08-06T01:02:54.244101Z","title":"Tutusaus, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-08T06:19:06.452226Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":136,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:54.244101Z"},"links":{"cited_paper":"/paper/2312.06434","citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:f925f4d6cb2b0ca22a9fe6479118a57ba791ece3ca56b29a88d7076e9d3697df","observation_id":"0e19f10f-04a5-4675-97bd-62bf6d2593ef","resolution":{"observed_at":"2026-08-06T01:02:54.244101Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","snapshot_observed_at":"2026-08-07T04:19:36.513613Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data","version":2},"cited_work":{"arxiv_id":"2312.06434","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.06434","snapshot_observed_at":"2026-07-10T18:27:31.497997Z","title":"Tutusaus, C","venue":"astro-ph.CO","work_id":"90ae291c-482d-48d4-8420-a8c035eba15b","year":2023},"citing_paper":{"arxiv_id":"2605.22599","last_updated":"2026-05-21T15:14:45Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-21T15:14:45Z","title":"The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-22T03:48:48.036434Z"},"links":{"cited_paper":"/paper/2312.06434","citing_paper":"/paper/2605.22599"},"observation_digest":"sha256:5464604cb7bd0ce92f34e5a59419449be28bee795c0e6d0f943911682ef81dd4","observation_id":"b8d3f918-3d54-4c1f-8969-b68e81721834","resolution":{"observed_at":"2026-05-22T03:51:01.812862Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","snapshot_observed_at":"2026-08-07T04:19:36.513613Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data","version":2},"cited_work":{"arxiv_id":"2312.06434","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.06434","snapshot_observed_at":"2026-07-10T18:27:31.497997Z","title":"Tutusaus, C","venue":"astro-ph.CO","work_id":"90ae291c-482d-48d4-8420-a8c035eba15b","year":2023},"citing_paper":{"arxiv_id":"2606.31977","last_updated":"2026-06-30T17:17:50Z","snapshot_observed_at":"2026-08-02T18:59:37.715063Z","submitted_at":"2026-06-30T17:17:50Z","title":"Constraining dark energy with complementary probes of large-scale structure","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-07-01T03:37:13.804621Z"},"links":{"cited_paper":"/paper/2312.06434","citing_paper":"/paper/2606.31977"},"observation_digest":"sha256:ff5824ec3f8aa3536d85fefe1dd57dbc0f0d1adc35f033f4b41c8ae9e89444a1","observation_id":"ae021971-53c8-4d1a-9885-80b7c15d8c86","resolution":{"observed_at":"2026-07-01T11:55:42.842753Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","snapshot_observed_at":"2026-08-07T04:19:36.513613Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data","version":2},"cited_work":{"arxiv_id":"2312.06434","doi":null,"metadata_source":"pith","pith_arxiv_id":"2312.06434","snapshot_observed_at":"2026-07-10T18:27:31.497997Z","title":"Tutusaus, C","venue":"astro-ph.CO","work_id":"90ae291c-482d-48d4-8420-a8c035eba15b","year":2023},"citing_paper":{"arxiv_id":"2607.07777","last_updated":"2026-07-08T17:38:46Z","snapshot_observed_at":"2026-08-05T11:19:33.253012Z","submitted_at":"2026-07-08T17:38:46Z","title":"The Status of Single Scalar Field Dark Energy","version":1},"reference_index":206,"source":"pdf_text","source_observed_at":"2026-07-10T18:19:17.740185Z"},"links":{"cited_paper":"/paper/2312.06434","citing_paper":"/paper/2607.07777"},"observation_digest":"sha256:aa0a88fc923d6cab3877b1b9e411701db3e176915ec67345b9145910d6b82039","observation_id":"fa527b4b-5f46-4bbb-b562-7390372a61e2","resolution":{"observed_at":"2026-07-10T18:27:31.499447Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2312.06434/citation-record","integrity":"/paper/2312.06434/integrity","json":"/paper/2312.06434/citation-record.json","paper":"/paper/2312.06434"},"outbound":[],"paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T04:19:36.513613Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2312.06434."}