{"as_of":"2026-08-15T03:39:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:42b8220984e9abbdd07edca49e5f79a235a9dbe2b459c8655ea6be594361b3c5","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":"2026-08-14T06:32:32.682623+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":"2026-08-14T05:15:37.227932Z","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":"2026-07-03T06:47:43.667883Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1801.04251","last_updated":"2018-11-12T19:58:10Z","snapshot_observed_at":"2026-08-14T19:55:34.970019Z","submitted_at":"2018-01-12T17:56:19Z","title":"Testing (modified) gravity with 3D and tomographic cosmic shear","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04251","snapshot_observed_at":"2026-08-14T05:15:37.227932Z","title":"Testing (modiﬁed) gravity with 3D and tomographic cosmic shear,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1909.01828","last_updated":"2020-02-11T23:29:28Z","snapshot_observed_at":"2026-08-14T06:01:35.593562Z","submitted_at":"2019-09-04T14:17:51Z","title":"hi_class: Background Evolution, Initial Conditions and Approximation Schemes","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-14T05:15:37.227932Z"},"links":{"cited_paper":"/paper/1801.04251","citing_paper":"/paper/1909.01828"},"observation_digest":"sha256:2bcd0acdba98be2c9bdb865790e6c9b11eef12db68d92bce9cbb73dd1caeca5d","observation_id":"c52576a9-8547-4be4-9e59-b33e875a93ff","resolution":{"observed_at":"2026-08-14T05:15:37.227932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04251","last_updated":"2018-11-12T19:58:10Z","snapshot_observed_at":"2026-08-14T19:55:34.970019Z","submitted_at":"2018-01-12T17:56:19Z","title":"Testing (modified) gravity with 3D and tomographic cosmic shear","version":2},"cited_work":{"arxiv_id":"1801.04251","doi":null,"metadata_source":"pith","pith_arxiv_id":"1801.04251","snapshot_observed_at":"2026-07-03T06:47:43.667883Z","title":"Testing (modified) gravity with 3D and tomographic cosmic shear","venue":"astro-ph.CO","work_id":"0b02e928-e750-40e3-94a0-e1a83be778fe","year":2018},"citing_paper":{"arxiv_id":"2606.10597","last_updated":"2026-07-23T02:03:26Z","snapshot_observed_at":"2026-08-14T17:43:09.302589Z","submitted_at":"2026-06-09T09:01:21Z","title":"Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-27T12:26:46.137299Z"},"links":{"cited_paper":"/paper/1801.04251","citing_paper":"/paper/2606.10597"},"observation_digest":"sha256:44c192cab2c257e6332233f5614a26efa3dfbca6a00c8cc7d774db24e2cdfc10","observation_id":"d32c2132-05f9-48de-8e9e-9d49e27ece56","resolution":{"observed_at":"2026-07-03T06:47:43.669173Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04251","last_updated":"2018-11-12T19:58:10Z","snapshot_observed_at":"2026-08-14T19:55:34.970019Z","submitted_at":"2018-01-12T17:56:19Z","title":"Testing (modified) gravity with 3D and tomographic cosmic shear","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04251","snapshot_observed_at":"2026-08-02T11:57:24.453946Z","title":"Spurio Mancini, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2606.10597","last_updated":"2026-07-23T02:03:26Z","snapshot_observed_at":"2026-08-14T17:43:09.302589Z","submitted_at":"2026-06-09T09:01:21Z","title":"Synergy between the gravitational potential decay rate and other structure growth probes in testing gravity","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-02T11:57:24.453946Z"},"links":{"cited_paper":"/paper/1801.04251","citing_paper":"/paper/2606.10597"},"observation_digest":"sha256:39ada26094af71ac9dbb20becaa4981261da37e3dacd408557fe28f38a0d80b0","observation_id":"8a6712f5-ede7-48ec-9187-d0d70b35d391","resolution":{"observed_at":"2026-08-02T11:57:24.453946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1801.04251","last_updated":"2018-11-12T19:58:10Z","snapshot_observed_at":"2026-08-14T19:55:34.970019Z","submitted_at":"2018-01-12T17:56:19Z","title":"Testing (modified) gravity with 3D and tomographic cosmic shear","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1801.04251","snapshot_observed_at":"2026-07-31T14:40:34.601100Z","title":"Spurio Mancini, R","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.28207","last_updated":"2026-07-30T13:47:00Z","snapshot_observed_at":"2026-08-14T17:25:58.645577Z","submitted_at":"2026-07-30T13:47:00Z","title":"Signatures of kinetic gravity braiding in cosmological probes of the gravitational field","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-31T14:40:34.601100Z"},"links":{"cited_paper":"/paper/1801.04251","citing_paper":"/paper/2607.28207"},"observation_digest":"sha256:90986e2e21d26c2c4be517fb478b7f23ea93010cdce2dca68416c9d5c438033e","observation_id":"ce56c46e-9fce-4a45-bb47-d4fb5a82e4c9","resolution":{"observed_at":"2026-07-31T14:40:34.601100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1801.04251/citation-record","integrity":"/paper/1801.04251/integrity","json":"/paper/1801.04251/citation-record.json","paper":"/paper/1801.04251"},"outbound":[],"paper":{"arxiv_id":"1801.04251","last_updated":"2018-11-12T19:58:10Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T19:55:34.970019Z","submitted_at":"2018-01-12T17:56:19Z","title":"Testing (modified) gravity with 3D and tomographic cosmic shear"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1801.04251."}