{"as_of":"2026-08-14T06:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3fd45ca29ef4bbbc1245a38e385f982a2dd1e1b78db572a63092ffa716c9055c","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T14:44:52.170478Z","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":"2026-07-01T11:55:42.795646Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-08-09T14:44:52.170478Z","title":"Carron, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.01751","last_updated":"2025-02-03T19:00:22Z","snapshot_observed_at":"2026-08-10T10:43:36.116218Z","submitted_at":"2025-02-03T19:00:22Z","title":"Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-09T14:44:52.170478Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2502.01751"},"observation_digest":"sha256:d46832f50c6545b1fcbf6e7c29def6fdcfe99638f3d4872e83db816305752683","observation_id":"205a4005-f54e-437e-a6cd-aace40b5d84e","resolution":{"observed_at":"2026-08-09T14:44:52.170478Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-08-03T20:12:23.305511Z","title":"Carron, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-08T22:41:12.425390Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.305511Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:c9d27322ae52dbb92e2306bd556cec67f2574bbe45f181d8350b38753ad7063b","observation_id":"b9006dac-69e9-4f3d-80fc-0cd7cf29ce19","resolution":{"observed_at":"2026-08-03T20:12:23.305511Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-08-03T18:35:00.450104Z","title":"Carron, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.05401","last_updated":"2026-07-25T18:57:19Z","snapshot_observed_at":"2026-08-04T00:50:50.770057Z","submitted_at":"2025-12-05T03:43:30Z","title":"The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-03T18:35:00.450104Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2512.05401"},"observation_digest":"sha256:5d2e054796863b43b81aac445c5d039421618c620aa8c7f75276962772267725","observation_id":"a5a994d9-7e75-4735-8e80-b73d6cd87c3c","resolution":{"observed_at":"2026-08-03T18:35:00.450104Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-08-03T17:24:59.347632Z","title":"Carron, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.09991","last_updated":"2026-06-01T10:52:35Z","snapshot_observed_at":"2026-08-14T00:06:22.195087Z","submitted_at":"2025-12-10T19:00:02Z","title":"Observational constraints on 3-forms dark energy","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-03T17:24:59.347632Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2512.09991"},"observation_digest":"sha256:8eb79fc6fc2fd1fe69d9707905f06d6bdcdf1abb7072c1ac6ff93d8031862c1b","observation_id":"1e96143f-0462-4529-933b-f61e3f596a15","resolution":{"observed_at":"2026-08-03T17:24:59.347632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":"2209.07395","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-07-01T11:55:42.795646Z","title":"Carron, A","venue":null,"work_id":"081a94e9-ef30-483e-993d-d46dd2d10aa5","year":2022},"citing_paper":{"arxiv_id":"2603.10787","last_updated":"2026-03-11T14:00:06Z","snapshot_observed_at":"2026-08-11T15:40:03.224454Z","submitted_at":"2026-03-11T14:00:06Z","title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","version":1},"reference_index":194,"source":"pdf_text","source_observed_at":"2026-05-15T13:14:03.491513Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2603.10787"},"observation_digest":"sha256:a95f9a84af3af70ae8eeacb36f64af7019d0bd88461b29a686596f4612f1777d","observation_id":"2ead5c37-10dc-4c65-a717-9ca400bd3427","resolution":{"observed_at":"2026-05-15T13:15:49.970970Z","resolver_source":"arxiv_id","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":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":"2209.07395","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-07-01T11:55:42.795646Z","title":"Carron, A","venue":null,"work_id":"081a94e9-ef30-483e-993d-d46dd2d10aa5","year":2022},"citing_paper":{"arxiv_id":"2606.00411","last_updated":"2026-05-29T23:05:25Z","snapshot_observed_at":"2026-08-10T17:21:07.504594Z","submitted_at":"2026-05-29T23:05:25Z","title":"The sound of dynamical dark energy and modified gravity","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-06-28T20:48:00.755241Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2606.00411"},"observation_digest":"sha256:c50697d5f7f5e93879c0dc630e17e7bf43d4ba3264785ef847f986effef8c96d","observation_id":"d02f8652-94ef-4023-a281-aebe385c6d26","resolution":{"observed_at":"2026-06-28T20:52:37.661907Z","resolver_source":"arxiv_id","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":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":"2209.07395","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-07-01T11:55:42.795646Z","title":"Carron, A","venue":null,"work_id":"081a94e9-ef30-483e-993d-d46dd2d10aa5","year":2022},"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":7,"source":"pdf_text","source_observed_at":"2026-07-01T03:37:13.804621Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2606.31977"},"observation_digest":"sha256:709a7f77cd337d508b46c14338bf2d3bff282ed2cf970f27dc42fd040b6c9b9c","observation_id":"0aa4fdf5-a025-4f4b-9b9b-0711aaa64741","resolution":{"observed_at":"2026-07-01T11:55:42.797634Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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":"2209.07395","last_updated":"2022-10-07T13:02:48Z","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.07395","snapshot_observed_at":"2026-07-31T05:27:07.674082Z","title":"and Lewis, A","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.24940","last_updated":"2026-07-27T18:00:27Z","snapshot_observed_at":"2026-08-07T23:11:43.152438Z","submitted_at":"2026-07-27T18:00:27Z","title":"EFT-Ramses: a code to simulate the effective field theory of dark energy","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-31T05:27:07.674082Z"},"links":{"cited_paper":"/paper/2209.07395","citing_paper":"/paper/2607.24940"},"observation_digest":"sha256:05a16edfda579d0204fcde5824236e54be7d163718bb6a301b5e8663ead41412","observation_id":"74dcaf2b-cca9-4fb8-95a4-ba50a0a09a6a","resolution":{"observed_at":"2026-07-31T05:27:07.674082Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2209.07395/citation-record","integrity":"/paper/2209.07395/integrity","json":"/paper/2209.07395/citation-record.json","paper":"/paper/2209.07395"},"outbound":[],"paper":{"arxiv_id":"2209.07395","last_updated":"2022-10-07T13:02:48Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T14:25:41.329665Z","submitted_at":"2022-09-15T15:55:57Z","title":"Planck ISW-lensing likelihood and the CMB temperature"},"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 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2209.07395."}