{"as_of":"2026-08-05T04:40:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:59d029f62c3252552e46eb0a4af773394929c905884ea569ee54f4886e84cbcf","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":"2026-08-04T06:34:03.388597+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":"2026-07-13T06:51:47.584044Z","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":"2026-07-08T01:44:25.980193Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2504.20478","last_updated":"2026-04-17T05:39:20Z","snapshot_observed_at":"2026-07-06T21:16:13.624880Z","submitted_at":"2025-04-29T07:19:58Z","title":"Tomographic Alcock-Paczynski Test with Marked Correlation Functions","version":5},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-22T18:56:46.117021Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2504.20478"},"observation_digest":"sha256:5baaa36470ea43697b810b205f7c92abcac97a39399d6267257abb7c0bd6e24e","observation_id":"79320e80-efda-4087-82ce-a5925268ef88","resolution":{"observed_at":"2026-05-22T18:56:58.004643Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2604.21050","last_updated":"2026-07-30T08:11:22Z","snapshot_observed_at":"2026-08-02T23:16:53.603712Z","submitted_at":"2026-04-22T19:48:11Z","title":"The Vacuum Displacement Principle: Theoretical Framework and Local Phenomenology","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-09T23:23:41.527408Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2604.21050"},"observation_digest":"sha256:4b953d1dbcac673463cc628c76d6e89181d5c7bb19dc7fc9480a46535039e6fb","observation_id":"a0a47ff8-b837-42ec-b0d9-846bb41296fc","resolution":{"observed_at":"2026-05-09T23:24:43.093653Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2604.21050","last_updated":"2026-07-30T08:11:22Z","snapshot_observed_at":"2026-08-02T23:16:53.603712Z","submitted_at":"2026-04-22T19:48:11Z","title":"The Vacuum Displacement Principle: Theoretical Framework and Local Phenomenology","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-05T02:05:21.835143Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2604.21050"},"observation_digest":"sha256:e60c8b4cca4563d99530361ee809be1fd1b8bb39ad42794697012f897d6d9105","observation_id":"cf1b0aa7-c4a1-44b1-bf48-16832afc204c","resolution":{"observed_at":"2026-07-05T02:10:36.469913Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2605.23367","last_updated":"2026-06-08T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-22T08:33:44Z","title":"Cosmological constraints from neighbor-density-weighted marked correlation functions","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-25T03:27:13.896349Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2605.23367"},"observation_digest":"sha256:948626a744345ae155b86c61b906611646ccc440be85a6c1bcb93415ef06a444","observation_id":"407e1332-f2ad-4194-aa0b-a45ee0986ce0","resolution":{"observed_at":"2026-05-25T03:30:17.428194Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2605.23367","last_updated":"2026-06-08T11:28:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-22T08:33:44Z","title":"Cosmological constraints from neighbor-density-weighted marked correlation functions","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-30T15:08:32.960489Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2605.23367"},"observation_digest":"sha256:0389b7678e8464df5d94b315f8e15df9cf328198853828f11606624dea368ce0","observation_id":"69b0f9d9-4e48-4d3b-b96b-ed46f76d1c95","resolution":{"observed_at":"2026-06-30T15:14:47.282233Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2605.27087","last_updated":"2026-06-02T03:39:14Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-26T14:35:10Z","title":"Cosmological Constraints from Bias-Robust Wavelet Scattering Statistics for Stage-IV Galaxy Surveys","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-29T15:49:18.200446Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2605.27087"},"observation_digest":"sha256:80e729141d5709b2e1643e1c813f8adfc8888dc9f316775e80e7bba5ff2a4243","observation_id":"944a2ee9-2e74-4b08-b1ab-b9c8877c4036","resolution":{"observed_at":"2026-06-29T16:33:39.534412Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":"1108.2637","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-08T01:44:25.980193Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","venue":"astro-ph.CO","work_id":"c4fa80c9-f7c0-472a-8c8f-8f000186cc4c","year":2011},"citing_paper":{"arxiv_id":"2607.06567","last_updated":"2026-07-10T06:39:12Z","snapshot_observed_at":"2026-08-02T03:10:04.985353Z","submitted_at":"2026-07-07T17:59:59Z","title":"Skipping the rungs! Calibrating distance indicators through their clustering with galaxies","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-08T01:43:22.553776Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2607.06567"},"observation_digest":"sha256:77893b354d3ff36e67036928a675371b22b6bf50ceb806251c540d4a497754cd","observation_id":"4dae2b0f-9e40-4afd-abb8-d3ee732ef12e","resolution":{"observed_at":"2026-07-08T01:44:25.981449Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.2637","snapshot_observed_at":"2026-07-13T06:51:47.584044Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.06567","last_updated":"2026-07-10T06:39:12Z","snapshot_observed_at":"2026-08-02T03:10:04.985353Z","submitted_at":"2026-07-07T17:59:59Z","title":"Skipping the rungs! Calibrating distance indicators through their clustering with galaxies","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-13T06:51:47.584044Z"},"links":{"cited_paper":"/paper/1108.2637","citing_paper":"/paper/2607.06567"},"observation_digest":"sha256:3bc1bdd8e1d651c8684a231763ddcf20b7a696068793a8061064b453dc77a4d5","observation_id":"3c60a96e-b63e-41ad-a010-bc432a7a38f8","resolution":{"observed_at":"2026-07-13T06:51:47.584044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1108.2637/citation-record","integrity":"/paper/1108.2637/integrity","json":"/paper/1108.2637/citation-record.json","paper":"/paper/1108.2637"},"outbound":[],"paper":{"arxiv_id":"1108.2637","last_updated":"2011-08-12T15:11:56Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:32:20.777676Z","submitted_at":"2011-08-12T15:11:56Z","title":"The WiggleZ Dark Energy Survey: measuring the cosmic expansion history using the Alcock-Paczynski test and distant supernovae"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1108.2637."}