{"as_of":"2026-08-10T18:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3176dec66ed954d3724c5de4132b5f8dc6514c18284919b4baf516e1fbd3b0bc","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":19,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":19,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":19,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":19,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T21:04:17.789776Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-08T21:04:17.789776Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04929","last_updated":"2025-05-14T14:57:09Z","snapshot_observed_at":"2026-08-08T20:55:05.610325Z","submitted_at":"2025-02-07T13:49:14Z","title":"Robustness of dark energy phenomenology across different parameterizations","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-08T21:04:17.789776Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2502.04929"},"observation_digest":"sha256:bb1f465826e736d74e85960f77a20360c0356dc901c77968e64f5468fe8f41cd","observation_id":"4ec5102a-1ba9-4878-a735-d25ff1769f1b","resolution":{"observed_at":"2026-08-08T21:04:17.789776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-04T18:59:22.954439Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.09562","last_updated":"2025-09-11T15:52:46Z","snapshot_observed_at":"2026-08-08T03:00:16.548546Z","submitted_at":"2025-09-11T15:52:46Z","title":"The simple way to measure evolving dark energy without prior-volume effects","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-04T18:59:22.954439Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2509.09562"},"observation_digest":"sha256:9f8966f3aafda012e208a1d3e4f4c61aa9d31cd588d62716db8c41ce9943f3f1","observation_id":"1d3db2fb-008e-4562-a387-8f0f181dd2d4","resolution":{"observed_at":"2026-08-04T18:59:22.954439Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-03T19:53:35.800014Z","title":"G., Paliathanasis, A., & Saridakis, E","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2511.22478","last_updated":"2026-06-30T07:30:00Z","snapshot_observed_at":"2026-08-09T07:04:27.807597Z","submitted_at":"2025-11-27T14:06:13Z","title":"Probing the sound speed and clustering of dark energy","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T19:53:35.800014Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2511.22478"},"observation_digest":"sha256:32219008a8a38691aef2e0fbaf076fca567a78da9b8a7a5488bedddb2ed6941e","observation_id":"66d6f4a3-88ae-4722-bdc9-cff4d4de00c4","resolution":{"observed_at":"2026-08-03T19:53:35.800014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-03T18:51:43.979266Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2512.04130","last_updated":"2026-07-26T05:14:02Z","snapshot_observed_at":"2026-08-09T18:20:38.058807Z","submitted_at":"2025-12-03T06:33:55Z","title":"Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\\omega_0\\omega_a$CDM","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:43.979266Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:7900665406298b9a724fed190a1b5560804d9fb944a3ae99275c5487c22ad5b0","observation_id":"b33f5638-dd46-4dab-804d-3d55f620ef6d","resolution":{"observed_at":"2026-08-03T18:51:43.979266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-03T15:40:03.472546Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2512.16551","last_updated":"2026-05-25T13:54:56Z","snapshot_observed_at":"2026-08-03T15:39:55.325698Z","submitted_at":"2025-12-18T13:55:56Z","title":"Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the impact on the $\\sigma_8$ tension","version":3},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-03T15:40:03.472546Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2512.16551"},"observation_digest":"sha256:190cd41a47355a1e0d04cec886206cb7003deaebe541c815bee76d9de197c418","observation_id":"30cac4a3-0d27-4cf0-b652-f539996f4bee","resolution":{"observed_at":"2026-08-03T15:40:03.472546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-03T14:40:55.482565Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.19888","last_updated":"2026-06-18T12:16:03Z","snapshot_observed_at":"2026-08-07T04:04:01.596809Z","submitted_at":"2025-12-22T21:27:32Z","title":"Observational constraints on early time non-phantom behaviour of dynamical dark energy","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-03T14:40:55.482565Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2512.19888"},"observation_digest":"sha256:3fcd1184534bd6ed5536cbef06d54b3479004c05eb28b72497406b24cb0230a4","observation_id":"3f77a340-4a7c-448d-9c45-e2ab77e54b92","resolution":{"observed_at":"2026-08-03T14:40:55.482565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-03T08:42:10.017858Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-08T14:24:16.036685Z","submitted_at":"2026-01-22T18:10:50Z","title":"Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy","version":2},"reference_index":202,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:10.017858Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:5106f22faedda9de46122886f05ed4b9f2ac9ce7420d88ed46b058657535c643","observation_id":"fdb4f0d5-173e-4485-935a-92a1341608b9","resolution":{"observed_at":"2026-08-03T08:42:10.017858Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2603.26560","last_updated":"2026-05-26T09:42:59Z","snapshot_observed_at":"2026-07-13T17:26:51.495350Z","submitted_at":"2026-03-27T16:25:41Z","title":"Exploring the interplay of late-time dynamical dark energy and new physics before recombination","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:37bc1f77c0eb9110dc0c85a3e4cb01c87f7efaee7e2ab3541db19dc26befc213","observation_id":"474c9306-1d7e-44d4-92fc-ed4c11b791b1","resolution":{"observed_at":"2026-05-14T23:13:15.184353Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2604.08895","last_updated":"2026-04-10T02:59:01Z","snapshot_observed_at":"2026-07-31T18:55:02.385910Z","submitted_at":"2026-04-10T02:59:01Z","title":"FolpsD: combining EFT and phenomenological approaches for joint power spectrum and bispectrum analyses","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-10T17:38:15.169909Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2604.08895"},"observation_digest":"sha256:a7d50ebbe1508f2494a09d25a239fc557485f6befe0e5c1af79d3531a2f6ebae","observation_id":"1799911b-f2b0-4d50-823f-6f64656a81f0","resolution":{"observed_at":"2026-05-11T06:26:00.089773Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2605.05114","last_updated":"2026-06-03T14:56:40Z","snapshot_observed_at":"2026-08-08T13:23:09.915860Z","submitted_at":"2026-05-06T16:45:33Z","title":"Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-08T16:57:42.506088Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2605.05114"},"observation_digest":"sha256:fe8375d514d91376011f8dda8a79315cb9e992e91f13b5c29c0d7ed3aaacf513","observation_id":"69d49b39-f6c7-43f7-9691-1860d0d59d17","resolution":{"observed_at":"2026-05-11T17:56:05.567011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2605.05114","last_updated":"2026-06-03T14:56:40Z","snapshot_observed_at":"2026-08-08T13:23:09.915860Z","submitted_at":"2026-05-06T16:45:33Z","title":"Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-30T23:23:06.869558Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2605.05114"},"observation_digest":"sha256:6cf4baba2b24ae127070e4cf0caad484140bac4df4d8a01fd284401ba195ce11","observation_id":"0cca8dae-28ee-4d73-afc0-d9a7d35864f6","resolution":{"observed_at":"2026-06-30T23:25:07.663384Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2605.22309","last_updated":"2026-07-15T09:02:22Z","snapshot_observed_at":"2026-08-06T01:35:32.177705Z","submitted_at":"2026-05-21T10:55:25Z","title":"Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-22T05:36:41.912431Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2605.22309"},"observation_digest":"sha256:173aef83ee1c82122ed41689c9524a3e048f14579f7e8ac9c9e65ab02ef48f03","observation_id":"77f3730a-fef6-4887-a243-56f41a1a1030","resolution":{"observed_at":"2026-05-22T05:41:08.695172Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-02T13:29:55.487937Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.22309","last_updated":"2026-07-15T09:02:22Z","snapshot_observed_at":"2026-08-06T01:35:32.177705Z","submitted_at":"2026-05-21T10:55:25Z","title":"Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-02T13:29:55.487937Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2605.22309"},"observation_digest":"sha256:f39a8dd52cdc6d71e78599a4156a1bfbb5fc8f1cacbfcfa5992b7fc195d59870","observation_id":"cb724ba9-4e21-4b95-b1a2-64d1188cc439","resolution":{"observed_at":"2026-08-02T13:29:55.487937Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2605.28644","last_updated":"2026-05-27T15:50:02Z","snapshot_observed_at":"2026-07-06T23:38:14.056361Z","submitted_at":"2026-05-27T15:50:02Z","title":"Exploring non-Poisson satellite occupation in HOD models and its impact on 2- and 3-point galaxy clustering","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-29T10:41:50.746173Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2605.28644"},"observation_digest":"sha256:3b6897b5429ce52541a051dca6770301c6a80e789c472aa3f52fc0b260fab02d","observation_id":"3950a6fc-7069-4d75-b287-a6c17f13a612","resolution":{"observed_at":"2026-06-29T10:43:18.397675Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2606.26237","last_updated":"2026-06-24T18:00:03Z","snapshot_observed_at":"2026-07-07T00:00:36.766142Z","submitted_at":"2026-06-24T18:00:03Z","title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-06-26T01:35:05.451125Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2606.26237"},"observation_digest":"sha256:64f1ae6692f5387676c9cd8bc191fa75217b7b9eac288e072af2d095090334b9","observation_id":"bda70f54-6493-47c3-9522-060612fbcc9b","resolution":{"observed_at":"2026-06-26T01:38:51.859705Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"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":103,"source":"pdf_text","source_observed_at":"2026-07-01T03:37:13.804621Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2606.31977"},"observation_digest":"sha256:7932de880be1be090b1d741fc7d2b158573cca2966a5680f60ca095ef48c580e","observation_id":"84b4f8d2-778a-4f34-b234-345bbad54cef","resolution":{"observed_at":"2026-07-01T11:55:42.873903Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":"2503.04602","doi":"10.48550/arxiv.2503.04602","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","venue":"ArXiv.org","work_id":"fdbfec0d-37e1-4707-b6fb-dc5dc2bba93a","year":2025},"citing_paper":{"arxiv_id":"2607.02498","last_updated":"2026-07-09T17:52:11Z","snapshot_observed_at":"2026-07-12T23:18:45.171074Z","submitted_at":"2026-07-02T17:57:15Z","title":"Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-03T06:27:31.520900Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2607.02498"},"observation_digest":"sha256:39d44cfe15113da399fda4a9c243460eb244e6d8d32e9f402beb9376d2ce7e61","observation_id":"c4e612d3-b261-44bd-84c9-3fbfcfe3ace1","resolution":{"observed_at":"2026-07-03T06:27:41.636165Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-07-12T08:00:27.085537Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.02498","last_updated":"2026-07-09T17:52:11Z","snapshot_observed_at":"2026-07-12T23:18:45.171074Z","submitted_at":"2026-07-02T17:57:15Z","title":"Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-12T08:00:27.085537Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2607.02498"},"observation_digest":"sha256:00476626cfb1fd73c0e599ef921587912c42fea458ae9fa833223af4e3b3b07d","observation_id":"5bb9ee6c-0616-472b-b4bc-965b689cc046","resolution":{"observed_at":"2026-07-12T08:00:27.085537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.04602","snapshot_observed_at":"2026-08-02T05:48:26.022291Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.13283","last_updated":"2026-07-14T21:36:00Z","snapshot_observed_at":"2026-08-07T20:25:34.943645Z","submitted_at":"2026-07-14T21:36:00Z","title":"The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions","version":1},"reference_index":218,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:26.022291Z"},"links":{"cited_paper":"/paper/2503.04602","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:972a8d9e1889852d51b4fddc5bd6f0f724943dc92192b1c6f26969b5feb421a0","observation_id":"40ad9ba8-29fd-4bde-9bbd-859ac66d52ac","resolution":{"observed_at":"2026-08-02T05:48:26.022291Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.04602/citation-record","integrity":"/paper/2503.04602/integrity","json":"/paper/2503.04602/citation-record.json","paper":"/paper/2503.04602"},"outbound":[],"paper":{"arxiv_id":"2503.04602","last_updated":"2025-04-15T13:08:41Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T17:24:11.337697Z","submitted_at":"2025-03-06T16:45:49Z","title":"Preference for evolving dark energy in light of the galaxy bispectrum"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2503.04602."}