{"as_of":"2026-08-14T23:16:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:75bc2ac3b4227ed8ed50c27bc45b8fde7421a48bae2d7cf7d6624b13d5eead8a","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":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T22:01:20.748500Z","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":"2026-07-04T05:19:35.753488Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-08-12T22:01:20.748500Z","title":"Sch¨ oneberg and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08097","last_updated":"2024-11-12T19:00:00Z","snapshot_observed_at":"2026-08-14T09:19:33.499151Z","submitted_at":"2024-11-12T19:00:00Z","title":"Atomic Dark Matter, Interacting Dark Radiation, and the Hubble Tension","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T22:01:20.748500Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2411.08097"},"observation_digest":"sha256:729b31bb097002a25350a290edc7302b10adf7315abf5860fb2d250fa662c455","observation_id":"0df45ca4-67a3-43f3-8482-a3f5e3b90135","resolution":{"observed_at":"2026-08-12T22:01:20.748500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-08-04T12:53:35.694520Z","title":"Sch¨ oneberg and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-14T00:44:55.106734Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:35.694520Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:f764f189c2b58dcad9a1f833e788a8158cb8dfcce06b8a52563e938a41815bc1","observation_id":"d3a0f0e5-2d79-4b0d-8958-8a2d2733cde0","resolution":{"observed_at":"2026-08-04T12:53:35.694520Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":"2206.11276","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-04T05:19:35.753488Z","title":"Sch¨ oneberg and G","venue":null,"work_id":"2fafb8fc-dd65-4262-9dcb-6feecb6ae5f1","year":2022},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:576c935dbedc96bd454df130c6f610cf254d310266bf7959b9acd5b0cdc820e7","observation_id":"b49d0632-cb4d-4010-93f1-e211a14fe7e8","resolution":{"observed_at":"2026-05-11T11:36:03.793345Z","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":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":"2206.11276","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-04T05:19:35.753488Z","title":"Sch¨ oneberg and G","venue":null,"work_id":"2fafb8fc-dd65-4262-9dcb-6feecb6ae5f1","year":2022},"citing_paper":{"arxiv_id":"2604.25813","last_updated":"2026-04-28T16:22:13Z","snapshot_observed_at":"2026-08-14T05:46:29.116219Z","submitted_at":"2026-04-28T16:22:13Z","title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","version":1},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-07T14:55:55.250283Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2604.25813"},"observation_digest":"sha256:9b63440d772204b960a9cdd0b2a3e5a37a77d7587ff5f2538b2a7aea8098876b","observation_id":"6bfccf20-12b8-4748-a509-bdbe465910c9","resolution":{"observed_at":"2026-05-12T00:36:16.199441Z","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":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":"2206.11276","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-04T05:19:35.753488Z","title":"Sch¨ oneberg and G","venue":null,"work_id":"2fafb8fc-dd65-4262-9dcb-6feecb6ae5f1","year":2022},"citing_paper":{"arxiv_id":"2604.26541","last_updated":"2026-04-29T11:12:54Z","snapshot_observed_at":"2026-08-12T14:37:11.867707Z","submitted_at":"2026-04-29T11:12:54Z","title":"The End of the First Act: Spectral Running, Interacting Dark Radiation, and the Hubble Tension in Light of ACT DR6 Data","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-07T12:38:23.880499Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2604.26541"},"observation_digest":"sha256:ce336e30cd917709ff4977d31aecde079af698c7ef3993bab69e82365f88adfc","observation_id":"bb4022ad-80d8-4e8a-85f6-199e09356789","resolution":{"observed_at":"2026-05-12T09:11:26.204920Z","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":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":"2206.11276","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-04T05:19:35.753488Z","title":"Sch¨ oneberg and G","venue":null,"work_id":"2fafb8fc-dd65-4262-9dcb-6feecb6ae5f1","year":2022},"citing_paper":{"arxiv_id":"2606.06495","last_updated":"2026-06-04T17:59:59Z","snapshot_observed_at":"2026-08-13T23:27:08.774753Z","submitted_at":"2026-06-04T17:59:59Z","title":"What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:e3bad06abe6969577949a8bc923754f21bf71c93b9644650c65657bb31f35ab6","observation_id":"636fda0f-bbac-4d1b-8122-5e99e92cd503","resolution":{"observed_at":"2026-07-02T15:37:06.542903Z","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":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":"2206.11276","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-04T05:19:35.753488Z","title":"Sch¨ oneberg and G","venue":null,"work_id":"2fafb8fc-dd65-4262-9dcb-6feecb6ae5f1","year":2022},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-14T03:18:00.674049Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":260,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:a6c4c889f701bfaa6955253e090dc99b2326ab6af1993cd16c29b8f5a1a17d1d","observation_id":"101839e1-38c0-465d-abb4-bf664ebdf855","resolution":{"observed_at":"2026-07-04T05:19:35.755048Z","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":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Sch¨ oneberg and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-14T03:18:00.674049Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":260,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:5f089cb3c9fcd3444d6dc8d18a84f731dff91567edc6ecb863452514134618fe","observation_id":"92e9e9b6-f989-4a2e-8fd8-045d522aa736","resolution":{"observed_at":"2026-07-15T10:41:50.733215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":"2206.11276","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-07-04T05:19:35.753488Z","title":"Sch¨ oneberg and G","venue":null,"work_id":"2fafb8fc-dd65-4262-9dcb-6feecb6ae5f1","year":2022},"citing_paper":{"arxiv_id":"2606.31362","last_updated":"2026-06-30T08:57:18Z","snapshot_observed_at":"2026-08-09T03:11:42.668077Z","submitted_at":"2026-06-30T08:57:18Z","title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","version":1},"reference_index":197,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:efcfecf90a14bfd8218637398e6f71c1a4035213418f45324fb0db7eaec03d40","observation_id":"b87fcb43-88ee-4183-9425-1eab6f388685","resolution":{"observed_at":"2026-07-01T11:25:45.604040Z","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":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-08-02T05:41:43.806878Z","title":"Sch¨ oneberg and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.13282","last_updated":"2026-07-14T21:35:59Z","snapshot_observed_at":"2026-08-13T03:17:59.749576Z","submitted_at":"2026-07-14T21:35:59Z","title":"The $H_0$ World Cup. I. Summary of the baseline group stage results","version":1},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-08-02T05:41:43.806878Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2607.13282"},"observation_digest":"sha256:261476d7320192b6055c1deff27bb2a15158c7218c28cf4a29e682b0640e5606","observation_id":"19a28691-ad67-4fd3-81b5-68b8289ff223","resolution":{"observed_at":"2026-08-02T05:41:43.806878Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-08-02T05:48:19.672460Z","title":"Sch¨ oneberg and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.13283","last_updated":"2026-07-14T21:36:00Z","snapshot_observed_at":"2026-08-14T14:19:11.939913Z","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":145,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:19.672460Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:9d158551627e35cf5033a9477389b8c348a1cd56f8cea0657da3ede83004a921","observation_id":"4d7d86f3-d7c2-488c-b2aa-3e76ff7dc991","resolution":{"observed_at":"2026-08-02T05:48:19.672460Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11276","snapshot_observed_at":"2026-08-01T08:08:43.504899Z","title":"Sch¨ oneberg and G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-12T13:23:10.903299Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:43.504899Z"},"links":{"cited_paper":"/paper/2206.11276","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:e338205c634b7263c6e67d39961b50b5f131c4cccef21624e61abe29ea47ae70","observation_id":"6a46950e-1306-4332-8290-71d987d7e6fe","resolution":{"observed_at":"2026-08-01T08:08:43.504899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2206.11276/citation-record","integrity":"/paper/2206.11276/integrity","json":"/paper/2206.11276/citation-record.json","paper":"/paper/2206.11276"},"outbound":[],"paper":{"arxiv_id":"2206.11276","last_updated":"2022-08-25T11:54:57Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T11:48:26.544378Z","submitted_at":"2022-06-22T18:00:02Z","title":"A step in the right direction? Analyzing the Wess Zumino Dark Radiation solution to the Hubble tension"},"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 12 inbound Pith citation observations for arXiv:2206.11276."}