{"as_of":"2026-08-20T00:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b5185e1ceb083d8205d882dac16fbc742ccc731c05554267ce1da9687df7f34a","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":16,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":16,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":16,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":16,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:00:38.148236Z","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":"2026-07-04T05:19:36.129495Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-10T18:12:34.780565Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.11571","last_updated":"2025-06-17T07:05:51Z","snapshot_observed_at":"2026-08-10T20:17:39.475166Z","submitted_at":"2025-01-20T16:20:59Z","title":"Illustrating the consequences of a misuse of $\\sigma_8$ in cosmology","version":2},"reference_index":228,"source":"pdf_text","source_observed_at":"2026-08-10T18:12:34.780565Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2501.11571"},"observation_digest":"sha256:62ece047efe72ce068126ad5c0483e576bde2f3379d12594ae0bee9c4a5b39fb","observation_id":"f24682c4-61b9-47d7-a1f3-08ae2e6df877","resolution":{"observed_at":"2026-08-10T18:12:34.780565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-07T20:33:58.153247Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.09810","last_updated":"2025-03-28T12:50:30Z","snapshot_observed_at":"2026-08-09T21:41:06.451790Z","submitted_at":"2025-02-13T23:02:39Z","title":"$\\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T20:33:58.153247Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2502.09810"},"observation_digest":"sha256:0b9a0d689265a53774aa166e2c51478ce7cf7e8c4325986397bde156c7e87e62","observation_id":"5040a965-0226-44e2-9cb4-58a973982e53","resolution":{"observed_at":"2026-08-07T20:33:58.153247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-16T05:00:38.148236Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.21813","last_updated":"2025-04-30T17:16:54Z","snapshot_observed_at":"2026-08-16T23:26:45.882526Z","submitted_at":"2025-04-30T17:16:54Z","title":"Turning a negative neutrino mass into a positive optical depth","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-16T05:00:38.148236Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2504.21813"},"observation_digest":"sha256:bf5288a86192533204d565d54ff8051856db7d654660017c39b76d6b5c5a76a4","observation_id":"bcb9b371-47b3-4ab2-9f25-44b4cab69d8f","resolution":{"observed_at":"2026-08-16T05:00:38.148236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-15T22:11:10.288816Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.08051","last_updated":"2025-05-27T06:00:57Z","snapshot_observed_at":"2026-08-16T23:26:47.901395Z","submitted_at":"2025-05-12T20:38:52Z","title":"Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-15T22:11:10.288816Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2505.08051"},"observation_digest":"sha256:ae949242d7d6b1e5efc10429ffd50b6d79a6b4c3525eac0c197a18017c256e8a","observation_id":"882eb87b-49d8-4e33-b1d4-f0db5172343b","resolution":{"observed_at":"2026-08-15T22:11:10.288816Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-07T10:52:56.684987Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.04306","last_updated":"2025-06-04T17:51:05Z","snapshot_observed_at":"2026-08-13T10:19:27.378849Z","submitted_at":"2025-06-04T17:51:05Z","title":"Can the universe experience an AdS landscape since matter-radiation equality?","version":1},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.684987Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2506.04306"},"observation_digest":"sha256:ec4f7f46791aeca8d5adc01a0dd488e31ddb5d818f11bf7ca5db7c5651016d2d","observation_id":"1d3f348b-8e41-4de7-90d5-b227739d8a9f","resolution":{"observed_at":"2026-08-07T10:52:56.684987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-04T12:53:38.034126Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"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":70,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:38.034126Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:a2238a9a21ebff603e44260382c5aebbfdace358fdba334340cfb22ad06db232","observation_id":"4c56ef15-fc5d-487c-8b05-5d61ab473c8c","resolution":{"observed_at":"2026-08-04T12:53:38.034126Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"citing_paper":{"arxiv_id":"2604.12587","last_updated":"2026-04-14T11:10:26Z","snapshot_observed_at":"2026-08-11T02:10:08.591061Z","submitted_at":"2026-04-14T11:10:26Z","title":"Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-10T14:37:32.848262Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2604.12587"},"observation_digest":"sha256:867f692e4964fb06449ad236229a0839c865584e7889e63b12125ba02687b307","observation_id":"67820e46-fff1-44da-946a-2910cfad0827","resolution":{"observed_at":"2026-05-10T14:45:48.020557Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-08-18T05:23:44.122534Z","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":152,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:66f7acd1a08d239c4c8100036b62e5e0bed59f390788b2f511993652f934aaa3","observation_id":"0ace725f-5dbc-4b53-8418-29cb1df63995","resolution":{"observed_at":"2026-05-11T11:41:02.093063Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"citing_paper":{"arxiv_id":"2605.26050","last_updated":"2026-05-25T17:12:16Z","snapshot_observed_at":"2026-08-12T22:00:57.664487Z","submitted_at":"2026-05-25T17:12:16Z","title":"Early- and Late-Time Modifications to $\\Lambda$CDM: Implications for the Hubble Tension","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-06-29T20:29:06.417337Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2605.26050"},"observation_digest":"sha256:345b4559fc2b0b0642d4c7d314252819f112a3338d44c6149960fa9def652403","observation_id":"2bf6fc49-d081-488f-b1c5-b953a8b8a1ad","resolution":{"observed_at":"2026-06-30T00:14:05.017286Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"citing_paper":{"arxiv_id":"2605.26116","last_updated":"2026-05-25T17:59:53Z","snapshot_observed_at":"2026-07-06T23:36:01.564747Z","submitted_at":"2026-05-25T17:59:53Z","title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","version":1},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:59eb995e4308679b8370b3571a454628372e4698eb8ae81e3ba6f37ccb2fd08d","observation_id":"20471d1f-86b1-4b12-9909-6a54e2a70840","resolution":{"observed_at":"2026-07-01T16:35:51.042720Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"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":82,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:7dc618336c63b3a12646be2f7d2afad0ca8d68344d33ab5ea648d75fff23633a","observation_id":"6af922df-1be0-4e0f-a061-3f08c7ca3cf6","resolution":{"observed_at":"2026-07-02T15:37:06.168347Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-15T03:29:17.716518Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":297,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:e86e813969d53a2b8309af325478d2a56683a99c02add49486d21cf345b41064","observation_id":"e71d6088-b8e4-44ea-a7ec-2fc95af62710","resolution":{"observed_at":"2026-07-04T05:19:36.130938Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-15T03:29:17.716518Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":297,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:e692f8b4b794b590a1a5499bb9888e2eca5d15671fbfea58a52ba855b19ee35b","observation_id":"fe4919bb-f0ff-43fd-805e-9da86366d9c7","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":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":"2311.00524","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-07-04T05:19:36.129495Z","title":"Efstathiou, E","venue":null,"work_id":"c37197ce-ac02-4fd3-99f8-dd5f5d0b728e","year":2024},"citing_paper":{"arxiv_id":"2606.31324","last_updated":"2026-06-30T08:27:42Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-30T08:27:42Z","title":"Cosmological Viability of Exponential Infrared $f(T)$ Gravity","version":1},"reference_index":129,"source":"pdf_text","source_observed_at":"2026-07-01T04:39:56.556632Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2606.31324"},"observation_digest":"sha256:1ca38a65d0efda8eb0dca2dd518f23c3bff223499fd51b97e3c65190226c40c6","observation_id":"c582d2a5-ac6d-4113-b25a-992725a711d1","resolution":{"observed_at":"2026-07-01T11:15:42.388034Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-02T05:48:26.439944Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"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":221,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:26.439944Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:a6b7b8997f74f7d4054ecf86b9f82b5d96db282958a21a92e66506f54c917c6b","observation_id":"bbef7105-fd19-407e-ab64-65d3ad721087","resolution":{"observed_at":"2026-08-02T05:48:26.439944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.00524","snapshot_observed_at":"2026-08-01T08:08:46.299482Z","title":"Efstathiou, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-18T04:16:34.790019Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":134,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:46.299482Z"},"links":{"cited_paper":"/paper/2311.00524","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:7a4d28a9cc22c2166d4279a2b06c1ab63d3eaa56cf5e2555edd916ed4427bbf0","observation_id":"3405390b-e21b-491e-b7b0-e64d224b3911","resolution":{"observed_at":"2026-08-01T08:08:46.299482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2311.00524/citation-record","integrity":"/paper/2311.00524/integrity","json":"/paper/2311.00524/citation-record.json","paper":"/paper/2311.00524"},"outbound":[],"paper":{"arxiv_id":"2311.00524","last_updated":"2023-11-01T13:51:33Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-18T01:52:36.801496Z","submitted_at":"2023-11-01T13:51:33Z","title":"Improved Planck constraints on axion-like early dark energy as a resolution of 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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2311.00524."}