{"as_of":"2026-08-12T06:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:95bee0ee54882b3ea29ce510009d1b039d7e5abfe79b293ae3feb33548b7f95a","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":23,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":23,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":23,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":23,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T17:19:39.465918Z","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":"2026-07-04T05:19:36.051419Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2211.04492","last_updated":"2022-11-08T19:00:16Z","snapshot_observed_at":"2026-08-01T18:06:39.805867Z","submitted_at":"2022-11-08T19:00:16Z","title":"The Hubble Tension and Early Dark Energy","version":1},"reference_index":140,"source":"pdf_text","source_observed_at":"2026-05-17T23:41:11.040188Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2211.04492"},"observation_digest":"sha256:99dc62cef98b85d584929eeca2cc887dd51656212db2a7ae9b6597d92b37efb9","observation_id":"194dd95a-ed97-405b-aec9-3159dd415b6e","resolution":{"observed_at":"2026-05-17T23:41:11.255396Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-05T12:06:17.634719Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.08840","last_updated":"2025-09-02T06:17:29Z","snapshot_observed_at":"2026-08-08T14:59:09.132548Z","submitted_at":"2025-09-02T06:17:29Z","title":"Alleviating the Hubble Tension via Cosmological Time Dilation in the meVSL Model","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-05T12:06:17.634719Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2509.08840"},"observation_digest":"sha256:7b5c1353ba296bfda2dcc46a0c5a85b331a4d1f1c10b3e892edf6397875da7e2","observation_id":"41f9a5e2-420b-4fec-8a8a-e248671dfabb","resolution":{"observed_at":"2026-08-05T12:06:17.634719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-04T13:24:31.663299Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.00852","last_updated":"2026-06-26T02:09:02Z","snapshot_observed_at":"2026-08-09T17:37:11.286930Z","submitted_at":"2025-10-01T13:06:16Z","title":"Alleviating Cosmological Tensions with the Hadrosymmetric Twin Higgs","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T13:24:31.663299Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2510.00852"},"observation_digest":"sha256:ef21c62eb8923a7f76d97f30f798ff44b8ca1f05116e99b4b191fa23f254f7f9","observation_id":"15e79c61-73fa-4722-8a8b-f81346c6f305","resolution":{"observed_at":"2026-08-04T13:24:31.663299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-04T12:53:34.355529Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-04T12:53:22.243014Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:34.355529Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:0d36d2ff60b8afd67ff2abb8c9eba3e3506bc6ff02855822fb500c63d8d017f7","observation_id":"ef95d76c-964b-4d4e-82fe-e77790cdc066","resolution":{"observed_at":"2026-08-04T12:53:34.355529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-04T09:59:20.686128Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-07T12:03:55.381688Z","submitted_at":"2025-10-14T15:24:50Z","title":"Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2","version":2},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:20.686128Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:d2e968413061bcab3bb427a17b8b5baf3ec47e1a88b8f0e68a220805c34467e8","observation_id":"8040d4c6-5cbf-4864-8335-b5af02318093","resolution":{"observed_at":"2026-08-04T09:59:20.686128Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-03T17:35:05.359097Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.09177","last_updated":"2025-12-09T22:51:47Z","snapshot_observed_at":"2026-08-06T16:53:45.987150Z","submitted_at":"2025-12-09T22:51:47Z","title":"Primordial magnetic field from chiral plasma instability with sourcing","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T17:35:05.359097Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2512.09177"},"observation_digest":"sha256:596eeaa14730f35105a4e3941929605e66fd275d38a9d9b7c12bc982952e1300","observation_id":"b6ca306e-fb87-4462-8f3a-934e948fefbc","resolution":{"observed_at":"2026-08-03T17:35:05.359097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"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":126,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:5b4631f4704be7194cce071f9ab2344912c9f1b0a17a9bd88975aebfdb556578","observation_id":"223444d5-9fe5-4d7a-9dcb-be21513cc87e","resolution":{"observed_at":"2026-05-14T23:13:15.908216Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2604.07327","last_updated":"2026-04-08T17:44:37Z","snapshot_observed_at":"2026-07-06T22:55:37.787732Z","submitted_at":"2026-04-08T17:44:37Z","title":"Primordial magnetic fields in the light of upcoming post-EoR Lyman-$\\alpha$ and 21-cm observations","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-10T17:49:57.964050Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2604.07327"},"observation_digest":"sha256:34ceb3d5f3478681737da53046871f0454f16be4cf9e4fd95e77be9fb8e9eb7c","observation_id":"2960ffba-468e-4a8c-bbd7-6cccacde3919","resolution":{"observed_at":"2026-05-11T06:01:00.875996Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"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":39,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:9f349cb492fbf89785bf0cf1fe7e342f19df2e286c5dba3f2379d69b814c4936","observation_id":"c4e101eb-88c3-49f5-993b-ab527970a95a","resolution":{"observed_at":"2026-05-10T13:00:24.833710Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2604.20768","last_updated":"2026-04-22T16:57:22Z","snapshot_observed_at":"2026-07-06T23:07:25.185196Z","submitted_at":"2026-04-22T16:57:22Z","title":"Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition","version":1},"reference_index":161,"source":"pdf_text","source_observed_at":"2026-05-09T23:54:19.807809Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2604.20768"},"observation_digest":"sha256:2e3614b18034f0b76d1e5bb1a7a156d2ccbc3cc7a7cd85d1b8846f74796f24ba","observation_id":"8d0c6a4e-51da-48e9-9731-004c729fc44c","resolution":{"observed_at":"2026-05-11T13:56:04.802021Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2604.25813","last_updated":"2026-04-28T16:22:13Z","snapshot_observed_at":"2026-08-11T17:31:33.518155Z","submitted_at":"2026-04-28T16:22:13Z","title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","version":1},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-05-07T14:55:55.250283Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2604.25813"},"observation_digest":"sha256:bf307f4358ce4a3e70bfa3cab0fe8f0061c514aaabc39b8b029f2be558744930","observation_id":"a85abbf0-4e1b-45d4-8819-2f05486ae4b8","resolution":{"observed_at":"2026-05-12T00:36:16.078173Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2605.14044","last_updated":"2026-05-13T19:06:49Z","snapshot_observed_at":"2026-08-11T17:15:40.035827Z","submitted_at":"2026-05-13T19:06:49Z","title":"The Magnetic Origin of Primordial Black Holes: Ultralight PBHs and Secondary GWs","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-15T02:09:52.351925Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2605.14044"},"observation_digest":"sha256:d2e655ab57e3378994a3bc903dac727147f906f20f5e325416a7231254cca366","observation_id":"aaaebe36-a11f-4c74-a083-e954e1bd5bfb","resolution":{"observed_at":"2026-05-15T02:13:30.935133Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2606.06495","last_updated":"2026-06-04T17:59:59Z","snapshot_observed_at":"2026-08-08T14:37:47.002746Z","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":36,"source":"pdf_text","source_observed_at":"2026-06-27T23:47:15.644279Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2606.06495"},"observation_digest":"sha256:165a2bdb59195ef9cc83fee437cca098bab85b275579206961862a7142d1c163","observation_id":"605ad1de-8d1c-490e-baf2-4dec18353bfe","resolution":{"observed_at":"2026-07-02T15:37:06.490668Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":215,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:3fecb27729a9238a84c8783e2890f7004695541bc55eb26c2790a254863d1d41","observation_id":"b4061d2b-aca0-4373-9a33-48141cb82f47","resolution":{"observed_at":"2026-07-04T05:19:36.053102Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":215,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:0c61191af21848113640053988d87ed0dd94a8a3ef0e4b80736eadd624dece7d","observation_id":"13c43475-d99e-4def-b57b-f76b062ff1ba","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":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":"2004.09487","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-04T05:19:36.051419Z","title":"Relieving the Hubble tension with primordial magnetic ﬁelds","venue":null,"work_id":"4d2ebcf7-e5ce-40d7-9c03-9ed2c86cd454","year":2020},"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":182,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:b49d98283e435a1f2a958ea27b50ed48cd1d5ed45202261c81712891486f17f7","observation_id":"85c9db1b-1107-4230-beed-c5d60492d22c","resolution":{"observed_at":"2026-07-01T11:25:45.592162Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-07-14T16:44:02.461654Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.09732","last_updated":"2026-07-02T07:56:02Z","snapshot_observed_at":"2026-08-04T12:51:14.408110Z","submitted_at":"2026-07-02T07:56:02Z","title":"Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-14T16:44:02.461654Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2607.09732"},"observation_digest":"sha256:81dbb09c91d1370c89f40732e02d34d7ccb9c30479be6967d4e99715d7760011","observation_id":"1bca37ab-377a-4dc9-990e-906c8598d1a2","resolution":{"observed_at":"2026-07-14T16:44:02.461654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-02T05:41:41.905085Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.13282","last_updated":"2026-07-14T21:35:59Z","snapshot_observed_at":"2026-08-09T22:31:41.159100Z","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":105,"source":"pdf_text","source_observed_at":"2026-08-02T05:41:41.905085Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2607.13282"},"observation_digest":"sha256:5d496203a1f3a654a360ade8d34ea28a5e4a26b2662a9e3a76fac3cff4c3b652","observation_id":"6982466a-941e-4701-8979-dc7866eae830","resolution":{"observed_at":"2026-08-02T05:41:41.905085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-02T05:48:17.320760Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"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":128,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:17.320760Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:158e9954e037536b285c9574c81a7f9719235c26500837aeff7aef26245f56d6","observation_id":"113fd2a5-bbd2-4da9-8b75-860a4d813d49","resolution":{"observed_at":"2026-08-02T05:48:17.320760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-01T16:50:21.401560Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.17875","last_updated":"2026-07-20T12:21:07Z","snapshot_observed_at":"2026-08-08T12:33:19.084496Z","submitted_at":"2026-07-20T12:21:07Z","title":"Magnetically assisted primordial scalar perturbations: Scalar-Induced Gravitational Waves","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-01T16:50:21.401560Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2607.17875"},"observation_digest":"sha256:552dc389ac78480a4b99cdcdc6d4fe52b8326279b639c445afc7292f8589bef6","observation_id":"15a628cd-8264-416f-ab84-123afdceea1e","resolution":{"observed_at":"2026-08-01T16:50:21.401560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-01T08:08:38.097897Z","title":"Jedamzik and L","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-08T21:46:06.090866Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:38.097897Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:6392b4d4bc3f24235f012069f84ef33fafa634e35fa9633c826770ee9b1a7a01","observation_id":"3062bba6-9cc1-4a40-9196-27c833ebe27e","resolution":{"observed_at":"2026-08-01T08:08:38.097897Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-01T07:20:08.114249Z","title":"Relieving the Hubble tension with primordial mag- netic fields,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-07-23T16:45:10Z","snapshot_observed_at":"2026-08-09T21:28:10.481411Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":196,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:08.114249Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:c56ac0456ea8d7af68aa7ccaf51f726ef1899fb87633559bfb62c2f2601f2f3c","observation_id":"9f678026-da8e-43cd-914e-31e52709f077","resolution":{"observed_at":"2026-08-01T07:20:08.114249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09487","snapshot_observed_at":"2026-08-10T17:19:39.465918Z","title":", keywords =","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2608.06978","last_updated":"2026-08-07T08:55:46Z","snapshot_observed_at":"2026-08-12T06:10:38.781620Z","submitted_at":"2026-08-07T08:55:46Z","title":"Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-10T17:19:39.465918Z"},"links":{"cited_paper":"/paper/2004.09487","citing_paper":"/paper/2608.06978"},"observation_digest":"sha256:18c0123a6afe4b7fb793f3c20023cf9dccac2a9ca2875b89f4f07503625a1e39","observation_id":"9e99f7c0-dc41-49c7-b34b-cd6da3cdc67b","resolution":{"observed_at":"2026-08-10T17:19:39.465918Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2004.09487/citation-record","integrity":"/paper/2004.09487/integrity","json":"/paper/2004.09487/citation-record.json","paper":"/paper/2004.09487"},"outbound":[],"paper":{"arxiv_id":"2004.09487","last_updated":"2020-09-14T19:53:09Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-06T22:50:36.359621Z","submitted_at":"2020-04-20T17:59:51Z","title":"Relieving the Hubble tension with primordial magnetic fields"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 inbound Pith citation observations for arXiv:2004.09487."}