{"as_of":"2026-08-17T05:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:dcb9f19c0f273e2f37438ad73319cb37e9b88eac535058cf6579c48f3e5fea47","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":"2026-08-16T06:30:59.297886+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":"2026-08-16T11:38:47.360879Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T20:07:33.199644Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"citing_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-08-16T02:36:16.088814Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"reference_index":189,"source":"pdf_text","source_observed_at":"2026-05-15T11:50:20.600831Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2103.01183"},"observation_digest":"sha256:7e0522eaabdad166869a4cfbb2ce10ac713198e67945ceb67941bd1138f30889","observation_id":"162c0d7b-4563-4d57-98b2-adac7231067b","resolution":{"observed_at":"2026-05-15T11:50:21.439237Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"citing_paper":{"arxiv_id":"2411.03773","last_updated":"2026-05-07T16:04:58Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-11-06T09:10:25Z","title":"Model-independent calibration of Gamma-Ray Bursts with neural networks","version":3},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-05-23T17:55:16.089703Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2411.03773"},"observation_digest":"sha256:32685bfba875adc5523d30bffd12f1bb1f55c02080bc112b2a8dcd131c7d873d","observation_id":"74d65fa3-f12d-4420-8471-4b5f50e7409e","resolution":{"observed_at":"2026-05-23T17:55:44.535619Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-12T04:57:06.685560Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.00931","last_updated":"2025-02-15T06:07:09Z","snapshot_observed_at":"2026-08-17T04:11:55.502412Z","submitted_at":"2024-12-01T18:41:32Z","title":"Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T04:57:06.685560Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2412.00931"},"observation_digest":"sha256:2330c36f271dc373e4789c2c856f07f293cac7867734a9d9e24cb72ab69467f0","observation_id":"e6b94e21-4f0a-4a30-bbdc-770e1b0c224c","resolution":{"observed_at":"2026-08-12T04:57:06.685560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-11T12:00:12.102201Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.14750","last_updated":"2024-12-19T11:29:57Z","snapshot_observed_at":"2026-08-13T16:22:12.867394Z","submitted_at":"2024-12-19T11:29:57Z","title":"Deep Learning Based Recalibration of SDSS and DESI BAO Alleviates Hubble and Clustering Tensions","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T12:00:12.102201Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2412.14750"},"observation_digest":"sha256:9fc105bf702658988c46809986d57c7b05dd80acfa92e42e4e9ec82ea563a225","observation_id":"9806b077-c90e-4cf9-90ab-856dea67c789","resolution":{"observed_at":"2026-08-11T12:00:12.102201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-11T00:53:46.992915Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.19240","last_updated":"2025-04-23T01:47:03Z","snapshot_observed_at":"2026-08-15T19:41:56.137910Z","submitted_at":"2024-12-26T14:51:09Z","title":"Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T00:53:46.992915Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2412.19240"},"observation_digest":"sha256:ae80c8e50dd62cfdd7afd5a824a740fbf414f243fc98d0f2f4fed73b75412578","observation_id":"0b2d2965-99f1-4962-97e0-5f848496eaf6","resolution":{"observed_at":"2026-08-11T00:53:46.992915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-16T11:38:47.360879Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.15127","last_updated":"2025-07-12T01:39:19Z","snapshot_observed_at":"2026-08-16T18:33:40.770191Z","submitted_at":"2025-04-21T14:22:41Z","title":"Reconstructing the redshift evolution of Type Ia supernovae absolute magnitude","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-16T11:38:47.360879Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2504.15127"},"observation_digest":"sha256:beecb8afeb5ec8b6620e1825d24187db03c1c65ad32de7b5a0adc5817af42adb","observation_id":"addeee3a-7504-42c5-bd5c-a42b5ae47efd","resolution":{"observed_at":"2026-08-16T11:38:47.360879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-03T18:51:50.045588Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"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":116,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:50.045588Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:d532fab10082e054bd3a02eb89b22e19f8cacec053df02797162fa670856411c","observation_id":"f1c012da-5b3a-4f46-9cff-43380bf7b0eb","resolution":{"observed_at":"2026-08-03T18:51:50.045588Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"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":146,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:3ae0ee8f3456c3ca81be84a45dfd4611a500fb04e595f4acdec06594c19c91ea","observation_id":"2b798510-7c0f-45c5-b76f-1c32b0ecece6","resolution":{"observed_at":"2026-05-14T23:13:15.361171Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"citing_paper":{"arxiv_id":"2603.27616","last_updated":"2026-04-09T07:03:12Z","snapshot_observed_at":"2026-07-06T22:51:00.579062Z","submitted_at":"2026-03-29T10:21:42Z","title":"Model-independent test of the cosmic distance duality relation with recent observational data","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-14T22:11:51.900263Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2603.27616"},"observation_digest":"sha256:f233f29c695ea170a4015f9cd103d452410f9f20c0a7b803ba80ea3022376f5e","observation_id":"7443b3e0-5f51-4859-934d-d69aa65c92be","resolution":{"observed_at":"2026-05-14T22:13:04.454519Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"citing_paper":{"arxiv_id":"2604.28013","last_updated":"2026-04-30T15:31:57Z","snapshot_observed_at":"2026-08-10T23:20:14.168556Z","submitted_at":"2026-04-30T15:31:57Z","title":"Cosmological intercept tension","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-07T05:59:51.789689Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2604.28013"},"observation_digest":"sha256:23b1bb14e100bdef8be96dddcd4a4a01923e39fb0e6dd2ee2738b99e3dbdc08c","observation_id":"c8fa934d-e577-4ddb-bf2c-0355177605a6","resolution":{"observed_at":"2026-05-12T10:26:30.965359Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"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":68,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:cd98d5bbf5e552cd5ce29e6cc1bac1e7f904582247b5e833e54d2c9706261724","observation_id":"3b3502d4-b592-45a9-856e-2ee33d838066","resolution":{"observed_at":"2026-07-04T05:19:36.011548Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"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":68,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:29af00c4da0ab03992b9280762bd79c99d4c1691c2bc91dd7b54a3089000d356","observation_id":"5cd4ecd8-7847-4587-8289-dd3b0b16d97a","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":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":"2101.08641","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-07-10T20:07:33.199644Z","title":"Camarena and V","venue":"astro-ph.CO","work_id":"5c844276-0f07-4144-b9e2-25a8513e5174","year":2021},"citing_paper":{"arxiv_id":"2607.06959","last_updated":"2026-07-08T03:35:59Z","snapshot_observed_at":"2026-08-17T04:57:28.562156Z","submitted_at":"2026-07-08T03:35:59Z","title":"KAN-LSTM-Transformer Neural Networks, MFV and Cosmological Parameters","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2607.06959"},"observation_digest":"sha256:07af8b4065e3f69a097effb54b1a7743db1974b1af1712c09132797dee123653","observation_id":"daa58351-459a-4abe-9792-7b3eae746355","resolution":{"observed_at":"2026-07-10T20:07:33.200927Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-02T05:48:24.134646Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"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":200,"source":"pdf_text","source_observed_at":"2026-08-02T05:48:24.134646Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2607.13283"},"observation_digest":"sha256:b8744a86058773c77f4cd834cdb277d12655d5c945e30ccc7db4f2874f500b62","observation_id":"ea928d4b-1fc3-432c-a01e-6bb283ab1f4f","resolution":{"observed_at":"2026-08-02T05:48:24.134646Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-01T08:08:54.700985Z","title":"Camarena and V","venue":null,"work_id":null,"year":2021},"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":207,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:54.700985Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:6cbd3f44319af1a7ecc18c663cf609beb79d8b53930c09f069d81e75f9876e21","observation_id":"f37513d0-d297-4360-98d3-2ecf4c5dff41","resolution":{"observed_at":"2026-08-01T08:08:54.700985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.08641","snapshot_observed_at":"2026-08-01T07:20:07.596914Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-08-14T16:46:31Z","snapshot_observed_at":"2026-08-17T04:12:21.368593Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:07.596914Z"},"links":{"cited_paper":"/paper/2101.08641","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:fc5c2e9d5c75cc5e1347130075c581f15b2640176f7364144ce459c235c365e0","observation_id":"36811469-731f-4963-813b-66b2ace0168b","resolution":{"observed_at":"2026-08-01T07:20:07.596914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2101.08641/citation-record","integrity":"/paper/2101.08641/integrity","json":"/paper/2101.08641/citation-record.json","paper":"/paper/2101.08641"},"outbound":[],"paper":{"arxiv_id":"2101.08641","last_updated":"2021-04-24T01:34:24Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T18:50:54.250616Z","submitted_at":"2021-01-21T14:41:23Z","title":"On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2101.08641."}