{"as_of":"2026-08-12T12:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e33b438325ff034ff054ac22dfc84fb084466a346aef7b199afc9c0258fe01ee","coverage":[{"denominator":120,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T12:59:39.191300Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2501.16492/citation-record","integrity":"/paper/2501.16492/integrity","json":"/paper/2501.16492/citation-record.json","paper":"/paper/2501.16492"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.712766Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.712766Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:0f596f5ed0edec695181cdad3e4bf0c274aa4e7f6b90fa54d23cb365721e13e9","observation_id":"5cbd6e82-fcb4-4fe1-922c-951b85222544","resolution":{"observed_at":"2026-08-10T12:59:38.712766Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.718113Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.718113Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:9096538b5e7ea3004b5f92147d3e09cc3db89d07c435344dc446e11e2b30e9f6","observation_id":"11ca24ec-598e-401c-80fc-debfd66c1fc1","resolution":{"observed_at":"2026-08-10T12:59:38.718113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.723754Z","title":"2V[ 4ZLOMa?\\⎽","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.723754Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:3a635faefcecb8906608c69518368b479548945027aede3aeb06301ccbe658b1","observation_id":"bc35f692-cb13-48e9-bdbb-370779fdbd9c","resolution":{"observed_at":"2026-08-10T12:59:38.723754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.781396Z","title":"G., et al., (1998), Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, The Astronomical Journal, 116(3), 1009","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.781396Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:ced0e084fd6ebd16cb08b149acb5f6d1fb615846e9aa36fb4df98aa3b5547684","observation_id":"c30bab41-f8c1-4162-a4c6-2d06ed6b5929","resolution":{"observed_at":"2026-08-10T12:59:38.781396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.787474Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.787474Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:ef12d34895169a420f3ad7dd4eb2583e5ef46e9ac0ae896af2bf47714a7bffab","observation_id":"16413ebb-a8ce-4b50-a568-4c8a49062ef0","resolution":{"observed_at":"2026-08-10T12:59:38.787474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.791839Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.791839Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:065a222694e2fe9ab731fe1fc3df2855d8d908237dab03f9ce9eb3149b74389a","observation_id":"16804894-f291-49e4-8828-f7b5a8cf2d80","resolution":{"observed_at":"2026-08-10T12:59:38.791839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.796887Z","title":null,"venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.796887Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:bcd93ef0151f9cf0134fe07209233612961603bdb5f660375ba197cc7b6e9207","observation_id":"f36cb2e9-2b83-4d09-a2c9-2de48f266aa8","resolution":{"observed_at":"2026-08-10T12:59:38.796887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.801280Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.801280Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:affece794966c8ff1413b23097ca13981aca68839d62106665c7c26667a25213","observation_id":"7b03f79e-6bde-4b6b-b86d-5a35bb42ad3f","resolution":{"observed_at":"2026-08-10T12:59:38.801280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.806119Z","title":"J., (1999), Quintessence, Cosmic Coincidence, and the Cosmological Constant, Physical Review Letters, 82(5), 896-899","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.806119Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:9583cf17ae9dd729c43f25a9f74844c97719695373ca84a1dc0796e9f3ee06fb","observation_id":"bea304d9-c48f-42cf-bb73-10435dc86026","resolution":{"observed_at":"2026-08-10T12:59:38.806119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.810289Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.810289Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:fca4ee49e5b7190a71da0863d1e126e494833945663b99fef4b89dcfb409b9cf","observation_id":"d7da76e8-2975-4d65-8ca5-06ac92155708","resolution":{"observed_at":"2026-08-10T12:59:38.810289Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.814658Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.814658Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:e19219abd554e538ebe074f430bb9950876bd467ef2b7737b040389a25a942cf","observation_id":"351d2b9e-f7f9-4bf2-aa6d-48567949ed7e","resolution":{"observed_at":"2026-08-10T12:59:38.814658Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0601213","last_updated":"2006-03-31T03:39:12Z","snapshot_observed_at":"2026-07-07T04:56:30.478178Z","submitted_at":"2006-01-29T22:31:37Z","title":"Introduction to Modified Gravity and Gravitational Alternative for Dark Energy","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0601213","snapshot_observed_at":"2026-08-10T12:59:38.818738Z","title":"and Odintsov S","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.818738Z"},"links":{"cited_paper":"/paper/hep-th/0601213","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:17081b1093aee891b398f06e5bbb08fef020868fff34f4f986ba36272bed56f9","observation_id":"52bc3091-1f33-4f83-914c-c6264c2ab4f0","resolution":{"observed_at":"2026-08-10T12:59:38.818738Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0307288","last_updated":"2003-09-19T07:45:56Z","snapshot_observed_at":"2026-07-07T04:47:52.261544Z","submitted_at":"2003-07-30T10:18:28Z","title":"Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0307288","snapshot_observed_at":"2026-08-10T12:59:38.823412Z","title":"D.,(2003), Phys","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.823412Z"},"links":{"cited_paper":"/paper/hep-th/0307288","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:73ade786907e9b47d3e9df1b6d307eba879aca13f04cbcffe9d8733b1537fe14","observation_id":"534d3de8-286e-4c1a-96d2-ffefd7a6b01e","resolution":{"observed_at":"2026-08-10T12:59:38.823412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1726","last_updated":"2010-06-04T00:50:27Z","snapshot_observed_at":"2026-07-06T01:37:50.026971Z","submitted_at":"2008-05-12T19:44:15Z","title":"f(R) Theories Of Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.1726","snapshot_observed_at":"2026-08-10T12:59:38.827811Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.827811Z"},"links":{"cited_paper":"/paper/0805.1726","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:2d50f86b39707990d29c9e30aae9e5c7422858eb77dd75bd347815a991589bc8","observation_id":"7981f016-ffc6-46de-a1fa-61fe657510a3","resolution":{"observed_at":"2026-08-10T12:59:38.827811Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.4928","last_updated":"2010-06-23T15:13:49Z","snapshot_observed_at":"2026-08-02T22:06:15.947617Z","submitted_at":"2010-02-26T07:01:02Z","title":"f(R) theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.4928","snapshot_observed_at":"2026-08-10T12:59:38.831928Z","title":"and Tsujikawa S.,(2010), Living Rev","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.831928Z"},"links":{"cited_paper":"/paper/1002.4928","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:ba504f9821a8e83df9c1d12cacf7cf2506ddf076f4010504676586d9c17a359a","observation_id":"0159d50e-ade9-44c3-9ada-7c4c5097b1e3","resolution":{"observed_at":"2026-08-10T12:59:38.831928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1108.6266","last_updated":"2011-09-02T14:20:59Z","snapshot_observed_at":"2026-08-03T18:01:11.531316Z","submitted_at":"2011-08-31T15:29:02Z","title":"Extended Theories of Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1108.6266","snapshot_observed_at":"2026-08-10T12:59:38.835970Z","title":"and De Laurentis M.,(2011), Phys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.835970Z"},"links":{"cited_paper":"/paper/1108.6266","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:8ec54080a4e651797aa1b20f02a47589a37e51d218b1fdb906e6c7ee83f42d81","observation_id":"080e6850-8ed3-46d4-a2f0-e70aa9faf682","resolution":{"observed_at":"2026-08-10T12:59:38.835970Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0201033","last_updated":"2002-01-10T17:42:19Z","snapshot_observed_at":"2026-07-07T03:15:16.005210Z","submitted_at":"2002-01-10T17:42:19Z","title":"Curvature Quintessence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0201033","snapshot_observed_at":"2026-08-10T12:59:38.840055Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.840055Z"},"links":{"cited_paper":"/paper/gr-qc/0201033","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:4ee85d820f0f45d62c6f9fae9a6913b71e8917b59ef923c6a713cbf52c620316","observation_id":"4fe44c9d-13c0-496c-8619-f6415b3b076f","resolution":{"observed_at":"2026-08-10T12:59:38.840055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0303041","last_updated":"2003-03-03T17:21:18Z","snapshot_observed_at":"2026-07-07T00:31:40.363455Z","submitted_at":"2003-03-03T17:21:18Z","title":"Quintessence without scalar fields","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0303041","snapshot_observed_at":"2026-08-10T12:59:38.844044Z","title":"and Troisi A., Recent Res","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.844044Z"},"links":{"cited_paper":"/paper/astro-ph/0303041","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:fc883854c2c467ef83f15706245275e4b53d624782ed7fe453f60ffeedde3a91","observation_id":"833b1559-359f-41e0-928c-2a6ecdc937e6","resolution":{"observed_at":"2026-08-10T12:59:38.844044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.853199Z","title":"M., 1993, ApJ, 413, L105","venue":null,"work_id":null,"year":1993},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.853199Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:2e58b5a81b6d7e7960d171754cf005feaf1033b10daaaa1ce931c4e2b7c706e0","observation_id":"44e386af-55e9-4d40-876a-1299befb4af7","resolution":{"observed_at":"2026-08-10T12:59:38.853199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.857468Z","title":"G., (1968), Comments on the Scalar-Tensor Theory, International Journal of Theoretical Physics, 1(1), 25–36, doi: 10.1007/BF00668828","venue":null,"work_id":null,"year":1968},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.857468Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:cab5ab95daa3b894dc88481a71d3ef7dd62da437d3ae587b6fa888bf3400a4fb","observation_id":"5ae22135-de84-46ec-ae1a-939fa58f4ef6","resolution":{"observed_at":"2026-08-10T12:59:38.857468Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.861696Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.861696Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:2aae20fb0eb63d6fbbaebdcbc46762e063318a9afd7b65706f46adefba3fdcbb","observation_id":"6e6b693b-27a7-4a94-b7c8-0744aca711b4","resolution":{"observed_at":"2026-08-10T12:59:38.861696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.865915Z","title":"A., (1970), Non-Linear Lagrangians and Cosmological Theory, Monthly Notices of the Royal Astronomical Society, 150(1), 1–8, doi: 10.1093/mnras/150.1.1","venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.865915Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:46fe1099b1f979aa29398d827b85c826ccfa91a5864ccc4bf1a5e9570adafdf8","observation_id":"7a0f0d0d-99b1-47d7-8722-8237a6243635","resolution":{"observed_at":"2026-08-10T12:59:38.865915Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.870099Z","title":"L., Tully R","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.870099Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:8b6277b4f46391450761ecd844b80c58e02a2566e8e6eaaa5bebf1ce0c5c9861","observation_id":"c53f5498-791b-4b84-8d4a-d2a24b13c613","resolution":{"observed_at":"2026-08-10T12:59:38.870099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1203.2290","last_updated":"2012-04-17T06:36:24Z","snapshot_observed_at":"2026-07-06T02:44:20.589849Z","submitted_at":"2012-03-08T17:56:09Z","title":"Cosmological measure with volume averaging and the vacuum energy problem","version":3},"cited_work":{"arxiv_id":"1203.2290","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.2290","snapshot_observed_at":"2026-08-10T12:59:40.024155Z","title":"Cosmological measure with volume averaging and the vacuum energy problem","venue":"gr-qc","work_id":"53f44b16-7cc6-4b02-a3b3-9fcf5f030b0d","year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.874134Z"},"links":{"cited_paper":"/paper/1203.2290","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:61c70dc56e5433f3973f42e3bd7643694888a87a39a4ededd7bfb8ec80ed2fc8","observation_id":"e3efe459-bfa6-4c6c-b53c-e333f0720a8f","resolution":{"observed_at":"2026-08-10T12:59:40.029075Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.878172Z","title":"& Burns, J.O., 1985, ApJ, 299, 5","venue":null,"work_id":null,"year":1985},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.878172Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:7c42699fb1d38013f245a46ba5169ce662e1c0a95e529eac98ea25c675ba7129","observation_id":"49918bc4-7d9a-4227-8bc8-cc95942b1c3e","resolution":{"observed_at":"2026-08-10T12:59:38.878172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0603240","last_updated":"2006-05-30T10:59:59Z","snapshot_observed_at":"2026-07-07T00:58:56.837254Z","submitted_at":"2006-03-09T17:55:04Z","title":"Dipole of the luminosity distance: a direct measure of H(z)","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0603240","snapshot_observed_at":"2026-08-10T12:59:38.882242Z","title":", Durrer R., and Kunz M.,(2006), Phys.Rev.Lett","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.882242Z"},"links":{"cited_paper":"/paper/astro-ph/0603240","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:465da85bed75eb8d5c3ebf80513dba438fcc17ad18c1eefac8392ff49c8e0456","observation_id":"2e77b418-66c9-4707-8425-cf0c9d67a98c","resolution":{"observed_at":"2026-08-10T12:59:38.882242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.886305Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.886305Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:6752c493b8f883e40856c0bd941c6638eee6e155d667794be910b64bba77d0c8","observation_id":"806b5e03-4642-4895-8314-6f859e908f44","resolution":{"observed_at":"2026-08-10T12:59:38.886305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1103.0007","last_updated":"2011-05-13T15:41:38Z","snapshot_observed_at":"2026-08-07T08:29:50.029418Z","submitted_at":"2011-02-28T21:00:02Z","title":"Too big to fail? The puzzling darkness of massive Milky Way subhaloes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1103.0007","snapshot_observed_at":"2026-08-10T12:59:38.890145Z","title":"415, L40?L44, [arXiv:astro-ph.CO/1103.0007]","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.890145Z"},"links":{"cited_paper":"/paper/1103.0007","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:77b13210be9f867b99ca999a61811a87425f74ae5eefd39538cc58cfcfa62f2c","observation_id":"fa3d16d5-a900-4613-927e-b6097a795c30","resolution":{"observed_at":"2026-08-10T12:59:38.890145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.2048","last_updated":"2012-03-21T16:16:26Z","snapshot_observed_at":"2026-08-12T09:46:29.894464Z","submitted_at":"2011-11-08T21:00:01Z","title":"The Milky Way's bright satellites as an apparent failure of LCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.2048","snapshot_observed_at":"2026-08-10T12:59:38.894084Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.894084Z"},"links":{"cited_paper":"/paper/1111.2048","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:c9ed6264a71710894b0d9caeaa8e95efa0733d2738ab5bcf2a1e84dbfad1fb0a","observation_id":"a8a33b9f-53b5-44cd-abfd-d07033cfba56","resolution":{"observed_at":"2026-08-10T12:59:38.894084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.898194Z","title":null,"venue":null,"work_id":null,"year":1970},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.898194Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:a59158fd381ddb238567b6b099948797c4260bc4112e9fee1ac9ae7fce0f6d8b","observation_id":"5f6ff6a6-fc17-4e04-988b-8da4f76f2c89","resolution":{"observed_at":"2026-08-10T12:59:38.898194Z","resolver_source":null,"status":"parse_uncertain"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.0961","last_updated":"2013-07-09T15:01:47Z","snapshot_observed_at":"2026-07-06T03:07:58.573900Z","submitted_at":"2013-03-05T09:22:38Z","title":"Constraining the Anisotropic Expansion of Universe","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.0961","snapshot_observed_at":"2026-08-10T12:59:38.902155Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.902155Z"},"links":{"cited_paper":"/paper/1303.0961","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:19727cd84edcd52545a247cc827f2e3eca785baf1d5b147f0b9eae66cb066fae","observation_id":"739892f4-7238-481d-b74f-aea9e33d3d13","resolution":{"observed_at":"2026-08-10T12:59:38.902155Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0706.1146","last_updated":"2007-07-16T15:29:42Z","snapshot_observed_at":"2026-07-06T01:28:25.918347Z","submitted_at":"2007-06-08T09:59:25Z","title":"Extended Theories of Gravity and their Cosmological and Astrophysical Applications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0706.1146","snapshot_observed_at":"2026-08-10T12:59:38.906406Z","title":"and Francaviglia M.,(2008) , Gen","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.906406Z"},"links":{"cited_paper":"/paper/0706.1146","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:fc3c995b59c6af3068c9a22811dea65ced134090ce95b3e2b07007365bd3beed","observation_id":"3dab6f93-e8a6-48a4-8530-fcb88c6ea4c5","resolution":{"observed_at":"2026-08-10T12:59:38.906406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1593","last_updated":"2013-06-07T06:10:20Z","snapshot_observed_at":"2026-07-06T03:08:08.856453Z","submitted_at":"2013-03-07T02:35:37Z","title":"Cosmological model with local symmetry of very special relativity and constraints on it from supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1593","snapshot_observed_at":"2026-08-10T12:59:38.910639Z","title":", Li M.-H","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.910639Z"},"links":{"cited_paper":"/paper/1303.1593","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:a08d4bfc1b03d8ab3e5dc02e5a0cd6e981dd4bbc558e69afc53a6cc811cc1ca9","observation_id":"ff5cd170-dc42-44b9-b69c-af6381bc61ba","resolution":{"observed_at":"2026-08-10T12:59:38.910639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.915206Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.915206Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:25a7eb047d78ed915c0c2954bcc0d9f93633c44a229381619f04df2e24ff95a3","observation_id":"72d3b90b-b992-4251-a19c-25167be91f8a","resolution":{"observed_at":"2026-08-10T12:59:38.915206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.919361Z","title":null,"venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.919361Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:00ec87b6c6af06532c0b430b7416f15390b1948ecdca78bd1a918c95a95404bd","observation_id":"e68d0171-8483-4c2a-859e-5f395c0a6310","resolution":{"observed_at":"2026-08-10T12:59:38.919361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.923376Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.923376Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:4f335da728da039ce2b5d74db08e047e93187170c7eab1066d611a22e375bc4e","observation_id":"0420dc17-a119-4979-a93f-ce55c7193bc5","resolution":{"observed_at":"2026-08-10T12:59:38.923376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.927585Z","title":null,"venue":null,"work_id":null,"year":1969},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.927585Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:8f892bcec13ac65fcebc29052ba314fe91f6ec45dca659942303bdf61253121e","observation_id":"80b54d5f-a54e-470f-97d5-2bc22b2c9785","resolution":{"observed_at":"2026-08-10T12:59:38.927585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.931882Z","title":"A., Strauss, M","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.931882Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:73f53906a6cdcfe72c0c50309858141f263dec7ff584229534814d4d4eef2788","observation_id":"8bc2747f-c9da-467d-b54b-8816f72e63a0","resolution":{"observed_at":"2026-08-10T12:59:38.931882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.935895Z","title":"1983, ARA&A, 21,109","venue":null,"work_id":null,"year":1983},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.935895Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:829bc5bdb22fe44436576ad3af39f6f06981535616846578b23d958e7f98a101","observation_id":"d046a1bc-7acf-454d-972c-f3ff97ddae29","resolution":{"observed_at":"2026-08-10T12:59:38.935895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.940118Z","title":"1982, ApJ, 254, 437","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.940118Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:8d5026f2e28091097e83db290280bbc778dd8b6753bae742dd2b37cf197ea913","observation_id":"34b95233-d9ac-42ca-a359-b4a1e5dad16e","resolution":{"observed_at":"2026-08-10T12:59:38.940118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.944259Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.944259Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:96e7b291c5d84317287eeb355467306cc0754fa3463740782e0f2b984bbacfa5","observation_id":"fe63bc47-f2cb-49e7-8eba-06ac236b40f9","resolution":{"observed_at":"2026-08-10T12:59:38.944259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.948662Z","title":"1987, ApJ, 313, L37","venue":null,"work_id":null,"year":1987},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.948662Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:0baf571761511b5c98a7f22765c8a32293170e3d6c97983c932538cb1dea3c20","observation_id":"ac3b312b-0905-447d-b0df-d79621b45642","resolution":{"observed_at":"2026-08-10T12:59:38.948662Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.952818Z","title":null,"venue":null,"work_id":null,"year":1915},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.952818Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:295144c750d93bb7562faa7bdeec0d49b87af42221c0fd8434b96204d2088143","observation_id":"47eadb2b-5e3e-49da-9eb7-90e0fc68e017","resolution":{"observed_at":"2026-08-10T12:59:38.952818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.956772Z","title":null,"venue":null,"work_id":null,"year":1917},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.956772Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:145613dd503a5b56482fe802fa91fa320db272cfcc997d9269730fd95db13019","observation_id":"6c9d150d-8710-489b-ab55-ac27360f22f9","resolution":{"observed_at":"2026-08-10T12:59:38.956772Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.960698Z","title":null,"venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.960698Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:700f895d0ce2d353adb3461d28963cb24e46ce9efe59a9a63c24bf8170fd7f59","observation_id":"a875073d-da7e-4e12-afc3-0169db794c6a","resolution":{"observed_at":"2026-08-10T12:59:38.960698Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.964579Z","title":"A., Watkins R., Hudson M","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.964579Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:e2fb1858c1eb06683be27bc2e63ad83fa449826b50367512505fd44dce091285","observation_id":"c02a0449-5bcc-4b9a-bad4-04d6bf5a6e4e","resolution":{"observed_at":"2026-08-10T12:59:38.964579Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.968475Z","title":"et al., 2013, AA, 560, A90","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.968475Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:f667ec4c199b25927b974785dec193b1a8563185e082b9d3731e073c190d400b","observation_id":"f0aafdc9-ad57-4a29-ac8d-0032fb6a3286","resolution":{"observed_at":"2026-08-10T12:59:38.968475Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.972109Z","title":"S., 1971, Nature, 231, 516","venue":null,"work_id":null,"year":1971},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.972109Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:049a1da8725c8ae518d69799bc6cfa14f46f80275d69cd905e9bcac9dd7f74ff","observation_id":"dc320586-deab-483d-b61e-cb44d3bfbde3","resolution":{"observed_at":"2026-08-10T12:59:38.972109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.976081Z","title":"et al., 2014, MNRAS, 445, 402392, 743","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.976081Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:35cd15179ce17a3cd07f609f1b79d6bdaf9545594a4ed4801072e5510fe71bef","observation_id":"6eafe515-cba4-411c-b2ec-8efdd8c8678a","resolution":{"observed_at":"2026-08-10T12:59:38.976081Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.980125Z","title":null,"venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.980125Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:bb81d0f9d82c499773d7108fcacd21665032ed1507676b2640be424c6c62f35c","observation_id":"66a52cc2-bcfc-4c5a-8bcf-ea06256e180b","resolution":{"observed_at":"2026-08-10T12:59:38.980125Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.983952Z","title":"J., Smith, R","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.983952Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:296b41b06e0f20673bd24b3f647d229b97bcdf2639dcc1e760eb5976143f4c48","observation_id":"becccb4a-13ee-46e1-9820-d9125de26b70","resolution":{"observed_at":"2026-08-10T12:59:38.983952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.988094Z","title":"Einasto, J., 1978, IAU Symp","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.988094Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:112f07ec23dd58266977cd482d79bbcd787aaeaee93483e122b24fd73111f1ac","observation_id":"1296d669-fa06-452d-b49c-90177dc6963e","resolution":{"observed_at":"2026-08-10T12:59:38.988094Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.992113Z","title":null,"venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.992113Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:3fa2b5210a9abf9dde2bbedf248687640909c01ac653b7aeb9cdd045fe55dd82","observation_id":"ec2f40f1-5763-4c54-9dca-b8a53794df92","resolution":{"observed_at":"2026-08-10T12:59:38.992113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:38.996315Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:38.996315Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:95a3929c7c496151c77ba506564ea6bafa74e252852a08c8f4571030d4a88cf2","observation_id":"aba46e9c-708d-4c97-820c-3862af227cfd","resolution":{"observed_at":"2026-08-10T12:59:38.996315Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:39.000381Z","title":", Kocevski D","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.000381Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:ec621741de8c39158b7e576ed0755d8eed71f6b81cb55d0a2fdf29bff988631a","observation_id":"331995fd-6ab2-4b05-80bb-ae0b4cfab1bf","resolution":{"observed_at":"2026-08-10T12:59:39.000381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:39.004465Z","title":"2009, ApJ, 691, 1479","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.004465Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:b330c91484719c1e0ad0939a386be994e3b33c42a5db5b46512794fc5706b5aa","observation_id":"6b07c2ff-ded6-471f-af8c-f0a788457dc0","resolution":{"observed_at":"2026-08-10T12:59:39.004465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:39.008721Z","title":", Ebeling H","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.008721Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:b95d10eb00d13fd7460ceeae3684726f30303162455bc2a6026a78bd13688c08","observation_id":"86aac2ed-81f4-4e68-be5b-96b36ac55f42","resolution":{"observed_at":"2026-08-10T12:59:39.008721Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.806463Z","title":"2011, ApJ, 732, 1","venue":null,"work_id":"c5ece98d-614b-4aa4-9bef-f492d81171bf","year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.016033Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:945e19eec64cba0a8ae99839a8571e8344de3830f0b48c60155af3662456c175","observation_id":"4318d634-c362-4713-a8ae-841be5797f04","resolution":{"observed_at":"2026-08-10T12:59:40.811358Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.791970Z","title":"2012, ArXiv e-prints","venue":null,"work_id":"5350b6ff-4f1b-4371-8a9f-ad43fb9f0807","year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.020251Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:fd18eb90fc9f9f99ece35401f38281d43ac591068254c4baaa4ead8b2b39f280","observation_id":"b2ce3658-383a-43a6-b123-d85cfde49945","resolution":{"observed_at":"2026-08-10T12:59:40.796441Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.777237Z","title":"et al., 1993, ApJ, 419, 1","venue":null,"work_id":"62c41ffb-8d6a-41ad-99b7-75bebe954cc6","year":1993},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.024488Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:81d75c656ec64d112cc522eb40945e5c4b19ebf90c7724659aafd972c67ff228","observation_id":"12b00f15-a5c0-4bc7-b80c-0edaa7355653","resolution":{"observed_at":"2026-08-10T12:59:40.781727Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:39.028660Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.028660Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:78c198fdf726765c5dc8f346cb749d0e0bba7f91704c4fcacd40f8f9ec35987b","observation_id":"a33d23ec-526c-48f3-92c6-3dcd4d1daa8c","resolution":{"observed_at":"2026-08-10T12:59:39.028660Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.753463Z","title":"1990, ApJ, 352,448","venue":null,"work_id":"5abb7335-69a8-4ef4-b5e2-5f21a81a630d","year":1990},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.032734Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:cdda1100345d8d355caea1945c51e0fe947e3f155a706043d75f4389a117d09f","observation_id":"bcd73ce9-496b-4996-b3bc-c68e3b6f5752","resolution":{"observed_at":"2026-08-10T12:59:40.757994Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.739256Z","title":"B., Mohayaee, R., & Colombi, S","venue":null,"work_id":"2ac75b4d-8aea-4299-93f7-74a85056f923","year":2010},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.036764Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:55f49b17fbf3a7defa7461df8cfe8084416587ccfe526260bcce008fb13d1abe","observation_id":"c9fbc984-4df8-456f-8f98-1bf765466f63","resolution":{"observed_at":"2026-08-10T12:59:40.743688Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.724389Z","title":null,"venue":null,"work_id":"b578fa9d-6f70-46b8-a1ac-a6965934dee5","year":null},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.040684Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:a600b8a97f2126f2f59e82667d5bd9bc7dec6c1b4e19032d69d7308e01d7b0d7","observation_id":"b54c046e-e417-43c4-9a70-c59f48d7a48a","resolution":{"observed_at":"2026-08-10T12:59:40.729257Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.710633Z","title":"M., Burstein D., Davies R","venue":null,"work_id":"652b6eec-edde-4785-bf08-bdfd214aeff1","year":1988},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.044773Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:ef562ceeeb69cc9f8a084a74b7e6e32f879d4fde1d713dc44d8b75d0cf53de99","observation_id":"ea2a57ee-01e8-48a3-80be-c5f89bd52c44","resolution":{"observed_at":"2026-08-10T12:59:40.714885Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.696542Z","title":"1989, MNRAS, 241, 325","venue":null,"work_id":"d0ae328f-cae3-433b-b378-899bb77d329f","year":1989},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.049152Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:bc3f640152d4863c9cd36a3aeea5ab63531b807828960c78ab80bc68eecef6d1","observation_id":"de5494bc-b52f-45e6-8ee1-e48838f07c5d","resolution":{"observed_at":"2026-08-10T12:59:40.701244Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.682261Z","title":"& Scott, D","venue":null,"work_id":"a794206f-201e-459a-aabc-54d12772a96a","year":2013},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.053253Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:4a32e755697c500e1b08910c7ee977128e1baab3923bf7b3b42f1bdee73a5f1f","observation_id":"78aba714-1c7e-4f24-accb-b5f5d5d71010","resolution":{"observed_at":"2026-08-10T12:59:40.687104Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.668298Z","title":"A., Ferreira P","venue":null,"work_id":"3e88825a-771c-47ed-80eb-1a75120f119c","year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.057214Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:284ee5025d50eb3b8d4474c5b307d15f5d10d653ee1fd8b27756d872dbccf285","observation_id":"be8b03a0-bdb8-4486-9953-0e72b65c715a","resolution":{"observed_at":"2026-08-10T12:59:40.672593Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1206.4055","last_updated":"2012-09-05T15:34:04Z","snapshot_observed_at":"2026-07-06T02:50:11.129175Z","submitted_at":"2012-06-18T20:00:29Z","title":"Is there Correlation between Fine Structure and Dark Energy Cosmic Dipoles?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.4055","snapshot_observed_at":"2026-08-10T12:59:39.061308Z","title":"and Perivolaropoulos L","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.061308Z"},"links":{"cited_paper":"/paper/1206.4055","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:535974c4d965f3e09935fa398c9f26eb68209ee633ee9581d7f064d403de07e1","observation_id":"de2ed78d-b0a9-4cce-bd83-52ed150dac2c","resolution":{"observed_at":"2026-08-10T12:59:39.061308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.3365","last_updated":"2012-05-15T13:36:21Z","snapshot_observed_at":"2026-08-10T20:42:41.294490Z","submitted_at":"2012-05-15T13:36:21Z","title":"Everything You Always Wanted To Know About The Cosmological Constant Problem (But Were Afraid To Ask)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.3365","snapshot_observed_at":"2026-08-10T12:59:39.065549Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.065549Z"},"links":{"cited_paper":"/paper/1205.3365","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:e857afff258b5c58e46ff4424df942c82adec691eff0791aafb6acdbd5f46ef7","observation_id":"a3c3177d-2dea-4a42-9a84-114007e3fd01","resolution":{"observed_at":"2026-08-10T12:59:39.065549Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.654156Z","title":null,"venue":null,"work_id":"063f07c5-9ebc-40c0-be98-e652e6a50656","year":1994},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.069822Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:0568a31c234387e76b771e5b554e311230f03c3e20bfb5fb9f94242466a7c7d5","observation_id":"50d4614f-0d72-40df-9f78-c50588b88feb","resolution":{"observed_at":"2026-08-10T12:59:40.658511Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"astro-ph/9903164","last_updated":"1999-03-11T01:02:43Z","snapshot_observed_at":"2026-07-07T01:25:03.823050Z","submitted_at":"1999-03-11T01:02:43Z","title":"Cold collapse and the core catastrophe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9903164","snapshot_observed_at":"2026-08-10T12:59:39.074061Z","title":null,"venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.074061Z"},"links":{"cited_paper":"/paper/astro-ph/9903164","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:3d3246a510d784a4eb67ee2317e3e6a5f7fb7641dbe19a296dc17f4d55437c61","observation_id":"fd86ee5b-f34b-4009-8182-0502fbc7a1e5","resolution":{"observed_at":"2026-08-10T12:59:39.074061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.640313Z","title":"& Davis, M","venue":null,"work_id":"492b9f3d-b601-485b-904d-2ce0df4da508","year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.078457Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:a2e5683269be699d8d1ef7704628b5ce87d3e7b5eeeecbf14eb59bc2bdfe4472","observation_id":"265acf90-d6fc-48eb-aa06-7fcd99aebf43","resolution":{"observed_at":"2026-08-10T12:59:40.644759Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.626559Z","title":"2011, ApJ, 735, 77","venue":null,"work_id":"968dabca-64ed-430a-9e08-15673c19ae6f","year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.082715Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:33568f92178e05295d5473d3b4767a3cc92b1ef95ad6177ec6a498694018b9eb","observation_id":"efac0984-c35e-464f-8c0d-e880745a8d1d","resolution":{"observed_at":"2026-08-10T12:59:40.630924Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"1011.2777","last_updated":"2011-04-15T14:58:26Z","snapshot_observed_at":"2026-07-06T02:19:05.048681Z","submitted_at":"2010-11-11T21:23:46Z","title":"The central slope of dark matter cores in dwarf galaxies: Simulations vs. THINGS","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1011.2777","snapshot_observed_at":"2026-08-10T12:59:39.087119Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.087119Z"},"links":{"cited_paper":"/paper/1011.2777","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:618cf1ef5627372ec753d34ce61f55c93f24b65327a68f6425b064e8ca0ca334","observation_id":"a9ce48fd-5429-4aae-be56-5310d98240ea","resolution":{"observed_at":"2026-08-10T12:59:39.087119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0306402","last_updated":"2003-06-19T19:39:10Z","snapshot_observed_at":"2026-07-07T00:34:15.172651Z","submitted_at":"2003-06-19T19:39:10Z","title":"New Light on Dark Matter","version":1},"cited_work":{"arxiv_id":"astro-ph/0306402","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0306402","snapshot_observed_at":"2026-08-10T12:59:39.877964Z","title":"New Light on Dark Matter","venue":"astro-ph","work_id":"20e157a4-2100-4640-80c8-0dbeb0d8ab74","year":2003},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.091727Z"},"links":{"cited_paper":"/paper/astro-ph/0306402","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:d57f7f29ffe653e121fa167f29e00a9ad6d8c18849a6faba65749908031a1b5d","observation_id":"bc1cb03a-f50c-415d-b13b-491a47873c3b","resolution":{"observed_at":"2026-08-10T12:59:39.882433Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.612700Z","title":null,"venue":null,"work_id":"212f094c-e4b4-499d-aa67-f336d5990deb","year":1981},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.096197Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:e72aef10cfa57c1117f0d1ee2cbc84d2b9e767b6d0dfce8279313f3dee23e2db","observation_id":"0d4d112c-a64d-4b02-82c6-85b447805154","resolution":{"observed_at":"2026-08-10T12:59:40.616921Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.599138Z","title":"et al.,(1999), ApJ, 517(2):565, 1999","venue":null,"work_id":"0ecc0a2e-7cc7-4c81-b440-c523f4e00843","year":1999},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.100351Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:cbb2433f721e01e10d66bafec1a8bb2da04a893976b1976658936433bf8d01fb","observation_id":"6c514fbe-e8c7-4612-b627-f0febcb54885","resolution":{"observed_at":"2026-08-10T12:59:40.603463Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":"astroph/9805201","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:39.855152Z","title":null,"venue":null,"work_id":"94917420-721b-48fb-9193-9be99f3b1d19","year":1998},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.104175Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:3c1da2770404f4525a7484c8ebec6742769b31bc8f9fe90583f51321b2567192","observation_id":"81196a3a-54f4-4263-8f7e-5bddaf4c3d7c","resolution":{"observed_at":"2026-08-10T12:59:39.862729Z","resolver_source":"raw_fallback","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.584970Z","title":"1990, MNRAS, 247, 1","venue":null,"work_id":"3a906748-836a-4bcf-a5ea-0c9131245c5a","year":1990},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.108169Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:b0fdb85da1ad7832947a165468a945c037d3cd3138006c2f0ce18f589af0f3d4","observation_id":"94a9d83e-7273-47d3-b27d-d77c31eab741","resolution":{"observed_at":"2026-08-10T12:59:40.589600Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.570937Z","title":"C., Edge, A","venue":null,"work_id":"47a70604-84e9-4bad-8cd5-a9b7f658e367","year":1991},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.112221Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:66e8b25b7aeeefb5187fd9cd6890854822e44e6ce42dfde3cc829bef98c6c3a3","observation_id":"462c842d-e75b-4a6d-a99a-2125919b8b08","resolution":{"observed_at":"2026-08-10T12:59:40.575419Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"2001.01743","last_updated":"2020-01-06T19:12:48Z","snapshot_observed_at":"2026-08-11T16:27:29.297676Z","submitted_at":"2020-01-06T19:12:48Z","title":"The cosmological bulk flow in QCDM model: (In)consistency with $\\Lambda CDM$","version":1},"cited_work":{"arxiv_id":"2001.01743","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.01743","snapshot_observed_at":"2026-08-10T12:59:39.680063Z","title":"The cosmological bulk flow in QCDM model: (In)consistency with $\\Lambda CDM$","venue":"astro-ph.CO","work_id":"a7b6e9e6-ff2d-4582-964b-275acad2ca8f","year":2020},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.116435Z"},"links":{"cited_paper":"/paper/2001.01743","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:08f7f7fde33460b51e354a62a854fcaa46800b65d2304144a3c4fa8f1fcf2ae6","observation_id":"4a33a873-948d-4a8a-87a0-d10e64396bca","resolution":{"observed_at":"2026-08-10T12:59:39.685023Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.557393Z","title":"1989, Nature, 338, 562","venue":null,"work_id":"1286f3ea-1bb3-4d6b-80c1-1fadd3bbc247","year":1989},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.120400Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:e472328a898c049144e459219a29a212423bcedb4a1a0fded9030c90f5205813","observation_id":"3646d7d1-7d1a-4c41-9ab3-12ae36c4ec53","resolution":{"observed_at":"2026-08-10T12:59:40.561684Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.544395Z","title":null,"venue":null,"work_id":"560adc92-9b40-485a-9efa-9d02b34d40c1","year":2018},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.124076Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:de0d8865ecfac1cc33af19097f427aefc6a7129c335c800b5c588df859b7d391","observation_id":"eaa90c40-e409-455c-a5f1-6430a0db5f7e","resolution":{"observed_at":"2026-08-10T12:59:40.548457Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.531440Z","title":null,"venue":null,"work_id":"f4e16877-e36c-4285-bef8-06501beaf3d6","year":2016},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.127819Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:3bc7f7b4ff96a80f09609c95dc8dbc24e74c691e317b2f2968262bb33a67babd","observation_id":"89655049-7b69-48fd-ba6b-a66b9364f097","resolution":{"observed_at":"2026-08-10T12:59:40.535521Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.517781Z","title":"1930, Harvard College Observatory Bulletin, 874, 9","venue":null,"work_id":"3ba6723a-892a-4f84-8009-69502e246749","year":1930},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.131973Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:8a254f33005fcae9aa4bd806c34e786f97fd327c5d3bf3bfe7a8e3090e818f0f","observation_id":"c282de56-33d2-40c4-a623-65851e9cfd2b","resolution":{"observed_at":"2026-08-10T12:59:40.522293Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.504313Z","title":"J., Peebles P","venue":null,"work_id":"0e71d078-33d9-4990-8179-d6534de3235f","year":1995},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.136016Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:62270f693f62766643e955c6495cd7d49ede1657becec2abecc697932e1e2954","observation_id":"e3f00827-e42d-427a-bb38-3600c8d40807","resolution":{"observed_at":"2026-08-10T12:59:40.508491Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.490727Z","title":null,"venue":null,"work_id":"30069222-cb33-4cb6-92c4-4f9daa82e8ba","year":2022},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.139925Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:88564f3e1a926fcb37fb06fdfa744feb01e92266f540a552cc118b578d1007a2","observation_id":"5fcd89b1-b23c-44f7-a702-d88a33c7fcfa","resolution":{"observed_at":"2026-08-10T12:59:40.495114Z","resolver_source":"raw_fallback","status":"unresolved"},"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":"1203.4197","last_updated":"2012-03-19T18:30:57Z","snapshot_observed_at":"2026-08-12T00:12:23.967540Z","submitted_at":"2012-03-19T18:30:57Z","title":"Is the Cosmological Coincidence a Problem?","version":1},"cited_work":{"arxiv_id":"1203.4197","doi":null,"metadata_source":"pith","pith_arxiv_id":"1203.4197","snapshot_observed_at":"2026-08-10T12:59:39.660354Z","title":"Is the Cosmological Coincidence a Problem?","venue":"astro-ph.CO","work_id":"34748a3f-cab1-4d36-bff0-0817e43d5f8c","year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.144057Z"},"links":{"cited_paper":"/paper/1203.4197","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:33d1d591b0ca0133257d45cd601b47e1c43857ebbe7da021f6c7ba4e14b9c51f","observation_id":"a19f21bf-29c8-46d4-9cbd-bd5b92a587ca","resolution":{"observed_at":"2026-08-10T12:59:39.665140Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.476968Z","title":"F., Gorenstein, M","venue":null,"work_id":"792f39ac-b235-4647-bbf0-e030c50bba59","year":1977},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.148781Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:78bd213ec292e09cf854d8038725d312881b4caf1a27151b4773b7d98a37ee6e","observation_id":"4c49e1e8-f69f-4486-8229-ba526fabf3f4","resolution":{"observed_at":"2026-08-10T12:59:40.481566Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.463615Z","title":"M., Masters K","venue":null,"work_id":"a609bb41-e514-4755-a2b7-b69c68fad443","year":null},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.152996Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:0c952f5c89fe5031015dd79d0be64589cad4edbb6381e046b304d6e428656e54","observation_id":"668e2885-6546-4e97-9e80-8a552cf3857c","resolution":{"observed_at":"2026-08-10T12:59:40.467978Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.450277Z","title":"A., (December 1979)","venue":null,"work_id":"80e17efd-49df-43fb-84ee-017d0e42373f","year":1979},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.157196Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:ea4db256efa4b22d108d72c4edeeab61da357e5a25434dc0cb820c7ea6525368","observation_id":"34c09121-b358-41b3-81e2-9acadd77d831","resolution":{"observed_at":"2026-08-10T12:59:40.454395Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.436899Z","title":"Huchra, John P","venue":null,"work_id":"ad508f0e-64b2-47f5-a89e-bafc9848eb86","year":1992},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.161379Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:f023f0dbf726b39bd3d7260a06f4d96a633c9b7e6ec72679b0045f99781ae574","observation_id":"a1d80f3c-0a22-4db6-a2f7-97abcc7821d2","resolution":{"observed_at":"2026-08-10T12:59:40.440964Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.423332Z","title":null,"venue":null,"work_id":"d7d9dd9a-5c74-4ba2-ac37-c158c553aaf7","year":1985},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.165656Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:6461f3a4c02e498a30ff870c184b67e805e9edb66249aadd02e3f757be5478f3","observation_id":"e6b2f1b0-3944-4535-9db9-6be6f6800de8","resolution":{"observed_at":"2026-08-10T12:59:40.427682Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.408438Z","title":null,"venue":null,"work_id":"98bd065d-eeb0-4826-95f1-5cfe910707bd","year":1981},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.169972Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:1a6e677a0aec5707bea8ea5f409b7abd746bf7aa35b351dd3d57456c2a96dfc8","observation_id":"d139e913-57e9-49a0-a8f1-ddae3fcd9ce0","resolution":{"observed_at":"2026-08-10T12:59:40.412903Z","resolver_source":"raw_fallback","status":"unresolved"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.394480Z","title":"B., Shaya E","venue":null,"work_id":"f79f9d7f-9612-438f-8c12-726e46f0a7c6","year":2008},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.174014Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:4272fe0564377a7fb1bda04585faa8e2698fe73851a4e20d42b781b73975a6f8","observation_id":"3ccfd701-caad-4241-b8e9-6868277988cf","resolution":{"observed_at":"2026-08-10T12:59:40.398898Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.380824Z","title":"J., Hudson, M","venue":null,"work_id":"357097ee-1b60-4206-8e6e-1fcb64018b32","year":2012},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.178160Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:d2cdf3f1f0822f4b8c39377a41c45ca6370c8e404ecfdd32eaf7582143c6e0ee","observation_id":"cd53d93a-e968-4f50-b87c-018ad74fae31","resolution":{"observed_at":"2026-08-10T12:59:40.385105Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":"0908.2243","last_updated":"2009-08-16T13:58:30Z","snapshot_observed_at":"2026-08-11T12:23:26.698995Z","submitted_at":"2009-08-16T13:58:30Z","title":"Tests of General Relativity on Astrophysical Scales","version":1},"cited_work":{"arxiv_id":"0908.2243","doi":null,"metadata_source":"pith","pith_arxiv_id":"0908.2243","snapshot_observed_at":"2026-08-10T12:59:39.638706Z","title":"Tests of General Relativity on Astrophysical Scales","venue":"astro-ph.CO","work_id":"2da91184-806b-49ea-9b34-d5ab0a99b2c6","year":2009},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.182552Z"},"links":{"cited_paper":"/paper/0908.2243","citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:aff0b8139222089d227f5e5d5e97c0346c3bdfbd039edf67e1146eb4ac136230","observation_id":"8b8e64d7-251e-4d84-a2e6-20798d10c659","resolution":{"observed_at":"2026-08-10T12:59:39.644741Z","resolver_source":"local_arxiv","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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.366713Z","title":",(2009), Lect.Notes Phys.800:147-177,2010","venue":null,"work_id":"d390b940-09ca-4577-afaa-d0f222d80e45","year":2009},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.187140Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:087bca930835808b5672a35b654050eb0c19b6edfbdefad746c49a0529d1eaf7","observation_id":"9893b3b8-a29b-4c1a-8f21-8334e9f1e97f","resolution":{"observed_at":"2026-08-10T12:59:40.371456Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T12:59:40.352422Z","title":"1987, ApJ, 322, 37","venue":null,"work_id":"604ccba3-d85a-4e1b-a426-9c0c17eb225b","year":1987},"citing_paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-10T12:59:39.191300Z"},"links":{"citing_paper":"/paper/2501.16492"},"observation_digest":"sha256:d104f719e875d755143f0297d979b08be5775fc96aa0ed03b49ac9232b292aad","observation_id":"a8f5e230-5604-49f0-ad16-2f4d2c953154","resolution":{"observed_at":"2026-08-10T12:59:40.356663Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"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"}}],"paper":{"arxiv_id":"2501.16492","last_updated":"2025-01-27T20:50:35Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-11T12:37:31.313130Z","submitted_at":"2025-01-27T20:50:35Z","title":"Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":1,"unresolved":68,"verified_exact":5,"verified_fuzzy":25},"total_outbound_references":120},"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 100 of 120 outbound references and 0 inbound Pith citation observations for arXiv:2501.16492."}