{"as_of":"2026-08-11T16:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:99570d7ac0ba21d702d5f5b239bbd01f61893899b569e660fdc6772d6d94bc9e","coverage":[{"denominator":39,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":39,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T12:56:51.730105Z","state":"measured"},{"denominator":39,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":39,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+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/2507.21359/citation-record","integrity":"/paper/2507.21359/integrity","json":"/paper/2507.21359/citation-record.json","paper":"/paper/2507.21359"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T12:56:52.047690Z","title":"Such transitions are highly sensitive to the parameterninF(R, T) =R+αT n, indicating that small deviations from 12 GR (n= 1) have rich phenomenological consequences","venue":null,"work_id":"7a02c5c4-5cff-44e5-ba5a-841221c6df0e","year":null},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.015187Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:be6be82450546adc88d5e71c983f2352b232acf79a89049542d6b812b23a4047","observation_id":"278f2415-970c-4089-91ed-9e653cc6e1b3","resolution":{"observed_at":"2026-08-06T12:56:52.050446Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:48.081370Z","title":"Particle Dark Matter: Evidence, Candidates and Con- straints,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.081370Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:8df81c839072fbf3ae0b25f694df252b7fd49ab4a313db53068852701f656fe2","observation_id":"cc187586-700a-48f5-941b-d7e4342bb338","resolution":{"observed_at":"2026-08-06T12:56:48.081370Z","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":"2026-08-06T12:56:48.182296Z","title":"Dark Matter Candidates from Particle Physics and Methods of Detection,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.182296Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:e03a618ae1544783c059bd9f780ec9af3c63c1a95ff0cc2c5d5b15d3b320211b","observation_id":"66db6b40-d069-4a6a-87e9-351841efe390","resolution":{"observed_at":"2026-08-06T12:56:48.182296Z","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":"2026-08-06T12:56:48.383199Z","title":"Small-Scale Challenges to the ΛCDM Paradigm,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.383199Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:b994962b3bd592f8cff7fb67ee2c6115d64449b1c0cd77126c98cf57a5a604b3","observation_id":"5df48603-80d3-4ec1-99a0-39675a4ef64a","resolution":{"observed_at":"2026-08-06T12:56:48.383199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.2476","last_updated":"2012-03-12T12:39:47Z","snapshot_observed_at":"2026-07-06T02:29:12.672489Z","submitted_at":"2011-06-13T16:06:49Z","title":"Modified Gravity and Cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.2476","snapshot_observed_at":"2026-08-06T12:56:48.572118Z","title":"Modified Gravity and Cosmology,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.572118Z"},"links":{"cited_paper":"/paper/1106.2476","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:816eec101a287bae188336e86352a626e1490bec3bf7a880050c0a878e8204a6","observation_id":"9d013353-53dd-41bd-b64b-cef229a0f75e","resolution":{"observed_at":"2026-08-06T12:56:48.572118Z","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":"2026-08-06T12:56:48.766961Z","title":"Extended Theories of Gravity,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.766961Z"},"links":{"cited_paper":"/paper/1108.6266","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:42ee6c09433e9608c1e7811952dbb226d4b04b1188245c34e43e1418f0c3ef04","observation_id":"e89a2ee6-3e48-400b-82b3-a1cb08554bf6","resolution":{"observed_at":"2026-08-06T12:56:48.766961Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.1039","last_updated":"2012-11-17T21:07:09Z","snapshot_observed_at":"2026-08-09T04:25:21.716850Z","submitted_at":"2012-06-28T18:51:56Z","title":"FRW Cosmology in F(R,T) gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.1039","snapshot_observed_at":"2026-08-06T12:56:48.927857Z","title":"Myrzakulov, Eur","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:48.927857Z"},"links":{"cited_paper":"/paper/1207.1039","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:54a8db5ca1fe2d40f9c13243374bbc71557d7dae65572fc92809ac5833ac8d8b","observation_id":"d0eb0c67-189c-4374-ad54-0f69fb8a83a5","resolution":{"observed_at":"2026-08-06T12:56:48.927857Z","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":"2026-08-06T12:56:49.110341Z","title":"f(R,T) gravity,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:49.110341Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:69e6a095441ff4c34e4fa3e1582fa55017474de0eb123893f79daf76d30fd3bb","observation_id":"83da963c-867d-4cec-98de-890d4e5fbabe","resolution":{"observed_at":"2026-08-06T12:56:49.110341Z","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":"2026-08-06T12:56:52.037053Z","title":"Myrzakulov Gravity in Vielbein Formalism: A Study in Weitzenb¨ ock Spacetime,","venue":null,"work_id":"dc01288d-0d45-4b1d-b540-efedb11e4f53","year":2025},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:49.288429Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:51fd4dd58c7e60b7f9b91acd7c89f43e55ff459218c2b9fb7bbb991b8a0231ad","observation_id":"b27c27ae-9762-4c06-9e54-45dec899064e","resolution":{"observed_at":"2026-08-06T12:56:52.039309Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:52.030741Z","title":"Metric-Affine Myrzakulov Gravity Theories: Models, Appli- cations and Theoretical Developments,","venue":null,"work_id":"6c45ee82-2669-44b1-88b7-b27a09b18595","year":2025},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:49.510280Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:07fd386ecb6e70b3695dcf6a299919e0dca3235a29469b997bc74d65be05443d","observation_id":"f85b1bf7-7029-4e78-8063-201d939f0dbe","resolution":{"observed_at":"2026-08-06T12:56:52.033193Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:52.024314Z","title":"Einstein–Gauss–Bonnet–Myrzakulov gravity fromR+ F(T, G),","venue":null,"work_id":"815c26ff-0a69-4ea4-9b90-bd4842c7dc8f","year":2025},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:49.690536Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:b0dd0d57ebdac59a377a3b8dc1392252ff89dba86a3cc5330d071737d7ac26aa","observation_id":"39b50410-2362-4707-91c7-40f038bae1ac","resolution":{"observed_at":"2026-08-06T12:56:52.026679Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:52.018575Z","title":"f(T) Teleparallel Gravity and Cosmology,","venue":null,"work_id":"19f99dc6-13bf-4056-b3dd-e8d8e4055ab3","year":2016},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:49.859120Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:8ac12d3cc9b92b81d5d556d91a947937f128d390fd6f4c702194e4f2f04d89fa","observation_id":"d44a0dd8-a383-487d-9f55-e65d1a4454a9","resolution":{"observed_at":"2026-08-06T12:56:52.020591Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:52.012742Z","title":"Teleparallel Palatini Theories,","venue":null,"work_id":"d736940f-551c-4df2-95d7-86fc8147f57b","year":2018},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.031387Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:7aca2de794fb469959e5bcc03f1166153b29369b4b07c7d541aea8f95d09c290","observation_id":"151a3df8-8fa1-4bed-a47c-cbe665bd6bc3","resolution":{"observed_at":"2026-08-06T12:56:52.014750Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.985322Z","title":"Dark Energy Survey Year 1 Results,","venue":null,"work_id":"379c6b9a-1659-43df-9206-da2e857d76ce","year":2018},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.144082Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:a84f19f087e7cfc8e28a1a661a91680ab34dcac49144082cec94aa0998652444","observation_id":"b75c29e0-2d48-46e8-9360-70bb5ef08624","resolution":{"observed_at":"2026-08-06T12:56:52.008855Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.964025Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":"5b90ca33-bbb5-4e68-8a1b-5905d9199d37","year":2020},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.223639Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:86950f76d82934c67a402aa34bc9cd0f6b90022a422b9eed39deea73c22b60bd","observation_id":"81f529e8-6f12-4c99-bb29-664f8c9371ec","resolution":{"observed_at":"2026-08-06T12:56:51.973308Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.938507Z","title":"Modified teleparallel gravity: Inflation without inflaton,","venue":null,"work_id":"9bc46d7b-1900-4735-b433-d1df1da07c80","year":2007},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.297889Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:c3b8df516ad4915f3ed37937314a237c2421f7e936a48dd5b55feea844357eaf","observation_id":"f7ab4bc3-a08f-4013-bf4c-462e75b8661c","resolution":{"observed_at":"2026-08-06T12:56:51.947950Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1309.3269","last_updated":"2014-08-11T12:06:47Z","snapshot_observed_at":"2026-07-06T03:22:53.179183Z","submitted_at":"2013-09-12T04:45:53Z","title":"Warm Intermediate Inflation in $F(T)$ Gravity","version":3},"cited_work":{"arxiv_id":"1309.3269","doi":null,"metadata_source":"pith","pith_arxiv_id":"1309.3269","snapshot_observed_at":"2026-08-06T12:56:51.827670Z","title":"Warm Intermediate Inflation in $F(T)$ Gravity","venue":"gr-qc","work_id":"b152bae8-8057-4ad3-976c-9d476a067f13","year":2013},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.352172Z"},"links":{"cited_paper":"/paper/1309.3269","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:84b6c34f7c67392888855460319319fca81529dc1c6d0e13b39d81e3b45cc722","observation_id":"8d38c35f-0f7d-475b-84f5-ee424dc06248","resolution":{"observed_at":"2026-08-06T12:56:51.830152Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.12296","last_updated":"2024-10-16T06:55:36Z","snapshot_observed_at":"2026-07-06T19:34:23.353138Z","submitted_at":"2024-10-16T06:55:36Z","title":"Warm non-minimally coupled Peccei-Quinn Inflation and de Sitter Swampland Conjecture","version":1},"cited_work":{"arxiv_id":"2410.12296","doi":null,"metadata_source":"pith","pith_arxiv_id":"2410.12296","snapshot_observed_at":"2026-08-06T12:56:51.818301Z","title":"Warm non-minimally coupled Peccei-Quinn Inflation and de Sitter Swampland Conjecture","venue":"gr-qc","work_id":"db290a15-9277-4214-911a-760d1e996ba7","year":2024},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.439923Z"},"links":{"cited_paper":"/paper/2410.12296","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:3b2f18c3a81e2c85ac0accd2c8bd3b8f741da3072c59ff8b69183669ade26931","observation_id":"72f7227b-5498-4d58-ac9b-8e7090b547eb","resolution":{"observed_at":"2026-08-06T12:56:51.820941Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.04174","last_updated":"2024-08-01T23:03:34Z","snapshot_observed_at":"2026-07-06T18:10:53.622248Z","submitted_at":"2024-05-07T10:19:18Z","title":"Gravity Rainbow Effects on Higher Curvature Modification of R2 inflation","version":3},"cited_work":{"arxiv_id":"2405.04174","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.04174","snapshot_observed_at":"2026-08-06T12:56:51.808782Z","title":"Gravity Rainbow Effects on Higher Curvature Modification of R2 inflation","venue":"gr-qc","work_id":"ef63cbd2-fe4e-45f1-b958-62b80a368dfd","year":2024},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.516496Z"},"links":{"cited_paper":"/paper/2405.04174","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:515041dfaccbb65298dfe98209f63602d90f43002272c0431b76ef1ec824d285","observation_id":"95e256f7-5f12-4f61-802c-bc9090b75fdc","resolution":{"observed_at":"2026-08-06T12:56:51.811445Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.00572","last_updated":"2023-07-08T04:04:12Z","snapshot_observed_at":"2026-08-11T09:34:53.091770Z","submitted_at":"2023-03-01T15:16:23Z","title":"Nonminimally-coupled warm Higgs inflation: Metric vs. Palatini Formulations","version":2},"cited_work":{"arxiv_id":"2303.00572","doi":null,"metadata_source":"pith","pith_arxiv_id":"2303.00572","snapshot_observed_at":"2026-08-06T12:56:51.796992Z","title":"Nonminimally-coupled warm Higgs inflation: Metric vs. Palatini Formulations","venue":"gr-qc","work_id":"4198f215-3343-455d-a9de-e46da5fe753a","year":2023},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.585722Z"},"links":{"cited_paper":"/paper/2303.00572","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:4b22118d643abdf3741f553cff1b45693d1f20b95118a614876b81dfc5cd5b73","observation_id":"ac0b99ab-932f-41f0-803b-26e8e95d1f8b","resolution":{"observed_at":"2026-08-06T12:56:51.801684Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.932043Z","title":"Modified gravity with negative and positive powers of the curvature,","venue":null,"work_id":"e93ee0dc-e908-4289-abe1-26e569267139","year":2003},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.661401Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:d98d44dbf6428281ca4878c4af32f80d02eb21e7906d933febd4ce44c3b5a5de","observation_id":"32c929a5-0f93-49e6-b426-26e9068b7ef5","resolution":{"observed_at":"2026-08-06T12:56:51.934177Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.926128Z","title":"Introduction to modified gravity and gravitational alternative for dark energy,","venue":null,"work_id":"e5e3f3c8-1afc-4823-b642-eb783c5150c8","year":2007},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.789686Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:037a97909517357ab448b367ac6699c63fe73a9084c48865ab7628d1e2aa7af6","observation_id":"4ee3fde3-bdf2-464b-a2e4-e1d2052d452d","resolution":{"observed_at":"2026-08-06T12:56:51.928389Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.920111Z","title":"Cosmographic analysis with Chebyshev poly- nomials,","venue":null,"work_id":"2967b353-0b29-4a5a-baa6-785511aa7019","year":2018},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.873560Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:1fe13a87f2428214b4066db0f3c6d5bafd6f60a5224c8bcf41b9d68eeb721cbe","observation_id":"2b776e0a-cb8e-4859-8e4a-1ebe969f7877","resolution":{"observed_at":"2026-08-06T12:56:51.922379Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.912580Z","title":"Dark torsion as the cosmic speed-up,","venue":null,"work_id":"f7a8e205-a760-4770-b238-c019771ca1fd","year":2009},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:50.963577Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:ab0125de66efbcbd537a8be814d6545604d034d1e322b168a94e3b9239db2309","observation_id":"75e0a5fd-6710-4eb6-bfb2-39ef6ada0a01","resolution":{"observed_at":"2026-08-06T12:56:51.915013Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.906091Z","title":"The Confrontation between General Relativity and Experiment,","venue":null,"work_id":"843ecd70-e711-4746-bfa5-930507151279","year":2014},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.105594Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:e4c2e53d271cee0913ea37c4796b703812cfda30cab4f96dcab6844cca18c997","observation_id":"807845d4-16ce-489d-b809-7ca7b8291720","resolution":{"observed_at":"2026-08-06T12:56:51.908289Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.899829Z","title":"Testing General Relativity with Present and Future Astrophysical Observa- tions,","venue":null,"work_id":"f1ce5f62-7060-4f6a-9542-97384e8adb2e","year":2015},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.249437Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:435c18d2cbd38c837276e200c1ad6320ff08ebccca44d0255f1c1ede58d6cf44","observation_id":"5317c7e2-5fd2-400d-9e85-c2377b6e0e9d","resolution":{"observed_at":"2026-08-06T12:56:51.902087Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.893679Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger,","venue":null,"work_id":"8b5d448c-4def-4fed-b137-21319745ddb1","year":2016},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.351147Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:86910dcb6dfcd8d31d9591497c075ada448a38cd39d97f3429303d9a28af7835","observation_id":"4ed28d6f-b89d-4ae2-b0d6-04cd609b2174","resolution":{"observed_at":"2026-08-06T12:56:51.895930Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.886741Z","title":"Dark Energy After GW170817: Dead Ends and the Road Ahead,","venue":null,"work_id":"97479466-309a-4d63-bcfd-bcbd2da3c8de","year":2017},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.468440Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:11d4449a0d3ea810b36cf50007176e4b81e3e65f1969adfae39b2548e703bb68","observation_id":"45911ac9-66cf-4676-974f-1453c25ae7ef","resolution":{"observed_at":"2026-08-06T12:56:51.889330Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.879712Z","title":"Capozziello, R","venue":null,"work_id":"ddc7b879-a7cf-47d0-8480-8f565274b025","year":2018},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.594792Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:3f063214596e11e0345856a9135d72cecfe16c5baa00852a2d456e90319905df","observation_id":"4fa454e6-d6eb-4cdb-8223-f738e89033c4","resolution":{"observed_at":"2026-08-06T12:56:51.882278Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.873206Z","title":"Berti et al., Class","venue":null,"work_id":"752fd43c-4efd-4786-964d-b00b50eab9d4","year":2015},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.707510Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:5820473fc47e798b74fb81a7544cf9ecb621cf00a18bcd4437d79177b8e725b0","observation_id":"95aa2e93-e3b4-4cf2-bc5a-0a5f123955f2","resolution":{"observed_at":"2026-08-06T12:56:51.875435Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.866751Z","title":null,"venue":null,"work_id":"762c0a09-76a1-4d7c-a128-04a8fa10ad87","year":2023},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.710039Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:47110ef5827949ab5e195eaceff199aa3b398ee511518e0bea24cd70f06b22ae","observation_id":"9aef7b6e-9648-4db7-90aa-9cd72db884a1","resolution":{"observed_at":"2026-08-06T12:56:51.868907Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.859948Z","title":"Windhorst et al., Nature Astronomy7, 384 (2023)","venue":null,"work_id":"dd7c8512-ded3-4fa1-aa49-49f436c3cb71","year":2023},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.712558Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:f5dad5f2febd40080041d5452a3d50a4c47193db5dc54142d0db4034a2b49262","observation_id":"b4e6c7d7-21fa-4266-8dd8-ad243689b37a","resolution":{"observed_at":"2026-08-06T12:56:51.862191Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.852996Z","title":"SPARC: Mass Models for 175 Disk Galaxies with Spitzer Photometry and Accurate Rotation Curves,","venue":null,"work_id":"84a685a1-cb52-4003-a6d8-f179bb6df068","year":2016},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.715206Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:66edeea4798814abe59c88c838bb3f19b7873d7330e510e73427007fbbf65e50","observation_id":"40618d28-4c25-4d9c-95bf-a3cbecc7ba8c","resolution":{"observed_at":"2026-08-06T12:56:51.855468Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+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":"2026-08-06T12:56:51.717710Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.717710Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:4ca047e870504297693fb5beba75dc976e04c4cbdbbf6ee78c159fd33b707633","observation_id":"4cc40c25-abbe-431f-bc02-0685210e10dc","resolution":{"observed_at":"2026-08-06T12:56:51.717710Z","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":"2026-08-06T12:56:51.720057Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.720057Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:19896128f6146a54b8c4c26e69855e541653c645a5f6486571745dcfd4ff9d3d","observation_id":"46f53707-ce5b-4d3c-8233-4256d501b2e9","resolution":{"observed_at":"2026-08-06T12:56:51.720057Z","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":"2026-08-06T12:56:51.722382Z","title":"KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.722382Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:9cf5b9ffc8a7fd1003ca80c62b70d3435ac9b69371fd74075b5d01fe9bb25644","observation_id":"e27eefe9-2c31-4a7c-8030-0476505a0cc3","resolution":{"observed_at":"2026-08-06T12:56:51.722382Z","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":"2026-08-06T12:56:51.725122Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological analysis of the DR12 galaxy sample,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.725122Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:04ffe1729c0f3019a408361e5b0c363ec97b833e7eec16b180fbad7c67240d52","observation_id":"7699695d-bb8c-4c85-bf26-37fc07b0bf25","resolution":{"observed_at":"2026-08-06T12:56:51.725122Z","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":"2026-08-06T12:56:51.727664Z","title":"The Pantheon+ Analysis: Cosmological Constraints,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.727664Z"},"links":{"citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:5061e9125273f9f15e0c77d3bc526dc11964858e3421d787010251647265ebd1","observation_id":"17fac542-b04e-491e-ba35-3d71c4496e07","resolution":{"observed_at":"2026-08-06T12:56:51.727664Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1110.3193","last_updated":"2011-10-14T12:57:07Z","snapshot_observed_at":"2026-07-06T02:35:48.625634Z","submitted_at":"2011-10-14T12:57:07Z","title":"Euclid Definition Study Report","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1110.3193","snapshot_observed_at":"2026-08-06T12:56:51.730105Z","title":"Euclid Definition Study Report,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T12:56:51.730105Z"},"links":{"cited_paper":"/paper/1110.3193","citing_paper":"/paper/2507.21359"},"observation_digest":"sha256:7489fb9dc280497708022ef4959476491e10db0715d421d255452883ea43293c","observation_id":"54042d00-cf44-40fd-a7ef-e6192142af3d","resolution":{"observed_at":"2026-08-06T12:56:51.730105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2507.21359","last_updated":"2025-07-28T22:04:23Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-11T09:34:51.981995Z","submitted_at":"2025-07-28T22:04:23Z","title":"Dark Matter Constraints in Myrzakulov $F(R,T)$ Gravity: A Vielbein Approach in Weitzenb\\\"{o}ck Spacetime with Observational Data"},"reference_resolution":{"displayed":39,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":14,"verified_exact":4,"verified_fuzzy":21},"total_outbound_references":39},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 39 of 39 outbound references and 0 inbound Pith citation observations for arXiv:2507.21359."}