{"as_of":"2026-08-22T21:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:30d8ef3fac1f935381adbbaa19fc84c80cd792fd08d2d9505158a57413e9006c","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":66,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":66,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-22T06:32:14.747728+00:00","state":"measured"},{"denominator":66,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":66,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:43:40.733495Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T05:19:35.645700Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-08-21T09:57:37.233643Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-13T09:13:23.547287Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1907.10625"},"observation_digest":"sha256:bba934e4e6666025ca12daa82309345d36107a6ab75a90c5149be3077e1854ee","observation_id":"672b7926-a66d-4f1d-b115-fafac42ccb67","resolution":{"observed_at":"2026-05-13T09:13:23.589150Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T15:21:27.669525Z","title":null,"venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.01391","last_updated":"2019-12-01T12:03:17Z","snapshot_observed_at":"2026-08-19T05:17:12.389236Z","submitted_at":"2019-08-04T19:35:10Z","title":"Cosmological constraints in extended parameter space from the Planck 2018 Legacy release","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T15:21:27.669525Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.01391"},"observation_digest":"sha256:99a31e3319e5060c2badddec373b3112cf6d28e70a4ed7d02f9acc354ba2d487","observation_id":"b5280d74-000d-4d9e-b698-8d47ec1bbe5c","resolution":{"observed_at":"2026-08-14T15:21:27.669525Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T15:16:19.728377Z","title":"C., Suyu, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.01626","last_updated":"2021-01-21T16:46:16Z","snapshot_observed_at":"2026-08-18T20:28:46.897711Z","submitted_at":"2019-08-05T14:01:03Z","title":"Analytic Calculation of Covariance between Cosmological Parameters from Correlated Data Sets, with an Application to SPTpol","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T15:16:19.728377Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.01626"},"observation_digest":"sha256:fedcd05831f6356cb8b1d7b916691d7bc84378f62b2042c80e723cc1e58e50c1","observation_id":"0eee4f46-fe1d-4bc6-9fca-011f7ff96475","resolution":{"observed_at":"2026-08-14T15:16:19.728377Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T14:40:46.886641Z","title":"C., Suyu S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.02892","last_updated":"2019-08-08T00:56:02Z","snapshot_observed_at":"2026-08-18T20:28:11.698521Z","submitted_at":"2019-08-08T00:56:02Z","title":"Measuring the distances to quasars at high redshifts with strong lensing","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-14T14:40:46.886641Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.02892"},"observation_digest":"sha256:503b681d33a13643a8d337ef2805a2d0e786f98100dac56e470308ef63eb9eb2","observation_id":"a5cf204f-8887-4c60-9c2c-0e77de7a76ab","resolution":{"observed_at":"2026-08-14T14:40:46.886641Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T14:24:14.495318Z","title":null,"venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.03324","last_updated":"2020-09-24T15:12:03Z","snapshot_observed_at":"2026-08-18T08:04:07.306356Z","submitted_at":"2019-08-09T06:00:26Z","title":"Resolving Hubble Tension with Quintom Dark Energy Model","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T14:24:14.495318Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.03324"},"observation_digest":"sha256:caadfb6ce406628c21e2597998ca7f3a47dae8a862a5af17c057affda4971849","observation_id":"5e6ee4a5-d805-441d-8176-3d9628722778","resolution":{"observed_at":"2026-08-14T14:24:14.495318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T14:14:09.072340Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.03663","last_updated":"2019-09-16T21:35:34Z","snapshot_observed_at":"2026-08-17T00:55:38.317018Z","submitted_at":"2019-08-10T01:40:10Z","title":"The Hubble Hunter's Guide","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T14:14:09.072340Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.03663"},"observation_digest":"sha256:a22d81135f98d488c3a66a9596e41676fb7620d3b24fad27d3c5cb20b5a37b1f","observation_id":"c82732a6-8ea8-45fd-afc9-458bb1e340d0","resolution":{"observed_at":"2026-08-14T14:14:09.072340Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T13:51:09.259600Z","title":null,"venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.04281","last_updated":"2020-07-01T09:13:30Z","snapshot_observed_at":"2026-08-15T17:08:59.798095Z","submitted_at":"2019-08-12T17:48:35Z","title":"Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions","version":2},"reference_index":281,"source":"pdf_text","source_observed_at":"2026-08-14T13:51:09.259600Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.04281"},"observation_digest":"sha256:cd950bef3234dfe6c880f06a7c06fab516da28db362ea2606e170c182a020bef","observation_id":"897f9d5b-709c-4c61-9337-210e32584cf4","resolution":{"observed_at":"2026-08-14T13:51:09.259600Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T13:42:33.008707Z","title":"H0LiCOW XIII. A 2.4% measure- ment of H0 from lensed quasars: 5 .3σ tension between early and late-Universe probes,","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-18T14:50:01.444766Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.008707Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:30a2d0b9aa405bdf08125fb90afce8fea74a1ca13b2c1361a35eb9eac42a406e","observation_id":"52b99a01-8e73-4bd3-b717-92db91538a9e","resolution":{"observed_at":"2026-08-14T13:42:33.008707Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T12:34:56.751432Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06995","last_updated":"2019-08-19T18:00:08Z","snapshot_observed_at":"2026-08-19T22:26:29.128543Z","submitted_at":"2019-08-19T18:00:08Z","title":"Oscillating scalar fields and the Hubble tension: a resolution with novel signatures","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T12:34:56.751432Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.06995"},"observation_digest":"sha256:5df923cc56c6fe4f35984a5ca6297284dd4ac4f8d5fb57986c89c0521694509f","observation_id":"6bb971f9-2e9b-4531-84c0-d87480971a72","resolution":{"observed_at":"2026-08-14T12:34:56.751432Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T12:25:23.674626Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.07267","last_updated":"2019-08-27T12:13:54Z","snapshot_observed_at":"2026-08-17T12:06:20.383298Z","submitted_at":"2019-08-20T10:51:59Z","title":"Cosmology With Low-Redshift Observations: No Signal For New Physics","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T12:25:23.674626Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.07267"},"observation_digest":"sha256:e6e89ea7d1c6d62deaa1db6738ec0ccbc4e2871f4ea9256e1dd1cd58aac3f398","observation_id":"af674eb4-716a-47ff-baa5-d24d38bb3e38","resolution":{"observed_at":"2026-08-14T12:25:23.674626Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T11:53:25.101406Z","title":"Wong et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08472","last_updated":"2020-04-15T14:39:51Z","snapshot_observed_at":"2026-08-21T03:17:22.482555Z","submitted_at":"2019-08-22T16:09:19Z","title":"Measuring $H_0$ with pulsar timing arrays","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:53:25.101406Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.08472"},"observation_digest":"sha256:0d73e2b03b30f28866bc29ab0747cd2b2d07f57768897727df5969eb8d9f625d","observation_id":"75791181-96cd-4203-9408-74c09b25f009","resolution":{"observed_at":"2026-08-14T11:53:25.101406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T10:35:40.651639Z","title":"C., Suyu, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.10883","last_updated":"2019-12-03T17:02:47Z","snapshot_observed_at":"2026-08-17T12:29:45.375713Z","submitted_at":"2019-08-28T18:01:02Z","title":"Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T10:35:40.651639Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.10883"},"observation_digest":"sha256:3e6b2139cc7e4bebf59e4a150cc3195a82b1ee7a5a320483c3b4952f89f1134f","observation_id":"707d3201-a33e-4a94-b7ee-c70e59297a31","resolution":{"observed_at":"2026-08-14T10:35:40.651639Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T10:19:13.061074Z","title":"H0LiCOW XIII. A 2.4% measurement ofH0 from lensed quasars: 5.3σ tension between early and late-Universe probes","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.11410","last_updated":"2019-08-29T18:25:49Z","snapshot_observed_at":"2026-08-18T20:27:51.918809Z","submitted_at":"2019-08-29T18:25:49Z","title":"High angular resolution gravitational wave astronomy","version":1},"reference_index":143,"source":"pdf_text","source_observed_at":"2026-08-14T10:19:13.061074Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1908.11410"},"observation_digest":"sha256:478898ca63fae71330a4a4c4764ca4256544509b394394febf3af6d6e9017f2c","observation_id":"2d408cdf-ddf6-43dd-866e-ed5be4ed3efb","resolution":{"observed_at":"2026-08-14T10:19:13.061074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T05:15:36.919799Z","title":"H0LiCOW XIII. A 2.4% measurement ofH0 from lensed quasars:5.3σtension between early and late-Universe probes,","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1909.01828","last_updated":"2020-02-11T23:29:28Z","snapshot_observed_at":"2026-08-14T06:01:35.593562Z","submitted_at":"2019-09-04T14:17:51Z","title":"hi_class: Background Evolution, Initial Conditions and Approximation Schemes","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T05:15:36.919799Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1909.01828"},"observation_digest":"sha256:70f6ae201b40e7bbf36bbf3b0985e019739881292c05692394808fef3b2ec5dc","observation_id":"cbbd59e6-13c0-4b4d-9d48-4a00b4396746","resolution":{"observed_at":"2026-08-14T05:15:36.919799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-14T05:10:14.052160Z","title":"C., Suyu, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1909.02005","last_updated":"2019-10-17T20:22:14Z","snapshot_observed_at":"2026-08-18T01:27:10.983099Z","submitted_at":"2019-09-04T18:00:00Z","title":"Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning","version":2},"reference_index":152,"source":"pdf_text","source_observed_at":"2026-08-14T05:10:14.052160Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1909.02005"},"observation_digest":"sha256:b8b71450aa14adb213cc3b5ebef5d02088e55c658f440b31e40d8e5e25820867","observation_id":"57cf5ccd-cac2-43d7-83ac-41dc2b37d246","resolution":{"observed_at":"2026-08-14T05:10:14.052160Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"1912.02622","last_updated":"2020-03-24T17:57:53Z","snapshot_observed_at":"2026-08-12T18:38:43.637331Z","submitted_at":"2019-12-05T14:57:00Z","title":"Science Case for the Einstein Telescope","version":4},"reference_index":193,"source":"pdf_text","source_observed_at":"2026-05-16T00:13:18.137293Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/1912.02622"},"observation_digest":"sha256:12890405b383c944367a9a2d04fb4e9f25e3dddeff7b830a6b35486ba4d6c678","observation_id":"93a4e5aa-849d-4f34-a9f9-e432cbd9b3c5","resolution":{"observed_at":"2026-05-16T00:13:18.585025Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2211.04492","last_updated":"2022-11-08T19:00:16Z","snapshot_observed_at":"2026-08-01T18:06:39.805867Z","submitted_at":"2022-11-08T19:00:16Z","title":"The Hubble Tension and Early Dark Energy","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-17T23:41:11.040188Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2211.04492"},"observation_digest":"sha256:250981bfdc1528cb22c860595129b11a5daa698efa5cafb921dd639fcb78f987","observation_id":"69ca9b8f-1d4a-45f7-84bd-949286b8e524","resolution":{"observed_at":"2026-05-17T23:41:11.418130Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-12T18:51:10.136900Z","title":"H0LiCOW XIII. A 2.4 % measurement of H0 from lensed quasars: 5.3σ tension between early and late-Universe probes,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.11923","last_updated":"2025-05-09T05:26:16Z","snapshot_observed_at":"2026-08-19T02:52:53.385337Z","submitted_at":"2024-11-18T06:09:59Z","title":"Late Time Phenomena in $f(T,\\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T18:51:10.136900Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2411.11923"},"observation_digest":"sha256:429bf521f50dcde7f63f052108d6813f7bb49044331b4760f2fdeed4e3a4b299","observation_id":"3ae2c279-4147-4742-955d-86c01b7051c2","resolution":{"observed_at":"2026-08-12T18:51:10.136900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-12T16:37:56.363214Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-19T15:12:27.506598Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.363214Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:7c8b5ded8ff1e70125ef046f53b2abbb17f81262018301808e87ab557e332c5e","observation_id":"54d8a352-db82-4621-b73f-c6d7b4aa7925","resolution":{"observed_at":"2026-08-12T16:37:56.363214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-11T21:12:38.205627Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.04959","last_updated":"2025-01-29T07:31:15Z","snapshot_observed_at":"2026-08-19T04:12:40.889815Z","submitted_at":"2024-12-06T11:25:46Z","title":"Neutrino masses from large-scale structures: future sensitivity and theory dependence","version":2},"reference_index":173,"source":"pdf_text","source_observed_at":"2026-08-11T21:12:38.205627Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2412.04959"},"observation_digest":"sha256:f0eef18a9368f1598de89c07dbfba34419b022a2084f52800f87640c96dc933a","observation_id":"c4c205de-60c2-4e13-ae2c-bbe84e04d41b","resolution":{"observed_at":"2026-08-11T21:12:38.205627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-11T13:41:23.627487Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.627487Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:a719b567bd71adcd48bb96a5bf877be403b8fe562fa63377ca62dd05604b0f66","observation_id":"331e37a2-de33-4f88-8df7-c7f3e317f158","resolution":{"observed_at":"2026-08-11T13:41:23.627487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-10T20:48:19.239916Z","title":"H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 σ tension between early- and late-Universe probes,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.07538","last_updated":"2025-04-26T14:21:38Z","snapshot_observed_at":"2026-08-16T12:59:00.797085Z","submitted_at":"2025-01-13T18:18:17Z","title":"Testing $\\gamma\\delta$CDM Model in the Redshift Bins","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T20:48:19.239916Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2501.07538"},"observation_digest":"sha256:6f7b4f590ea26fd4ac951ae86520d4d42f6f5ee2ba13fca5f40c7e2b89d03ef3","observation_id":"759cd80d-2d75-4448-82f8-e6ee87765d19","resolution":{"observed_at":"2026-08-10T20:48:19.239916Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-10T13:41:25.765490Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.16292","last_updated":"2026-07-08T13:46:40Z","snapshot_observed_at":"2026-08-18T20:22:46.215222Z","submitted_at":"2025-01-27T18:31:32Z","title":"Line-of-sight shear in SLACS strong lenses I: shear and mass model parametrisations","version":3},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-10T13:41:25.765490Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2501.16292"},"observation_digest":"sha256:249fb54d029aa9cf38552b919a9403547de40bb82a5e17a87b18ff1a992d3bd6","observation_id":"bd868135-4977-4622-9f77-322330857dac","resolution":{"observed_at":"2026-08-10T13:41:25.765490Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-09T05:41:24.134509Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.03190","last_updated":"2025-07-27T14:01:59Z","snapshot_observed_at":"2026-08-19T03:58:23.897477Z","submitted_at":"2025-02-05T14:07:08Z","title":"Exploring Hubble Tension Alleviation through Neutrino-Coupled Perturbed $f(R)$ Gravity","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-09T05:41:24.134509Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2502.03190"},"observation_digest":"sha256:6583d16693f63cfbf985986410b42d4ef83e31051859887dc67826234904e062","observation_id":"509cd822-c496-4881-a436-1f5dad83c672","resolution":{"observed_at":"2026-08-09T05:41:24.134509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-16T12:43:40.733495Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2504.12205","last_updated":"2025-09-05T12:05:34Z","snapshot_observed_at":"2026-08-19T15:50:59.813841Z","submitted_at":"2025-04-16T15:54:06Z","title":"Barrow and Tsallis entropies after the DESI DR2 BAO data","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-16T12:43:40.733495Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2504.12205"},"observation_digest":"sha256:779efb4d930a68b52987c3e9b03a0d9946d36fbebca20f9b054a3b356baf275f","observation_id":"e6607ec5-89e1-4e8c-8bd5-a7589cf47ffd","resolution":{"observed_at":"2026-08-16T12:43:40.733495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-16T05:58:50.938406Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2504.19523","last_updated":"2025-04-28T06:41:32Z","snapshot_observed_at":"2026-08-19T04:54:47.337704Z","submitted_at":"2025-04-28T06:41:32Z","title":"Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-16T05:58:50.938406Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2504.19523"},"observation_digest":"sha256:2aabfa15d813d6a32f472a17dc50b4e2f00530fd05abb6b7df1acb607e1f2a5b","observation_id":"572189c6-e670-477d-899a-cc9a77e3e212","resolution":{"observed_at":"2026-08-16T05:58:50.938406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-15T23:39:45.942087Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.04336","last_updated":"2025-07-23T19:10:27Z","snapshot_observed_at":"2026-08-17T21:26:13.566598Z","submitted_at":"2025-05-07T11:33:48Z","title":"In search of an interaction in the dark sector through Gaussian Process and ANN approaches","version":2},"reference_index":124,"source":"pdf_text","source_observed_at":"2026-08-15T23:39:45.942087Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2505.04336"},"observation_digest":"sha256:5a24954f76bd0afee9b9dde74ae4565d212e3f138f5f465a63396e43f491c0de","observation_id":"a6d39f51-9db7-4a21-98c3-41112d9fca84","resolution":{"observed_at":"2026-08-15T23:39:45.942087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-15T23:21:48.430715Z","title":"C., Suyu, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.05032","last_updated":"2026-06-08T07:05:34Z","snapshot_observed_at":"2026-08-22T08:22:16.406989Z","submitted_at":"2025-05-08T08:11:38Z","title":"Gravitational Lenses in UNIONS and Euclid (GLUE) I: A Search for Strong Gravitational Lenses in UNIONS with Subaru, CFHT, and Pan-STARRS Data","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-15T23:21:48.430715Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2505.05032"},"observation_digest":"sha256:1afe4b0d7b6fe62906064a19aade29a86ce1aeb373377b5d346d3ae6d8c8d4c7","observation_id":"361422fc-cb93-4fd4-baa4-d19bd335c8ca","resolution":{"observed_at":"2026-08-15T23:21:48.430715Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-07T15:09:32.185536Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.16158","last_updated":"2025-09-09T00:51:51Z","snapshot_observed_at":"2026-08-15T14:59:20.207138Z","submitted_at":"2025-05-22T02:57:53Z","title":"Confirming HSC strong lens candidates with DESI Spectroscopy. I. Project overview and first results","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-07T15:09:32.185536Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2505.16158"},"observation_digest":"sha256:e216f9bd46b9b90bb4883837424bc17f37ed0e5728beeb4da3a929221e9d7ab1","observation_id":"829eb098-8e3a-422e-9752-f541c61dea02","resolution":{"observed_at":"2026-08-07T15:09:32.185536Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-07T14:56:32.085585Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.17262","last_updated":"2025-05-22T20:16:33Z","snapshot_observed_at":"2026-08-19T06:11:22.169245Z","submitted_at":"2025-05-22T20:16:33Z","title":"A Joint Analysis of Strong Lensing and Type Ia Supernovae to Determine the Hubble Constant","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-07T14:56:32.085585Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2505.17262"},"observation_digest":"sha256:f85b22254f2384a6ac937d27c550f63d04cc99e8b870d96b03734bdeb259540a","observation_id":"5e19de9d-c3cf-4c5b-b0dc-5611af5fa11c","resolution":{"observed_at":"2026-08-07T14:56:32.085585Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-07T13:42:40.047705Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.21359","last_updated":"2025-05-27T15:52:14Z","snapshot_observed_at":"2026-08-16T06:46:25.246040Z","submitted_at":"2025-05-27T15:52:14Z","title":"Teleparallel dark energy in a nonflat universe","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T13:42:40.047705Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2505.21359"},"observation_digest":"sha256:47daf7eff3dfb28d54514684ddcbdc9f0d036493bdd219cc655eaaf41fbd5c1f","observation_id":"74a0b1e8-ac2a-48c2-b0f6-7815bbb32248","resolution":{"observed_at":"2026-08-07T13:42:40.047705Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-07T11:35:05.009418Z","title":"Wong, S.H","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.02235","last_updated":"2025-06-02T20:28:10Z","snapshot_observed_at":"2026-08-15T01:47:37.918115Z","submitted_at":"2025-06-02T20:28:10Z","title":"A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T11:35:05.009418Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2506.02235"},"observation_digest":"sha256:d5df16f2ebbd34bc44cc0c4d949e82b0c144e962cc8352202a6ac48bd6794cc6","observation_id":"1bdbe924-39f3-4c83-8511-9e24058b497a","resolution":{"observed_at":"2026-08-07T11:35:05.009418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-07T00:54:42.125603Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.12709","last_updated":"2025-07-01T13:57:37Z","snapshot_observed_at":"2026-08-22T01:16:50.768676Z","submitted_at":"2025-06-15T03:43:47Z","title":"Constraints on Dark Energy Models Using Late Universe Probes","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T00:54:42.125603Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2506.12709"},"observation_digest":"sha256:4f1bafad00647d6de4dc29bc4c75697cdd5575579885a9092c5fd9c5b7770c4d","observation_id":"8822c8cf-7f05-41af-ba48-5c914bdfccbe","resolution":{"observed_at":"2026-08-07T00:54:42.125603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2506.13537","last_updated":"2026-04-05T09:39:17Z","snapshot_observed_at":"2026-08-15T12:25:05.072231Z","submitted_at":"2025-06-16T14:26:18Z","title":"Revisiting $\\Lambda$CDM extensions in light of re-analyzed CMB data","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-19T09:23:33.941977Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2506.13537"},"observation_digest":"sha256:98eaea48658ed77bc4114cbb5132c3a995ae4b0c384287c8679e4b49d1159d25","observation_id":"21878802-dd17-4ec9-914a-1ff46032840b","resolution":{"observed_at":"2026-05-19T09:27:15.246162Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-06T22:33:05.808065Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.21477","last_updated":"2025-06-26T17:07:20Z","snapshot_observed_at":"2026-08-20T20:32:46.462474Z","submitted_at":"2025-06-26T17:07:20Z","title":"Quasar cosmology II: joint analyses with Cosmic Microwave Background","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T22:33:05.808065Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2506.21477"},"observation_digest":"sha256:4da80655de38f87282e5f88375440bd6362059995f38c7f29219d7183445679f","observation_id":"29f9af78-97ba-4d5a-976d-0e41d12554b1","resolution":{"observed_at":"2026-08-06T22:33:05.808065Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-05T23:23:30.848557Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.05436","last_updated":"2026-05-27T07:37:45Z","snapshot_observed_at":"2026-08-19T00:43:08.425664Z","submitted_at":"2025-08-07T14:25:53Z","title":"Constraints on DBI dark energy with chameleon mechanism","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-05T23:23:30.848557Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2508.05436"},"observation_digest":"sha256:4090cc5ad4b0dd0255d32367c9d4d38cd5eb4142d917ea6adf614b6e7be42e46","observation_id":"e7ef1245-18d9-4412-8b22-c6715a9de37e","resolution":{"observed_at":"2026-08-05T23:23:30.848557Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-05T15:19:52.142482Z","title":"C., Suyu, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.20087","last_updated":"2025-08-27T17:55:25Z","snapshot_observed_at":"2026-08-17T23:37:34.529838Z","submitted_at":"2025-08-27T17:55:25Z","title":"Strong Lens Discoveries in DESI Legacy Imaging Surveys DR10 with Two Deep Learning Architectures","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-05T15:19:52.142482Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2508.20087"},"observation_digest":"sha256:3a5c0b22f6f31216e5f3e835799c31020ef24c2b49ff068fd03b5eac6b6257a5","observation_id":"1089a028-05fa-42d3-937c-3ae2e58ec6ac","resolution":{"observed_at":"2026-08-05T15:19:52.142482Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-05T14:43:16.181718Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.20971","last_updated":"2026-06-14T15:39:47Z","snapshot_observed_at":"2026-08-15T21:32:35.239373Z","submitted_at":"2025-08-28T16:25:22Z","title":"Cosmo-Learn: code for learning cosmology using different methods and mock data","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-05T14:43:16.181718Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2508.20971"},"observation_digest":"sha256:07c79d56f8b4eb17e2b27aaa01849f722e0a05008f2ac4761c06bce0a1eb8db6","observation_id":"79523969-2769-453b-9523-34e7da003088","resolution":{"observed_at":"2026-08-05T14:43:16.181718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2509.09202","last_updated":"2026-04-12T17:53:51Z","snapshot_observed_at":"2026-08-16T20:14:42.800239Z","submitted_at":"2025-09-11T07:18:09Z","title":"Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-18T18:14:18.793821Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2509.09202"},"observation_digest":"sha256:edee118bbc3988958c20fdcf98ccdef54b7d1e5dfa0095de950f358825c81e97","observation_id":"eca84f24-f591-49b0-b2db-6452a2d8c9e2","resolution":{"observed_at":"2026-05-18T18:16:43.508753Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-04T18:49:51.345465Z","title":"A 2.4 per cent measurement ofH 0 from lensed quasars: 5.3σtension between early- and late-Universe probes,Mon","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2509.09678","last_updated":"2025-09-11T17:59:46Z","snapshot_observed_at":"2026-08-15T10:09:50.196701Z","submitted_at":"2025-09-11T17:59:46Z","title":"Cosmic $\\tau$ensions Indirectly Correlate with Reionization Optical Depth","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T18:49:51.345465Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2509.09678"},"observation_digest":"sha256:860a276c08c43ea292acfdb01a1d8a92778f37de0f7d06adb95035fa1a993cbd","observation_id":"ef491685-1352-479f-a967-ac6a3a58ee2f","resolution":{"observed_at":"2026-08-04T18:49:51.345465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-03T23:23:54.260139Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.06332","last_updated":"2026-07-29T03:18:47Z","snapshot_observed_at":"2026-08-22T00:10:58.312134Z","submitted_at":"2025-11-09T11:16:28Z","title":"Bayesian and Machine-Learning Analyses of Nonminimal $f(Q)$ Gravity and $H_0$ Tension","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T23:23:54.260139Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2511.06332"},"observation_digest":"sha256:aff1edeb938ddb9221c642044ca2667e8ad1c9594babc9c0aa2f2fcffc299a82","observation_id":"f0e8edd1-014f-428d-b7d0-35277ecd0d6e","resolution":{"observed_at":"2026-08-03T23:23:54.260139Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-03T22:55:44.453554Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.08486","last_updated":"2026-06-01T07:28:08Z","snapshot_observed_at":"2026-08-06T23:45:29.322816Z","submitted_at":"2025-11-11T17:26:43Z","title":"Accelerated inference of microlensed gravitational waves with machine learning","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T22:55:44.453554Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2511.08486"},"observation_digest":"sha256:3c9d7508ce80f08da7c2e96152aed55070a6aa5aaec8664decb365f61a442fd4","observation_id":"d73b9306-cc38-4416-8187-8b8a92cd0305","resolution":{"observed_at":"2026-08-03T22:55:44.453554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-03T13:11:13.143620Z","title":"Wong, S.H","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2601.00495","last_updated":"2026-07-17T23:50:20Z","snapshot_observed_at":"2026-08-14T08:24:24.486521Z","submitted_at":"2026-01-01T22:28:11Z","title":"Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-03T13:11:13.143620Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2601.00495"},"observation_digest":"sha256:0f2125fcb0865d63ffa9f1daf2448e12e857258e8c0ba41c2ed651c1e241dab5","observation_id":"917e55b8-2701-4f83-b757-07350f43b3c2","resolution":{"observed_at":"2026-08-03T13:11:13.143620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2601.14222","last_updated":"2026-04-27T15:45:53Z","snapshot_observed_at":"2026-08-16T10:25:36.389340Z","submitted_at":"2026-01-20T18:32:34Z","title":"Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension","version":2},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-05-16T12:15:01.997389Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2601.14222"},"observation_digest":"sha256:08e50588570ae721624ae98e62235a9ed709ad52a9afb5245c9e1537f60b44ce","observation_id":"89d933e4-bb04-48d7-8789-d5958abc5bc9","resolution":{"observed_at":"2026-05-16T12:17:52.408499Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-03T08:28:47.100141Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2601.17281","last_updated":"2026-07-22T16:31:27Z","snapshot_observed_at":"2026-08-19T13:46:26.748996Z","submitted_at":"2026-01-24T03:41:53Z","title":"Dissipative Unimodular Gravity: Linking Energy Diffusion to Bulk Viscosity as an Alternative to $\\Lambda$CDM under DESI DR2 Data","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T08:28:47.100141Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2601.17281"},"observation_digest":"sha256:6791c3ba556e396d25a9f3f4f504b7c9cda2cc56a700167d4043d0b1708738d9","observation_id":"ffde3bfc-3f54-438e-833b-80e4f2606277","resolution":{"observed_at":"2026-08-03T08:28:47.100141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-03T06:51:31.536615Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2601.21820","last_updated":"2026-05-28T08:19:01Z","snapshot_observed_at":"2026-08-13T13:08:09.900415Z","submitted_at":"2026-01-29T15:04:37Z","title":"Forecasting Constraints on Cosmology and Modified Gravitational-wave Propagation by Combining Strongly Lensed Gravitational Waves and Galaxy Surveys","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T06:51:31.536615Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2601.21820"},"observation_digest":"sha256:bf1b4a85b95b78c664ee159c9835f3bf09e8409c56acc0bc921aff7c6c8759fa","observation_id":"10e92a62-89b1-401a-9758-590e5c92d866","resolution":{"observed_at":"2026-08-03T06:51:31.536615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2602.11093","last_updated":"2026-04-18T16:30:32Z","snapshot_observed_at":"2026-08-08T00:16:50.248213Z","submitted_at":"2026-02-11T18:01:44Z","title":"New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-16T02:22:49.920780Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2602.11093"},"observation_digest":"sha256:472cfdbb689977cf129f6fb2875d43bc139a221f5da6e81173780d75b6cdcd0c","observation_id":"674893b3-51cf-4791-a430-6d8ba38600e8","resolution":{"observed_at":"2026-05-16T02:27:10.633226Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2602.22840","last_updated":"2026-04-04T03:04:57Z","snapshot_observed_at":"2026-08-13T10:30:16.011557Z","submitted_at":"2026-02-26T10:27:19Z","title":"Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-15T19:26:47.797586Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2602.22840"},"observation_digest":"sha256:54c3d5b19382bdf52fcddfba360b449f194f7872df6298c09ec27b51d5208598","observation_id":"97d894ad-a904-4e3e-8b87-3ba5dd6d23af","resolution":{"observed_at":"2026-05-15T19:30:17.222826Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2604.27511","last_updated":"2026-04-30T07:09:56Z","snapshot_observed_at":"2026-08-11T15:02:56.009662Z","submitted_at":"2026-04-30T07:09:56Z","title":"Finding Strongly Lensed Supernovae from Blended Light Curves","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-07T10:06:15.598465Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2604.27511"},"observation_digest":"sha256:f4baf35c59ddb580d4a3f9d691a00525e6869ec228df5df70cddc67d5d6112e9","observation_id":"1624a35b-bb47-4657-9e09-f7c88b71a383","resolution":{"observed_at":"2026-05-12T09:36:27.602839Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2605.02181","last_updated":"2026-05-04T03:25:33Z","snapshot_observed_at":"2026-08-14T10:47:53.071058Z","submitted_at":"2026-05-04T03:25:33Z","title":"Beyond collective fluctuations: probing micro-image swarms in lensed quasars with intensity interferometry","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-08T19:23:33.877340Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2605.02181"},"observation_digest":"sha256:d16308ac9c2e276b4bfc31cfad6536a3eeda2273f5e83bc7b7f6373af2514cf1","observation_id":"059ee935-bc50-4fa9-b9cc-2b9382d21b90","resolution":{"observed_at":"2026-05-09T05:55:30.670868Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2605.03008","last_updated":"2026-08-15T01:29:57Z","snapshot_observed_at":"2026-08-20T23:09:31.129532Z","submitted_at":"2026-05-04T18:00:06Z","title":"Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations","version":1},"reference_index":148,"source":"arxiv_source","source_observed_at":"2026-05-08T17:57:29.069633Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2605.03008"},"observation_digest":"sha256:c1cce252f20d28335403be652a3ca7cc677fcf7a6f5cd46ea4be786977915e1a","observation_id":"a35853bf-a4e9-409e-b98f-ac494a55c408","resolution":{"observed_at":"2026-05-09T06:55:43.615512Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2605.19476","last_updated":"2026-07-14T05:19:43Z","snapshot_observed_at":"2026-08-15T01:27:29.695101Z","submitted_at":"2026-05-19T07:28:18Z","title":"Prospect of Measuring the Cosmic Dipole by Associating Strongly Lensed Gravitational Waves with Galaxy Surveys","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-20T03:03:06.326603Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2605.19476"},"observation_digest":"sha256:eb61fab0347609c9ce4fcf0903ce7f407ad54579d986a694ac0e000fcb1cbb9c","observation_id":"20e1582a-c873-458a-8035-3069b137cdd2","resolution":{"observed_at":"2026-05-20T03:03:21.294466Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2605.21310","last_updated":"2026-05-20T15:37:58Z","snapshot_observed_at":"2026-08-17T02:55:31.042897Z","submitted_at":"2026-05-20T15:37:58Z","title":"Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-21T03:33:53.198336Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2605.21310"},"observation_digest":"sha256:283f4f04014d53b78474c4d9bc0f495d6089f8c9f369a0cfabcb9cd86a7dd70a","observation_id":"b62fa737-cb77-4d5d-9046-f61f3e70ea8e","resolution":{"observed_at":"2026-05-21T03:33:56.392803Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2605.28658","last_updated":"2026-05-27T15:57:34Z","snapshot_observed_at":"2026-08-07T14:47:20.363975Z","submitted_at":"2026-05-27T15:57:34Z","title":"Measuring the Hubble constant with strongly lensed gravitational waves from space-based detector networks","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-29T10:38:35.290637Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2605.28658"},"observation_digest":"sha256:4aede48ea6f1f840edb20df13636ab45ffd126cec4258d6e9b0d8104394faa37","observation_id":"f6389c71-f5f1-48e2-9c52-dbc82edd3e4b","resolution":{"observed_at":"2026-06-29T11:13:21.260077Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2606.02097","last_updated":"2026-06-01T11:28:21Z","snapshot_observed_at":"2026-08-14T01:42:29.390361Z","submitted_at":"2026-06-01T11:28:21Z","title":"Redshift Duality with Pantheon+SH0ES in a Planck-anchored Flat $\\Lambda$CDM Framework: Implications for Hubble Tension and Observational Inference","version":1},"reference_index":104,"source":"arxiv_source","source_observed_at":"2026-06-28T13:17:56.799399Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.02097"},"observation_digest":"sha256:2631bfd4478b3588a2b2ff73d113ba4b329c53ef75a76636d7ef5afdbcd47d3a","observation_id":"fb49520c-b774-422b-8aeb-213ca7e65602","resolution":{"observed_at":"2026-07-02T00:46:23.807124Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2606.03634","last_updated":"2026-06-02T13:31:54Z","snapshot_observed_at":"2026-07-06T23:43:50.943530Z","submitted_at":"2026-06-02T13:31:54Z","title":"Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays","version":1},"reference_index":120,"source":"pdf_text","source_observed_at":"2026-06-28T08:37:43.649043Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.03634"},"observation_digest":"sha256:269470757a3cc9b6770bf2a98c834ba5e812c37869b818bf6c2cd44e72464ec3","observation_id":"59726dda-f534-467f-8ced-de518eeb9de5","resolution":{"observed_at":"2026-07-02T04:56:39.524171Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2606.05281","last_updated":"2026-06-03T18:00:00Z","snapshot_observed_at":"2026-08-03T00:56:47.377000Z","submitted_at":"2026-06-03T18:00:00Z","title":"Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-06-28T05:20:29.507384Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.05281"},"observation_digest":"sha256:6adcc69be3289dec3b8494947974bbf989e11e4234e5c843577ff1f357037955","observation_id":"63ec8c09-7bbc-475d-ae64-84654acfa234","resolution":{"observed_at":"2026-07-02T10:06:51.597644Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2606.12822","last_updated":"2026-06-11T02:35:35Z","snapshot_observed_at":"2026-07-06T23:51:40.528967Z","submitted_at":"2026-06-11T02:35:35Z","title":"Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-27T06:23:50.957273Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.12822"},"observation_digest":"sha256:19af7de5525c3c7bc053308de3e44f38c8e3627b5db662d80fd651809bad6ce1","observation_id":"6982afdd-ce92-4b04-94db-e5548b97946a","resolution":{"observed_at":"2026-07-03T15:38:33.888692Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2606.19905","last_updated":"2026-06-18T08:02:10Z","snapshot_observed_at":"2026-08-13T00:28:53.387043Z","submitted_at":"2026-06-18T08:02:10Z","title":"Cosmological Constraints on Minimal Cubic Galileon Models in Teleparallel Gravity","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-26T16:55:10.910021Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.19905"},"observation_digest":"sha256:e370717018fd57a0a6c8fb261675074ac18837eb5db654ca9263e626b1fcc270","observation_id":"71934149-e5b1-4f9b-a8dc-0d8b39f2929d","resolution":{"observed_at":"2026-07-04T04:39:34.082726Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":"1907.04869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-04T05:19:35.645700Z","title":"Wong et al","venue":null,"work_id":"113e274d-4e5b-44f4-a664-0dc6161bd260","year":2020},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-15T03:29:17.716518Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":174,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:d286dc2338c39e56d3d1115351b1f19b2914188e0dc5203d3c0d3425c27a4de8","observation_id":"1a5a48e4-587f-410f-b904-dba14e9b3a67","resolution":{"observed_at":"2026-07-04T05:19:35.647603Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-08-15T03:29:17.716518Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":174,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:24d47807bcdc7d095e0c5ed43b8e8e746ebb171af96d33e6e2a5162ae4c796a7","observation_id":"a6bffb32-92ff-488f-800f-473cd40dabe3","resolution":{"observed_at":"2026-07-15T10:41:50.733215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-12T00:47:44.012023Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.03672","last_updated":"2026-07-07T05:23:35Z","snapshot_observed_at":"2026-08-17T08:48:15.875345Z","submitted_at":"2026-07-04T02:58:17Z","title":"Hubble constant measurement with 13 bright standard sirens from binary black hole mergers inside active galactic nuclei","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-12T00:47:44.012023Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2607.03672"},"observation_digest":"sha256:368bf144167700770fef9c71ef94f53794ef84eb0e06b47a2359ce38aced92e8","observation_id":"c08ee99e-8e82-47d2-838f-b908b2df39cc","resolution":{"observed_at":"2026-07-12T00:47:44.012023Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-07-11T06:44:15.468115Z","title":"A 2.4 per cent measurement of H _ 0 from lensed quasars: 5.3 tension between early- and late-Universe probes","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2607.05502","last_updated":"2026-07-06T18:00:02Z","snapshot_observed_at":"2026-08-19T15:31:54.007221Z","submitted_at":"2026-07-06T18:00:02Z","title":"The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models","version":1},"reference_index":162,"source":"arxiv_source","source_observed_at":"2026-07-11T06:44:15.468115Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2607.05502"},"observation_digest":"sha256:a76faf5617b23aafe38de19dd91c5b3209f0ce95a8dfe0b655828a9da3c7ab70","observation_id":"d1c50a81-a8bd-4d02-8fc7-9ff8c0bcdc3d","resolution":{"observed_at":"2026-07-11T06:44:15.468115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-02T02:52:21.117388Z","title":"H0LiCOW XIII. A 2.4% measurement ofH0 from lensed quasars: 5.3σ tension between early- and late-Universe probes","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14211","last_updated":"2026-07-15T18:00:01Z","snapshot_observed_at":"2026-08-15T18:59:57.704560Z","submitted_at":"2026-07-15T18:00:01Z","title":"Non-Primordial Contribution to the Cosmic Microwave Background","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-02T02:52:21.117388Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2607.14211"},"observation_digest":"sha256:ddcf44cc5f0a44e3ef8fb9e60e643d0271ad55f91944236ac6082636fae4a964","observation_id":"a001a48e-1e2e-4ee3-a9a2-e2913d2d8d4d","resolution":{"observed_at":"2026-08-02T02:52:21.117388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-01T19:06:47.108814Z","title":"A 2.4 per cent measurement of H _ 0 from lensed quasars: 5.3 tension between early- and late-Universe probes","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"2607.17144","last_updated":"2026-07-19T09:00:22Z","snapshot_observed_at":"2026-08-16T19:02:57.032508Z","submitted_at":"2026-07-19T09:00:22Z","title":"Microlensing of Microlensing: Effects of Random Stars on the Double-Source-Plane Gravitational Lens","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-01T19:06:47.108814Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2607.17144"},"observation_digest":"sha256:a696eb6152cb98d27cb9f16141e65fc1d38659f3b988e7753cf33062d9184151","observation_id":"46c1f119-99b1-4baa-9b77-1f62ab8c81e6","resolution":{"observed_at":"2026-08-01T19:06:47.108814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-01T07:20:07.524287Z","title":"H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3 σ tension between early- and late-Universe probes,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-08-14T16:46:31Z","snapshot_observed_at":"2026-08-19T23:10:52.542376Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:07.524287Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:9b6188f94e919a1431404c4f37479172ce2587680a8907f397fd93dbb52185f9","observation_id":"bca4bec7-5efd-42ab-b600-c0e6e8e688a7","resolution":{"observed_at":"2026-08-01T07:20:07.524287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1907.04869/citation-record","integrity":"/paper/1907.04869/integrity","json":"/paper/1907.04869/citation-record.json","paper":"/paper/1907.04869"},"outbound":[],"paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 66 inbound Pith citation observations for arXiv:1907.04869."}