{"as_of":"2026-08-15T17:23:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c16d6df355f879990b3fb16fe9081344fc74ba20108344f691ad31eee245b6e7","coverage":[{"denominator":43,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":43,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:42:33.118270Z","state":"measured"},{"denominator":43,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":43,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/1908.04619/citation-record","integrity":"/paper/1908.04619/integrity","json":"/paper/1908.04619/citation-record.json","paper":"/paper/1908.04619"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-14T13:42:32.991338Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:32.991338Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:99125723f7070c46bd0f6c6f4ebd32fa3fa9f298fd4c6fd27111fd610fe020d1","observation_id":"8b50e1f6-efed-4404-961e-d3294e52dec0","resolution":{"observed_at":"2026-08-14T13:42:32.991338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01589","last_updated":"2016-06-17T14:55:14Z","snapshot_observed_at":"2026-08-15T15:19:00.841595Z","submitted_at":"2015-02-05T15:08:33Z","title":"Planck 2015 results. XIII. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01589","snapshot_observed_at":"2026-08-14T13:42:32.995074Z","title":"Planck 2015 results. XIII. Cosmological parameters,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:32.995074Z"},"links":{"cited_paper":"/paper/1502.01589","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:58cbbbed47cefc4204e9a1bd4add4505dc3cc624467c3e765ecb9f95e2ba6ce8","observation_id":"32adee23-51e2-4d03-8a88-39be01225aea","resolution":{"observed_at":"2026-08-14T13:42:32.995074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07603","last_updated":"2019-03-27T15:38:08Z","snapshot_observed_at":"2026-08-14T21:43:57.540409Z","submitted_at":"2019-03-18T17:50:59Z","title":"Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07603","snapshot_observed_at":"2026-08-14T13:42:32.998559Z","title":"Large Magellanic Cloud Cepheid Stan- dards Provide a 1% Foundation for the Determina- tion of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:32.998559Z"},"links":{"cited_paper":"/paper/1903.07603","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:330d3afd4088b82774b015aa951aa96b8064430078d3f9b116829e679bd602ba","observation_id":"a12083d4-42c6-4c88-b2a4-db04925db543","resolution":{"observed_at":"2026-08-14T13:42:32.998559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.10655","last_updated":"2018-05-25T17:29:35Z","snapshot_observed_at":"2026-08-14T19:21:05.545475Z","submitted_at":"2018-04-27T19:18:44Z","title":"Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.10655","snapshot_observed_at":"2026-08-14T13:42:33.001955Z","title":"Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.001955Z"},"links":{"cited_paper":"/paper/1804.10655","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:c238a18d624b7b038c009edc66eabc446d3e0bdbef863599a801050ddbff11dc","observation_id":"cdba0c49-b47d-4dbc-8508-c9b119144d37","resolution":{"observed_at":"2026-08-14T13:42:33.001955Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.01424","last_updated":"2016-06-09T20:24:48Z","snapshot_observed_at":"2026-08-14T22:02:56.475749Z","submitted_at":"2016-04-05T21:00:26Z","title":"A 2.4% Determination of the Local Value of the Hubble Constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.01424","snapshot_observed_at":"2026-08-14T13:42:33.005351Z","title":"A 2.4% Determination of the Local Value of the Hubble Constant,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.005351Z"},"links":{"cited_paper":"/paper/1604.01424","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:a66ff968a8b0a8d3d0d6641bc8c25a55b6d0076bdf6a0fe720b0b95e04c34467","observation_id":"db090d89-edf7-48b6-af39-9b927e8b0b34","resolution":{"observed_at":"2026-08-14T13:42:33.005351Z","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":"2026-08-15T13:30:22.129548Z","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":"2026-08-15T12:40:00.802794Z","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:c5d4e4b69e7c02ff7a824af9ea7bb839a0774a73ef455a7c1dc005d491c07ca3","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":"1907.05922","last_updated":"2019-07-12T18:56:31Z","snapshot_observed_at":"2026-08-14T16:06:17.561878Z","submitted_at":"2019-07-12T18:56:31Z","title":"The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.05922","snapshot_observed_at":"2026-08-14T13:42:33.012157Z","title":"The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.012157Z"},"links":{"cited_paper":"/paper/1907.05922","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:286c482209c605f253bb67cce5166532009cc2ff2a64c06080d104a3554a6d86","observation_id":"b29a1791-a6cf-48a6-92d7-99fdc3fef464","resolution":{"observed_at":"2026-08-14T13:42:33.012157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.00993","last_updated":"2019-10-14T23:31:05Z","snapshot_observed_at":"2026-08-14T15:24:08.025366Z","submitted_at":"2019-08-02T18:09:29Z","title":"Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.00993","snapshot_observed_at":"2026-08-14T13:42:33.015063Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.015063Z"},"links":{"cited_paper":"/paper/1908.00993","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:0ac742d42c7601da8920078ce4b845902a25f5b22841d1638be8775e0beebddc","observation_id":"9ac6b5e5-f875-4dd3-82d1-bfb1f2eaf251","resolution":{"observed_at":"2026-08-14T13:42:33.015063Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-08-15T06:22:52.301428Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10625","snapshot_observed_at":"2026-08-14T13:42:33.018014Z","title":"Tensions between the Early and the Late Universe,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.018014Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:6415d50fafa8b1e2a5ee019939a57f5358deed57ce50c58d4bbdc30f7a79eb8e","observation_id":"1751e9e3-5141-44d2-96cc-7252eea13ed4","resolution":{"observed_at":"2026-08-14T13:42:33.018014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.11298","last_updated":"2019-05-20T10:57:21Z","snapshot_observed_at":"2026-08-14T17:09:27.419823Z","submitted_at":"2019-02-28T18:57:40Z","title":"Measuring the Homogeneity of the Universe Using Polarization Drift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.11298","snapshot_observed_at":"2026-08-14T13:42:33.020863Z","title":"Measuring the Homo- geneity of the Universe Using Polarization Drift,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.020863Z"},"links":{"cited_paper":"/paper/1902.11298","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:4359e954be77e4f33732f66da83f78122df916d65df74db909e1f86c30e5b3bf","observation_id":"bd8936ac-859c-48c6-bf04-e6e52da4ef0b","resolution":{"observed_at":"2026-08-14T13:42:33.020863Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.03114","last_updated":"2017-02-24T12:45:19Z","snapshot_observed_at":"2026-08-14T21:53:24.934015Z","submitted_at":"2016-06-09T20:47:06Z","title":"The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys","version":2},"cited_work":{"arxiv_id":"1606.03114","doi":null,"metadata_source":"pith","pith_arxiv_id":"1606.03114","snapshot_observed_at":"2026-08-14T13:42:33.379207Z","title":"The Alcock Paczynski test with Baryon Acoustic Oscillations: systematic effects for future surveys","venue":"astro-ph.CO","work_id":"385b7828-83a3-47ad-976a-b238dd8f5a18","year":2016},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.023754Z"},"links":{"cited_paper":"/paper/1606.03114","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:84631fba5a302ae92bed54d42e54f88257edb99a72d3b09e61f0e2cfaba413a9","observation_id":"7a6c272a-cdb0-4d80-bcc4-82acb3e7dae3","resolution":{"observed_at":"2026-08-14T13:42:33.382797Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-14T19:02:24.105988Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-08-14T13:42:33.026622Z","title":"Model independent H(z) reconstruction using the cosmic in- verse distance ladder,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.026622Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:96e35de9cf3f23b9d5c6ae2b09dbd102e107b261f9e0f36af850a8bf1cd047ee","observation_id":"9b641a45-95c1-4f3a-8e4f-40025c603aab","resolution":{"observed_at":"2026-08-14T13:42:33.026622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.00180","last_updated":"2016-06-01T09:03:30Z","snapshot_observed_at":"2026-08-15T15:59:06.115749Z","submitted_at":"2016-06-01T09:03:30Z","title":"Cosmology and Fundamental Physics with the Euclid Satellite","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.00180","snapshot_observed_at":"2026-08-14T13:42:33.029696Z","title":"Cosmology and fundamental physics with the Euclid satellite,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.029696Z"},"links":{"cited_paper":"/paper/1606.00180","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:0dd552561b486bc8f120f5ae1df3e2f34b3961912c5b106966d1a9922681a4f4","observation_id":"a6b98857-1ba7-40a1-9ec2-e7b910605139","resolution":{"observed_at":"2026-08-14T13:42:33.029696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02743","last_updated":"2018-11-07T03:12:27Z","snapshot_observed_at":"2026-08-14T18:03:00.382832Z","submitted_at":"2018-11-07T03:12:27Z","title":"Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.02743","snapshot_observed_at":"2026-08-14T13:42:33.032601Z","title":"Cosmology with Phase 1 of the Square Kilometre Array: Red Book 2018: Technical speciﬁcations and performance forecasts,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.032601Z"},"links":{"cited_paper":"/paper/1811.02743","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:46dbe157bbc5d5d30b02c2ffa926a992a504f01573658a0fabc5348ffb40984d","observation_id":"01a509d7-bd45-4aad-9737-a8ce6d46cf76","resolution":{"observed_at":"2026-08-14T13:42:33.032601Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.07562","last_updated":"2016-01-22T02:10:19Z","snapshot_observed_at":"2026-08-14T22:30:54.543307Z","submitted_at":"2015-09-24T23:00:32Z","title":"Extending cosmological tests of General Relativity with the Square Kilometre Array","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.07562","snapshot_observed_at":"2026-08-14T13:42:33.035586Z","title":"Extending cosmological tests of General Rela- tivity with the Square Kilometre Array,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.035586Z"},"links":{"cited_paper":"/paper/1509.07562","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:83abdccaec2f5bafe6a95d53b6c695c1603193a6be99accf4885fd6e3782a9c0","observation_id":"1a8a8f1f-9fe4-493f-9537-6f2279050653","resolution":{"observed_at":"2026-08-14T13:42:33.035586Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1609.00019","last_updated":"2016-08-31T20:01:02Z","snapshot_observed_at":"2026-08-14T21:41:53.476869Z","submitted_at":"2016-08-31T20:01:02Z","title":"Baryonic acoustic oscillations from 21cm intensity mapping: the Square Kilometre Array case","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1609.00019","snapshot_observed_at":"2026-08-14T13:42:33.038546Z","title":"Bary- onic acoustic oscillations from 21 cm intensity mapping: the Square Kilometre Array case,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.038546Z"},"links":{"cited_paper":"/paper/1609.00019","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:c20365680f4a10c6b6bb0b7b112bf5bfc58d459dcb0692b45769f884db9cf5bd","observation_id":"2ec75991-d6b1-40c8-9331-10163c47d153","resolution":{"observed_at":"2026-08-14T13:42:33.038546Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1402.5429","last_updated":"2014-02-21T21:24:00Z","snapshot_observed_at":"2026-08-14T23:43:47.053948Z","submitted_at":"2014-02-21T21:24:00Z","title":"Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1402.5429","snapshot_observed_at":"2026-08-14T13:42:33.041411Z","title":"Evidence for a Lower Value for H0 from Cosmic Chronometers Data?,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.041411Z"},"links":{"cited_paper":"/paper/1402.5429","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:1c13314146c469cb6d53edade61b04daa11176511a42c87dc5daa8483a5730d5","observation_id":"898adc03-b2e6-4641-a430-c43be8d7d6c3","resolution":{"observed_at":"2026-08-14T13:42:33.041411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.01202","last_updated":"2016-10-01T14:17:12Z","snapshot_observed_at":"2026-08-14T21:37:12.801970Z","submitted_at":"2016-10-01T14:17:12Z","title":"Model-independent determination on $H_0$ using the latest $H(z)$ data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.01202","snapshot_observed_at":"2026-08-14T13:42:33.044357Z","title":"Model-independent deter- mination of H0 using the latest cosmic chronometer data,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.044357Z"},"links":{"cited_paper":"/paper/1610.01202","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:b9e3b6d2599745b2669f9a197d1fa1f54733b8952c0537272d9a43fdb8b1e11e","observation_id":"fdbc4bc8-dec9-4ada-9a88-3afd822749db","resolution":{"observed_at":"2026-08-14T13:42:33.044357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.01505","last_updated":"2018-04-09T12:09:27Z","snapshot_observed_at":"2026-08-14T19:48:48.024744Z","submitted_at":"2018-02-05T16:36:45Z","title":"$H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.01505","snapshot_observed_at":"2026-08-14T13:42:33.047219Z","title":"H0 from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.047219Z"},"links":{"cited_paper":"/paper/1802.01505","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:7b88ed501293fd98818983de39d69ad32e47ba978a6e58753843ad1f3dc2e97d","observation_id":"90f89aa4-2158-4382-b097-08b8d2251fc7","resolution":{"observed_at":"2026-08-14T13:42:33.047219Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.2832","last_updated":"2012-05-31T16:02:21Z","snapshot_observed_at":"2026-08-15T04:13:13.371419Z","submitted_at":"2012-04-12T20:00:11Z","title":"Reconstruction of dark energy and expansion dynamics using Gaussian processes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.2832","snapshot_observed_at":"2026-08-14T13:42:33.049983Z","title":"Reconstruc- tion of dark energy and expansion dynamics us- ing Gaussian processes,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.049983Z"},"links":{"cited_paper":"/paper/1204.2832","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:55f5e5200fdbebb492a7d1cb8ae68d6813508a3d8cf0e1d31291094e1fa4aa23","observation_id":"011802d3-3174-47ad-9d93-43fc95bd2dd9","resolution":{"observed_at":"2026-08-14T13:42:33.049983Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.2272","last_updated":"2012-07-10T16:52:06Z","snapshot_observed_at":"2026-08-15T04:13:28.446386Z","submitted_at":"2012-04-10T20:01:57Z","title":"Gaussian Process Cosmography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.2272","snapshot_observed_at":"2026-08-14T13:42:33.053083Z","title":"Gaussian Process Cosmography,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.053083Z"},"links":{"cited_paper":"/paper/1204.2272","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:89626c1a16f0ae6667ae6265534b4726d3a0a2710c62d01f8069046f608fc135","observation_id":"c43e6dec-ea7c-4e6e-b41a-61a9edf72c37","resolution":{"observed_at":"2026-08-14T13:42:33.053083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1308.4099","last_updated":"2013-12-05T11:10:24Z","snapshot_observed_at":"2026-08-15T00:06:23.001774Z","submitted_at":"2013-08-19T18:59:49Z","title":"Null tests of the cosmological constant using supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1308.4099","snapshot_observed_at":"2026-08-14T13:42:33.056050Z","title":"Null tests of the cosmological constant using supernovae,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.056050Z"},"links":{"cited_paper":"/paper/1308.4099","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:5b1267d6f8257cba59f78bf7cd5cb107f0f137eb4cb0343c8cb1ebef8839120a","observation_id":"3c105e43-e2da-4db5-90f0-1cc478c5e8ae","resolution":{"observed_at":"2026-08-14T13:42:33.056050Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1602.01015","last_updated":"2016-02-02T17:22:44Z","snapshot_observed_at":"2026-08-14T22:12:00.231742Z","submitted_at":"2016-02-02T17:22:44Z","title":"Non-parametric reconstruction of cosmological matter perturbations","version":1},"cited_work":{"arxiv_id":"1602.01015","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.01015","snapshot_observed_at":"2026-08-14T13:42:33.285677Z","title":"Non-parametric reconstruction of cosmological matter perturbations","venue":"astro-ph.CO","work_id":"5bd9ebe6-1377-4eec-ad45-cfb8ffac9dcf","year":2016},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.058851Z"},"links":{"cited_paper":"/paper/1602.01015","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:704f590000068a47df6740ad87b93abca31e12bfe1255dbb54180678a8439179","observation_id":"452b990f-04b4-44de-b90d-82a9ab756a58","resolution":{"observed_at":"2026-08-14T13:42:33.289349Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.00027","last_updated":"2018-10-17T15:37:02Z","snapshot_observed_at":"2026-08-14T19:20:22.703599Z","submitted_at":"2018-04-30T18:00:03Z","title":"Model-independent reconstruction of the linear anisotropic stress $\\eta$","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.00027","snapshot_observed_at":"2026-08-14T13:42:33.062018Z","title":"Model- independent reconstruction of the linear anisotropic stress η,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.062018Z"},"links":{"cited_paper":"/paper/1805.00027","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:96f64c0b76302c2d4ac442ac5899c46c31ab1598044d75470731e834d46c24ff","observation_id":"2b121c74-e80d-46b4-b9bd-e38b6cc718a9","resolution":{"observed_at":"2026-08-14T13:42:33.062018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.02333","last_updated":"2018-12-06T03:20:17Z","snapshot_observed_at":"2026-08-14T17:47:45.865230Z","submitted_at":"2018-12-06T03:20:17Z","title":"Null test for interactions in the dark sector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.02333","snapshot_observed_at":"2026-08-14T13:42:33.064954Z","title":"Null test for interactions in the dark sec- tor,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.064954Z"},"links":{"cited_paper":"/paper/1812.02333","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:92622296414e5ebd0ae6a557ad9c0a4cb9a26a6c448beebfac3fdc84787f0bcb","observation_id":"1f0928dd-616f-4209-8029-cb35eeb9e0ff","resolution":{"observed_at":"2026-08-14T13:42:33.064954Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.09900","last_updated":"2018-07-16T21:19:43Z","snapshot_observed_at":"2026-08-14T19:11:22.720597Z","submitted_at":"2018-05-24T21:09:46Z","title":"The impact of the cosmic variance on $H_0$ on cosmological analyses","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.09900","snapshot_observed_at":"2026-08-14T13:42:33.068055Z","title":"Impact of the cosmic vari- ance on H0 on cosmological analyses,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.068055Z"},"links":{"cited_paper":"/paper/1805.09900","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:03726d021c9523817c854744363fcdca7ead318009a477669bdc76d2c855a81c","observation_id":"a2c2319f-e340-487c-ab9f-17e240561894","resolution":{"observed_at":"2026-08-14T13:42:33.068055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.04966","last_updated":"2019-09-11T06:57:24Z","snapshot_observed_at":"2026-08-14T18:16:16.342337Z","submitted_at":"2018-10-11T11:55:22Z","title":"How does an incomplete sky coverage affect the Hubble Constant variance?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.04966","snapshot_observed_at":"2026-08-14T13:42:33.071052Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.071052Z"},"links":{"cited_paper":"/paper/1810.04966","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:9716b7ad810bcb88e0439f4f85ebb6d051c540172adc9f29d6c7722643e32a0f","observation_id":"49794afe-a283-4562-8ae9-d8de34614a28","resolution":{"observed_at":"2026-08-14T13:42:33.071052Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.06531","last_updated":"2018-07-06T15:54:34Z","snapshot_observed_at":"2026-08-14T20:02:31.509106Z","submitted_at":"2017-12-18T17:16:23Z","title":"A 2 per cent Hubble constant measurement from standard sirens within 5 years","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.06531","snapshot_observed_at":"2026-08-14T13:42:33.074326Z","title":"A two per cent Hubble constant measurement from standard sirens within ﬁve years,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.074326Z"},"links":{"cited_paper":"/paper/1712.06531","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:7517f731b45d749dd7cd368dce6b6cd2cf99bf2cf441be915c9deabf04984bbf","observation_id":"561e5cd2-718b-458a-bc18-1fd61f88ecd4","resolution":{"observed_at":"2026-08-14T13:42:33.074326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.06085","last_updated":"2018-07-04T09:16:33Z","snapshot_observed_at":"2026-08-14T19:25:13.142923Z","submitted_at":"2018-04-17T07:49:35Z","title":"Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.06085","snapshot_observed_at":"2026-08-14T13:42:33.077387Z","title":"Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.077387Z"},"links":{"cited_paper":"/paper/1804.06085","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:49c29f7d5b1db1ba70a010de35730140230609d6937d8f8708a2fc2586b52d9d","observation_id":"32adf742-3b1a-4e3f-a484-2ff6a86a833d","resolution":{"observed_at":"2026-08-14T13:42:33.077387Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1804.07337","last_updated":"2018-06-30T13:23:55Z","snapshot_observed_at":"2026-08-14T19:24:07.056131Z","submitted_at":"2018-04-19T18:59:34Z","title":"Measuring the Hubble constant with neutron star black hole mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1804.07337","snapshot_observed_at":"2026-08-14T13:42:33.080198Z","title":"Measuring the Hubble con- stant with neutron star black hole mergers,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.080198Z"},"links":{"cited_paper":"/paper/1804.07337","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:0472902ebb5cd57da59fcdb9e05987f205405a213281d057e40761039684727d","observation_id":"eeb7043f-c5c0-4f81-8283-9f3fc2cb67e6","resolution":{"observed_at":"2026-08-14T13:42:33.080198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.11723","last_updated":"2019-10-07T16:57:08Z","snapshot_observed_at":"2026-08-14T17:51:51.520195Z","submitted_at":"2018-11-28T18:24:13Z","title":"Unbiased Hubble constant estimation from binary neutron star mergers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.11723","snapshot_observed_at":"2026-08-14T13:42:33.083096Z","title":"Unbiased Hubble constant estimation from binary neutron star mergers,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.083096Z"},"links":{"cited_paper":"/paper/1811.11723","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:8d47a53be12436b45e1730f41492a50c08c477e252766d9ad2950636aa238c52","observation_id":"0c83b4f5-4ae4-4cea-9e99-6fa18abc3a16","resolution":{"observed_at":"2026-08-14T13:42:33.083096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.07775","last_updated":"2018-12-19T06:38:08Z","snapshot_observed_at":"2026-08-15T15:17:57.182912Z","submitted_at":"2018-12-19T06:38:08Z","title":"Will Gravitational Wave Sirens Determine the Hubble Constant?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.07775","snapshot_observed_at":"2026-08-14T13:42:33.085929Z","title":"Will Grav- itational Wave Sirens Determine the Hubble Constant?,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.085929Z"},"links":{"cited_paper":"/paper/1812.07775","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:fd491adce89b5fe9d7eefc3d35b130ba31afe68115fd2e00d9b0288536ea45e4","observation_id":"edc2e001-3de8-479e-9541-7a85dabb10c3","resolution":{"observed_at":"2026-08-14T13:42:33.085929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.11122","last_updated":"2019-07-01T15:24:25Z","snapshot_observed_at":"2026-08-14T16:26:01.650335Z","submitted_at":"2019-05-27T11:10:28Z","title":"Gravitational wave standard sirens and cosmological parameter measurement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.11122","snapshot_observed_at":"2026-08-14T13:42:33.088871Z","title":"Gravitational wave standard sirens and cosmological parameter measurement,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.088871Z"},"links":{"cited_paper":"/paper/1905.11122","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:aa5a70d80d75746bc904973c6a02fe00386ea9eb5dae95c28ca3d98f486d632b","observation_id":"333d42fa-4c44-47da-aefc-725449a45d32","resolution":{"observed_at":"2026-08-14T13:42:33.088871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.03404","last_updated":"2019-01-11T16:12:29Z","snapshot_observed_at":"2026-08-14T19:47:16.792171Z","submitted_at":"2018-02-09T19:00:04Z","title":"Prospects for resolving the Hubble constant tension with standard sirens","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1802.03404","snapshot_observed_at":"2026-08-14T13:42:33.091714Z","title":"Prospects for resolving the Hubble constant tension with standard sirens,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.091714Z"},"links":{"cited_paper":"/paper/1802.03404","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:6213bef1abe9d39d5bda8b9b468786f4e46058a3ce5d0382440545ac013f8eba","observation_id":"e03ab12c-23a5-4380-9ccf-44e2329854b3","resolution":{"observed_at":"2026-08-14T13:42:33.091714Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.12097","last_updated":"2019-11-08T11:01:21Z","snapshot_observed_at":"2026-08-15T01:46:45.260340Z","submitted_at":"2019-03-28T16:31:04Z","title":"A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\\gamma$-ray attenuation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.12097","snapshot_observed_at":"2026-08-14T13:42:33.094691Z","title":"A new measurement of the Hubble constant and matter content of the Universe using extra- galactic background lightγ-ray attenuation,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.094691Z"},"links":{"cited_paper":"/paper/1903.12097","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:1aebf23d3d9f1c78c18f39fa4e186803d409249338ea709b518cd273dcdb1b01","observation_id":"64f342f8-0b88-45e9-86ce-dc97d1a46a26","resolution":{"observed_at":"2026-08-14T13:42:33.094691Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05951","last_updated":"2017-10-16T18:28:23Z","snapshot_observed_at":"2026-08-14T20:23:13.923413Z","submitted_at":"2017-10-16T18:28:23Z","title":"An independent determination of the local Hubble constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05951","snapshot_observed_at":"2026-08-14T13:42:33.097661Z","title":"An independent determi- nation of the local Hubble constant,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.097661Z"},"links":{"cited_paper":"/paper/1710.05951","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:3440548a8a57298e2469139883be8ea6d980a8f2b7ce7812df92c7905e11d8bd","observation_id":"ae0d7093-560a-43d3-8ace-c124b1747c13","resolution":{"observed_at":"2026-08-14T13:42:33.097661Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00403","last_updated":"2017-11-01T15:42:57Z","snapshot_observed_at":"2026-08-15T12:26:41.534677Z","submitted_at":"2017-11-01T15:42:57Z","title":"Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00403","snapshot_observed_at":"2026-08-14T13:42:33.100689Z","title":"Dark En- ergy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.100689Z"},"links":{"cited_paper":"/paper/1711.00403","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:34dd7ac781f9445097bfe24cd76298b9cf1e89dda81fe3d30173d13b21806186","observation_id":"9480866b-3714-4977-9de0-1fe0cb609699","resolution":{"observed_at":"2026-08-14T13:42:33.100689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.09149","last_updated":"2017-09-21T03:36:34Z","snapshot_observed_at":"2026-08-14T20:51:10.435134Z","submitted_at":"2017-06-28T07:39:24Z","title":"A measurement of the Hubble constant using galaxy redshift surveys","version":2},"cited_work":{"arxiv_id":"1706.09149","doi":null,"metadata_source":"pith","pith_arxiv_id":"1706.09149","snapshot_observed_at":"2026-08-14T13:42:33.169935Z","title":"A measurement of the Hubble constant using galaxy redshift surveys","venue":"astro-ph.CO","work_id":"31eaf40f-0eb3-491f-a442-3ee797f3d27e","year":2017},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.103468Z"},"links":{"cited_paper":"/paper/1706.09149","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:f23e5a0fc7f2c662b3f4caaa6160ad6f0c9d64f5d3af7389d206bf3521eaaa4c","observation_id":"07f820ef-cf40-42ab-a84e-0e82d4660c6f","resolution":{"observed_at":"2026-08-14T13:42:33.175101Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05835","last_updated":"2017-10-16T16:57:20Z","snapshot_observed_at":"2026-08-14T20:23:19.810604Z","submitted_at":"2017-10-16T16:57:20Z","title":"A gravitational-wave standard siren measurement of the Hubble constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.05835","snapshot_observed_at":"2026-08-14T13:42:33.106268Z","title":"A gravitational- wave standard siren measurement of the Hubble con- stant,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.106268Z"},"links":{"cited_paper":"/paper/1710.05835","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:019e4b16e0b4c6968103ab37193154cd2a3c3f079fbbecab072cf7e47b7ef9f2","observation_id":"89b564f2-b34e-4ad3-8ce5-cce88d6a64b4","resolution":{"observed_at":"2026-08-14T13:42:33.106268Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.10216","last_updated":"2020-01-16T07:28:28Z","snapshot_observed_at":"2026-08-14T16:27:09.904801Z","submitted_at":"2019-05-24T13:10:23Z","title":"Debiasing Cosmic Gravitational Wave Sirens","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.10216","snapshot_observed_at":"2026-08-14T13:42:33.109100Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.109100Z"},"links":{"cited_paper":"/paper/1905.10216","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:da09e92ecc8ab85443b7d73e3cf09ace193212b9b01c009a286ba2800a072a27","observation_id":"9f36a042-da64-4485-aa45-48ef86fe6400","resolution":{"observed_at":"2026-08-14T13:42:33.109100Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.00036","snapshot_observed_at":"2026-08-14T13:42:33.112153Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey De- sign,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.112153Z"},"links":{"cited_paper":"/paper/1611.00036","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:d125c1ec9c4076dfd52bf4e52a3ab73e3ebbf225340230c6f8055399c32642bd","observation_id":"9b6ac58e-e158-4ba6-8dd0-c9a4f9318604","resolution":{"observed_at":"2026-08-14T13:42:33.112153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.06099","last_updated":"2017-09-18T18:00:22Z","snapshot_observed_at":"2026-08-15T01:11:25.450557Z","submitted_at":"2017-09-18T18:00:22Z","title":"MeerKLASS: MeerKAT Large Area Synoptic Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.06099","snapshot_observed_at":"2026-08-14T13:42:33.115197Z","title":"MeerKLASS: MeerKAT Large Area Synoptic Survey,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.115197Z"},"links":{"cited_paper":"/paper/1709.06099","citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:a9f808487f2bb54df7991d32f77e62924df392b288bf2056f3ed3ae7c7dd7f55","observation_id":"f2831f9e-3d3d-43e6-bcd1-828d79e1888a","resolution":{"observed_at":"2026-08-14T13:42:33.115197Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:42:33.464617Z","title":null,"venue":null,"work_id":"1ee5d113-107d-439d-99d7-157a755438bb","year":null},"citing_paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T13:42:33.118270Z"},"links":{"citing_paper":"/paper/1908.04619"},"observation_digest":"sha256:18e8e96bfa2f2ec5aaad628e08abfb4b3fab0f33fc062ad6189ccdd6ee1f033b","observation_id":"28f81bce-2a8a-4e4c-a340-8346cc168c77","resolution":{"observed_at":"2026-08-14T13:42:33.467659Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.04619","last_updated":"2020-05-01T16:31:01Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T12:40:00.802794Z","submitted_at":"2019-08-13T13:02:29Z","title":"The Hubble constant tension with next-generation galaxy surveys"},"reference_resolution":{"displayed":43,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":40,"verified_exact":3,"verified_fuzzy":0},"total_outbound_references":43},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 43 of 43 outbound references and 0 inbound Pith citation observations for arXiv:1908.04619."}