{"as_of":"2026-08-15T03:17:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:600ef9b6c4db9bd554bfde2b52ce02b3a643dc42649ed274b7f71a3aa39cdbef","coverage":[{"denominator":65,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":65,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T13:02:34.002583Z","state":"measured"},{"denominator":67,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":67,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T05:58:02.828055Z","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":"2026-05-17T23:41:11.669355Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.06100","snapshot_observed_at":"2026-08-14T05:58:02.828055Z","title":"Jeong and M","venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"1909.00568","last_updated":"2020-01-29T08:59:46Z","snapshot_observed_at":"2026-08-14T14:52:57.914578Z","submitted_at":"2019-09-02T07:02:31Z","title":"B-mode Power Spectrum of CMB via Polarized Compton Scattering","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T05:58:02.828055Z"},"links":{"cited_paper":"/paper/1908.06100","citing_paper":"/paper/1909.00568"},"observation_digest":"sha256:09a6b8d2dbce3d5e8dbd5d414b9e87cd3b036baa35c4489df72e255b7c97883a","observation_id":"3e7a397e-2284-4b57-b574-e5138fba0b59","resolution":{"observed_at":"2026-08-14T05:58:02.828055Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"cited_work":{"arxiv_id":"1908.06100","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1908.06100","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","venue":null,"work_id":"c6fc87e2-8e59-4f36-8847-0a33112a946e","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":122,"source":"pdf_text","source_observed_at":"2026-05-17T23:41:11.040188Z"},"links":{"cited_paper":"/paper/1908.06100","citing_paper":"/paper/2211.04492"},"observation_digest":"sha256:8b00c8bc994f438e644fdae30c4bb5cffde27cbc987441d9b062f92da5207c73","observation_id":"f4b20cfe-7f7d-4b54-a4fa-f4f5202ee3ef","resolution":{"observed_at":"2026-05-17T23:41:11.671796Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1908.06100/citation-record","integrity":"/paper/1908.06100/integrity","json":"/paper/1908.06100/citation-record.json","paper":"/paper/1908.06100"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1706.02739","last_updated":"2017-06-08T19:38:32Z","snapshot_observed_at":"2026-08-14T20:55:12.300186Z","submitted_at":"2017-06-08T19:38:32Z","title":"Cosmology at at Crossroads: Tension with the Hubble Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.02739","snapshot_observed_at":"2026-08-14T13:02:33.700256Z","title":"Cosmology at a Crossroads,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.700256Z"},"links":{"cited_paper":"/paper/1706.02739","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:5559dd47444a0c2a6c175a3521012fdbf43645313db212badd441bcc3cfe94f9","observation_id":"765fa9eb-e24a-4443-ac86-bf5129bd7773","resolution":{"observed_at":"2026-08-14T13:02:33.700256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.00007","last_updated":"2017-11-08T21:59:10Z","snapshot_observed_at":"2026-08-14T20:50:26.078713Z","submitted_at":"2017-06-30T18:00:04Z","title":"Clarifying the Hubble constant tension with a Bayesian hierarchical model of the local distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.00007","snapshot_observed_at":"2026-08-14T13:02:33.706279Z","title":"Clarify- ing the Hubble constant tension with a Bayesian hierar- chical model of the local distance ladder,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.706279Z"},"links":{"cited_paper":"/paper/1707.00007","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:6ea0f0bd30f6b107a4726f004d8627ff73e265ae67e7e83390b6f12e7d26632f","observation_id":"052c5c9a-0fa6-4b2d-a390-e454a2bc6aa4","resolution":{"observed_at":"2026-08-14T13:02:33.706279Z","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":"2026-07-06T08:09:59.842324Z","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":"2026-08-14T13:02:33.710952Z","title":"Tensions between the Early and the Late Universe,","venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.710952Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:0eeae8fe07ed430685f3f41e1a812bf2f0d0fecc28a2daeb9bbe0916bf93c8a8","observation_id":"f9334589-6ab0-4dc6-880b-e56b880387a5","resolution":{"observed_at":"2026-08-14T13:02:33.710952Z","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":"2026-08-14T13:02:33.715569Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.715569Z"},"links":{"cited_paper":"/paper/1604.01424","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:1965566dc3d3ddf43c419fa300056bd528d81f7ccf9aa267bf3891c67d8e61a6","observation_id":"2fe23858-ad51-4779-824f-ab2163903a35","resolution":{"observed_at":"2026-08-14T13:02:33.715569Z","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":"2026-08-14T13:02:33.721147Z","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":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.721147Z"},"links":{"cited_paper":"/paper/1804.10655","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:bf2162614516e93c3aba5ab44292aec1673cf81ad5d5db78e1377f2477b197f8","observation_id":"a4728fb2-4e85-4ad5-990f-ee6ff3715219","resolution":{"observed_at":"2026-08-14T13:02:33.721147Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.01790","last_updated":"2017-01-25T08:29:41Z","snapshot_observed_at":"2026-08-14T21:49:30.579039Z","submitted_at":"2016-07-06T20:00:04Z","title":"H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: $H_0$ to 3.8% precision from strong lensing in a flat $\\Lambda$CDM model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.01790","snapshot_observed_at":"2026-08-14T13:02:33.726592Z","title":"H0LiCOW – V. New COSMOGRAIL time delays of HE 0435-1223: H0 to 3.8 per cent pre- cision from strong lensing in a ﬂat ΛCDM model,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.726592Z"},"links":{"cited_paper":"/paper/1607.01790","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:f134b2703cb477a43846324b401a9dd370ac02790896d575a8b6f448a7577dc5","observation_id":"3d991ce6-0aa5-4475-8141-a045ca4b5ed4","resolution":{"observed_at":"2026-08-14T13:02:33.726592Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.01274","last_updated":"2019-05-24T16:29:15Z","snapshot_observed_at":"2026-08-14T18:32:58.081187Z","submitted_at":"2018-09-05T00:18:39Z","title":"H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.01274","snapshot_observed_at":"2026-08-14T13:02:33.731500Z","title":"H0LiCOW - IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.731500Z"},"links":{"cited_paper":"/paper/1809.01274","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:b6a423d10a119438a66dba0159fc3c93d2c826170a72db4a94aab21b2d3bb225","observation_id":"cc841474-6890-4bc0-b0e2-f47a01c36b99","resolution":{"observed_at":"2026-08-14T13:02:33.731500Z","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":"2026-08-14T23:01:13.900835Z","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":"2026-08-14T13:02:33.736241Z","title":"Planck 2015 results. XIII. Cosmological parameters,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.736241Z"},"links":{"cited_paper":"/paper/1502.01589","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:fb4c7a63da8e4fecf49003cfbf6da7224f1e74b29ee00e4a5c3ed35126ace857","observation_id":"ef2dc855-8ce1-4358-b689-cb906e1cb01b","resolution":{"observed_at":"2026-08-14T13:02:33.736241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","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":"2026-08-14T13:02:33.740553Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.740553Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:0cd6b1c2efb3b80a9e7a226289c8b88725f49efd31f24b96b6c03e92b742ce2e","observation_id":"fb59a740-8d55-45bd-b4c1-2f7ee52d45b3","resolution":{"observed_at":"2026-08-14T13:02:33.740553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.3461","last_updated":"2014-02-08T11:43:07Z","snapshot_observed_at":"2026-08-14T23:55:19.967350Z","submitted_at":"2013-11-14T11:33:37Z","title":"H0 Revisited","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.3461","snapshot_observed_at":"2026-08-14T13:02:33.744775Z","title":"H0 Revisited,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.744775Z"},"links":{"cited_paper":"/paper/1311.3461","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:0f4554f263db3bde527dc7789ce7fd65327dbd5d22e9d37bb367def20d580a19","observation_id":"52dcfa58-6605-45c5-ac67-f8c2b9186dec","resolution":{"observed_at":"2026-08-14T13:02:33.744775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.00055","last_updated":"2016-02-17T19:11:23Z","snapshot_observed_at":"2026-08-14T22:25:27.961745Z","submitted_at":"2015-10-31T01:34:26Z","title":"Quantifying discordance in the 2015 Planck CMB spectrum","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.00055","snapshot_observed_at":"2026-08-14T13:02:33.749153Z","title":"Quanti- fying discordance in the 2015 Planck CMB spectrum,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.749153Z"},"links":{"cited_paper":"/paper/1511.00055","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:f166a3d3585ce15ee2af641c5f9432d1700d93848dc2ce011efaa2954e58f4b6","observation_id":"73db2e9c-3544-4d8f-96d6-85961fb7d98d","resolution":{"observed_at":"2026-08-14T13:02:33.749153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.02487","last_updated":"2017-04-21T10:01:03Z","snapshot_observed_at":"2026-08-14T21:44:59.627118Z","submitted_at":"2016-08-08T15:26:32Z","title":"Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.02487","snapshot_observed_at":"2026-08-14T13:02:33.753000Z","title":"Planck in- termediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.753000Z"},"links":{"cited_paper":"/paper/1608.02487","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:963a1d7a19c39ded215c76b0ab52e4bcd0ee311ac96b55997b335b7e10561949","observation_id":"d4bd6030-2a49-4948-be85-85cc59932837","resolution":{"observed_at":"2026-08-14T13:02:33.753000Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00537","last_updated":"2019-04-25T00:24:38Z","snapshot_observed_at":"2026-08-14T18:05:33.676369Z","submitted_at":"2018-11-01T17:57:56Z","title":"Sounds Discordant: Classical Distance Ladder & $\\Lambda$CDM -based Determinations of the Cosmological Sound Horizon","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.00537","snapshot_observed_at":"2026-08-14T13:02:33.757404Z","title":"Sounds Discordant: Classical Dis- tance Ladder & ΛCDM -based Determinations of the Cosmological Sound Horizon,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.757404Z"},"links":{"cited_paper":"/paper/1811.00537","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:36369b0f9abd49de9d7a55a2775bb92df303a3479d33f58e18223d66f894485c","observation_id":"ca6aee83-f791-4e46-a82c-3103ba702623","resolution":{"observed_at":"2026-08-14T13:02:33.757404Z","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":"2026-08-14T13:02:33.762351Z","title":"Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Be- yond LambdaCDM,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.762351Z"},"links":{"cited_paper":"/paper/1903.07603","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:7d026af2c29d39705fce52998bb580de116f021ff123b81ecabfd26deb480c88","observation_id":"e3985b94-7b1f-4b31-a443-9c21c44387dd","resolution":{"observed_at":"2026-08-14T13:02:33.762351Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.08096","last_updated":"2019-03-19T16:32:39Z","snapshot_observed_at":"2026-08-14T16:59:57.867349Z","submitted_at":"2019-03-19T16:32:39Z","title":"A distance to the Large Magellanic Cloud that is precise to one per cent","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.08096","snapshot_observed_at":"2026-08-14T13:02:33.766688Z","title":"A distance to the Large Magellanic Cloud that is precise to one per cent,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.766688Z"},"links":{"cited_paper":"/paper/1903.08096","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:5257469d6b89ecbcd3b19d90e975c5528d2fc75fd015372e529829a75d74feef","observation_id":"cd20c712-6d12-499f-ae00-2918034ec6b6","resolution":{"observed_at":"2026-08-14T13:02:33.766688Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-14T13:02:33.771776Z","title":"The Hubble Constant de- termined through an inverse distance ladder includ- ing quasar time delays and Type Ia supernovae,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.771776Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:48992cdeeafbbf088fee08541bafad524c3b3ad67aef046a3ff5cf91a6b3cc95","observation_id":"d774dced-0ceb-4913-b315-5c03f89c1568","resolution":{"observed_at":"2026-08-14T13:02:33.771776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.09781","last_updated":"2019-12-02T18:17:16Z","snapshot_observed_at":"2026-08-14T16:27:40.625367Z","submitted_at":"2019-05-23T17:12:01Z","title":"Model-independent determination of $H_0$ and $\\Omega_{K0}$ from strong lensing and type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.09781","snapshot_observed_at":"2026-08-14T13:02:33.775832Z","title":"Model- independent determination of H0 and Ω K0 from strong lensing and type Ia supernovae,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.775832Z"},"links":{"cited_paper":"/paper/1905.09781","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:b5b04e4204adec6774dc4c9cd75ab8657040e598205548c979b7ec158fdffb87","observation_id":"f783d5c0-d92f-47cf-9626-5e5e3e4125bd","resolution":{"observed_at":"2026-08-14T13:02:33.775832Z","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":"2026-08-14T13:02:33.781602Z","title":null,"venue":null,"work_id":null,"year":1907},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.781602Z"},"links":{"cited_paper":"/paper/1907.05922","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:620593c525859ccf277f1ccab279b26eb2e3e1829435a44e296645aac4088e68","observation_id":"ad8276fe-290d-4d85-841e-e7e95c68194d","resolution":{"observed_at":"2026-08-14T13:02:33.781602Z","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":"2026-08-14T13:02:33.788072Z","title":null,"venue":null,"work_id":null,"year":1908},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.788072Z"},"links":{"cited_paper":"/paper/1908.00993","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:baae7c3d300c0831be3642f16f97e0569545dd0f6b8bb8e8fe86ae184a6cb161","observation_id":"a3b96e12-4866-4de3-9e1f-261faeb29fef","resolution":{"observed_at":"2026-08-14T13:02:33.788072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9401003","last_updated":"1994-01-04T04:43:27Z","snapshot_observed_at":"2026-07-07T01:09:16.203858Z","submitted_at":"1994-01-04T04:43:27Z","title":"Small-Scale Cosmic Microwave Background Anisotropies as a Probe of the Geometry of the Universe","version":1},"cited_work":{"arxiv_id":"astro-ph/9401003","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9401003","snapshot_observed_at":"2026-08-14T13:02:34.783613Z","title":"Small-Scale Cosmic Microwave Background Anisotropies as a Probe of the Geometry of the Universe","venue":"astro-ph","work_id":"737f1895-7692-43ea-8716-69d245ce35e9","year":1994},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.794201Z"},"links":{"cited_paper":"/paper/astro-ph/9401003","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:3e15652a0e98347c8aad74fed1d425f68bb490a060b4086f8840138818ea92dd","observation_id":"6aa74e87-c744-42d3-aedc-37e5ff9b7770","resolution":{"observed_at":"2026-08-14T13:02:34.787293Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9507080","last_updated":"1995-07-21T19:46:04Z","snapshot_observed_at":"2026-07-07T01:11:30.626114Z","submitted_at":"1995-07-21T19:46:04Z","title":"Weighing the Universe with the Cosmic Microwave Background","version":1},"cited_work":{"arxiv_id":"astro-ph/9507080","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/9507080","snapshot_observed_at":"2026-08-14T13:02:34.768509Z","title":"Weighing the Universe with the Cosmic Microwave Background","venue":"astro-ph","work_id":"f49c0081-81d3-4be7-8591-ad0b9d70b16c","year":1995},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.799863Z"},"links":{"cited_paper":"/paper/astro-ph/9507080","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:740c4ca56080ae844c84e7b259d1c283f7f3a32ee937f770eb8231807c646641","observation_id":"863d9491-47bc-4cfb-b7cf-eb630b50e48d","resolution":{"observed_at":"2026-08-14T13:02:34.771975Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1608.01309","last_updated":"2016-11-06T23:41:15Z","snapshot_observed_at":"2026-08-14T21:45:33.346929Z","submitted_at":"2016-08-03T20:00:01Z","title":"Early dark energy, the Hubble-parameter tension, and the string axiverse","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.01309","snapshot_observed_at":"2026-08-14T13:02:33.805033Z","title":"Dark energy at early times, the Hubble parameter, and the string axiverse,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.805033Z"},"links":{"cited_paper":"/paper/1608.01309","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:450cd3c79f4e0ab9c916051c6626a3fd925f77976751919cca4f8e8489c4485d","observation_id":"331f8283-fd8c-4b55-958a-cfce17a852b1","resolution":{"observed_at":"2026-08-14T13:02:33.805033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.05617","last_updated":"2016-10-20T11:40:06Z","snapshot_observed_at":"2026-08-14T21:47:44.301416Z","submitted_at":"2016-07-19T14:55:13Z","title":"The trouble with $H_0$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.05617","snapshot_observed_at":"2026-08-14T13:02:33.812363Z","title":"The trouble with H0,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.812363Z"},"links":{"cited_paper":"/paper/1607.05617","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:8523f4a3305ef43798366c7a4ffef785f58eb5655d1c15e513fda281637be0f2","observation_id":"39aa59d8-6299-4812-a7c0-3a1cd38d7f6a","resolution":{"observed_at":"2026-08-14T13:02:33.812363Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.04083","last_updated":"2019-06-11T10:04:20Z","snapshot_observed_at":"2026-08-14T18:01:28.256190Z","submitted_at":"2018-11-09T19:00:00Z","title":"Early Dark Energy Can Resolve The Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.04083","snapshot_observed_at":"2026-08-14T13:02:33.816312Z","title":"Early Dark Energy Can Resolve The Hubble Tension,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.816312Z"},"links":{"cited_paper":"/paper/1811.04083","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:7880af2f71220706a7fbe48ae5b3b2e9a87e68f2a215aa94526702f3ff4bf483","observation_id":"dddc7aa8-d1c9-4fd1-a0ff-f10571393c11","resolution":{"observed_at":"2026-08-14T13:02:33.816312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.02333","last_updated":"2018-10-04T17:27:44Z","snapshot_observed_at":"2026-08-14T18:19:23.402656Z","submitted_at":"2018-10-04T17:27:44Z","title":"Phenomenology of Modified Gravity at Recombination","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.02333","snapshot_observed_at":"2026-08-14T13:02:33.821846Z","title":"Phenomenology of Modiﬁed Gravity at Recombination,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.821846Z"},"links":{"cited_paper":"/paper/1810.02333","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:58f8fcd78e8c6bf9ad3198ec2b0c6a04f24e9cd924f843475654e8ccdbc0f41e","observation_id":"c9b8d937-553c-4f7a-9658-e0368febd286","resolution":{"observed_at":"2026-08-14T13:02:33.821846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.00534","last_updated":"2019-04-02T14:25:47Z","snapshot_observed_at":"2026-08-14T17:22:11.245313Z","submitted_at":"2019-02-01T19:38:17Z","title":"The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.00534","snapshot_observed_at":"2026-08-14T13:02:33.826236Z","title":"The Neu- trino Puzzle: Anomalies, Interactions, and Cosmological Tensions,","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.826236Z"},"links":{"cited_paper":"/paper/1902.00534","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:6243542f23a6834f5e191a20f606e8cf76e2665093d027513d5512a4ab9c99b0","observation_id":"cdd93b6c-ad32-4c17-af13-80472596eb15","resolution":{"observed_at":"2026-08-14T13:02:33.826236Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.02727","last_updated":"2019-11-18T14:50:48Z","snapshot_observed_at":"2026-08-14T16:35:55.200142Z","submitted_at":"2019-05-07T18:00:01Z","title":"Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.02727","snapshot_observed_at":"2026-08-14T13:02:33.830697Z","title":"Constraining the Self-Interacting Neutrino In- terpretation of the Hubble Tension,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.830697Z"},"links":{"cited_paper":"/paper/1905.02727","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:f5f477c9dd187b13286cbe262acc00dda864a3a850474c60e9ddf2ef1bbd4750","observation_id":"73f7d67e-345d-408a-82b6-980c617dc822","resolution":{"observed_at":"2026-08-14T13:02:33.830697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02625","last_updated":"2019-04-23T02:27:31Z","snapshot_observed_at":"2026-08-14T16:51:39.784858Z","submitted_at":"2019-04-04T15:55:22Z","title":"$\\Lambda$CDM or self-interacting neutrinos? - how CMB data can tell the two models apart","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02625","snapshot_observed_at":"2026-08-14T13:02:33.835168Z","title":"ΛCDM or self-interacting neutri- nos? - how CMB data can tell the two models apart,","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.835168Z"},"links":{"cited_paper":"/paper/1904.02625","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:d9dea2a503b328ddcd833a35053ce2eeff8e024c3ef5fe3c10be8a38980a57e5","observation_id":"ff13851a-a376-494d-86a8-9311426fcc4e","resolution":{"observed_at":"2026-08-14T13:02:33.835168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01016","last_updated":"2023-10-07T21:58:58Z","snapshot_observed_at":"2026-08-14T16:53:29.165074Z","submitted_at":"2019-04-01T18:00:00Z","title":"Rock 'n' Roll Solutions to the Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01016","snapshot_observed_at":"2026-08-14T13:02:33.839305Z","title":"Rock ’n’ Roll Solutions to the Hubble Tension,","venue":null,"work_id":null,"year":1904},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.839305Z"},"links":{"cited_paper":"/paper/1904.01016","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:781f4865d6027e3a954424fbb4a9a251911cdeaae5f4ac1ab306a7f676183481","observation_id":"c40cd67a-7889-472a-b454-3935430b5a05","resolution":{"observed_at":"2026-08-14T13:02:33.839305Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12618","last_updated":"2019-10-30T01:54:52Z","snapshot_observed_at":"2026-08-14T16:24:16.637427Z","submitted_at":"2019-05-29T17:59:01Z","title":"Acoustic Dark Energy: Potential Conversion of the Hubble Tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12618","snapshot_observed_at":"2026-08-14T13:02:33.842958Z","title":"Acous- tic Dark Energy: Potential Conversion of the Hubble Tension,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.842958Z"},"links":{"cited_paper":"/paper/1905.12618","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:fe4d59e7257e3eba409ee4a766b48936db8967cce01efd78ce661d00b2e1d493","observation_id":"d19851ea-6d32-4819-9aef-d9028044b6d4","resolution":{"observed_at":"2026-08-14T13:02:33.842958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1606.00634","last_updated":"2016-09-01T13:28:22Z","snapshot_observed_at":"2026-08-14T21:54:32.269412Z","submitted_at":"2016-06-02T11:44:54Z","title":"Reconciling Planck with the local value of $H_0$ in extended parameter space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1606.00634","snapshot_observed_at":"2026-08-14T13:02:33.846944Z","title":"Reconciling Planck with the local value of H0 in extended parameter space,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.846944Z"},"links":{"cited_paper":"/paper/1606.00634","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:23f822d78b8daa910bc8d007135557c9c52bc7a7b951fe598e58f6892c967707","observation_id":"86dfe383-b1e4-4591-9d49-edd77ffa6492","resolution":{"observed_at":"2026-08-14T13:02:33.846944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.00762","last_updated":"2017-04-03T18:55:55Z","snapshot_observed_at":"2026-08-14T21:08:30.643294Z","submitted_at":"2017-04-03T18:55:55Z","title":"Constraining Dark Energy Dynamics in Extended Parameter Space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.00762","snapshot_observed_at":"2026-08-14T13:02:33.851267Z","title":"Constraining Dark Energy Dynamics in Extended Pa- rameter Space,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.851267Z"},"links":{"cited_paper":"/paper/1704.00762","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:4418d8c2f6f5aab5dfc94633283b4502a97da1a7bc283d7a38ecd6a03790b0a7","observation_id":"2db33997-3a08-4d6d-a62b-03b64aab4f81","resolution":{"observed_at":"2026-08-14T13:02:33.851267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.02153","last_updated":"2017-10-05T18:00:07Z","snapshot_observed_at":"2026-08-14T20:26:27.553476Z","submitted_at":"2017-10-05T18:00:07Z","title":"A Vacuum Phase Transition Solves $H_0$ Tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.02153","snapshot_observed_at":"2026-08-14T13:02:33.855970Z","title":"Vac- uum phase transition solves the H0 tension,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.855970Z"},"links":{"cited_paper":"/paper/1710.02153","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:838f993438a5d0c4bf59c5685e07dce39e7f4752edf76e4b585cd84904f8731d","observation_id":"167b5eeb-4cdb-4942-ba35-4e0e6ee9c2fe","resolution":{"observed_at":"2026-08-14T13:02:33.855970Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.08342","last_updated":"2017-04-26T20:36:07Z","snapshot_observed_at":"2026-08-14T21:04:28.265532Z","submitted_at":"2017-04-26T20:36:07Z","title":"Can interacting dark energy solve the $H_0$ tension?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.08342","snapshot_observed_at":"2026-08-14T13:02:33.860344Z","title":"Can inter- acting dark energy solve the H0 tension?,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.860344Z"},"links":{"cited_paper":"/paper/1704.08342","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:e8558579cc9981ad6d7119f65e0a5de0d653dd85a6f0f0091b957789dc465272","observation_id":"f43fa766-62a1-4175-91cf-330172bb7249","resolution":{"observed_at":"2026-08-14T13:02:33.860344Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10636","last_updated":"2019-10-21T19:29:34Z","snapshot_observed_at":"2026-08-14T17:45:41.642071Z","submitted_at":"2019-02-27T17:01:54Z","title":"Alleviating the $H_0$ and $\\sigma_8$ anomalies with a decaying dark matter model","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10636","snapshot_observed_at":"2026-08-14T13:02:33.864643Z","title":"Alleviating theH0 and σ8 anomalies with a decaying dark matter model,","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.864643Z"},"links":{"cited_paper":"/paper/1902.10636","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:a6f86adecbc8f527fdf6cb5bdcdfbecc04843913146c9eeefbd4a3b24d9cabe3","observation_id":"cd8970fa-2332-40c7-b207-a01cd49b5689","resolution":{"observed_at":"2026-08-14T13:02:33.864643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.06220","last_updated":"2019-03-21T18:55:03Z","snapshot_observed_at":"2026-08-14T17:43:43.057290Z","submitted_at":"2019-03-14T18:57:42Z","title":"Late universe decaying dark matter can relieve the H_0 tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.06220","snapshot_observed_at":"2026-08-14T13:02:33.868295Z","title":"Late uni- verse decaying dark matter can relieve the H0 tension,","venue":null,"work_id":null,"year":1903},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.868295Z"},"links":{"cited_paper":"/paper/1903.06220","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:ebefb932dfac5611c412b7c55b0cfb3e835d0714d432d81eca77879e28e645aa","observation_id":"ce942209-7361-4f6e-b36a-6613ac1ef76c","resolution":{"observed_at":"2026-08-14T13:02:33.868295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1707.06547","last_updated":"2018-01-31T16:29:48Z","snapshot_observed_at":"2026-08-14T20:46:22.150286Z","submitted_at":"2017-07-20T14:33:32Z","title":"Elucidating $\\Lambda$CDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.06547","snapshot_observed_at":"2026-08-14T13:02:33.872824Z","title":"Elucidating ΛCDM: Im- pact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.872824Z"},"links":{"cited_paper":"/paper/1707.06547","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:4f466009fb400a333d45f081cac2bb9c940c04ce205dc1fcf23a9a3d00641d39","observation_id":"e44372ba-9494-4505-992f-62a2ffa2ca19","resolution":{"observed_at":"2026-08-14T13:02:33.872824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.3366","last_updated":"2011-06-16T22:41:18Z","snapshot_observed_at":"2026-07-06T02:29:26.831866Z","submitted_at":"2011-06-16T22:41:18Z","title":"The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.3366","snapshot_observed_at":"2026-08-14T13:02:33.878898Z","title":"The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Con- stant,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.878898Z"},"links":{"cited_paper":"/paper/1106.3366","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:5cd00b78f73f1fd35df230485c86df044aa06a31502b01d77f96424663029800","observation_id":"6d9a1b9b-c9b3-479a-a58e-3247f98ea03b","resolution":{"observed_at":"2026-08-14T13:02:33.878898Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3242","last_updated":"2015-01-21T19:36:11Z","snapshot_observed_at":"2026-08-14T23:19:56.921026Z","submitted_at":"2014-09-10T20:02:29Z","title":"The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1409.3242","snapshot_observed_at":"2026-08-14T13:02:33.885109Z","title":"The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance mea- 6 sure at z = 0.15,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.885109Z"},"links":{"cited_paper":"/paper/1409.3242","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:3a41432234c2098f9774ffcd9b75c45cf1905ced1ae2107fccd78846e74754a5","observation_id":"a4f94f55-d89d-48f3-bc17-313ec93a12e7","resolution":{"observed_at":"2026-08-14T13:02:33.885109Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03155","last_updated":"2016-07-11T20:29:52Z","snapshot_observed_at":"2026-08-14T21:48:51.809084Z","submitted_at":"2016-07-11T20:29:52Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03155","snapshot_observed_at":"2026-08-14T13:02:33.889529Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.889529Z"},"links":{"cited_paper":"/paper/1607.03155","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:57dc736c5a61fa75ab6b63989459350b54c03ded3adc37a6db9d6cdd3b22702d","observation_id":"ce5611b6-0819-4ecc-a51c-4caa4b757f4d","resolution":{"observed_at":"2026-08-14T13:02:33.889529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.08165","last_updated":"2017-07-13T13:51:22Z","snapshot_observed_at":"2026-08-14T21:19:09.402047Z","submitted_at":"2017-01-27T19:00:03Z","title":"Dynamical dark energy in light of the latest observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.08165","snapshot_observed_at":"2026-08-14T13:02:33.894367Z","title":"Dynamical dark energy in light of the latest observations,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.894367Z"},"links":{"cited_paper":"/paper/1701.08165","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:a4c46d04f3d65ee657b1b234deec601c8eb79a12bc8d8bba18826c8251c6bceb","observation_id":"ef17fa3f-a345-4d36-a126-d35faa134d32","resolution":{"observed_at":"2026-08-14T13:02:33.894367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.02474","last_updated":"2018-09-02T20:45:21Z","snapshot_observed_at":"2026-08-14T19:38:47.042676Z","submitted_at":"2018-03-06T23:42:17Z","title":"The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.02474","snapshot_observed_at":"2026-08-14T13:02:33.898573Z","title":"Implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.898573Z"},"links":{"cited_paper":"/paper/1803.02474","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:2a878d0009f039edcb7b0573039c7d6f88c5e19860e20789b9e25fb21003c8ed","observation_id":"2f6231ae-0095-407d-af3e-a93e998ebc00","resolution":{"observed_at":"2026-08-14T13:02:33.898573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9611125","last_updated":"1996-11-15T18:24:05Z","snapshot_observed_at":"2026-07-07T01:15:03.940917Z","submitted_at":"1996-11-15T18:24:05Z","title":"Statistics of Cosmic Microwave Background Polarization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9611125","snapshot_observed_at":"2026-08-14T13:02:33.903407Z","title":"Statistics of cosmic microwave background polariza- tion,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.903407Z"},"links":{"cited_paper":"/paper/astro-ph/9611125","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:89073edc5ce2bf0cd50e1cf5433c0d7093799f3345836ed7d6329f1d13e71f1d","observation_id":"6298e8ff-8e9c-42c1-a95a-d0653d7c355b","resolution":{"observed_at":"2026-08-14T13:02:33.903407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9609170","last_updated":"1997-03-02T17:59:12Z","snapshot_observed_at":"2026-07-07T01:14:30.808201Z","submitted_at":"1996-09-25T15:36:04Z","title":"An All-Sky Analysis of Polarization in the Microwave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9609170","snapshot_observed_at":"2026-08-14T13:02:33.908187Z","title":"An all sky analysis of polarization in the microwave background,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.908187Z"},"links":{"cited_paper":"/paper/astro-ph/9609170","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:e61c0a80715538a222598cc2e8f5f79459812775daa6c4573fe1b58ca403e7d4","observation_id":"dce77b1c-f59f-4900-a3ff-7cafe46103f1","resolution":{"observed_at":"2026-08-14T13:02:33.908187Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9609132","last_updated":"1996-09-19T11:50:52Z","snapshot_observed_at":"2026-07-07T01:14:30.808201Z","submitted_at":"1996-09-19T11:50:52Z","title":"A Probe of Primordial Gravity Waves and Vorticity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9609132","snapshot_observed_at":"2026-08-14T13:02:33.913141Z","title":"A Probe of primordial gravity waves and vorticity,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.913141Z"},"links":{"cited_paper":"/paper/astro-ph/9609132","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:4cd647243b853f0ca1f625514c5d161d4ddbf98b9ca1987837584361a7e9966f","observation_id":"634549e6-73b0-4d8a-9f4f-629e5c94ad02","resolution":{"observed_at":"2026-08-14T13:02:33.913141Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9609169","last_updated":"1997-03-02T17:58:44Z","snapshot_observed_at":"2026-07-07T01:14:30.808201Z","submitted_at":"1996-09-25T03:20:46Z","title":"Signature of Gravity Waves in Polarization of the Microwave Background","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9609169","snapshot_observed_at":"2026-08-14T13:02:33.917366Z","title":"Signature of gravity waves in polarization of the microwave background,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.917366Z"},"links":{"cited_paper":"/paper/astro-ph/9609169","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:425f605cfeeef0541847d80399c13477c8f522aaee1dba0f45fe42cce996d4f5","observation_id":"516673d3-6b2b-4dff-8334-79d28eed831a","resolution":{"observed_at":"2026-08-14T13:02:33.917366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.06042","last_updated":"2015-10-20T20:12:45Z","snapshot_observed_at":"2026-08-14T22:27:00.800382Z","submitted_at":"2015-10-20T20:12:45Z","title":"The Quest for B Modes from Inflationary Gravitational Waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.06042","snapshot_observed_at":"2026-08-14T13:02:33.922922Z","title":"The Quest for B Modes from Inﬂationary Gravitational Waves,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.922922Z"},"links":{"cited_paper":"/paper/1510.06042","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:4bb7ba9c0d6cb4ebe2eee1587527bbd172cfce72cbf4022603279d5cd3640c86","observation_id":"76e33d11-f28e-4a56-a480-86cfad12e5c5","resolution":{"observed_at":"2026-08-14T13:02:33.922922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1408.4788","last_updated":"2014-08-20T19:59:40Z","snapshot_observed_at":"2026-08-14T23:22:29.109723Z","submitted_at":"2014-08-20T19:59:40Z","title":"CLASS: The Cosmology Large Angular Scale Surveyor","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1408.4788","snapshot_observed_at":"2026-08-14T13:02:33.926669Z","title":"Essinger-Hileman et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.926669Z"},"links":{"cited_paper":"/paper/1408.4788","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:8807afbe35b4c236d0ad51d6b9b4d31b4355ff813d86a71e612062d61aeaac34","observation_id":"c6d04094-1f5c-4a2b-a86c-f6c1cb08dd57","resolution":{"observed_at":"2026-08-14T13:02:33.926669Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1311.2847","last_updated":"2013-11-12T17:30:22Z","snapshot_observed_at":"2026-08-14T23:55:36.786817Z","submitted_at":"2013-11-12T17:30:22Z","title":"Mission design of LiteBIRD","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1311.2847","snapshot_observed_at":"2026-08-14T13:02:33.930308Z","title":"Mission design of LiteBIRD,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.930308Z"},"links":{"cited_paper":"/paper/1311.2847","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:58e79288ef726060cbdb1bba65f5f68e4a1898a058ca10dfad0df0c472036e15","observation_id":"562480cf-1bd5-435f-a289-ba138b1645c0","resolution":{"observed_at":"2026-08-14T13:02:33.930308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1808.07445","last_updated":"2019-03-01T10:51:03Z","snapshot_observed_at":"2026-08-15T01:11:26.803228Z","submitted_at":"2018-08-22T17:19:17Z","title":"The Simons Observatory: Science goals and forecasts","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1808.07445","snapshot_observed_at":"2026-08-14T13:02:33.934076Z","title":"The Simons Observatory: Science goals and fore- casts,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.934076Z"},"links":{"cited_paper":"/paper/1808.07445","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:37f519304ed681a3cce9381170ef392c2c27cdee9c5d56b2544db1d9401f98d4","observation_id":"193c0149-f4be-4baf-a32a-f680be4f4812","resolution":{"observed_at":"2026-08-14T13:02:33.934076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.02743","last_updated":"2016-10-10T00:35:39Z","snapshot_observed_at":"2026-08-14T21:36:01.073428Z","submitted_at":"2016-10-10T00:35:39Z","title":"CMB-S4 Science Book, First Edition","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.02743","snapshot_observed_at":"2026-08-14T13:02:33.938144Z","title":"CMB- S4 Science Book, First Edition,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.938144Z"},"links":{"cited_paper":"/paper/1610.02743","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:2035386143dc2a71886a68da065f52bb7972ee721741801e8e12579a58e5077e","observation_id":"3aa2879e-743b-4f01-b418-faf1d9171ef9","resolution":{"observed_at":"2026-08-14T13:02:33.938144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.10541","last_updated":"2019-03-05T16:34:33Z","snapshot_observed_at":"2026-08-14T17:10:51.309790Z","submitted_at":"2019-02-26T18:25:42Z","title":"PICO: Probe of Inflation and Cosmic Origins","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.10541","snapshot_observed_at":"2026-08-14T13:02:33.942339Z","title":"PICO: Probe of Inﬂation and Cosmic Origins,","venue":null,"work_id":null,"year":1902},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.942339Z"},"links":{"cited_paper":"/paper/1902.10541","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:764b664350aa563ea8b58b4c6a0226583751f7d106bde30f59ee98bf7a2441ec","observation_id":"638e102a-d438-4412-868d-2de7e97d8dea","resolution":{"observed_at":"2026-08-14T13:02:33.942339Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9803150","last_updated":"1998-03-13T02:48:14Z","snapshot_observed_at":"2026-07-07T01:20:15.654204Z","submitted_at":"1998-03-13T02:48:14Z","title":"Gravitational Lensing Effect on Cosmic Microwave Background Polarization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9803150","snapshot_observed_at":"2026-08-14T13:02:33.946652Z","title":"Gravitational lensing eﬀect on cosmic microwave background polarization,","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.946652Z"},"links":{"cited_paper":"/paper/astro-ph/9803150","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:9c0f4a8a7f901574c89c6074f2c2a2a67a84de2607c821fec8a86cfb6167133c","observation_id":"50a2db7c-aa8f-4f9e-9199-99bea2df5daa","resolution":{"observed_at":"2026-08-14T13:02:33.946652Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0412581","last_updated":"2004-12-21T23:05:11Z","snapshot_observed_at":"2026-08-11T15:00:52.855507Z","submitted_at":"2004-12-21T23:05:11Z","title":"Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0412581","snapshot_observed_at":"2026-08-14T13:02:33.952422Z","title":"Cosmic mi- crowave background ﬂuctuations from gravitational waves: An Analytic approach,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.952422Z"},"links":{"cited_paper":"/paper/astro-ph/0412581","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:04305ae1f550936e6a358c6720d4ec544e4107e0d1eafb37ff5913e7da83f154","observation_id":"07b33a29-b831-45d9-abad-e93d1be4d951","resolution":{"observed_at":"2026-08-14T13:02:33.952422Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703179","last_updated":"2007-05-11T07:22:13Z","snapshot_observed_at":"2026-08-05T18:35:36.188137Z","submitted_at":"2007-03-08T20:47:19Z","title":"Tensor Microwave Background Fluctuations for Large Multipole Order","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703179","snapshot_observed_at":"2026-08-14T13:02:33.956714Z","title":"Tensor Microwave Back- ground Fluctuations for Large Multipole Order,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.956714Z"},"links":{"cited_paper":"/paper/astro-ph/0703179","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:899e0b8160a9ab8d79565d3cbd107fec2441f13c1c4ccd44aac79077451d16f7","observation_id":"b821011b-b49a-46f6-a0d6-55461fc3958a","resolution":{"observed_at":"2026-08-14T13:02:33.956714Z","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":"2026-08-14T13:02:35.168040Z","title":"Small scale ﬂuc- tuations of relic radiation,","venue":null,"work_id":"6af8fe40-5b7c-459c-bd4d-3e60305d9c7a","year":1970},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.960146Z"},"links":{"citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:149bc9134321ec1be278c809d04cf935aaa99cb03853f86cc52b6afc7c851f6c","observation_id":"8cb2661a-ca3a-4fa0-8b9b-32af726666b7","resolution":{"observed_at":"2026-08-14T13:02:35.171904Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:02:35.155309Z","title":"Primeval adiabatic per- turbation in an expanding universe,","venue":null,"work_id":"de2b3286-6ddd-4186-8b90-f62739adb9bf","year":1970},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.964127Z"},"links":{"citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:32e955de4b225803ba347eb001b1d351caff02e86852fb00f8bc30eea954e766","observation_id":"72c60755-aaab-4dbf-acea-985d6c154526","resolution":{"observed_at":"2026-08-14T13:02:35.158798Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"ph/9705219","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T13:02:34.351163Z","title":"Detectability of inﬂationary gravitational waves with microwave back- ground polarization,","venue":null,"work_id":"24484a2a-5141-4b7b-831b-fa0ef80e1c44","year":1998},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.967903Z"},"links":{"citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:6c6a5ea6f8f31bdbd70950df61e039ee8cb5c351ae39cf1f863ff02430d97e5c","observation_id":"1ab5302e-3d66-43fd-bb65-dcf72b6c4df5","resolution":{"observed_at":"2026-08-14T13:02:34.356805Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9909281","last_updated":"1999-09-15T23:01:20Z","snapshot_observed_at":"2026-08-14T02:38:12.353418Z","submitted_at":"1999-09-15T23:01:20Z","title":"A Polarization Pursuers' Guide","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9909281","snapshot_observed_at":"2026-08-14T13:02:33.972890Z","title":"Polar- ization pursuers’ guide,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.972890Z"},"links":{"cited_paper":"/paper/astro-ph/9909281","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:a3df76572648c059f1864896a98c60b9f689abb92b39349e214ec998606c5c49","observation_id":"8b23dd46-f68b-48e9-94c1-467b77a59d8b","resolution":{"observed_at":"2026-08-14T13:02:33.972890Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9512139","last_updated":"1996-05-23T17:57:30Z","snapshot_observed_at":"2026-07-07T01:12:30.057746Z","submitted_at":"1995-12-20T22:29:37Z","title":"Cosmological-Parameter Determination with Microwave Background Maps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9512139","snapshot_observed_at":"2026-08-14T13:02:33.977922Z","title":"Cosmological parameter determination with microwave background maps,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.977922Z"},"links":{"cited_paper":"/paper/astro-ph/9512139","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:4eebad5f9de031cd2a53ab38765d6747d82392aa2e0bf1271117acb318d2b6ec","observation_id":"e4e26267-ceda-4fa6-9990-115d7774eee1","resolution":{"observed_at":"2026-08-14T13:02:33.977922Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.00176","last_updated":"2018-05-29T10:03:19Z","snapshot_observed_at":"2026-08-14T19:40:51.614887Z","submitted_at":"2018-03-01T02:41:43Z","title":"Reconstruction of primordial tensor power spectra from B-mode polarization of the cosmic microwave background","version":2},"cited_work":{"arxiv_id":"1803.00176","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.00176","snapshot_observed_at":"2026-08-14T13:02:34.255650Z","title":"Reconstruction of primordial tensor power spectra from B-mode polarization of the cosmic microwave background","venue":"astro-ph.CO","work_id":"75dcca2a-6c8d-4ae9-8dff-24110804baa3","year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.982198Z"},"links":{"cited_paper":"/paper/1803.00176","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:c2c2ef578f920c87b1ece0445880a81887f8eb872b56dfbb52ae4fa5c0dde8f6","observation_id":"9792a597-48f2-43ce-8850-c601ae3c1999","resolution":{"observed_at":"2026-08-14T13:02:34.259908Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202434","last_updated":"2002-05-14T22:55:07Z","snapshot_observed_at":"2026-08-02T10:39:55.492577Z","submitted_at":"2002-02-23T01:41:20Z","title":"Separation of Gravitational-Wave and Cosmic-Shear Contributions to Cosmic Microwave Background Polarization","version":2},"cited_work":{"arxiv_id":"astro-ph/0202434","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0202434","snapshot_observed_at":"2026-08-14T13:02:34.076021Z","title":"Separation of Gravitational-Wave and Cosmic-Shear Contributions to Cosmic Microwave Background Polarization","venue":"astro-ph","work_id":"3ea9fa83-4414-4ebe-8cb6-86b9c8b95674","year":2002},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.986634Z"},"links":{"cited_paper":"/paper/astro-ph/0202434","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:931522c6af917bc20f15b70f4e5e7e5411d740f29f385b3bb29786e8962b5892","observation_id":"db59ffa1-adec-458e-b134-40551fb788d7","resolution":{"observed_at":"2026-08-14T13:02:34.152977Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202286","last_updated":"2002-02-15T19:02:21Z","snapshot_observed_at":"2026-07-07T00:25:03.686623Z","submitted_at":"2002-02-15T19:02:21Z","title":"A limit on the detectability of the energy scale of inflation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0202286","snapshot_observed_at":"2026-08-14T13:02:33.993061Z","title":"A Limit on the detectability of the energy scale of inﬂation,","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.993061Z"},"links":{"cited_paper":"/paper/astro-ph/0202286","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:c7d0d3b956e675f54c0146bb9736f4b3d38c801e84ebb82341f8fda017af4402","observation_id":"fb3af0df-aa06-4356-92d8-2fcf1309b9e2","resolution":{"observed_at":"2026-08-14T13:02:33.993061Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9911177","last_updated":"2000-06-01T12:13:06Z","snapshot_observed_at":"2026-07-07T01:29:40.678750Z","submitted_at":"1999-11-10T17:57:36Z","title":"Efficient Computation of CMB anisotropies in closed FRW models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9911177","snapshot_observed_at":"2026-08-14T13:02:33.997435Z","title":"Eﬃcient com- putation of CMB anisotropies in closed FRW models,","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.997435Z"},"links":{"cited_paper":"/paper/astro-ph/9911177","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:3d7f4bb407b79fcadad7d6d31ea1647c7087cf5db412f0555732847ee26bec3b","observation_id":"d68191e3-483e-4f71-80ca-1c7d55c16a17","resolution":{"observed_at":"2026-08-14T13:02:33.997435Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.11038","last_updated":"2018-02-27T12:57:43Z","snapshot_observed_at":"2026-08-14T20:18:51.633042Z","submitted_at":"2017-10-30T16:11:11Z","title":"Future cosmic microwave background delensing with galaxy surveys","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.11038","snapshot_observed_at":"2026-08-14T13:02:34.002583Z","title":"Future cosmic microwave background de- lensing with galaxy surveys,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:34.002583Z"},"links":{"cited_paper":"/paper/1710.11038","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:bb32c709e849addb37d1bc74c766951ac0dcd6fb0bc30efb258e088670a7fdd5","observation_id":"824b7f67-17cd-4fe1-9763-ee2469d44550","resolution":{"observed_at":"2026-08-14T13:02:34.002583Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T13:11:18.819085Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension"},"reference_resolution":{"displayed":65,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":58,"verified_exact":5,"verified_fuzzy":2},"total_outbound_references":65},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 65 of 65 outbound references and 2 inbound Pith citation observations for arXiv:1908.06100."}