{"as_of":"2026-08-06T19:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:095ac67f584f6a3f2d3e458a48f81d1d84080a3b45723fcafb57cca29859cb7c","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T04:36:15.905132Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T05:19:36.039985Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"reference_index":187,"source":"pdf_text","source_observed_at":"2026-05-15T11:50:20.600831Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2103.01183"},"observation_digest":"sha256:69899f118320e94ef1bc29fad71aa88925a9537166632ca8f5cca301af716e61","observation_id":"33efe2c3-6b09-41de-95a6-586384453b8f","resolution":{"observed_at":"2026-05-15T11:50:21.433289Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2603.26560","last_updated":"2026-05-26T09:42:59Z","snapshot_observed_at":"2026-07-13T17:26:51.495350Z","submitted_at":"2026-03-27T16:25:41Z","title":"Exploring the interplay of late-time dynamical dark energy and new physics before recombination","version":2},"reference_index":148,"source":"pdf_text","source_observed_at":"2026-05-14T23:13:02.830649Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2603.26560"},"observation_digest":"sha256:455e1aa946385d090f1cf0ad8d6216a57bc8bab6623483b131da68e642bfd0ee","observation_id":"73d70cdb-7903-4ad9-a04d-47bae92eb81a","resolution":{"observed_at":"2026-05-14T23:13:14.878356Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2604.12587","last_updated":"2026-04-14T11:10:26Z","snapshot_observed_at":"2026-07-06T23:00:46.620106Z","submitted_at":"2026-04-14T11:10:26Z","title":"Impact of the SNe Ia Magnitude Transition at 20 Mpc on Cosmological Parameter Estimation","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-10T14:37:32.848262Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2604.12587"},"observation_digest":"sha256:5292d6f79dc538161df21463a2e6f85fcffb2d6b19c69e95454e598bb4b7abb7","observation_id":"8c0aea13-b8af-4459-a755-0217b1e790f1","resolution":{"observed_at":"2026-05-10T14:40:32.891482Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2604.28013","last_updated":"2026-04-30T15:31:57Z","snapshot_observed_at":"2026-07-06T23:13:20.516759Z","submitted_at":"2026-04-30T15:31:57Z","title":"Cosmological intercept tension","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-07T05:59:51.789689Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2604.28013"},"observation_digest":"sha256:936cd5a99d566a6152e35cd4c7b736a3d59ebfd1b0d61e5d518a5b3fbdb4e369","observation_id":"5bc01e29-d16d-42ea-9530-80c76d674df8","resolution":{"observed_at":"2026-05-12T10:26:30.988101Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2605.20748","last_updated":"2026-05-20T05:49:49Z","snapshot_observed_at":"2026-08-03T02:21:57.786789Z","submitted_at":"2026-05-20T05:49:49Z","title":"Probing late-time deviations from $\\Lambda$CDM with a quadratic dark energy expansion","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-21T02:43:57.001089Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2605.20748"},"observation_digest":"sha256:b7a7b0c3380256bf590d49705e240c27965980fc881effe40494882b43b6f1c0","observation_id":"497bfa87-82ce-436d-88de-6594f7a1f39b","resolution":{"observed_at":"2026-05-21T02:44:25.335053Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2606.12822","last_updated":"2026-06-11T02:35:35Z","snapshot_observed_at":"2026-07-06T23:51:40.528967Z","submitted_at":"2026-06-11T02:35:35Z","title":"Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-27T06:23:50.957273Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2606.12822"},"observation_digest":"sha256:b417b65200ba7f982dfd8f176ca242cec7ce73ab08a9970e14ca8a930a7ceb97","observation_id":"affdd0cd-6b9c-4c00-9a25-b34a7dfac872","resolution":{"observed_at":"2026-07-03T15:38:33.902530Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:2a1b3d4b3e43168d9ac478517270606bf11fcd044eca6b904e781f572b86fdd9","observation_id":"06bf75e6-b54b-42b0-936c-5536c7fc7e01","resolution":{"observed_at":"2026-07-04T05:19:36.042322Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Benevento, W","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:a792ee235378cb76b6530b64e1e41fe3e5ccc77af93d70be057b5e2c1d9b7a81","observation_id":"56e276d3-80a0-41fd-abf3-cd37309be2f9","resolution":{"observed_at":"2026-07-15T10:41:50.733215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":"2002.11707","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-07-04T05:19:36.039985Z","title":"Benevento, W","venue":null,"work_id":"f0f4c2bc-74e9-4806-866c-8a9c36d0ef1f","year":2020},"citing_paper":{"arxiv_id":"2606.31362","last_updated":"2026-06-30T08:57:18Z","snapshot_observed_at":"2026-07-07T00:05:02.977105Z","submitted_at":"2026-06-30T08:57:18Z","title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","version":1},"reference_index":263,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:e6ab27086706d6a25f3df36af01b3e82e249ccd7260b2c267e6e660ade7c9b1e","observation_id":"5dc2a70e-22fd-417e-978f-aa2ac153bb85","resolution":{"observed_at":"2026-07-01T11:25:45.145003Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-08-01T07:20:08.202560Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-07-23T16:45:10Z","snapshot_observed_at":"2026-08-03T22:55:05.115829Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":220,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:08.202560Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:97f3599efec4dcff2490d34a5233b6e33870e04af6b9e25b880b782c03f0a5a5","observation_id":"ff8c245a-6ec8-4d6d-a629-8a3ea45f088a","resolution":{"observed_at":"2026-08-01T07:20:08.202560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.11707","snapshot_observed_at":"2026-08-03T04:36:15.905132Z","title":", keywords =","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2607.29562","last_updated":"2026-07-31T15:52:41Z","snapshot_observed_at":"2026-08-06T12:51:31.367817Z","submitted_at":"2026-07-31T15:52:41Z","title":"Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-03T04:36:15.905132Z"},"links":{"cited_paper":"/paper/2002.11707","citing_paper":"/paper/2607.29562"},"observation_digest":"sha256:f6e05dc02c7aa17700989da4c3ea32989beef9e7e7257f1b587454ac3ad8a33e","observation_id":"6c3ae35c-7619-4975-953f-224bbf501918","resolution":{"observed_at":"2026-08-03T04:36:15.905132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2002.11707/citation-record","integrity":"/paper/2002.11707/integrity","json":"/paper/2002.11707/citation-record.json","paper":"/paper/2002.11707"},"outbound":[],"paper":{"arxiv_id":"2002.11707","last_updated":"2020-05-22T08:09:01Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-06T17:08:12.466325Z","submitted_at":"2020-02-26T18:56:38Z","title":"Can Late Dark Energy Transitions Raise the Hubble constant?"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2002.11707."}