{"as_of":"2026-08-07T15:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f1294bd90f6c077ded5f9a5b38c2e43a3788a2cbb87e48051b5b2483db43290d","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T00:50:26.634012Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-04T05:19:36.284309Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"citing_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},"reference_index":213,"source":"arxiv_source","source_observed_at":"2026-05-10T14:40:47.851452Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/1807.06209"},"observation_digest":"sha256:3a6d5e4ebf77bde0843a5b130d8374d83450d84e18fc732fe6cd5b44ed2e686f","observation_id":"b301b261-8255-4eac-8867-c87573a6d568","resolution":{"observed_at":"2026-05-10T14:45:45.247668Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-08-07T00:50:26.634012Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.13288","last_updated":"2025-06-16T09:30:34Z","snapshot_observed_at":"2026-08-07T00:34:06.683776Z","submitted_at":"2025-06-16T09:30:34Z","title":"Decay of dark energy into dark matter in a metric $f(R)$ gravity: effective running Hubble constant","version":1},"reference_index":2019,"source":"pdf_text","source_observed_at":"2026-08-07T00:50:26.634012Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2506.13288"},"observation_digest":"sha256:a2c772fac21c56111ddb548f13c290e7d3bf621d0c2cdee6f9a08e274e90a370","observation_id":"842c4b5f-397e-4b12-a13f-b23ad45d9954","resolution":{"observed_at":"2026-08-07T00:50:26.634012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-08-04T12:53:42.042493Z","title":"Lemos, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.01974","last_updated":"2026-01-19T10:15:04Z","snapshot_observed_at":"2026-08-04T12:53:22.243014Z","submitted_at":"2025-10-02T12:47:51Z","title":"BAO miscalibration cannot rescue late-time solutions to the Hubble tension","version":2},"reference_index":114,"source":"pdf_text","source_observed_at":"2026-08-04T12:53:42.042493Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2510.01974"},"observation_digest":"sha256:99c4ce66a7509577f0c17a964eefa30bfd5e4a2866ce1f4df3fe434512dcd855","observation_id":"c607a696-3a5b-4e2a-a342-93c0857104b6","resolution":{"observed_at":"2026-08-04T12:53:42.042493Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:fe1c4dba3f7a00c4b7eef46e57e455641a2bfd4d0aa7936d94b0d836606b71ed","observation_id":"9ca43234-45d9-4e2f-bd1e-9fe7e21075fb","resolution":{"observed_at":"2026-05-11T11:41:01.782737Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"citing_paper":{"arxiv_id":"2604.25813","last_updated":"2026-04-28T16:22:13Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-28T16:22:13Z","title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-07T14:55:55.250283Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2604.25813"},"observation_digest":"sha256:a685595ae83c394042cea4eb5318a03639324c2b9ed59d1bc693588da030c83b","observation_id":"8354c15a-5cc3-45e1-93fe-ffb55e218363","resolution":{"observed_at":"2026-05-12T00:36:16.666246Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"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":48,"source":"pdf_text","source_observed_at":"2026-05-07T05:59:51.789689Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2604.28013"},"observation_digest":"sha256:5997f5a2fa6f1c4636f3893c529431782331370c19d8a04fb9b29a0672f3ae01","observation_id":"e90d331c-1b33-47fa-9cdd-fd5d00c575f1","resolution":{"observed_at":"2026-05-12T10:26:30.823989Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"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":83,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:37324713575a0f24a64fb02561024786143518e4fc47ee0f05bacf4d8a9eb568","observation_id":"96229edb-d8b8-4af0-9672-30867cdd1e84","resolution":{"observed_at":"2026-07-04T05:19:36.285783Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Lemos, E","venue":null,"work_id":null,"year":2019},"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":83,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:b1490d50e4a88dbbb007206b57e5e143bfc454a9ce0d0134ba63ffe01ca51aec","observation_id":"51f7b2bb-5dc3-40b0-a966-ca545ac4fe45","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":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"citing_paper":{"arxiv_id":"2606.31324","last_updated":"2026-06-30T08:27:42Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-30T08:27:42Z","title":"Cosmological Viability of Exponential Infrared $f(T)$ Gravity","version":1},"reference_index":231,"source":"pdf_text","source_observed_at":"2026-07-01T04:39:56.556632Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2606.31324"},"observation_digest":"sha256:768b917481c5dcb1d265719974c7b6d3e2bd4cf1f3e43cd12583f6314d1b5763","observation_id":"da5f12e1-9950-4629-8871-d71a003ddab6","resolution":{"observed_at":"2026-07-01T11:15:42.772816Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":"1806.06781","doi":null,"metadata_source":"pith","pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-07-04T05:19:36.284309Z","title":"Lemos, E","venue":"astro-ph.CO","work_id":"622d3fdf-2d36-42c2-86c2-673686677675","year":2018},"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":252,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:81a38d5a8de4169aebf34d2335a84f9ec9f316136f608e992fd1d12677531782","observation_id":"bf7986c0-05fc-41a5-851c-98a414c78748","resolution":{"observed_at":"2026-07-01T11:25:45.139796Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-08-01T11:25:06.305129Z","title":"Lemos, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.19915","last_updated":"2026-07-22T08:45:43Z","snapshot_observed_at":"2026-08-07T04:48:41.686709Z","submitted_at":"2026-07-22T08:45:43Z","title":"QCD CP-violation scenario for a revised cosmological dynamics: analysis of the binned Pantheon Sample of Super Novae Ia","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-01T11:25:06.305129Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2607.19915"},"observation_digest":"sha256:5f2c252967d0b1d4b9234ed16686b118ca31e5034a201fd8a56c2d31be9337a8","observation_id":"bfaf077a-38c4-479e-b014-ec4079408b3f","resolution":{"observed_at":"2026-08-01T11:25:06.305129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-08-01T08:08:53.541724Z","title":"Lemos, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-03T05:59:43.108747Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":195,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:53.541724Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:4e45648b48c427c169a93fc9bc4669727417623f3f641cf95bb53c2c8d230737","observation_id":"6d533520-676e-431b-9729-bab6393dd846","resolution":{"observed_at":"2026-08-01T08:08:53.541724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1806.06781","snapshot_observed_at":"2026-08-03T04:36:18.669134Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.29562","last_updated":"2026-07-31T15:52:41Z","snapshot_observed_at":"2026-08-07T10:30:32.981654Z","submitted_at":"2026-07-31T15:52:41Z","title":"Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-03T04:36:18.669134Z"},"links":{"cited_paper":"/paper/1806.06781","citing_paper":"/paper/2607.29562"},"observation_digest":"sha256:b1542f8eddaf8872db86a546a5b1cb3588ab6a20b26ddb3d1285cd4f271d04f1","observation_id":"4d520092-5730-4e44-96a8-0edd938e49a8","resolution":{"observed_at":"2026-08-03T04:36:18.669134Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1806.06781/citation-record","integrity":"/paper/1806.06781/integrity","json":"/paper/1806.06781/citation-record.json","paper":"/paper/1806.06781"},"outbound":[],"paper":{"arxiv_id":"1806.06781","last_updated":"2018-07-19T15:44:09Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T15:50:55.905442Z","submitted_at":"2018-06-18T15:44:55Z","title":"Model independent $H(z)$ reconstruction using the cosmic inverse distance ladder"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:1806.06781."}