{"as_of":"2026-08-07T19:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f822f66d62652c98855936c4ea8d4feb02956db8e147fadc67b6691623b8726c","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T22:34:14.051012Z","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":"2026-05-24T01:45:55.429947Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2111.11526","last_updated":"2021-11-22T20:50:01Z","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys","version":1},"cited_work":{"arxiv_id":"2111.11526","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2111.11526","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cayuso, R","venue":null,"work_id":"5d74fc9f-e03d-46f4-8492-043ec6db2b5d","year":2023},"citing_paper":{"arxiv_id":"2405.00809","last_updated":"2026-05-08T03:41:52Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-05-01T18:47:04Z","title":"Kinetic Sunyaev Zel'dovich velocity reconstruction from Planck and unWISE","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-24T01:45:11.697720Z"},"links":{"cited_paper":"/paper/2111.11526","citing_paper":"/paper/2405.00809"},"observation_digest":"sha256:66a81990428ed8da4cad0efd83c0fd1970130975fda0654303df9393729cf6fe","observation_id":"5be168b4-4f35-47df-9296-06e31956c5ca","resolution":{"observed_at":"2026-05-24T01:45:55.432923Z","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":"2111.11526","last_updated":"2021-11-22T20:50:01Z","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.11526","snapshot_observed_at":"2026-08-06T22:34:14.051012Z","title":"Cayuso, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.21657","last_updated":"2025-06-26T18:00:00Z","snapshot_observed_at":"2026-08-07T07:03:02.125895Z","submitted_at":"2025-06-26T18:00:00Z","title":"Velocity Reconstruction from KSZ: Measuring $f_{NL}$ with ACT and DESILS","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T22:34:14.051012Z"},"links":{"cited_paper":"/paper/2111.11526","citing_paper":"/paper/2506.21657"},"observation_digest":"sha256:2caddf607d2fe3b839740f8582dbe4d413f97d1f437735d670897113f7611f5b","observation_id":"67e7f2e7-99d8-41e0-89f2-aa6279b490ff","resolution":{"observed_at":"2026-08-06T22:34:14.051012Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.11526","last_updated":"2021-11-22T20:50:01Z","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.11526","snapshot_observed_at":"2026-08-06T18:51:35.151092Z","title":"C., Johnson, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2507.07346","last_updated":"2025-07-25T13:32:05Z","snapshot_observed_at":"2026-08-06T18:41:02.083986Z","submitted_at":"2025-07-10T00:19:11Z","title":"CLASS_SZ II: Notes and Examples of Fast and Accurate Calculations of Halo Model, Large Scale Structure and Cosmic Microwave Background Observables","version":3},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-06T18:51:35.151092Z"},"links":{"cited_paper":"/paper/2111.11526","citing_paper":"/paper/2507.07346"},"observation_digest":"sha256:60736a75ab981fe7bca660956014c7e89db09c32f82f1ec774d493ee372fa890","observation_id":"2cff55b8-ad72-4613-9a11-8f4762e041fc","resolution":{"observed_at":"2026-08-06T18:51:35.151092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.11526","last_updated":"2021-11-22T20:50:01Z","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys","version":1},"cited_work":{"arxiv_id":"2111.11526","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2111.11526","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cayuso, R","venue":null,"work_id":"5d74fc9f-e03d-46f4-8492-043ec6db2b5d","year":2023},"citing_paper":{"arxiv_id":"2511.05653","last_updated":"2026-05-14T20:34:31Z","snapshot_observed_at":"2026-08-03T18:34:12.779343Z","submitted_at":"2025-11-07T19:00:02Z","title":"Probing Dark Energy Microphysics with kSZ Tomography","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-21T19:32:05.723072Z"},"links":{"cited_paper":"/paper/2111.11526","citing_paper":"/paper/2511.05653"},"observation_digest":"sha256:22b520f6866e1c94e3100df8822319fa7954ed9908294d64fb556d5a0d0b64e4","observation_id":"f9443eb6-4b30-4bd7-b03d-c11eb8a514f4","resolution":{"observed_at":"2026-05-21T19:34:20.386196Z","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":"2111.11526","last_updated":"2021-11-22T20:50:01Z","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys","version":1},"cited_work":{"arxiv_id":"2111.11526","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2111.11526","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cayuso, R","venue":null,"work_id":"5d74fc9f-e03d-46f4-8492-043ec6db2b5d","year":2023},"citing_paper":{"arxiv_id":"2604.04867","last_updated":"2026-04-06T17:16:00Z","snapshot_observed_at":"2026-08-05T17:24:18.281615Z","submitted_at":"2026-04-06T17:16:00Z","title":"Measurement of the galaxy-velocity power spectrum of DESI tracers with the kinematic Sunyaev-Zeldovich effect using DESI DR2 and ACT DR6","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-10T19:39:45.988015Z"},"links":{"cited_paper":"/paper/2111.11526","citing_paper":"/paper/2604.04867"},"observation_digest":"sha256:5c688ff82baf0329a56ef57dcc812a4e38bdadbe5fa2afd9cf12f2187e04d709","observation_id":"c0a3e512-53eb-488b-8ba4-a0a9e52f3480","resolution":{"observed_at":"2026-05-10T22:40:49.769433Z","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":"2111.11526","last_updated":"2021-11-22T20:50:01Z","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.11526","snapshot_observed_at":"2026-08-01T21:31:43.299171Z","title":"Cayuso, R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.16071","last_updated":"2026-07-17T15:54:33Z","snapshot_observed_at":"2026-08-04T10:08:52.485016Z","submitted_at":"2026-07-17T15:54:33Z","title":"Constraints on the remote quadrupole field from the polarized Sunyaev Zel'dovich effect","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-01T21:31:43.299171Z"},"links":{"cited_paper":"/paper/2111.11526","citing_paper":"/paper/2607.16071"},"observation_digest":"sha256:37a00968c95b82191755fe5e94c8fafd7f97a556e3425ec372c1c5fc007f9468","observation_id":"a39d8b49-16de-4d76-b288-90fb5a5d905d","resolution":{"observed_at":"2026-08-01T21:31:43.299171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2111.11526/citation-record","integrity":"/paper/2111.11526/integrity","json":"/paper/2111.11526/citation-record.json","paper":"/paper/2111.11526"},"outbound":[],"paper":{"arxiv_id":"2111.11526","last_updated":"2021-11-22T20:50:01Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T12:11:05.526931Z","submitted_at":"2021-11-22T20:50:01Z","title":"Velocity reconstruction with the cosmic microwave background and galaxy surveys"},"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 6 inbound Pith citation observations for arXiv:2111.11526."}