{"as_of":"2026-08-20T20:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3e24a97bb0a8cb1a3d97cf7cb4b5a8c8ccab59bf254d16924359c7b94841531c","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T18:51:42.560410Z","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":"2026-07-01T16:45:51.209108Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":"1105.0419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-07-01T16:45:51.209108Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","venue":"astro-ph.CO","work_id":"255b5599-53a5-4b5e-af26-ed5d4282ad8f","year":2011},"citing_paper":{"arxiv_id":"2304.05202","last_updated":"2025-12-22T05:26:10Z","snapshot_observed_at":"2026-08-14T20:36:34.318271Z","submitted_at":"2023-04-11T13:13:13Z","title":"The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth","version":3},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2304.05202"},"observation_digest":"sha256:fec20035ec48145dede1991cfcc776e9529d2d82cbdd71e1b9fb4f0e53994646","observation_id":"35fe2aef-ab4e-47c1-b801-7669f3d9be69","resolution":{"observed_at":"2026-05-21T13:38:51.412386Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-08-07T18:51:42.560410Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.10264","last_updated":"2025-04-10T17:38:46Z","snapshot_observed_at":"2026-08-19T21:36:29.298768Z","submitted_at":"2025-02-14T16:17:23Z","title":"An overview of what current data can (and cannot yet) say about evolving dark energy","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T18:51:42.560410Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2502.10264"},"observation_digest":"sha256:79a7f0aa0bd88eb2a76bdfd8c74e35f4ec21bed8d6dde17283f080b514027f60","observation_id":"ae098055-0f6b-47d4-ac47-7dcebd9083ff","resolution":{"observed_at":"2026-08-07T18:51:42.560410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-08-07T00:54:40.327624Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.12709","last_updated":"2025-07-01T13:57:37Z","snapshot_observed_at":"2026-08-10T02:08:50.780247Z","submitted_at":"2025-06-15T03:43:47Z","title":"Constraints on Dark Energy Models Using Late Universe Probes","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T00:54:40.327624Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2506.12709"},"observation_digest":"sha256:2fa72c0508f406912b4b1f1039fa76eba3ce46194703dd4c662af3b201de8e69","observation_id":"8e893b48-5e92-4118-9b15-74d916d96e49","resolution":{"observed_at":"2026-08-07T00:54:40.327624Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":"1105.0419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-07-01T16:45:51.209108Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","venue":"astro-ph.CO","work_id":"255b5599-53a5-4b5e-af26-ed5d4282ad8f","year":2011},"citing_paper":{"arxiv_id":"2507.05207","last_updated":"2026-04-10T05:44:06Z","snapshot_observed_at":"2026-08-03T03:36:09.305498Z","submitted_at":"2025-07-07T17:16:40Z","title":"Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-19T05:52:58.864730Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2507.05207"},"observation_digest":"sha256:02b7ae66da1ab1f1b0addaea296d197859bee9da8e0dbc292a06928b06519174","observation_id":"0018ac5a-e143-4d49-9e26-d107c009515c","resolution":{"observed_at":"2026-05-19T05:57:08.488140Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":"1105.0419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-07-01T16:45:51.209108Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","venue":"astro-ph.CO","work_id":"255b5599-53a5-4b5e-af26-ed5d4282ad8f","year":2011},"citing_paper":{"arxiv_id":"2509.09202","last_updated":"2026-04-12T17:53:51Z","snapshot_observed_at":"2026-08-16T20:14:42.800239Z","submitted_at":"2025-09-11T07:18:09Z","title":"Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-18T18:14:18.793821Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2509.09202"},"observation_digest":"sha256:f922ab882c45e47e8b3c6aea7cb415d87b38c469a62bf99ec93d64c762009398","observation_id":"2991a878-50bc-48a3-a3fc-cda3ed644011","resolution":{"observed_at":"2026-05-18T18:16:43.209612Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":"1105.0419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-07-01T16:45:51.209108Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","venue":"astro-ph.CO","work_id":"255b5599-53a5-4b5e-af26-ed5d4282ad8f","year":2011},"citing_paper":{"arxiv_id":"2605.18659","last_updated":"2026-05-18T17:05:30Z","snapshot_observed_at":"2026-07-06T23:29:29.105126Z","submitted_at":"2026-05-18T17:05:30Z","title":"Faster CMB lensing with control variates","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-20T09:06:47.937607Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2605.18659"},"observation_digest":"sha256:47f3b6c79a2080eca043db21cff8e628a73546d40a21df4cf42b1eb94f0e5c82","observation_id":"c7ecab76-2b3e-4dc6-83fe-fa182452f867","resolution":{"observed_at":"2026-05-20T09:08:09.641901Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":"1105.0419","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-07-01T16:45:51.209108Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","venue":"astro-ph.CO","work_id":"255b5599-53a5-4b5e-af26-ed5d4282ad8f","year":2011},"citing_paper":{"arxiv_id":"2605.26116","last_updated":"2026-05-25T17:59:53Z","snapshot_observed_at":"2026-07-06T23:36:01.564747Z","submitted_at":"2026-05-25T17:59:53Z","title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:c227580dfc178cf471b6a9eafafd49b01717f2ec5256150b9f7a1a758a2284f7","observation_id":"8fe801c9-99b8-4786-9f9f-9911a0c70d87","resolution":{"observed_at":"2026-07-01T16:45:51.210384Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.0419","snapshot_observed_at":"2026-08-02T06:19:43.440161Z","title":"Sherwin et al.,Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements,Phys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.13128","last_updated":"2026-07-14T18:00:00Z","snapshot_observed_at":"2026-08-19T03:39:22.194375Z","submitted_at":"2026-07-14T18:00:00Z","title":"Dark Energy and Neutrino Flavor from the Weak Axion","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-02T06:19:43.440161Z"},"links":{"cited_paper":"/paper/1105.0419","citing_paper":"/paper/2607.13128"},"observation_digest":"sha256:9d21ccf5e692e0ceae7c10f9cccdf563c892eb48e90f082d1c302dbf203f1f85","observation_id":"ce9ae834-3edb-4e04-afe2-1d3d93c7f9f7","resolution":{"observed_at":"2026-08-02T06:19:43.440161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1105.0419/citation-record","integrity":"/paper/1105.0419/integrity","json":"/paper/1105.0419/citation-record.json","paper":"/paper/1105.0419"},"outbound":[],"paper":{"arxiv_id":"1105.0419","last_updated":"2011-08-01T19:35:04Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T20:14:37.445264Z","submitted_at":"2011-05-02T19:52:29Z","title":"Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1105.0419."}