{"as_of":"2026-08-13T12:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:443f48516a1180865b1831d0d0177a5f6ec11bf9a4464ed8ebc0ce8c683c0002","coverage":[{"denominator":51,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":51,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T16:37:56.637483Z","state":"measured"},{"denominator":51,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":51,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2411.13379/citation-record","integrity":"/paper/2411.13379/integrity","json":"/paper/2411.13379/citation-record.json","paper":"/paper/2411.13379"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T16:37:57.869168Z","title":null,"venue":null,"work_id":"73419af0-e59a-408a-8259-7f6fe6dd99d9","year":1998},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.281014Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:0a49bc43456c097756ee264c5e4b2d4804b75d8cd02399b288d1f5823033a8d4","observation_id":"9700e13f-53d6-496b-90dc-b46442282d36","resolution":{"observed_at":"2026-08-12T16:37:57.874943Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.844805Z","title":"Perlmutter, M","venue":null,"work_id":"ab5d5558-b9c7-4c4c-b875-ffc7fd768079","year":1999},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.288175Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:08d55943093580a35cb0c7313048fabb4eb0a664fc0325afb75c7e011ef673aa","observation_id":"49abacdd-09f7-4f74-8308-53e6f3519700","resolution":{"observed_at":"2026-08-12T16:37:57.851731Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1201.2434","last_updated":"2013-03-06T20:33:04Z","snapshot_observed_at":"2026-08-13T04:43:19.108867Z","submitted_at":"2012-01-11T22:12:48Z","title":"Observational Probes of Cosmic Acceleration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.2434","snapshot_observed_at":"2026-08-12T16:37:56.297477Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.297477Z"},"links":{"cited_paper":"/paper/1201.2434","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:51af456c7a63bd45d26489b9921e06d408ec3d29b709437296734808ab81d13c","observation_id":"46282f48-baa0-44b5-860a-055ff14ed1c1","resolution":{"observed_at":"2026-08-12T16:37:56.297477Z","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":"2026-08-12T16:37:57.823497Z","title":null,"venue":null,"work_id":"2ad223ea-9d7b-4735-bd3d-2fafd51518a2","year":2013},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.303485Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:0ee881e3f6d6fa726fef666d141d98dd5dce57d472685f9f8b637dc7e941d42a","observation_id":"d863c16f-06d0-49d9-9512-405bba099cea","resolution":{"observed_at":"2026-08-12T16:37:57.828633Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1303.5076","last_updated":"2014-03-20T13:12:41Z","snapshot_observed_at":"2026-08-12T19:39:05.589825Z","submitted_at":"2013-03-20T20:10:16Z","title":"Planck 2013 results. XVI. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.5076","snapshot_observed_at":"2026-08-12T16:37:56.309839Z","title":"Collaboration, Planck 2013 results","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.309839Z"},"links":{"cited_paper":"/paper/1303.5076","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:bd1653d79f2cd1b5ceb1fbdfc0735a100993480459aab31817c81c9ed4b15e39","observation_id":"a5c3389e-732c-4995-8c12-771c8663e1f4","resolution":{"observed_at":"2026-08-12T16:37:56.309839Z","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":"2026-08-04T11:38:00.035477Z","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":"2026-08-12T16:37:56.316986Z","title":"Collaboration, Planck 2015 results","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.316986Z"},"links":{"cited_paper":"/paper/1502.01589","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:184041d3dd7950331c3a191efdab3089d9228d438843979f781c4caaf3e8f423","observation_id":"deff8066-7526-406e-9dc1-8b598478ffb5","resolution":{"observed_at":"2026-08-12T16:37:56.316986Z","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T16:37:56.324455Z","title":"Weinberg, The cosmological constant problem, Rev","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.324455Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:f49f8d109dad95431f02b7ab7c798ced9c9271c69538113a430a2a5773110f35","observation_id":"4a8b6fd5-6533-489b-9db3-87b5f5f07bc1","resolution":{"observed_at":"2026-08-12T16:37:56.324455Z","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":"2026-08-12T16:37:57.790550Z","title":"Zlatev, L","venue":null,"work_id":"793cd80a-3c7f-46d3-8985-c670891fb195","year":1999},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.331584Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:64241f41f7ba9a752f55e59d6c320b07f5e2f489fe3a421f9be7da2a653ad28a","observation_id":"007fc638-e5a9-455f-a953-1622e75cb2e0","resolution":{"observed_at":"2026-08-12T16:37:57.795875Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.04256","last_updated":"2019-09-02T22:12:33Z","snapshot_observed_at":"2026-08-12T15:52:42.048317Z","submitted_at":"2017-07-13T18:00:00Z","title":"Small-Scale Challenges to the $\\Lambda$CDM Paradigm","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1707.04256","snapshot_observed_at":"2026-08-12T16:37:56.339537Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.339537Z"},"links":{"cited_paper":"/paper/1707.04256","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:ed91e922b267d9c977a6844960f30a0685cc1662fa604e9fe1621b3c3b8a5cf0","observation_id":"36e94db9-0473-4b24-a363-d4872f3ba08c","resolution":{"observed_at":"2026-08-12T16:37:56.339537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.03624","last_updated":"2020-01-10T19:00:06Z","snapshot_observed_at":"2026-08-07T08:40:54.490186Z","submitted_at":"2020-01-10T19:00:06Z","title":"The Expansion of the Universe is Faster than Expected","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.03624","snapshot_observed_at":"2026-08-12T16:37:56.350280Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.350280Z"},"links":{"cited_paper":"/paper/2001.03624","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:a95e3615662c098785fb7ff11b2335e8fbfc25a26e44752f044132dd4f92b95d","observation_id":"0e4f9aff-4e65-4d64-88f8-de523d2bca84","resolution":{"observed_at":"2026-08-12T16:37:56.350280Z","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":"2026-08-12T16:37:57.768002Z","title":null,"venue":null,"work_id":"defa7b07-e60c-4a0b-95a1-147b5140f141","year":2019},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.356734Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:290d1b4e9da817af4d217a0607e9a7ff8adf744221f3a314f51a1426b42fc9f1","observation_id":"a652b9dc-985c-4875-8f1e-db4bf298f4bb","resolution":{"observed_at":"2026-08-12T16:37:57.776174Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-11T03:46:12.939306Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-12T16:37:56.363214Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.363214Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:47866c193ad02def9b0a63b1993177aacbf0a4f4c542d9a83d843b3ecc4ce966","observation_id":"54d8a352-db82-4621-b73f-c6d7b4aa7925","resolution":{"observed_at":"2026-08-12T16:37:56.363214Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09148","last_updated":"2019-01-27T01:32:21Z","snapshot_observed_at":"2026-07-06T07:04:00.428335Z","submitted_at":"2018-09-24T18:22:04Z","title":"Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09148","snapshot_observed_at":"2026-08-12T16:37:56.371877Z","title":"Hikage et al., Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data, Publ","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.371877Z"},"links":{"cited_paper":"/paper/1809.09148","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:a5053e367a1e370cd5fbd833a4003ff06eaba1900ed04d3753386db734ca5f4b","observation_id":"9dfee8b3-cb3b-44d7-95f5-5b2764a70bed","resolution":{"observed_at":"2026-08-12T16:37:56.371877Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1812.06076","last_updated":"2019-11-18T14:09:46Z","snapshot_observed_at":"2026-08-10T13:15:44.332954Z","submitted_at":"2018-12-14T18:51:54Z","title":"KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1812.06076","snapshot_observed_at":"2026-08-12T16:37:56.378099Z","title":"Hildebrandt et al., KiDS+VIKING-450: Cosmic shear tomography with optical and infrared data, Astron","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.378099Z"},"links":{"cited_paper":"/paper/1812.06076","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:74a77e249a2844c68b552897097c17fd0b663f8622f5bc9f34089c3667df7ecc","observation_id":"a5bbb11b-5bed-447c-a3b0-3d5137e087cd","resolution":{"observed_at":"2026-08-12T16:37:56.378099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.15633","last_updated":"2020-10-13T16:23:19Z","snapshot_observed_at":"2026-08-08T14:13:08.264394Z","submitted_at":"2020-07-30T17:54:56Z","title":"KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.15633","snapshot_observed_at":"2026-08-12T16:37:56.384151Z","title":"Asgari et al., KiDS-1000 cosmology: Cosmic shear constraints and comparison between two point statistics, Astron","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.384151Z"},"links":{"cited_paper":"/paper/2007.15633","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:9f9d37882b4249a7607e05b79c72768a445d2379aafbce4654c182add85014c5","observation_id":"b240eea7-3f4b-4f1c-9a99-9d6723427006","resolution":{"observed_at":"2026-08-12T16:37:56.384151Z","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":"2026-08-12T16:37:57.741797Z","title":"Amon et al","venue":null,"work_id":"697887de-fc28-4064-8e81-bf31c4e97208","year":2022},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.390938Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:eb75bfe787ba42772afae1585922232e0577d8eb546e51739eed5b090d0514f1","observation_id":"30612a93-67a1-41b9-aee8-3cf282f56e7c","resolution":{"observed_at":"2026-08-12T16:37:57.747236Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.721831Z","title":"Caldwell, A phantom menace? cosmological consequences of a dark energy component with super-negative equation of state, Phys","venue":null,"work_id":"77002c03-6e41-419e-bf6f-e373ab8cc71b","year":2002},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.395784Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:e9d5533b53b8ab44ee1c2f9b17ed7e6a3c97ef35c1d4d96992eda56f189cb6be","observation_id":"ae9dc058-14ab-4d04-ac3a-bbceb5056d15","resolution":{"observed_at":"2026-08-12T16:37:57.729194Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.702241Z","title":"Kamenshchik, U","venue":null,"work_id":"5f2a4b1c-a21d-46fc-a82e-48d98670270b","year":2001},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.401234Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:313fe655990d608a447e72cdc1dddbdc19d0f8cae77a49613689e2433bb88976","observation_id":"daf172ff-9b50-46aa-8702-1b272159836f","resolution":{"observed_at":"2026-08-12T16:37:57.708224Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.669926Z","title":"Nojiri and S","venue":null,"work_id":"67d2fc0b-fc66-437e-89c3-c9a3fc8b679d","year":2003},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.406431Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:882ab8b2e36c2bd6f38c931da9fd6839c83a5436e3f5c8319564a5a9e4e02fce","observation_id":"adbd19af-3350-4a68-bb1e-6bde0bcc211e","resolution":{"observed_at":"2026-08-12T16:37:57.677837Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0005016","last_updated":"2000-05-25T20:51:15Z","snapshot_observed_at":"2026-07-07T04:36:32.875811Z","submitted_at":"2000-05-02T00:30:42Z","title":"4D Gravity on a Brane in 5D Minkowski Space","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0005016","snapshot_observed_at":"2026-08-12T16:37:56.412698Z","title":null,"venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.412698Z"},"links":{"cited_paper":"/paper/hep-th/0005016","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:181ef818c5dc08c05ef22d3993f2bbc62cd133f2b27fd1e9e3a33322f8172740","observation_id":"664cca42-6c89-4f18-b866-8268b8bc1cf4","resolution":{"observed_at":"2026-08-12T16:37:56.412698Z","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":"2026-08-12T16:37:57.648920Z","title":"Eckart, The thermodynamics of irreversible processes","venue":null,"work_id":"db5aa00f-baed-471b-9156-68cb52166294","year":1940},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.418441Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:c42706a19b4f02cecb3c4a980a67bc762033a315b580f19fc062c5dcff3528a4","observation_id":"bcaaa8f3-2ec5-4ad9-8a3c-7a2fcd1392ef","resolution":{"observed_at":"2026-08-12T16:37:57.654926Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.625721Z","title":"Di Prisco, L","venue":null,"work_id":"71e3df81-de6d-4580-aefb-cf0d4a7ef923","year":2000},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.425129Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:ab8b26ceae47092f8f4e67bbf5ed3145a7d0c1e98894e52209c03284a3dffb3d","observation_id":"cd1eea56-ba38-46f1-8f21-7f8a6e171cfe","resolution":{"observed_at":"2026-08-12T16:37:57.633171Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.599517Z","title":"Zimdahl, D","venue":null,"work_id":"714d7cf1-9777-47d2-9eff-343a90cfa43a","year":2001},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.431451Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:48a0320ee23a78ca824ca207cdc1f06b9c37b7b6d788e0096ec884575b915883","observation_id":"e8b44c11-dc42-4d86-a9e3-7e2e602abbb3","resolution":{"observed_at":"2026-08-12T16:37:57.606820Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.568750Z","title":"Velten and D","venue":null,"work_id":"dde81d16-5b11-4774-bbb6-4ea8d7985ec7","year":2012},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.437582Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:3187ca6982889399d3ac235a17856074a5564fbd9881f1a53c69ec1b7f6e21ee","observation_id":"d1e74c68-7000-4559-a00e-08f4c9a2a8b6","resolution":{"observed_at":"2026-08-12T16:37:57.577731Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.540906Z","title":"Ren and X.-H","venue":null,"work_id":"2ca46b85-c2c8-4a20-87e3-423f1575bc4e","year":2006},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.446513Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:a578873bf12beb6b639d6fa90b72af9b8d42dbdcce2893b386baee6954ca0a7b","observation_id":"a7a7da52-6d1d-4b47-9458-db143af93b55","resolution":{"observed_at":"2026-08-12T16:37:57.547669Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.520104Z","title":"Xin-He and D","venue":null,"work_id":"286d35bb-da04-464e-9e62-664b1f8d1950","year":2009},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.453926Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:44f9aa495861bb9066c89b14d2dea18ae2718a1a94d115fe070d9729499bfccb","observation_id":"c5f35c53-e886-4915-aa78-3021e7abc44d","resolution":{"observed_at":"2026-08-12T16:37:57.526466Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.494869Z","title":"Colistete, J","venue":null,"work_id":"690a8e79-d7c4-4141-b2e9-2399a00baeb7","year":2007},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.460842Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:bfbaf6ee2a7db4fdedb6c9e7a2445f31fbe543f13bcd90e2f826894139e3a13c","observation_id":"9609b4ed-62ee-4617-954f-2a00f91d132c","resolution":{"observed_at":"2026-08-12T16:37:57.502124Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1611.01023","last_updated":"2016-10-30T07:39:26Z","snapshot_observed_at":"2026-07-06T05:17:14.601493Z","submitted_at":"2016-10-30T07:39:26Z","title":"FLRW viscous cosmological models","version":1},"cited_work":{"arxiv_id":"1611.01023","doi":null,"metadata_source":"pith","pith_arxiv_id":"1611.01023","snapshot_observed_at":"2026-08-12T16:37:56.777252Z","title":"FLRW viscous cosmological models","venue":"physics.gen-ph","work_id":"ddb57b77-0121-44a7-86a1-3538582fdc82","year":2016},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.468519Z"},"links":{"cited_paper":"/paper/1611.01023","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:85e6acb9cf1a729ebfc2c75444713acad7d91c69bcb4c48b0a6fdb06460761e5","observation_id":"135a219c-fa5b-40cb-8a2e-485a41c5525d","resolution":{"observed_at":"2026-08-12T16:37:56.783810Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.472356Z","title":null,"venue":null,"work_id":"3618d603-e71c-48d4-9096-d117f9a82fbd","year":2018},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.475350Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:ce12065edf8908cc6b3933d468e90bde8cc30ada28879f5c3bd1fd4407bebac0","observation_id":"f3857043-9759-40c5-ae0d-402103bc98ee","resolution":{"observed_at":"2026-08-12T16:37:57.479285Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.449105Z","title":"Wang and G.-B","venue":null,"work_id":"8e8f46d4-a9b2-4c65-8e2f-5831e45fd025","year":2018},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.482291Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:c13099b5015829ecc778fda64df76cf917aac4986a052c0b103785539dff5429","observation_id":"af9ff4e7-c0b9-4567-8a01-55687ac713e3","resolution":{"observed_at":"2026-08-12T16:37:57.455893Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.05228","last_updated":"2021-11-01T14:41:59Z","snapshot_observed_at":"2026-07-06T10:32:16.643169Z","submitted_at":"2021-01-13T17:43:04Z","title":"Probing the effects of primordial black holes on 21-cm EDGES signal along with interacting dark energy and dark matter - baryon scattering","version":3},"cited_work":{"arxiv_id":"2101.05228","doi":null,"metadata_source":"pith","pith_arxiv_id":"2101.05228","snapshot_observed_at":"2026-08-12T16:37:56.751950Z","title":"Probing the effects of primordial black holes on 21-cm EDGES signal along with interacting dark energy and dark matter - baryon scattering","venue":"astro-ph.CO","work_id":"bbbb5a49-2850-4385-9e6a-220d647d1b5e","year":2021},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.489298Z"},"links":{"cited_paper":"/paper/2101.05228","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:28f9484fc2a33c28acace952ad2cc7f359376f759aafd3df5467d6e91b801522","observation_id":"5a373e80-ed5d-4df6-a5c4-e8f42606560c","resolution":{"observed_at":"2026-08-12T16:37:56.757845Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.09177","last_updated":"2022-10-22T05:56:54Z","snapshot_observed_at":"2026-08-04T03:59:40.277316Z","submitted_at":"2022-07-19T10:23:45Z","title":"Global 21-cm brightness temperature in viscous dark energy models","version":3},"cited_work":{"arxiv_id":"2207.09177","doi":null,"metadata_source":"pith","pith_arxiv_id":"2207.09177","snapshot_observed_at":"2026-08-12T16:37:56.715127Z","title":"Global 21-cm brightness temperature in viscous dark energy models","venue":"astro-ph.CO","work_id":"80e262d0-c481-41dd-b401-5a97a48199c0","year":2022},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.497132Z"},"links":{"cited_paper":"/paper/2207.09177","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:74e02c28f808a442be189370b57f7d979cb0aba4771bce5ca7ce699685d8ea68","observation_id":"21ccb377-0f4b-4e51-9456-8f03772d41f0","resolution":{"observed_at":"2026-08-12T16:37:56.724696Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0807.3548","last_updated":"2008-11-03T20:24:22Z","snapshot_observed_at":"2026-08-10T08:38:42.878658Z","submitted_at":"2008-07-23T17:40:33Z","title":"Two new diagnostics of dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0807.3548","snapshot_observed_at":"2026-08-12T16:37:56.505773Z","title":"Sahni, A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.505773Z"},"links":{"cited_paper":"/paper/0807.3548","citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:3abdbcdcd4ccc61b861280375472a9d1d293d7ac9d7942a184cd5c1ea8e4d65e","observation_id":"a98d9165-d3eb-44a4-be64-90b853c97039","resolution":{"observed_at":"2026-08-12T16:37:56.505773Z","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":"2026-08-12T16:37:57.426530Z","title":null,"venue":null,"work_id":"c96a72d6-fa1f-433a-be86-b8621d93d72a","year":2020},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.511689Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:b974b44088eaf8df4c496fe1d03b7228b3334fb246e1740cfe2353157219ea87","observation_id":"259cf6cb-ea83-4aa5-bb47-0718783c7104","resolution":{"observed_at":"2026-08-12T16:37:57.432857Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.405242Z","title":null,"venue":null,"work_id":"9621e689-d0fb-4813-9ced-e895d9cb6aed","year":2007},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.517740Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:1ce00c803066fc9f8611a37654bd65ef0fa67bc67c222e27174a94e2b5b2db84","observation_id":"ed0e5726-202a-4de6-b909-a25f40812822","resolution":{"observed_at":"2026-08-12T16:37:57.412109Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.382298Z","title":"Di Valentino, A","venue":null,"work_id":"6833ba31-dfe9-451e-a27a-4d3ce8600126","year":2020},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.524290Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:2303ec3526b4057eff140584ed1c1a0589f4d9b9fcf43edeb60f7ba6af4953ec","observation_id":"1d7c2ca9-a04c-4de4-853e-12e8b3730929","resolution":{"observed_at":"2026-08-12T16:37:57.392410Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.360370Z","title":null,"venue":null,"work_id":"b1411686-7857-438e-a887-f96a69eb1776","year":2015},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.532698Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:b72e9a845aca52d0d1f49aabe3c7edc131e5e9cbc79f93decd291d17f467823b","observation_id":"46f7d768-9b5b-4f4d-8d74-86840936d8a6","resolution":{"observed_at":"2026-08-12T16:37:57.366863Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.327513Z","title":"Bertolami, F","venue":null,"work_id":"791bde94-0983-4725-be73-80da6d7f97ed","year":2007},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.539206Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:a0428892765071d2b7527ae8ae07b4d9272056ec0519988f1f4920308a3332ac","observation_id":"917f269f-f427-4f71-9961-837273f7acf4","resolution":{"observed_at":"2026-08-12T16:37:57.336410Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.304172Z","title":null,"venue":null,"work_id":"9b3869a1-8a57-4b41-a483-868627b99adb","year":2011},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.550729Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:9fb6cf23353eb00bb4607d4183b16378d68d38c6750d66f0941f837032408d25","observation_id":"1263514b-9fe4-4707-ab41-b23d30300dba","resolution":{"observed_at":"2026-08-12T16:37:57.310499Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.276921Z","title":"Santos, W","venue":null,"work_id":"567f85fe-f34b-4de4-bda8-0b3dc06f0e34","year":2017},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.558212Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:d92b8d1e53060b86853e3117d01a29e358dbce123f8064b99fba037009dc4e9d","observation_id":"c240cd38-d027-45ba-80d7-2336c7131a1c","resolution":{"observed_at":"2026-08-12T16:37:57.283510Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.246628Z","title":null,"venue":null,"work_id":"b1131b2d-2e02-4230-88b6-3203b716f7b0","year":2018},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.563812Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:be11c5880c1c6805bd8306d4437182226c8038aea34bf27585f0563a80df70de","observation_id":"4f9bd704-d5f3-4bdb-85ce-e09bbe64413a","resolution":{"observed_at":"2026-08-12T16:37:57.253636Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.223769Z","title":"Le Delliou, R","venue":null,"work_id":"aef94498-5b08-47ef-a765-b2364a9bd88d","year":2019},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.572499Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:81985182fbf21aa1bf468cc918ced0fcc237248ddc618fcc85804e7f91734dd1","observation_id":"f3d72d5c-6d2c-4846-9c2a-c1c51747cfbe","resolution":{"observed_at":"2026-08-12T16:37:57.230856Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.200358Z","title":"Gavela, D","venue":null,"work_id":"500d358d-2e4e-4ad9-b524-addd8ead4e86","year":2009},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.578969Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:b6ddab5228a9b4e17584641ad056ab9f984a905b07937bf77420293bb4bae36d","observation_id":"0f3f5e08-4c9a-4eeb-8548-a332409979c0","resolution":{"observed_at":"2026-08-12T16:37:57.209145Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.172844Z","title":null,"venue":null,"work_id":"9730dfa2-eb41-486d-a383-bfd7963d4acb","year":2009},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.585260Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:8a2d253c1418d9a1787843490d79292202ec91fe0b585f1d889d4b77c90eead3","observation_id":"702333e0-e364-4ecb-a956-1b857a109504","resolution":{"observed_at":"2026-08-12T16:37:57.179708Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.145666Z","title":"Visser, Jerk, snap, and the cosmological equation of state, Class","venue":null,"work_id":"acde256e-db92-4faa-9cc8-cb41f3a1b9c5","year":2003},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.591884Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:fe6afb5c2380cf8111eecb80e8acc71a9ee0f61b900344b2fcae97ef1159b922","observation_id":"1fb421a7-3926-4d71-9c3b-d3b62676434a","resolution":{"observed_at":"2026-08-12T16:37:57.153877Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.119346Z","title":null,"venue":null,"work_id":"83a910da-82f6-4fa6-90cf-0ab1afe168df","year":2013},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.597882Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:db0c7224b42e100d68c7cd66801f593c5b647c011fe992a1de46214a2048736b","observation_id":"6216bb73-9546-4ca9-a0f2-63e14433f463","resolution":{"observed_at":"2026-08-12T16:37:57.129773Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.096139Z","title":"Shafieloo, V","venue":null,"work_id":"157106db-2899-4312-84cd-7ba97ae126fd","year":2012},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.604802Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:010de612c996a05a6262390f40371482664a37e0bbbf413a505fac172440e2e0","observation_id":"dc01d224-15f6-4f34-abb3-893acdcccf7e","resolution":{"observed_at":"2026-08-12T16:37:57.102753Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.065559Z","title":"Blake et al., The WiggleZ Dark Energy Survey: mapping the distance–redshift relation with baryon acoustic oscillations, Mon","venue":null,"work_id":"ce0bf4e6-75bc-4945-86a8-7bc451a1b6e2","year":2011},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.614328Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:d3f6c32a792e4655ad0f73f89f0cc82983bcd60c01529e0fb0b103bf09c6943e","observation_id":"a1a03f1e-615e-472e-9154-a9acd7089215","resolution":{"observed_at":"2026-08-12T16:37:57.075508Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.038454Z","title":null,"venue":null,"work_id":"6aeec314-73bd-4242-8a58-568e64769009","year":2012},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.620847Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:63a6337dcab8d1eeebf5317aa1811c0bc2253a6e1fe25fb2d2c33ec1d2ec158d","observation_id":"13e2a71d-d5c4-4c09-a3a4-923e6f8d2ea0","resolution":{"observed_at":"2026-08-12T16:37:57.045139Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:57.013668Z","title":"Haario, M","venue":null,"work_id":"e7883401-0f52-457d-80fa-e6d938ca0b84","year":2006},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.631576Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:731225ba69aa50367d0e269dd7197b211b17bb8d8ac635b675c981f7ab611832","observation_id":"1b3119bd-6aa7-4eda-a2e0-9c37cd4d850f","resolution":{"observed_at":"2026-08-12T16:37:57.021311Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-12T16:37:56.991929Z","title":"Haario, E","venue":null,"work_id":"9ff1e4ad-bd8f-43fc-8037-19742818b1e7","year":2001},"citing_paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T16:37:56.637483Z"},"links":{"citing_paper":"/paper/2411.13379"},"observation_digest":"sha256:ce36180abd1ae56f2904d95da16c2beddfe1473cc42096c43ff0ef009f744303","observation_id":"10901167-3350-40e9-a24b-3321de683c24","resolution":{"observed_at":"2026-08-12T16:37:56.998627Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.13379","last_updated":"2024-11-20T15:00:42Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-12T16:26:49.486800Z","submitted_at":"2024-11-20T15:00:42Z","title":"Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario"},"reference_resolution":{"displayed":51,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":24,"verified_exact":3,"verified_fuzzy":24},"total_outbound_references":51},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 0 inbound Pith citation observations for arXiv:2411.13379."}