{"as_of":"2026-08-12T12:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c4850ce08f95b356cd5a6ab1242bf98ba0c55ff4670a8169c02e30b3cf717977","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":74,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":74,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":74,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T22:56:28.794850Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"doi_reference","source_observed_at":"2026-07-09T22:56:37.381487Z","state":"measured"}],"external_citation_measurements":[{"count":6862,"observed_at":"2026-07-09T22:56:37.381487Z","source":"doi_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-05-12T23:40:20.792511Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/1611.00036"},"observation_digest":"sha256:de294e6a16526100b2bed152fb4337abeeeafbc4cf561393c59b0f33b5498a61","observation_id":"8c1d8b4d-cd41-4354-b304-48a316f9554b","resolution":{"observed_at":"2026-05-12T23:40:21.676702Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"1907.06854","last_updated":"2019-07-16T06:05:49Z","snapshot_observed_at":"2026-07-06T08:07:57.308057Z","submitted_at":"2019-07-16T06:05:49Z","title":"$\\Lambda$CDM-like models with future singularities","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-24T21:13:25.514919Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/1907.06854"},"observation_digest":"sha256:12e121f728146a7f8c71c9df0bcff27eeaed99cfe17769b102df6899003f1f0e","observation_id":"b607a7d4-c85e-43e8-9bcc-17fe8c5d51de","resolution":{"observed_at":"2026-05-24T21:14:56.753561Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"1907.06880","last_updated":"2019-07-16T07:59:49Z","snapshot_observed_at":"2026-07-06T08:08:00.259644Z","submitted_at":"2019-07-16T07:59:49Z","title":"Finite scale factor and future singularities","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-24T21:08:32.275550Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/1907.06880"},"observation_digest":"sha256:b61cdab3f006127b94beffc6c0bf7569750b93dfe69f1cab5dbe682b1c40c51f","observation_id":"de4c1a5c-cbcc-4470-b706-b6e33ccb5cc4","resolution":{"observed_at":"2026-05-24T21:09:56.679685Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-05-12T18:07:31.131298Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2112.04510"},"observation_digest":"sha256:67b4e66daa59f1756869ada9611d7c1267af808190ad4d93d455f86b54280734","observation_id":"b557940a-0303-44d9-9a49-bf2bfb59acfe","resolution":{"observed_at":"2026-05-12T18:07:31.254307Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-11T22:56:28.794850Z","title":"Komatsu et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.03065","last_updated":"2024-12-04T06:34:46Z","snapshot_observed_at":"2026-08-12T11:17:45.852183Z","submitted_at":"2024-12-04T06:34:46Z","title":"Chebyshev cosmography in the framework of extended symmetric teleparallel theory","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T22:56:28.794850Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2412.03065"},"observation_digest":"sha256:81af6fc105a3e7c10c7d739776d7ec9c9817d592b82bb011ed1fab78dd1af584","observation_id":"78342d57-a2c2-49af-a611-6fae061a5edc","resolution":{"observed_at":"2026-08-11T22:56:28.794850Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-11T18:15:34.012138Z","title":"Komatsu and others, ApJS 192, 18 (2011), 1001.4538","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.08151","last_updated":"2025-06-05T09:13:24Z","snapshot_observed_at":"2026-08-12T09:21:05.923193Z","submitted_at":"2024-12-11T07:11:41Z","title":"Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-11T18:15:34.012138Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2412.08151"},"observation_digest":"sha256:0fc25fcdef8c22c7e4c481e2431e80ed72e29d072c2d799bb839f94a3706e3ad","observation_id":"bf364545-581f-44c3-aeb9-d3846214d930","resolution":{"observed_at":"2026-08-11T18:15:34.012138Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-11T17:13:30.669211Z","title":"Komatsu et al.,Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.09344","last_updated":"2024-12-12T15:11:40Z","snapshot_observed_at":"2026-08-11T17:03:20.601855Z","submitted_at":"2024-12-12T15:11:40Z","title":"Revisiting Universal Extra-Dimension Model with Gravity Mediated Decays","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T17:13:30.669211Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2412.09344"},"observation_digest":"sha256:cd51266ccbe36cb18b41780c029e18020ac2c73a991fae548e849a98d03d8cdb","observation_id":"a120fc00-dd9f-4ef0-b056-8c112dac5327","resolution":{"observed_at":"2026-08-11T17:13:30.669211Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-11T11:05:02.704508Z","title":"Komatsu, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.15849","last_updated":"2024-12-25T08:40:53Z","snapshot_observed_at":"2026-08-11T23:48:04.573895Z","submitted_at":"2024-12-20T12:46:05Z","title":"Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T11:05:02.704508Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2412.15849"},"observation_digest":"sha256:251d69beb7bb66e7f4a597aa1bf0d96ac4538733df2bfa9d8fb1b8f393ce5ded","observation_id":"8411b22b-a5c5-4715-84fa-de5318231b10","resolution":{"observed_at":"2026-08-11T11:05:02.704508Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-11T05:35:41.394366Z","title":"Komatsu et al., Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.17494","last_updated":"2025-08-31T11:42:43Z","snapshot_observed_at":"2026-08-12T08:48:19.234921Z","submitted_at":"2024-12-23T11:44:37Z","title":"Analysing Ultra High Energy Cosmic Rays' Anisotropy in $\\boldsymbol{f(R, T)}$ Gravity Theory","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-11T05:35:41.394366Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2412.17494"},"observation_digest":"sha256:d2ca2508555fd7bd3b19d5bb40c22d70fe1ba737d6bbe73e2254d19313d04c96","observation_id":"eebfd2d6-7cb0-491d-960d-960642e75b51","resolution":{"observed_at":"2026-08-11T05:35:41.394366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-10T22:48:20.279300Z","title":"Komatsu et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.00769","last_updated":"2025-02-26T10:16:34Z","snapshot_observed_at":"2026-08-11T12:59:21.802381Z","submitted_at":"2025-01-01T08:15:33Z","title":"Prospects for measuring neutrino mass with 21-cm forest","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-10T22:48:20.279300Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2501.00769"},"observation_digest":"sha256:55eb4757f77d3e37dc8f2d17b3ef9c32e3bf05017c365249515fc88938c8ab65","observation_id":"1d0385c0-aaaf-4f94-bab8-cfaed8948fbf","resolution":{"observed_at":"2026-08-10T22:48:20.279300Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-10T23:17:30.308002Z","title":"Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2501.01546","last_updated":"2025-05-06T08:07:33Z","snapshot_observed_at":"2026-08-11T19:56:47.754182Z","submitted_at":"2024-12-30T07:27:57Z","title":"Beam test performance of a prototype muon trigger detector for the PSI muEDM experiment","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-10T23:17:30.308002Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2501.01546"},"observation_digest":"sha256:d1105ea353240777649ea98603970c26edf5ffcb11522a04df8e83ee7b3bb5c2","observation_id":"17f3d71f-6ee5-4deb-9d92-dcda7934afd2","resolution":{"observed_at":"2026-08-10T23:17:30.308002Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-08T12:07:01.052191Z","title":"Komatsu, K.M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2502.07654","last_updated":"2025-02-11T15:43:29Z","snapshot_observed_at":"2026-08-08T20:39:53.330026Z","submitted_at":"2025-02-11T15:43:29Z","title":"Planck PR4 (NPIPE) map-space cosmic birefringence","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-08T12:07:01.052191Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2502.07654"},"observation_digest":"sha256:df7baff7943451e94d625abb7db916aa201b2f05095c0c3cb64111d5e19f7fa6","observation_id":"3f9a61c8-60b2-4a34-95e6-5100a854a9d6","resolution":{"observed_at":"2026-08-08T12:07:01.052191Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2503.16355","last_updated":"2026-05-19T08:31:27Z","snapshot_observed_at":"2026-07-06T20:56:09.656767Z","submitted_at":"2025-03-20T17:13:57Z","title":"DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-22T23:07:09.906749Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2503.16355"},"observation_digest":"sha256:fc4a82c21a3ae0d41ad7e866ef5343a944818534c24edbc93fddeefd38d08dc0","observation_id":"4216d045-893d-448f-a35d-4acde677e072","resolution":{"observed_at":"2026-05-22T23:07:14.070658Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-07T15:23:42.901316Z","title":"Komatsu et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2505.15540","last_updated":"2025-05-21T14:03:30Z","snapshot_observed_at":"2026-08-09T06:30:01.220642Z","submitted_at":"2025-05-21T14:03:30Z","title":"Quasinormal Modes of Schwarzschild Black Holes in the Dehnen-(1, 4, 5/2) Type Dark Matter Halos","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T15:23:42.901316Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2505.15540"},"observation_digest":"sha256:a6aaf9d9cd6c4caf8ed8402d63e77bd900564705f9274bd3561ca760d4d5352b","observation_id":"dcb21b88-b1e2-47b9-b3ea-bd64ce3d41f4","resolution":{"observed_at":"2026-08-07T15:23:42.901316Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-07T12:07:26.487602Z","title":"Komatsu et al","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2506.00684","last_updated":"2025-05-31T19:34:44Z","snapshot_observed_at":"2026-08-10T07:01:45.544999Z","submitted_at":"2025-05-31T19:34:44Z","title":"Forecast Constraints on Bouncing Cosmology from High Frequency Gravitational Waves Using Superconducting LC Circuits and Resonant Cavities","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T12:07:26.487602Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2506.00684"},"observation_digest":"sha256:8d37fad28d1fca5f52b6cdfdaf002ae6a27ef2a84603388b08e6d5892829b4e9","observation_id":"98ff0f4f-bc08-4c34-9c82-44f9d5fcf418","resolution":{"observed_at":"2026-08-07T12:07:26.487602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-06T20:32:38.768234Z","title":"Komatsu et al., Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation , Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.02685","last_updated":"2025-07-03T14:51:54Z","snapshot_observed_at":"2026-08-08T01:54:30.855147Z","submitted_at":"2025-07-03T14:51:54Z","title":"Axion USR Inflation","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T20:32:38.768234Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2507.02685"},"observation_digest":"sha256:6b30217a3501f3292c1234e432a7a0f232b372b20bfec6058cf92fb537667391","observation_id":"c96ac1e5-c331-473c-b537-476462599bf1","resolution":{"observed_at":"2026-08-06T20:32:38.768234Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-06T19:10:44.150899Z","title":"Komatsuet al.(WMAP), Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.06544","last_updated":"2025-07-09T04:57:39Z","snapshot_observed_at":"2026-08-08T21:29:37.875213Z","submitted_at":"2025-07-09T04:57:39Z","title":"Power Law Plateau Inflation and Primary Gravitational Waves in the light of ACT","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-06T19:10:44.150899Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2507.06544"},"observation_digest":"sha256:b8e14c84a87c67f0bc9c56f94441318b72060849b0d619e74a1e98358f862f17","observation_id":"20d2a4d0-2433-452a-8919-931a1e981e58","resolution":{"observed_at":"2026-08-06T19:10:44.150899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-06T15:12:38.161171Z","title":"Komatsuet al.(WMAP), Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2507.16589","last_updated":"2026-06-23T13:43:52Z","snapshot_observed_at":"2026-08-08T06:56:16.966820Z","submitted_at":"2025-07-22T13:45:38Z","title":"Cosmological preference for a positive neutrino mass at 2.7$\\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data","version":3},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-06T15:12:38.161171Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2507.16589"},"observation_digest":"sha256:759d716d19181b28181680d8a6e17ab6491b52e2bfda78e16a1a0a1ddc59a2ef","observation_id":"b6f63b8a-84bb-48e8-9014-5fba63293d36","resolution":{"observed_at":"2026-08-06T15:12:38.161171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-04T22:56:12.266986Z","title":"Komatsu, K.M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.07092","last_updated":"2025-09-08T18:00:05Z","snapshot_observed_at":"2026-08-04T22:56:04.649080Z","submitted_at":"2025-09-08T18:00:05Z","title":"Why Cosmic Voids Matter: Pristine Evolution","version":1},"reference_index":138,"source":"pdf_text","source_observed_at":"2026-08-04T22:56:12.266986Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2509.07092"},"observation_digest":"sha256:e0c417b91de7b51e356cc175b64ce94e75627262aafe4256d1102009a22e6673","observation_id":"c94be2ad-3b17-425a-b90f-f089965515f0","resolution":{"observed_at":"2026-08-04T22:56:12.266986Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2509.13654","last_updated":"2026-04-14T13:07:43Z","snapshot_observed_at":"2026-08-06T16:29:44.262121Z","submitted_at":"2025-09-17T02:59:36Z","title":"Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-18T16:55:42.473876Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2509.13654"},"observation_digest":"sha256:cf39eaebdcf42807a0446fed4e728ef789e8275c5c9fd3a4195f166ba5ac24a1","observation_id":"94239bc0-8219-4898-905a-5bfe5d08af7e","resolution":{"observed_at":"2026-05-18T16:56:38.217339Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-04T16:19:43.772001Z","title":"Komatsu, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2509.14751","last_updated":"2026-06-06T07:08:18Z","snapshot_observed_at":"2026-08-09T17:59:13.628251Z","submitted_at":"2025-09-18T08:54:47Z","title":"Probing initial isocurvature perturbation with 21cm one-point statistics","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-04T16:19:43.772001Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2509.14751"},"observation_digest":"sha256:281c3b1f785c8c0050c93829280cb8b4d8126e4ea23cc78a097e37d67e948e11","observation_id":"417bd0ea-b2ca-4185-aaea-ca3cf1e58953","resolution":{"observed_at":"2026-08-04T16:19:43.772001Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-04T13:15:32.122967Z","title":"Komatsu, K.M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2510.01121","last_updated":"2026-06-03T17:40:08Z","snapshot_observed_at":"2026-08-12T07:23:15.608603Z","submitted_at":"2025-10-01T17:07:37Z","title":"CosmoUiT: A Vision Transformer-UNet Hybrid for Fast and Accurate Emulation of 21-cm Maps from the Epoch of Reionization","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-04T13:15:32.122967Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2510.01121"},"observation_digest":"sha256:a8af273ea7a55b5cbf78dfb536aaea9cbec3c76d89a5486ac1643ac64ac600dd","observation_id":"f10d1fbc-5a31-4974-bfa2-817ead723366","resolution":{"observed_at":"2026-08-04T13:15:32.122967Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2510.13770","last_updated":"2026-05-08T01:20:55Z","snapshot_observed_at":"2026-08-11T05:08:44.069129Z","submitted_at":"2025-10-15T17:19:24Z","title":"Gauge-independent Gravitational Waves from Cogenesis in a $B-L$ Conserving Universe","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2510.13770"},"observation_digest":"sha256:513642a10863c8999934487f13b88ce8225f0ac24de420643ac5e8024cdd69a3","observation_id":"7037c0a1-613f-4c46-9a07-79643b411742","resolution":{"observed_at":"2026-05-18T07:06:02.149898Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-04T00:26:05.903280Z","title":"Komatsuet al.(WMAP), Astrophys","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.01612","last_updated":"2026-06-18T21:25:41Z","snapshot_observed_at":"2026-08-05T17:56:23.069298Z","submitted_at":"2025-11-03T14:19:16Z","title":"Running of the spectral index: Reconciling the CMB with the Lyman-$\\alpha$ Forest","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-04T00:26:05.903280Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2511.01612"},"observation_digest":"sha256:41bc35ba51d1ea5610adefb814a6b33a0956c5300a657d27d1000e58f0803cfe","observation_id":"8c5b6051-7072-4af7-b83c-5f9bf3d91c79","resolution":{"observed_at":"2026-08-04T00:26:05.903280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2511.09306","last_updated":"2026-05-20T08:58:17Z","snapshot_observed_at":"2026-07-06T22:35:37.039024Z","submitted_at":"2025-11-12T13:17:24Z","title":"Self-Interaction of Super-Resonant Dark Matter","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-21T19:49:36.832677Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2511.09306"},"observation_digest":"sha256:264666b2f00ca197648c17f4b54b447f37f934e6a8b2bb06c2ae552a8d8f78e1","observation_id":"652bd85c-05b1-4b2a-8201-c29ae9305d7a","resolution":{"observed_at":"2026-05-21T19:50:33.646888Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2601.17117","last_updated":"2026-04-25T12:29:32Z","snapshot_observed_at":"2026-08-09T12:22:25.235151Z","submitted_at":"2026-01-23T19:00:02Z","title":"Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-16T11:34:12.521105Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2601.17117"},"observation_digest":"sha256:4499368a6aa5e71ed2cbe98ddded917f83126a56abbd39cf97d5d02b413c6c64","observation_id":"2e137c48-7cb9-4941-b461-0c704f02a5e5","resolution":{"observed_at":"2026-05-16T11:37:48.975198Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2602.20237","last_updated":"2026-04-21T11:08:14Z","snapshot_observed_at":"2026-07-06T22:46:49.536946Z","submitted_at":"2026-02-23T19:00:00Z","title":"Linking Leptogenesis and Asymmetric Dark Matter: A Testable Framework for Neutrino Mass and the Matter-Antimatter Asymmetry","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-15T19:49:58.834025Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2602.20237"},"observation_digest":"sha256:32f660efbc307bab835a723ff9a1b087e5a6282a681f52e16deff5c90087be20","observation_id":"cdd29133-752c-4fb9-9856-36afa41c4e05","resolution":{"observed_at":"2026-05-15T19:50:17.190883Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-02T20:12:34.446668Z","title":"Komatsu, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2602.23913","last_updated":"2026-06-01T10:10:58Z","snapshot_observed_at":"2026-08-02T20:12:33.769011Z","submitted_at":"2026-02-27T11:02:50Z","title":"Probing inflationary features with galaxy ultraviolet luminosity function observables","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-02T20:12:34.446668Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2602.23913"},"observation_digest":"sha256:4acb1719393cad4bd8b8a80646a049bf05dcc36098df137d0688f750b18a7b2f","observation_id":"2fbefcec-3665-4389-a988-99fa8f5b4c22","resolution":{"observed_at":"2026-08-02T20:12:34.446668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-02T18:35:43.152852Z","title":"Komatsu, K","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2603.09270","last_updated":"2026-07-22T07:14:15Z","snapshot_observed_at":"2026-08-09T11:44:48.266368Z","submitted_at":"2026-03-10T06:56:54Z","title":"Statistical consistency of sign-switching vacuum energy with cosmological observations","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-02T18:35:43.152852Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2603.09270"},"observation_digest":"sha256:4826acb7842538f607e86808a475c873491cf9951294683da432bed19e70dc60","observation_id":"40780749-5002-4dd3-ac5f-e376a078e4cf","resolution":{"observed_at":"2026-08-02T18:35:43.152852Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2603.25331","last_updated":"2026-04-06T11:41:23Z","snapshot_observed_at":"2026-08-11T14:34:57.588170Z","submitted_at":"2026-03-26T11:19:36Z","title":"Jet Power Estimates of FSRQs PKS 1441+25 and Ton 599 from Broadband SED Modeling","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-15T00:55:48.761801Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2603.25331"},"observation_digest":"sha256:cd9ce808a0dce9143e7ce2752def5647b0207c9534bd645307185d2a7d5effe2","observation_id":"f22fdd68-0edf-4799-9934-7d3f3b43c54a","resolution":{"observed_at":"2026-05-15T00:58:25.215908Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2604.26072","last_updated":"2026-04-28T19:21:36Z","snapshot_observed_at":"2026-07-06T23:11:48.524898Z","submitted_at":"2026-04-28T19:21:36Z","title":"Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-07T14:42:49.502885Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2604.26072"},"observation_digest":"sha256:5d999f41f32ac1ecaf36386e5545e13bce41508a1ff86cda1392c6d8c164b2fa","observation_id":"b3e93b76-0f4a-48e6-91fc-06ca206fb082","resolution":{"observed_at":"2026-05-12T00:41:24.823969Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.02723","last_updated":"2026-05-04T15:22:39Z","snapshot_observed_at":"2026-08-11T16:23:17.189483Z","submitted_at":"2026-05-04T15:22:39Z","title":"Euclid preparation. CosmoPostProcess: A simulation calibrated framework for weak lensing selection bias in richness-selected galaxy clusters","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-05-08T18:17:47.203929Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.02723"},"observation_digest":"sha256:84e83cb9a4498a5fa665ca835e85717da389835557478bb52cc6c4987f59e54c","observation_id":"a9a95638-7872-4af5-9eae-91e145e87b20","resolution":{"observed_at":"2026-05-08T18:18:55.592089Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.03008","last_updated":"2026-05-04T18:00:06Z","snapshot_observed_at":"2026-08-11T12:47:45.058279Z","submitted_at":"2026-05-04T18:00:06Z","title":"Environmental Quenching of High-Redshift Galaxies: Interpreting JWST Observations with Simulations","version":1},"reference_index":147,"source":"arxiv_source","source_observed_at":"2026-05-08T17:57:29.069633Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.03008"},"observation_digest":"sha256:3ca80dbd42d2757e0929952a3eec06f1781073004475eeb5b617dfd16165671c","observation_id":"71d13492-a3c8-4d77-bc45-db13a2dd2461","resolution":{"observed_at":"2026-05-08T17:58:53.092800Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.03124","last_updated":"2026-05-04T20:04:41Z","snapshot_observed_at":"2026-07-06T23:16:05.372336Z","submitted_at":"2026-05-04T20:04:41Z","title":"Nowhere Left to Hide: Uncovering All of the Massive Young Embedded Star Clusters in the Antennae with JWST","version":1},"reference_index":248,"source":"arxiv_source","source_observed_at":"2026-05-08T17:31:55.999847Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.03124"},"observation_digest":"sha256:89b9f7df4b3c9c46b7019ad1367f61311ca34cd6a9778ceee771b3f626328ab8","observation_id":"aee6d22d-a68b-4881-8828-38acd22483bf","resolution":{"observed_at":"2026-05-08T17:33:47.283931Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.03171","last_updated":"2026-05-04T21:29:31Z","snapshot_observed_at":"2026-08-11T16:45:19.545809Z","submitted_at":"2026-05-04T21:29:31Z","title":"Nb$_3$Sn Thin Films Using a Cu-Sn Route for Dark Matter Detection","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-08T02:37:56.916734Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.03171"},"observation_digest":"sha256:86dc0b425239d1a9e8e76148eec0b56ae9f7f70068bbb9fca7e12c740c6d4e8e","observation_id":"c57c1c19-68d3-49a2-9805-830811dcb7b1","resolution":{"observed_at":"2026-05-12T10:51:30.472362Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.04537","last_updated":"2026-05-06T06:31:20Z","snapshot_observed_at":"2026-08-11T15:16:48.606707Z","submitted_at":"2026-05-06T06:31:20Z","title":"Investigating the Effects of Bars on Star Formation and Nuclear Activity of Galaxies Using DESI Survey Data","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-08T17:53:45.673744Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.04537"},"observation_digest":"sha256:84bc09945ceebf44e246d1feaa458b08c75107b907a4dda411cf29978ddd7fb8","observation_id":"928499a9-1c03-43cf-8c2c-30e3d30cc33e","resolution":{"observed_at":"2026-05-08T17:53:51.950542Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.08775","last_updated":"2026-05-09T08:03:03Z","snapshot_observed_at":"2026-08-11T01:29:31.390601Z","submitted_at":"2026-05-09T08:03:03Z","title":"Chasing the neutrino blazar candidates II: SED modeling with hadronic model","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-12T01:35:20.923291Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.08775"},"observation_digest":"sha256:543c3def4e80843ee49b81ca1ef107e86684ea2f7e9a59fca121485908fa7c89","observation_id":"e9be9446-e2b5-4e9c-abd6-a43a71d727c3","resolution":{"observed_at":"2026-05-12T01:36:14.118507Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.11083","last_updated":"2026-05-13T07:25:34Z","snapshot_observed_at":"2026-08-02T20:20:51.304949Z","submitted_at":"2026-05-11T18:00:10Z","title":"FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-05-13T01:06:12.360464Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.11083"},"observation_digest":"sha256:2b98b651eceb2fce874456571d7d90db135962222239b1cab4d1a64301b2b3eb","observation_id":"238ebcd8-3cd1-4c5e-ada7-4caf34392476","resolution":{"observed_at":"2026-05-13T01:06:59.886010Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.11083","last_updated":"2026-05-13T07:25:34Z","snapshot_observed_at":"2026-08-02T20:20:51.304949Z","submitted_at":"2026-05-11T18:00:10Z","title":"FLAMINGO: The thermal history of the Universe from tSZ effect cross-correlations and its dependencies on cosmology and baryon physics","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.11083"},"observation_digest":"sha256:cf67bd9af5d27d8fc584dac0502b06a727038dd0db92d98eec287ecb3af8c20e","observation_id":"2e0eb9a2-b27e-4c5b-adfe-6c0b64789440","resolution":{"observed_at":"2026-05-14T21:07:58.076529Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.11370","last_updated":"2026-05-12T00:48:34Z","snapshot_observed_at":"2026-08-11T14:31:28.300742Z","submitted_at":"2026-05-12T00:48:34Z","title":"Transonic accretion and the analogue gravity in multi-component elliptical galaxies hosting pseudo-Schwarzschild black holes","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-05-13T02:25:04.077026Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.11370"},"observation_digest":"sha256:753ad79728fc8396449f4daba47191e7efd2feee3d817282f74ece80245958ee","observation_id":"5e780e3f-61fc-4c18-9c5b-4b9cb40949ea","resolution":{"observed_at":"2026-05-13T02:27:06.458488Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.12599","last_updated":"2026-05-12T18:00:03Z","snapshot_observed_at":"2026-08-11T13:39:11.248654Z","submitted_at":"2026-05-12T18:00:03Z","title":"One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.12599"},"observation_digest":"sha256:0409cf6bf75011881fda7c583af78893c52bd9245941f70fc6cbf4384644e870","observation_id":"624380cf-900b-4aa8-88b3-696d030faed8","resolution":{"observed_at":"2026-05-14T20:47:57.279264Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.14128","last_updated":"2026-05-13T21:27:59Z","snapshot_observed_at":"2026-08-11T17:02:21.391194Z","submitted_at":"2026-05-13T21:27:59Z","title":"Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-15T02:10:02.249132Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.14128"},"observation_digest":"sha256:90be02ad4fbea6ad4c10f80a8dbf3ce18b44033e692eb6431004c3fce339b5bc","observation_id":"004cc843-9fc4-4d4a-a91e-52958c2e314e","resolution":{"observed_at":"2026-05-15T02:13:29.778057Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.15275","last_updated":"2026-05-14T18:00:03Z","snapshot_observed_at":"2026-07-06T23:26:37.362117Z","submitted_at":"2026-05-14T18:00:03Z","title":"The Simulated Oxygen Shortage (SOS): Mapping the Missing OVI in Simulated Dwarf Galaxies to Subgrid Physics","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.15275"},"observation_digest":"sha256:87708ae455af8273b46d3c0bd4f3a56ce2d2f060fa8c28d2484d9a884d7819de","observation_id":"ea36de5e-aeaf-4ed6-be4a-f5d440f0899d","resolution":{"observed_at":"2026-05-19T15:47:38.374571Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.17040","last_updated":"2026-07-20T15:48:43Z","snapshot_observed_at":"2026-08-10T22:29:32.789186Z","submitted_at":"2026-05-16T15:21:05Z","title":"PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.17040"},"observation_digest":"sha256:05a2c3584d113d969abf71c6686d2bbef124a719eb59f1128c13aea8a81f743d","observation_id":"536681d7-0bea-4636-8134-e06d15ea4af5","resolution":{"observed_at":"2026-05-20T15:38:26.219286Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.23489","last_updated":"2026-05-22T10:51:03Z","snapshot_observed_at":"2026-08-02T00:51:08.034872Z","submitted_at":"2026-05-22T10:51:03Z","title":"A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz","version":1},"reference_index":270,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.23489"},"observation_digest":"sha256:564b3fc90eb2cd3b1efdbce0286530ebafa5d960035ec29e80a007dff9decac0","observation_id":"7fb8a4a5-8dc6-4c58-884a-0973d4165795","resolution":{"observed_at":"2026-05-25T03:56:35.752064Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.23746","last_updated":"2026-05-22T15:20:11Z","snapshot_observed_at":"2026-08-02T08:23:53.526666Z","submitted_at":"2026-05-22T15:20:11Z","title":"Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.23746"},"observation_digest":"sha256:1c621d17afa52f882aeda298b32060ba27e7534ba6366ee942afee1865f7684e","observation_id":"b05722b1-8c2f-4196-bb10-ab52f912a17f","resolution":{"observed_at":"2026-05-25T03:35:17.684149Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2605.24429","last_updated":"2026-05-23T06:52:38Z","snapshot_observed_at":"2026-08-02T23:33:21.154084Z","submitted_at":"2026-05-23T06:52:38Z","title":"Changing-look Active Galactic Nuclei from SDSS, LAMOST and DESI Survey","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-06-30T13:25:30.436887Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2605.24429"},"observation_digest":"sha256:47916184634ee3c7bbd0aa46f3f32175027d9a8c9a80565c180f6cd0d48e9447","observation_id":"59eb35db-8786-4b67-8b67-597e548364de","resolution":{"observed_at":"2026-06-30T13:34:40.015474Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.00205","last_updated":"2026-05-29T18:00:00Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-29T18:00:00Z","title":"Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages","version":1},"reference_index":133,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.00205"},"observation_digest":"sha256:be0126b010d68f455e73e226cc3797a631afb92d8e35f7bc7144f3bfa733ddc5","observation_id":"ceacd153-4179-4aec-b56c-45dde439f67f","resolution":{"observed_at":"2026-06-28T21:52:40.169975Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.01775","last_updated":"2026-06-01T06:58:26Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-01T06:58:26Z","title":"Reconnection-Driven Injection and Stochastic Reacceleration during Cosmological Magnetogenesis","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-06-28T13:45:09.551932Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.01775"},"observation_digest":"sha256:e671ecf995a49a86126a7ea8e9c75a59a554fc0dbdc172ba3d7f057c6859dc41","observation_id":"abcaf812-72fd-4e50-835b-4518baf92532","resolution":{"observed_at":"2026-06-28T14:42:18.465028Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.02566","last_updated":"2026-06-01T17:55:45Z","snapshot_observed_at":"2026-07-06T23:42:58.036516Z","submitted_at":"2026-06-01T17:55:45Z","title":"Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-28T13:54:30.765345Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.02566"},"observation_digest":"sha256:2730a8e218c9fb2ff7f5d6b157bbc2985a299b07f38845dce62f59a23ecb74f9","observation_id":"08c7248f-cc53-41ce-9d0f-d8251573dfac","resolution":{"observed_at":"2026-06-28T14:02:17.279088Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.05005","last_updated":"2026-06-03T15:26:36Z","snapshot_observed_at":"2026-07-06T23:45:02.342193Z","submitted_at":"2026-06-03T15:26:36Z","title":"Neutrino mass constraints in interacting dark energy models after DESI DR2","version":1},"reference_index":170,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:4a3b5094a75318789f5b55ffad4a2207da48418e7072a4afcacdb1acc0a42242","observation_id":"e91783fa-f316-4126-9166-eb6930f53195","resolution":{"observed_at":"2026-07-02T10:56:52.525872Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.05323","last_updated":"2026-06-03T18:09:59Z","snapshot_observed_at":"2026-08-09T05:42:05.099605Z","submitted_at":"2026-06-03T18:09:59Z","title":"Strong [OIII]$+$H$\\beta$ emitters dominated the ionizing budget at $z\\sim7$","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-28T05:02:43.589726Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.05323"},"observation_digest":"sha256:9a4dc8a5ecd98930a3fcb6659012ff5c4428489b46eb4b50462d964ee5321431","observation_id":"c82664df-92fc-4128-9293-0531f3323d7e","resolution":{"observed_at":"2026-06-28T06:01:41.247947Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.05853","last_updated":"2026-06-04T08:27:25Z","snapshot_observed_at":"2026-08-01T21:34:07.002669Z","submitted_at":"2026-06-04T08:27:25Z","title":"Reconstructing dark energy with fewer assumptions","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-06-28T00:07:32.911711Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.05853"},"observation_digest":"sha256:b9fe5f8c59904dba030adcb5df8ee508182183bdb83f19401fbe30788d782abd","observation_id":"aae19247-7f40-4613-a447-1bf63f61a604","resolution":{"observed_at":"2026-07-02T14:57:04.210636Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.09997","last_updated":"2026-06-08T18:00:04Z","snapshot_observed_at":"2026-08-04T22:55:21.549658Z","submitted_at":"2026-06-08T18:00:04Z","title":"A universal model for the accretion rates and formation times of dark matter halos","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-06-27T15:34:25.812471Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.09997"},"observation_digest":"sha256:340523b790d447cca8fc08e5be7b86a8995af3bdf948826304eb5447cfefeb4b","observation_id":"0e7c33a6-402d-4ac9-b570-48a1eabff4af","resolution":{"observed_at":"2026-06-27T15:41:01.380155Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.17145","last_updated":"2026-06-15T18:00:02Z","snapshot_observed_at":"2026-08-12T07:59:50.896970Z","submitted_at":"2026-06-15T18:00:02Z","title":"OpenGadget3 GPU solver tests","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.17145"},"observation_digest":"sha256:c1c8af9bf73008a32812042d2719b42893673173ed4d25d8873b563eed995c15","observation_id":"7a6fe1a2-833f-46d1-aaf0-d620c01102fb","resolution":{"observed_at":"2026-06-27T02:50:23.863827Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.19104","last_updated":"2026-06-17T14:17:18Z","snapshot_observed_at":"2026-08-06T13:21:21.913983Z","submitted_at":"2026-06-17T14:17:18Z","title":"PHANTOM: A MATLAB and Octave Toolbox Connecting Linear Field Statistics to Dark Matter Halo Observables","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-06-26T19:45:14.793850Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.19104"},"observation_digest":"sha256:178cc9e190f4cf350cec6334c5a95ddade29d93c63fe68539f134bfbc5bd080b","observation_id":"444015fd-4640-47ba-bf4a-55d646fa17b5","resolution":{"observed_at":"2026-06-26T19:49:50.415831Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.19459","last_updated":"2026-06-17T18:01:12Z","snapshot_observed_at":"2026-08-03T04:16:59.150089Z","submitted_at":"2026-06-17T18:01:12Z","title":"Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-06-26T19:37:19.656550Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.19459"},"observation_digest":"sha256:f9c107eed9075a9c5fbb9939698e301c55bcb0e7100125bceb8583e5f66f7f76","observation_id":"81e07216-b1d9-4d05-b8f0-cce45bae0a4d","resolution":{"observed_at":"2026-06-26T19:39:50.573650Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.20175","last_updated":"2026-06-18T12:44:30Z","snapshot_observed_at":"2026-08-05T04:01:18.497219Z","submitted_at":"2026-06-18T12:44:30Z","title":"A Consistent Comparison of Intracluster Light Assembly in Simulations I. Redshift Evolution and Progenitor Galaxies","version":1},"reference_index":105,"source":"arxiv_source","source_observed_at":"2026-06-26T16:52:24.672846Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.20175"},"observation_digest":"sha256:73e956e2b3a8a62d9f0dbdc6417136377d55593368bf77a307b09e87c4c49e64","observation_id":"893b62de-9b9a-4d6f-ac0a-1c6d351894e0","resolution":{"observed_at":"2026-06-26T16:59:36.363066Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.22431","last_updated":"2026-06-21T10:44:26Z","snapshot_observed_at":"2026-08-08T10:46:01.971731Z","submitted_at":"2026-06-21T10:44:26Z","title":"An Interplay Between Fractional Calculus and Holographic Dark Energy","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-06-26T10:12:54.212718Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.22431"},"observation_digest":"sha256:9f2f224fd3b090f98c67a759b8669f1cb7962da71edc509d05235670a2fe0a79","observation_id":"8298524d-8fc9-43b8-8ce6-11c10bd11af8","resolution":{"observed_at":"2026-06-26T10:19:18.790573Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.23798","last_updated":"2026-06-22T18:00:04Z","snapshot_observed_at":"2026-08-04T20:08:29.004762Z","submitted_at":"2026-06-22T18:00:04Z","title":"The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-06-26T07:50:38.631331Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.23798"},"observation_digest":"sha256:15663310cddd76efb2a5e82ed6efa5c869e5292aaa40da16a9774d3beea670d9","observation_id":"1f691b3b-8a5e-453e-9246-848fe72a71a1","resolution":{"observed_at":"2026-06-26T09:09:16.730081Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.26445","last_updated":"2026-06-24T23:14:13Z","snapshot_observed_at":"2026-08-02T06:35:29.874763Z","submitted_at":"2026-06-24T23:14:13Z","title":"Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium","version":1},"reference_index":151,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.26445"},"observation_digest":"sha256:5945d707cf2464f9f849eb96c26600918fdf73f3c2803781dc86c7808dd0dac0","observation_id":"5f19173d-8483-4f80-b2fa-73cfa815dfd7","resolution":{"observed_at":"2026-06-27T01:00:20.757567Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.27021","last_updated":"2026-06-25T13:32:47Z","snapshot_observed_at":"2026-07-07T00:01:15.803410Z","submitted_at":"2026-06-25T13:32:47Z","title":"SMR: Scheduler with Multi-Channel Map-Encoded Reinforcement Learning for Radio Telescopes","version":1},"reference_index":128,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.27021"},"observation_digest":"sha256:87686f9b05525b6295e8b568c48482d11e9393b01eed134c1c0079ab17efac46","observation_id":"a6c95ff0-b7fc-42f2-8de0-3f06840cc437","resolution":{"observed_at":"2026-06-26T03:08:56.579885Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2606.30719","last_updated":"2026-06-29T18:00:01Z","snapshot_observed_at":"2026-07-07T00:04:34.491408Z","submitted_at":"2026-06-29T18:00:01Z","title":"Global trends in morphology from massive to dwarf galaxies","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-01T02:06:55.056595Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2606.30719"},"observation_digest":"sha256:d38b824505bd29d467c26d4661c57f6b8902163582b2fe42539d4ac1e7546da5","observation_id":"24651481-9d54-4a49-ad0b-7d65b1d3cad2","resolution":{"observed_at":"2026-07-01T02:55:18.951364Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2607.01177","last_updated":"2026-07-01T17:08:22Z","snapshot_observed_at":"2026-07-07T00:06:44.379624Z","submitted_at":"2026-07-01T17:08:22Z","title":"Preheating and oscillon formation in Einstein-scalar-Gauss-Bonnet gravity","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-02T08:19:59.728866Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.01177"},"observation_digest":"sha256:7bf92af495044a1dacb82e8423e1ff5561ba4875f0d449c84f91d6b7024d57ce","observation_id":"ec0ae1a7-a985-48fb-a813-2c991c0bdb17","resolution":{"observed_at":"2026-07-02T08:26:47.615670Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-12T07:56:00.734481Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.02654","last_updated":"2026-07-02T18:00:01Z","snapshot_observed_at":"2026-08-02T08:48:50.697615Z","submitted_at":"2026-07-02T18:00:01Z","title":"The youth of the intracluster medium. I. A non-parametric characterisation of the gas and electron number density profiles of $z \\simeq 2$ protoclusters","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-12T07:56:00.734481Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.02654"},"observation_digest":"sha256:f88d238a3a3bb4dbb7c5079fe6360a19a26e5bfd31fdf1979df3161ade1a5d43","observation_id":"22bd147c-501f-4fd4-b63d-16787a179d83","resolution":{"observed_at":"2026-07-12T07:56:00.734481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2607.06112","last_updated":"2026-07-07T10:22:33Z","snapshot_observed_at":"2026-08-03T04:30:54.160026Z","submitted_at":"2026-07-07T10:22:33Z","title":"Starobinsky Inflation in k-Essence Framework: Attractor Dynamics, Reheating, and Consistency with ACT DR6","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-08T16:33:14.129159Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.06112"},"observation_digest":"sha256:6f52542e61b8bded67be413e47535d5b2577dae6d998e35759f18b52268bc177","observation_id":"f0cf5f1a-b3c8-4eb6-a5df-e4feba1e94d5","resolution":{"observed_at":"2026-07-08T16:35:10.096446Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2607.06933","last_updated":"2026-07-08T02:52:51Z","snapshot_observed_at":"2026-08-02T14:02:00.881352Z","submitted_at":"2026-07-08T02:52:51Z","title":"Constructing a Mock Galaxy Catalog for the All-sky SPECtroscopic Survey of Nearby Galaxies (A-SPEC) Using the Machine-assisted Semi-Simulation Model","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-09T22:50:50.117291Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.06933"},"observation_digest":"sha256:524b2e40528763216970b67b65b405b48fab6ff17c185deec1a6e90e0af459f1","observation_id":"bb9d3dbd-c63a-4d4e-bf8b-5ad8fc31486d","resolution":{"observed_at":"2026-07-09T22:56:37.382760Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2607.07476","last_updated":"2026-07-08T14:38:12Z","snapshot_observed_at":"2026-08-07T07:41:34.280749Z","submitted_at":"2026-07-08T14:38:12Z","title":"First Demonstration of a Hybrid Cherenkov and Scintillation Detector in a Proof-of-Principle Axion Search at a Beam Dump","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.07476"},"observation_digest":"sha256:e6eab4ce15172d10aaa94265a6f8a0cd676afbc4e0e2862e5ace46379f0c5cbf","observation_id":"c7a1f6b3-84e2-45cd-a6d9-cd09ba9d48cb","resolution":{"observed_at":"2026-07-09T09:56:10.115342Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":"1001.4538","doi":"10.1088/0067-0049/192/2/18","metadata_source":"doi_reference","pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","venue":"astro-ph.CO","work_id":"bc0d9ff3-7bb4-4fc3-a649-2461f4e24142","year":2011},"citing_paper":{"arxiv_id":"2607.07610","last_updated":"2026-07-08T16:28:32Z","snapshot_observed_at":"2026-08-02T06:49:42.238535Z","submitted_at":"2026-07-08T16:28:32Z","title":"Gamma-ray bursts reveal the history and faint contributors of cosmic reionization","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-09T05:25:12.742172Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.07610"},"observation_digest":"sha256:ba1cf67422b758746c6938617d22d935ca10ccbea70b8bf954fdb3edaa000dfc","observation_id":"22e7adef-9725-4334-af38-e198136c872d","resolution":{"observed_at":"2026-07-09T05:26:01.712198Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T10:49:13.805271+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-07-13T04:41:12.165957Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09209","last_updated":"2026-07-10T08:56:40Z","snapshot_observed_at":"2026-08-01T19:30:08.283612Z","submitted_at":"2026-07-10T08:56:40Z","title":"Performance of morphological classifiers for galaxy mergers compared to current machine learning methods","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-13T04:41:12.165957Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.09209"},"observation_digest":"sha256:b6f05f1b8d44b6115706d7c984c757b2c291b8aea83f2e607cef114baed2ce92","observation_id":"e3aa9e34-949e-47e4-824b-cac798e0c9fc","resolution":{"observed_at":"2026-07-13T04:41:12.165957Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-02T00:36:14.133338Z","title":"Komatsu, K.M","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.14982","last_updated":"2026-07-16T13:35:45Z","snapshot_observed_at":"2026-08-09T21:46:07.384435Z","submitted_at":"2026-07-16T13:35:45Z","title":"Testing the Isotropy of the Universe with the CHIME/FRB Catalog I","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-02T00:36:14.133338Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.14982"},"observation_digest":"sha256:e78d3a74e8891fccce3013198a3b3294dfc196cc8319cfb4f3f44b29629d6ab2","observation_id":"0779d709-8569-4b94-b8a6-05e922cc5da7","resolution":{"observed_at":"2026-08-02T00:36:14.133338Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-01T22:12:34.713620Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15850","last_updated":"2026-07-17T11:08:01Z","snapshot_observed_at":"2026-08-06T20:42:12.266596Z","submitted_at":"2026-07-17T11:08:01Z","title":"Standard Reconstruction Shifts the Optimal Input Scale for CNN-Based Density-Field Reconstruction","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-01T22:12:34.713620Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2607.15850"},"observation_digest":"sha256:33cc097edf8395e0c4cdf5e55f04feb97345be9d04fd5ce9a7da682b20815bcd","observation_id":"0d559c5a-9616-41f3-bf30-bfa8079ef7eb","resolution":{"observed_at":"2026-08-01T22:12:34.713620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-08T16:24:48.371617Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.05281","last_updated":"2026-08-05T18:00:02Z","snapshot_observed_at":"2026-08-09T23:10:29.385260Z","submitted_at":"2026-08-05T18:00:02Z","title":"On the Origin of the Ly$\\alpha$ Damping Wing in Galaxies at $8\\le z \\le 10$: Explorations using the NINJA Simulations","version":1},"reference_index":271,"source":"arxiv_source","source_observed_at":"2026-08-08T16:24:48.371617Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2608.05281"},"observation_digest":"sha256:dffdfd749cd1ce4f3b67b8014805f4aa6b2cfba370302f7085c66fe66715c1b8","observation_id":"8260ff0b-83e5-4a88-8b4a-de194ea5838f","resolution":{"observed_at":"2026-08-08T16:24:48.371617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1001.4538","snapshot_observed_at":"2026-08-10T04:15:20.823925Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.06619","last_updated":"2026-08-06T22:10:11Z","snapshot_observed_at":"2026-08-12T12:11:25.025547Z","submitted_at":"2026-08-06T22:10:11Z","title":"Average soft X-ray surface brightness profile of massive galaxy clusters in Magneticum simulations","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-10T04:15:20.823925Z"},"links":{"cited_paper":"/paper/1001.4538","citing_paper":"/paper/2608.06619"},"observation_digest":"sha256:b4225c38d8d7980c0907d72bd68cd5ec13bbd46df24a7c30c92517d638f40b70","observation_id":"58b56c01-93fe-4460-a0db-6ba8d6d253ce","resolution":{"observed_at":"2026-08-10T04:15:20.823925Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1001.4538/citation-record","integrity":"/paper/1001.4538/integrity","json":"/paper/1001.4538/citation-record.json","paper":"/paper/1001.4538"},"outbound":[],"paper":{"arxiv_id":"1001.4538","last_updated":"2010-11-09T05:54:31Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:02:45.077111Z","submitted_at":"2010-01-25T21:24:29Z","title":"Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 74 inbound Pith citation observations for arXiv:1001.4538."}