{"as_of":"2026-08-20T01:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:14e4275651c12bc41a741b30d17b1bc4a1a696fbb2f29286c8147342e10c9d26","coverage":[{"denominator":45,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":45,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T04:19:29.699242Z","state":"measured"},{"denominator":46,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":46,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-20T21:32:19.408159Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-20T21:33:46.056054Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"cited_work":{"arxiv_id":"2602.05575","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2602.05575","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"32fb17b5-61ed-41ed-b095-bbf0c0d2521c","year":2026},"citing_paper":{"arxiv_id":"2605.12482","last_updated":"2026-05-16T20:11:42Z","snapshot_observed_at":"2026-08-11T09:39:54.485379Z","submitted_at":"2026-05-12T17:57:38Z","title":"Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-05-20T21:32:19.408159Z"},"links":{"cited_paper":"/paper/2602.05575","citing_paper":"/paper/2605.12482"},"observation_digest":"sha256:ae8870852845265a43204fe760b7652566d17422fca9e5fb33b8356ad7bc3c0c","observation_id":"587b5b25-816c-49d7-b898-8331681f5db7","resolution":{"observed_at":"2026-06-03T02:05:13.278423Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2602.05575/citation-record","integrity":"/paper/2602.05575/integrity","json":"/paper/2602.05575/citation-record.json","paper":"/paper/2602.05575"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9812133","last_updated":"1998-12-08T03:27:34Z","snapshot_observed_at":"2026-08-14T18:17:06.144059Z","submitted_at":"1998-12-08T03:27:34Z","title":"Measurements of Omega and Lambda from 42 High-Redshift Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9812133","snapshot_observed_at":"2026-08-03T04:19:26.301096Z","title":"Measurements of Ω and Λ from 42 High Redshift Supernovae,","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.301096Z"},"links":{"cited_paper":"/paper/astro-ph/9812133","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:2511232369ae2e93da6004ee44cad40536948c4a4914fd36ea3b29327f5da92f","observation_id":"08404f97-cd44-4de0-ad0e-95e0bede5ef1","resolution":{"observed_at":"2026-08-03T04:19:26.301096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-08-03T04:19:26.376073Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s −1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.376073Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:da4746634a8b93ea15ddb6d7ae3ab1615ab32484a0b4a528c6b20157a2b368c1","observation_id":"cd79b22e-cbd1-4827-b45d-2f5219e7d4de","resolution":{"observed_at":"2026-08-03T04:19:26.376073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-03T04:19:26.469364Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.469364Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:d2f9b0b6d76c7ad3a6ed45dbf01807ea6923952673e0799bbe2b89ec4696c6b3","observation_id":"0059f30e-204d-4ead-997d-6a78900b0ca7","resolution":{"observed_at":"2026-08-03T04:19:26.469364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.15633","last_updated":"2020-10-13T16:23:19Z","snapshot_observed_at":"2026-08-18T07:43:05.270334Z","submitted_at":"2020-07-30T17:54:56Z","title":"KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.15633","snapshot_observed_at":"2026-08-03T04:19:26.538817Z","title":"KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statis- tics,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.538817Z"},"links":{"cited_paper":"/paper/2007.15633","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:9492d1cc88b41386e195e0401cb985d404416ae2ef7bd60288d871b566eb1a02","observation_id":"3da439f1-57ab-4762-9293-51a0cbb7d150","resolution":{"observed_at":"2026-08-03T04:19:26.538817Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.07128","last_updated":"2022-03-14T14:22:40Z","snapshot_observed_at":"2026-08-16T17:14:47.127548Z","submitted_at":"2022-03-14T14:22:40Z","title":"Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.07128","snapshot_observed_at":"2026-08-03T04:19:26.604099Z","title":"Dark energy survey year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space,","venue":null,"work_id":null,"year":1942},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.604099Z"},"links":{"cited_paper":"/paper/2203.07128","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:9ad70343b9a65b0b0a7936ab455d44b6b632da5f0994c1bfb0e61854e28e48c7","observation_id":"9dab9629-6dba-4fc1-8e31-46510598ec12","resolution":{"observed_at":"2026-08-03T04:19:26.604099Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T04:19:26.696703Z","title":"A New Type of Isotropic Cosmological Models Without Singularity,","venue":null,"work_id":null,"year":1980},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.696703Z"},"links":{"citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:8d2f7852fc6c9f0e6b78e1d4384012f1d25d33be3b87d3e5c76e324e9a43c7ba","observation_id":"9e60a1c1-15b6-46fc-8e66-5abe7b081cf2","resolution":{"observed_at":"2026-08-03T04:19:26.696703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1002.4928","last_updated":"2010-06-23T15:13:49Z","snapshot_observed_at":"2026-08-15T05:25:28.959546Z","submitted_at":"2010-02-26T07:01:02Z","title":"f(R) theories","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1002.4928","snapshot_observed_at":"2026-08-03T04:19:26.793618Z","title":"f(R) theories,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.793618Z"},"links":{"cited_paper":"/paper/1002.4928","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:7e7cc91c51bdb806ecde6338435735d659594a92efeae8ea5c89149a8bec8d15","observation_id":"ba5ef9df-d3d6-48f1-bea0-c66e8bdb3ac2","resolution":{"observed_at":"2026-08-03T04:19:26.793618Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.08702","last_updated":"2017-12-14T18:01:01Z","snapshot_observed_at":"2026-08-16T11:39:14.492142Z","submitted_at":"2017-08-29T11:28:28Z","title":"Cosmic History of Chameleonic Dark Matter in $F(R)$ Gravity","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.08702","snapshot_observed_at":"2026-08-03T04:19:26.887323Z","title":"Cosmic History of Chameleonic Dark Matter inF(R) Gravity,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.887323Z"},"links":{"cited_paper":"/paper/1708.08702","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:86b0b1b5a0cbb0b0c57a6accb877db6238b2fa2b5c83501b984245b923bb8659","observation_id":"952ac073-ad8c-426f-a467-d3c81484fe99","resolution":{"observed_at":"2026-08-03T04:19:26.887323Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1726","last_updated":"2010-06-04T00:50:27Z","snapshot_observed_at":"2026-08-17T15:19:12.963977Z","submitted_at":"2008-05-12T19:44:15Z","title":"f(R) Theories Of Gravity","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.1726","snapshot_observed_at":"2026-08-03T04:19:26.994191Z","title":"f(R) Theories Of Gravity,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.994191Z"},"links":{"cited_paper":"/paper/0805.1726","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:4cbf95f326fdc018b5a06951872a20f796c21371e4a543a55894dc9dd69267c8","observation_id":"193da6f7-acc9-4626-9615-025c461e94e4","resolution":{"observed_at":"2026-08-03T04:19:26.994191Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0601213","last_updated":"2006-03-31T03:39:12Z","snapshot_observed_at":"2026-08-15T22:15:45.230199Z","submitted_at":"2006-01-29T22:31:37Z","title":"Introduction to Modified Gravity and Gravitational Alternative for Dark Energy","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"hep-th/0601213","snapshot_observed_at":"2026-08-03T04:19:27.092871Z","title":"Introduction to modified gravity and gravitational alternative for dark energy,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.092871Z"},"links":{"cited_paper":"/paper/hep-th/0601213","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:2039de392814dce39e2fd2d66d0cd7594aa8d200e407540c5dd95a188099984a","observation_id":"c626b181-c32b-4bbf-a5fe-9bb943b15369","resolution":{"observed_at":"2026-08-03T04:19:27.092871Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.5276","last_updated":"2013-11-30T13:20:53Z","snapshot_observed_at":"2026-08-15T00:09:45.489359Z","submitted_at":"2013-07-19T16:38:22Z","title":"Parametrized modified gravity constraints after Planck","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.5276","snapshot_observed_at":"2026-08-03T04:19:27.192161Z","title":"Parametrized modified gravity constraints after Planck,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.192161Z"},"links":{"cited_paper":"/paper/1307.5276","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:0904542430a903ad2078cf87c29c42d8f081a8ab3d2f497b34b8a4826c09f79a","observation_id":"90d00d9c-590c-4979-8fa4-2579b57ce483","resolution":{"observed_at":"2026-08-03T04:19:27.192161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.3009","last_updated":"2011-04-11T16:20:38Z","snapshot_observed_at":"2026-08-15T05:24:08.146505Z","submitted_at":"2010-03-15T19:53:23Z","title":"Constraints on f(R) gravity from probing the large-scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.3009","snapshot_observed_at":"2026-08-03T04:19:27.273032Z","title":"Constraints on f(R) gravity from probing the large-scale structure,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.273032Z"},"links":{"cited_paper":"/paper/1003.3009","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:1e33e37ea02825aa0933886bbfd9c0b1be510e248c72b2474e70ba9f0e4f575c","observation_id":"e82860d4-f681-4e7a-8af1-0a8e2450353b","resolution":{"observed_at":"2026-08-03T04:19:27.273032Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05976","last_updated":"2018-06-14T19:36:36Z","snapshot_observed_at":"2026-08-18T05:59:19.726871Z","submitted_at":"2017-12-16T15:44:45Z","title":"Do cosmological data rule out $f(\\mathcal{R})$ with $w\\neq-1$?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1712.05976","snapshot_observed_at":"2026-08-03T04:19:27.361591Z","title":"Do cosmological data rule outf(R) withw̸=−1?","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.361591Z"},"links":{"cited_paper":"/paper/1712.05976","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:c5049cb4611dbe8fe3187b9895c9d2b50ce5df6e9b24a1ab737dd5775e2f6671","observation_id":"b6ac1e4f-3e26-4b8c-8e9d-9a4a445fea31","resolution":{"observed_at":"2026-08-03T04:19:27.361591Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1401.3980","last_updated":"2014-04-07T05:57:35Z","snapshot_observed_at":"2026-08-14T23:48:10.028954Z","submitted_at":"2014-01-16T10:43:36Z","title":"Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1401.3980","snapshot_observed_at":"2026-08-03T04:19:27.456847Z","title":"Constraining models of f(R) gravity with Planck and WiggleZ power spectrum data,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.456847Z"},"links":{"cited_paper":"/paper/1401.3980","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:6001f386d976664aee3cde76526e7b37197c84d0e4834fb40b61d83f74e78cab","observation_id":"b9810deb-64eb-4669-b70d-bb491f3d09dd","resolution":{"observed_at":"2026-08-03T04:19:27.456847Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.0133","last_updated":"2015-08-08T11:33:22Z","snapshot_observed_at":"2026-08-14T23:09:40.704278Z","submitted_at":"2014-11-29T18:12:04Z","title":"New constraints on $f(R)$ gravity from clusters of galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.0133","snapshot_observed_at":"2026-08-03T04:19:27.553088Z","title":"New constraints onf(R) gravity from clusters of galaxies,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.553088Z"},"links":{"cited_paper":"/paper/1412.0133","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:3b5cfc17cedf198005fef22d0523aeea7ce7e2d3cbb3c713504806069d8c8be5","observation_id":"d2c50d2f-ea31-4cb9-98ad-d1258a847a7d","resolution":{"observed_at":"2026-08-03T04:19:27.553088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01136","last_updated":"2015-03-29T22:29:13Z","snapshot_observed_at":"2026-08-14T23:01:27.119700Z","submitted_at":"2015-02-04T09:24:23Z","title":"Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01136","snapshot_observed_at":"2026-08-03T04:19:27.619280Z","title":"Probingf(R) cosmology with sterile neutrinos via measurements of scale- dependent growth rate of structure,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.619280Z"},"links":{"cited_paper":"/paper/1502.01136","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:53b9e06d82cabbdbbe3db63574e154bbb88e8c800cd6524a8d210f0079fbf5e4","observation_id":"5528f5f6-b09b-4eab-b5c8-426e94a0353b","resolution":{"observed_at":"2026-08-03T04:19:27.619280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.0728","last_updated":"2013-03-25T14:13:04Z","snapshot_observed_at":"2026-08-15T00:37:11.724423Z","submitted_at":"2012-12-04T14:10:48Z","title":"Testing General Relativity with 21 cm intensity mapping","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.0728","snapshot_observed_at":"2026-08-03T04:19:27.686651Z","title":"Testing General Relativity with 21-cm intensity mapping,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.686651Z"},"links":{"cited_paper":"/paper/1212.0728","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:0c9c43a26ac8c0d86995edb1402f8e8f41bf4222214c634b894379cf4476080a","observation_id":"7647844c-c364-4285-a876-8c3083bfd96b","resolution":{"observed_at":"2026-08-03T04:19:27.686651Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401340","last_updated":"2004-01-16T14:19:04Z","snapshot_observed_at":"2026-08-19T23:42:13.144697Z","submitted_at":"2004-01-16T14:19:04Z","title":"Neutral hydrogen surveys for high redshift galaxy clusters and proto-clusters","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401340","snapshot_observed_at":"2026-08-03T04:19:27.764846Z","title":"Neutral hydrogen surveys for high redshift galaxy clusters and proto-clusters,","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.764846Z"},"links":{"cited_paper":"/paper/astro-ph/0401340","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:739a24f50b354973dd669ddc6c58fab373bec56841d588dc71f52562954cee1d","observation_id":"a2412f4d-7900-4cee-93d4-549ecc10f043","resolution":{"observed_at":"2026-08-03T04:19:27.764846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9608010","last_updated":"1996-08-01T21:42:55Z","snapshot_observed_at":"2026-08-15T20:17:14.292207Z","submitted_at":"1996-08-01T21:42:55Z","title":"21-cm Tomography of the Intergalactic Medium at High Redshift","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9608010","snapshot_observed_at":"2026-08-03T04:19:27.835512Z","title":"21-CM tomography of the intergalactic medium at high redshift,","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.835512Z"},"links":{"cited_paper":"/paper/astro-ph/9608010","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:1ed72fd774d245fd82ae9aa46c8b5b40811d51b030ffb4b0ef79bf2612d926dc","observation_id":"3aab425f-5e33-4955-9ac3-be7184d66214","resolution":{"observed_at":"2026-08-03T04:19:27.835512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1511.01131","last_updated":"2015-11-03T21:58:00Z","snapshot_observed_at":"2026-08-14T22:24:58.428847Z","submitted_at":"2015-11-03T21:58:00Z","title":"The 21-cm Line as a Probe of Reionization","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1511.01131","snapshot_observed_at":"2026-08-03T04:19:27.907029Z","title":"The 21-cm Line as a Probe of Reionization,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:27.907029Z"},"links":{"cited_paper":"/paper/1511.01131","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:a12a20a4a67ece5c2159c29d7b86b568208dae976a4a55cf875e2cd7e85d7e71","observation_id":"bcd9094c-7723-42e1-8737-fef2e1fe9638","resolution":{"observed_at":"2026-08-03T04:19:27.907029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.12595","last_updated":"2019-09-27T10:15:55Z","snapshot_observed_at":"2026-08-11T21:52:15.349311Z","submitted_at":"2019-09-27T10:15:55Z","title":"Astrophysics from the 21-cm background","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.12595","snapshot_observed_at":"2026-08-03T04:19:28.009075Z","title":"Astrophysics from the 21-cm background,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.009075Z"},"links":{"cited_paper":"/paper/1909.12595","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:c7511db7eb73cb65835e4d062906277988a43ef933c43f9f375d39d1d0ffb62e","observation_id":"be4d57f6-b428-4217-8a67-543e5d673a6d","resolution":{"observed_at":"2026-08-03T04:19:28.009075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01633","last_updated":"2021-10-12T14:27:25Z","snapshot_observed_at":"2026-08-16T18:12:28.763375Z","submitted_at":"2021-07-04T14:06:48Z","title":"The BINGO Project I: Baryon Acoustic Oscillations from Integrated Neutral Gas Observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01633","snapshot_observed_at":"2026-08-03T04:19:28.131594Z","title":"The BINGO project - I. Baryon acoustic oscillations from integrated neutral gas observations,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.131594Z"},"links":{"cited_paper":"/paper/2107.01633","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:7f95999069efd144b272dac1205d0b083507e9f8cac02bb90527b76cc2216a0b","observation_id":"d519590d-93d5-4702-bb17-ef91d3085b98","resolution":{"observed_at":"2026-08-03T04:19:28.131594Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01634","last_updated":"2021-12-13T20:33:35Z","snapshot_observed_at":"2026-08-16T18:12:29.129362Z","submitted_at":"2021-07-04T14:06:49Z","title":"The BINGO Project II: Instrument Description","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01634","snapshot_observed_at":"2026-08-03T04:19:28.231797Z","title":"The BINGO project - II. Instrument description,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.231797Z"},"links":{"cited_paper":"/paper/2107.01634","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:2f5cb51ea630c224314cab6a8cd0f588770483453522e90f5faacbef90e91ca5","observation_id":"42275813-7143-4297-b03d-32add3f6f424","resolution":{"observed_at":"2026-08-03T04:19:28.231797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01635","last_updated":"2022-03-18T15:05:24Z","snapshot_observed_at":"2026-08-16T18:12:28.375298Z","submitted_at":"2021-07-04T14:06:50Z","title":"The BINGO Project III: Optical design and optimisation of the focal plane","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01635","snapshot_observed_at":"2026-08-03T04:19:28.350724Z","title":"The BINGO Project - III. Optical design and optimization of the focal plane,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.350724Z"},"links":{"cited_paper":"/paper/2107.01635","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:91f89def7fc028999fae32523da5149f8ca98abd9522eb21789fed09b21a1502","observation_id":"1b4c1c4e-997c-4ebe-84f6-33a2cb2bfed7","resolution":{"observed_at":"2026-08-03T04:19:28.350724Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01636","last_updated":"2021-10-14T11:02:11Z","snapshot_observed_at":"2026-08-16T18:12:28.661119Z","submitted_at":"2021-07-04T14:06:51Z","title":"The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01636","snapshot_observed_at":"2026-08-03T04:19:28.452394Z","title":"The BINGO project - IV. Simulations for mission performance assessment and preliminary component separation steps,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.452394Z"},"links":{"cited_paper":"/paper/2107.01636","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:5c4283ee4b5d25b16ec0d3dbd303782e8f03d0d24a42ff52454d769abb433436","observation_id":"474be6ba-93a5-459c-a149-27e373ddf91e","resolution":{"observed_at":"2026-08-03T04:19:28.452394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01637","last_updated":"2022-04-01T06:01:14Z","snapshot_observed_at":"2026-08-16T18:12:28.571647Z","submitted_at":"2021-07-04T14:06:52Z","title":"The BINGO Project V: Further steps in Component Separation and Bispectrum Analysis","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01637","snapshot_observed_at":"2026-08-03T04:19:28.549040Z","title":"The BINGO project - V. Further steps in component separation and bispectrum analysis,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.549040Z"},"links":{"cited_paper":"/paper/2107.01637","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:27f1615c55a7f1a985fa29205b2ef9df44ddd61f07507dd4552f5c48ad845a3f","observation_id":"19094bc2-a008-4669-a449-a285f39c3e8d","resolution":{"observed_at":"2026-08-03T04:19:28.549040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01638","last_updated":"2021-07-04T14:06:53Z","snapshot_observed_at":"2026-08-16T18:12:28.386489Z","submitted_at":"2021-07-04T14:06:53Z","title":"The BINGO Project VI: HI Halo Occupation Distribution and Mock Building","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01638","snapshot_observed_at":"2026-08-03T04:19:28.644180Z","title":"The BINGO project - VI. HI halo occupation distribution and mock building,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.644180Z"},"links":{"cited_paper":"/paper/2107.01638","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:66b45b4b8329ab6cb1875790a6de70e5f957fbafb36f7db27e6900daa31115c8","observation_id":"2984650b-bd6a-4b20-bbcc-20979d4ed80b","resolution":{"observed_at":"2026-08-03T04:19:28.644180Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01639","last_updated":"2021-12-13T14:08:42Z","snapshot_observed_at":"2026-08-16T18:12:28.271989Z","submitted_at":"2021-07-04T14:06:54Z","title":"The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.01639","snapshot_observed_at":"2026-08-03T04:19:28.700942Z","title":"The BINGO project - VII. Cosmological forecasts from 21 cm intensity mapping,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.700942Z"},"links":{"cited_paper":"/paper/2107.01639","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:60210b3d9fde98494e5fb39ab013802754e56b4f1e2e61d4aab22bc6d11aedb0","observation_id":"fade4bec-7e71-475e-b5f2-72249673c6b9","resolution":{"observed_at":"2026-08-03T04:19:28.700942Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.06805","last_updated":"2023-11-02T16:29:35Z","snapshot_observed_at":"2026-08-18T04:16:52.903465Z","submitted_at":"2023-08-13T16:32:21Z","title":"The BINGO Project IX: Search for Fast Radio Bursts -- A Forecast for the BINGO Interferometry System","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.06805","snapshot_observed_at":"2026-08-03T04:19:28.746924Z","title":"The BINGO Project - IX. Search for fast radio bursts – A forecast for the BINGO interferometry system,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.746924Z"},"links":{"cited_paper":"/paper/2308.06805","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:d9dea6dafa243eb672f459f03c4cf87f325a8cc79940a0045249c723fd44003a","observation_id":"67cb2dc1-2aed-4b26-b749-f6566b953f39","resolution":{"observed_at":"2026-08-03T04:19:28.746924Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T04:19:28.802183Z","title":"The BINGO/ABDUS Project: Forecast for Cosmological Parameters from a Mock Fast Radio Burst Survey,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.802183Z"},"links":{"citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:b6d78f733441f0acb3d55d9109eb7b81215a6bf980649cb0affe0d8d21e10b89","observation_id":"8e48ecd8-d30c-4e0b-90c9-066d2a1a4cc2","resolution":{"observed_at":"2026-08-03T04:19:28.802183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02743","last_updated":"2018-11-07T03:12:27Z","snapshot_observed_at":"2026-08-19T13:26:57.386753Z","submitted_at":"2018-11-07T03:12:27Z","title":"Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.02743","snapshot_observed_at":"2026-08-03T04:19:28.857174Z","title":"Cosmology with Phase 1 of the Square Kilometre Array: Red Book 2018: Technical specifications and performance forecasts,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.857174Z"},"links":{"cited_paper":"/paper/1811.02743","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:acda5ded038244aea537cbcd0535dee48ceccb156be75dc4db2fa94c2f272127","observation_id":"5ea04ee6-e03b-4974-b312-4cc5918114cb","resolution":{"observed_at":"2026-08-03T04:19:28.857174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0610532","last_updated":"2007-01-15T01:03:20Z","snapshot_observed_at":"2026-08-15T10:59:52.551365Z","submitted_at":"2006-10-18T02:58:37Z","title":"The Large Scale Structure of f(R) Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0610532","snapshot_observed_at":"2026-08-03T04:19:28.922019Z","title":"The Large Scale Structure of f(R) Gravity,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.922019Z"},"links":{"cited_paper":"/paper/astro-ph/0610532","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:a6c6c255a9a95a04c50205ff984753f7f466d4cb3d904be568fd993a25b65774","observation_id":"b4ae756d-6806-471e-b5f6-7f3444db5eb5","resolution":{"observed_at":"2026-08-03T04:19:28.922019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.1158","last_updated":"2007-05-08T23:45:59Z","snapshot_observed_at":"2026-08-15T10:41:21.408621Z","submitted_at":"2007-05-08T23:45:59Z","title":"Models of f(R) Cosmic Acceleration that Evade Solar-System Tests","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.1158","snapshot_observed_at":"2026-08-03T04:19:28.978069Z","title":"Models of f(R) Cosmic Acceleration that Evade Solar-System Tests,","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:28.978069Z"},"links":{"cited_paper":"/paper/0705.1158","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:d991493721a53b86e516d551fe006f45c5098b534c3ebfd0900459797b77fc6a","observation_id":"01f90218-512e-497d-9b64-14e6319e8997","resolution":{"observed_at":"2026-08-03T04:19:28.978069Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-03T04:19:26.202827Z","title":"Here we want to focus on the effective anisotropy and the modified Poisson equations that generally describe the deflections of modified gravities from GR","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:26.202827Z"},"links":{"citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:a9e6ba68c0bd70ce94e5c5507d3af400948a6ef6b4c32fdbaa4cf92ea51df2e6","observation_id":"d6257623-033a-4cfa-9ea1-64e79262d467","resolution":{"observed_at":"2026-08-03T04:19:26.202827Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0709.0296","last_updated":"2010-01-16T21:14:11Z","snapshot_observed_at":"2026-08-15T10:33:01.086557Z","submitted_at":"2007-09-04T18:14:41Z","title":"The pattern of growth in viable f(R) cosmologies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0709.0296","snapshot_observed_at":"2026-08-03T04:19:29.067573Z","title":"The pattern of growth in viable f(R) cosmologies,","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.067573Z"},"links":{"cited_paper":"/paper/0709.0296","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:37c3c0de5d7eec97cc6357d011cf4fac9f6bd14b2a694ea86229a4d68ffc3e47","observation_id":"191f0256-85c7-4377-9381-cf5eb4fc6924","resolution":{"observed_at":"2026-08-03T04:19:29.067573Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.6880","last_updated":"2012-10-25T15:42:43Z","snapshot_observed_at":"2026-08-15T00:41:49.703417Z","submitted_at":"2012-10-25T15:42:43Z","title":"Practical solutions for perturbed f(R) gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.6880","snapshot_observed_at":"2026-08-03T04:19:29.149330Z","title":"Practical solutions for perturbed f(R) gravity,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.149330Z"},"links":{"cited_paper":"/paper/1210.6880","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:70e5a916478bc95111e524de243c5b04d212b5d35decb00178faa833a8e3a5b1","observation_id":"0c593486-d7a3-488f-a1e1-ccf1cc82a6a3","resolution":{"observed_at":"2026-08-03T04:19:29.149330Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1022","last_updated":"2014-11-19T10:30:04Z","snapshot_observed_at":"2026-08-14T23:35:11.345203Z","submitted_at":"2014-05-05T19:59:52Z","title":"Effective Field Theory of Cosmic Acceleration: constraining dark energy with CMB data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1022","snapshot_observed_at":"2026-08-03T04:19:29.208374Z","title":"Effective Field Theory of Cosmic Acceleration: constraining dark energy with CMB data,","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.208374Z"},"links":{"cited_paper":"/paper/1405.1022","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:fa5966c00f8d6799d37fb5603e456c595e99061a27095596c88542b7c7e20834","observation_id":"c7900519-4577-452f-86d7-e83e3df34b4a","resolution":{"observed_at":"2026-08-03T04:19:29.208374Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.05667","last_updated":"2023-08-16T09:13:07Z","snapshot_observed_at":"2026-08-16T15:34:22.757071Z","submitted_at":"2023-05-09T17:59:36Z","title":"New MGCAMB tests of gravity with CosmoMC and Cobaya","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05667","snapshot_observed_at":"2026-08-03T04:19:29.267168Z","title":"New MGCAMB tests of gravity with CosmoMC and Cobaya,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.267168Z"},"links":{"cited_paper":"/paper/2305.05667","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:03df04dc8dee2f1ed0812908ba63f3753749cad0b71847dc0a448adaa4c7456f","observation_id":"a41f7f4b-4250-42f2-ae10-21ca7628c350","resolution":{"observed_at":"2026-08-03T04:19:29.267168Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1106.4543","last_updated":"2011-07-23T12:01:53Z","snapshot_observed_at":"2026-08-15T04:43:10.430903Z","submitted_at":"2011-06-22T20:00:00Z","title":"Testing gravity with CAMB and CosmoMC","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1106.4543","snapshot_observed_at":"2026-08-03T04:19:29.330947Z","title":"Testing gravity with CAMB and CosmoMC,","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.330947Z"},"links":{"cited_paper":"/paper/1106.4543","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:44b3642d6f876622544f71b78aab39d7691519ee53fbdbf8221b35d18e6882f2","observation_id":"d9f0b5ca-f638-4f00-bd30-d8a0758894dd","resolution":{"observed_at":"2026-08-03T04:19:29.330947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0909.2045","last_updated":"2010-04-15T12:12:07Z","snapshot_observed_at":"2026-08-18T08:53:35.650655Z","submitted_at":"2009-09-11T11:46:05Z","title":"New constraints on parametrised modified gravity from correlations of the CMB with large scale structure","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0909.2045","snapshot_observed_at":"2026-08-03T04:19:29.410006Z","title":"New constraints on parametrised modified gravity from correlations of the CMB with large scale structure,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.410006Z"},"links":{"cited_paper":"/paper/0909.2045","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:a1976b964210de836212e4f09c188312927221134604767d9b85783d8c6c0dfd","observation_id":"fcbd5106-f893-4774-9a95-089627087c13","resolution":{"observed_at":"2026-08-03T04:19:29.410006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01796","last_updated":"2022-01-11T14:33:50Z","snapshot_observed_at":"2026-08-16T18:41:50.413112Z","submitted_at":"2021-03-02T15:07:21Z","title":"Forecasts on Interacting Dark Energy from 21-cm Angular Power Spectrum with BINGO and SKA observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01796","snapshot_observed_at":"2026-08-03T04:19:29.457239Z","title":"Forecasts on interacting dark energy from the 21-cm angular power spectrum with BINGO and SKA observations,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.457239Z"},"links":{"cited_paper":"/paper/2103.01796","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:a4d70d583f5f12ccdd7955058c03da620936d3e4e85bb2a1ecf19cf5dc453fe4","observation_id":"58eee00e-6e05-4ce4-906d-845fea67bbbf","resolution":{"observed_at":"2026-08-03T04:19:29.457239Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.12132","last_updated":"2019-07-28T19:48:00Z","snapshot_observed_at":"2026-08-14T16:01:26.350289Z","submitted_at":"2019-07-28T19:48:00Z","title":"Impact of $1/f$ noise on cosmological parameter constraints for SKA intensity mapping","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.12132","snapshot_observed_at":"2026-08-03T04:19:29.513132Z","title":"Impact of 1/fnoise on cosmological parameter constraints for SKA intensity mapping,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.513132Z"},"links":{"cited_paper":"/paper/1907.12132","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:47ee57e0459e22c3ef1d6fd6e88fa57293968e6bf8f571d406968fc57c7458c5","observation_id":"2a611e76-c5f3-4de8-af7f-699291ea0392","resolution":{"observed_at":"2026-08-03T04:19:29.513132Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1405.1452","last_updated":"2015-05-07T01:08:12Z","snapshot_observed_at":"2026-08-14T23:35:00.124999Z","submitted_at":"2014-05-06T20:46:41Z","title":"Late-time cosmology with 21cm intensity mapping experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1405.1452","snapshot_observed_at":"2026-08-03T04:19:29.572119Z","title":"Late-time cosmology with 21cm intensity mapping experiments,","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.572119Z"},"links":{"cited_paper":"/paper/1405.1452","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:fbbd1fa9464038420797080616b799fcd880e25a0d3dd871534ea45d4203c654","observation_id":"e830e3a1-9e84-41e8-b1ff-96048fcb021a","resolution":{"observed_at":"2026-08-03T04:19:29.572119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.3552","last_updated":"2010-02-12T19:04:40Z","snapshot_observed_at":"2026-08-15T05:33:36.820592Z","submitted_at":"2009-11-18T14:29:17Z","title":"Projected Constraints on Modified Gravity Cosmologies from 21 cm Intensity Mapping","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.3552","snapshot_observed_at":"2026-08-03T04:19:29.640031Z","title":"Projected Constraints on Modified Gravity Cosmologies from 21cm Intensity Mapping,","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.640031Z"},"links":{"cited_paper":"/paper/0911.3552","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:3e488e5af7a0088c25ba4b90fa3782de3e5f7300c3954839892373df06f12112","observation_id":"53d71e38-424e-4771-a194-c9d8c1adb980","resolution":{"observed_at":"2026-08-03T04:19:29.640031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.6487","last_updated":"2012-10-01T08:41:25Z","snapshot_observed_at":"2026-08-15T00:51:53.538833Z","submitted_at":"2012-07-27T08:30:43Z","title":"Recovering 3D clustering information with angular correlations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.6487","snapshot_observed_at":"2026-08-03T04:19:29.699242Z","title":"Recovering 3D clustering information with angular correlations,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-03T04:19:29.699242Z"},"links":{"cited_paper":"/paper/1207.6487","citing_paper":"/paper/2602.05575"},"observation_digest":"sha256:fc0c651c9aec88eb2f7c5aa75163035a04bcd3f8d7ce67db6c5c0d788bbed13a","observation_id":"c011fd6f-d6e0-4984-b19f-1eb0f7970054","resolution":{"observed_at":"2026-08-03T04:19:29.699242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2602.05575","last_updated":"2026-02-05T11:58:37Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-18T07:43:39.865871Z","submitted_at":"2026-02-05T11:58:37Z","title":"Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys"},"reference_resolution":{"displayed":45,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":45,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":45},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 45 of 45 outbound references and 1 inbound Pith citation observation for arXiv:2602.05575."}