{"as_of":"2026-08-11T01:24:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b3edc8cffce968b48a9ff42142deb5b5801aae44d8e480df60b10d1a0919ae16","coverage":[{"denominator":81,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":81,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":81,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":81,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2607.06346/citation-record","integrity":"/paper/2607.06346/integrity","json":"/paper/2607.06346/citation-record.json","paper":"/paper/2607.06346"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"0903.4895","last_updated":"2009-09-17T21:48:52Z","snapshot_observed_at":"2026-07-06T01:52:42.338116Z","submitted_at":"2009-03-27T20:03:05Z","title":"Residual Gas Motions in the Intracluster Medium and Bias in Hydrostatic Measurements of Mass Profiles of Clusters","version":2},"cited_work":{"arxiv_id":"0903.4895","doi":null,"metadata_source":"pith","pith_arxiv_id":"0903.4895","snapshot_observed_at":"2026-07-08T09:14:46.706325Z","title":"Residual Gas Motions in the Intracluster Medium and Bias in Hydrostatic Measurements of Mass Profiles of Clusters","venue":"astro-ph.CO","work_id":"06e3239b-00ca-4c82-9c4c-7ff8c4c56666","year":2009},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0903.4895","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:b2987263c8c6cbb14bd5baccf3d4db82bbff5711391c58dd662fb7aa6ba439ef","observation_id":"b983dd48-6c4c-4279-9644-da8f9697fa00","resolution":{"observed_at":"2026-07-08T09:14:46.708013Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.03558","last_updated":"2016-09-12T20:00:00Z","snapshot_observed_at":"2026-08-07T06:46:45.753213Z","submitted_at":"2016-09-12T20:00:00Z","title":"Turbulence and Vorticity in Galaxy Clusters Generated by Structure Formation","version":1},"cited_work":{"arxiv_id":"1609.03558","doi":"10.1093/mnras/stw2351","metadata_source":"openalex","pith_arxiv_id":"1609.03558","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"and Jones, T","venue":"astro-ph.CO","work_id":"f37d7044-4c26-4ae4-97a3-22cb92d6610d","year":2016},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1609.03558","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:7915d682fd335c576ccd45acd4b56cfb27124fe2ec0aba6f4c9c00b5fc6979e3","observation_id":"fce89def-cba3-4bd9-87f3-36c2f240da6a","resolution":{"observed_at":"2026-07-08T09:14:46.843736Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:51.379735+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:51.379735+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3576","last_updated":"2014-12-17T14:31:49Z","snapshot_observed_at":"2026-07-06T03:54:16.458401Z","submitted_at":"2014-09-11T20:00:11Z","title":"The Matryoshka Run (II): Time Dependent Turbulence Statistics, Stochastic Particle Acceleration and Microphysics Impact in a Massive Galaxy Cluster","version":2},"cited_work":{"arxiv_id":"1409.3576","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.3576","snapshot_observed_at":"2026-07-10T19:37:33.264201Z","title":"The Matryoshka Run (II): Time Dependent Turbulence Statistics, Stochastic Particle Acceleration and Microphysics Impact in a Massive Galaxy Cluster","venue":"astro-ph.CO","work_id":"396096e5-adac-4c6c-8267-7912b9b0dcbd","year":2014},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1409.3576","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:4a1784a3689394742921699ee8239e288bf7efb1bf2585a316f1c8e874f015d9","observation_id":"409cfc8f-749c-4914-96f1-1b4002353fc8","resolution":{"observed_at":"2026-07-08T09:14:46.797256Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0908.0610","last_updated":"2009-10-02T02:04:08Z","snapshot_observed_at":"2026-08-01T14:52:15.489878Z","submitted_at":"2009-08-05T07:57:16Z","title":"Characteristic Lengths of Magnetic Field in Magnetohydrodynamic Turbulence","version":2},"cited_work":{"arxiv_id":"0908.0610","doi":"10.1088/0004-637x/705/1/l90","metadata_source":"pith","pith_arxiv_id":"0908.0610","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Characteristic Lengths of Magnetic Field in Magnetohydrodynamic Turbulence","venue":"astro-ph.CO","work_id":"322732ed-c1ca-46f6-a377-b1e99980a1e5","year":2009},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0908.0610","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:5db6983471aa363d17bf99400361c06680218c9f8606bab41a3212b64157693d","observation_id":"c391ae87-3c59-4b86-8976-20f3d8e6eb61","resolution":{"observed_at":"2026-07-08T09:14:46.744539Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:51.917476+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:51.917476+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2011","doi":"10.1111/j.1365-2966.2011","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417","venue":null,"work_id":"d145e33f-f528-4886-b1e5-0963b1b5c030","year":2011},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:ea9eca02588949d2d45c93bc1a2a1736bc18344ef36130190d62ba63845bdf4e","observation_id":"fca966fc-245b-4262-a9f0-ff1c6708ca4e","resolution":{"observed_at":"2026-07-08T09:14:46.923154Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/175121","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2: Strong alfvenic turbulence","venue":"The Astrophysical Journal","work_id":"b2a31e83-ca5d-410d-ac58-3ebfabfd1f6d","year":1995},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:6314c08293c66680698130791df986d051831db68f38bfcec51c60be93b84f57","observation_id":"8a03da73-67dd-4a50-9d69-73d23e141473","resolution":{"observed_at":"2026-07-08T09:14:46.917954Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T15:38:19.617801+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T15:38:19.617801+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-10T15:38:19.617801+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02673","last_updated":"2017-11-07T19:00:02Z","snapshot_observed_at":"2026-08-01T06:33:30.616532Z","submitted_at":"2017-11-07T19:00:02Z","title":"Resolved magnetic dynamo action in the simulated intracluster medium","version":1},"cited_work":{"arxiv_id":"1711.02673","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.02673","snapshot_observed_at":"2026-07-08T09:14:46.751110Z","title":"Resolved magnetic dynamo action in the simulated intracluster medium","venue":"astro-ph.CO","work_id":"ff47c889-496b-4bae-8433-dd7e7f0f7dc3","year":2017},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.02673","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:42a5b4d36c1bec949623fcd028fe78be954e717bca3ee28c4b74448c851361cc","observation_id":"29f79751-7f6a-4138-bde3-a748047103e0","resolution":{"observed_at":"2026-07-08T09:14:46.752687Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.08737","last_updated":"2015-07-31T03:02:55Z","snapshot_observed_at":"2026-08-01T09:49:50.614727Z","submitted_at":"2015-07-31T03:02:55Z","title":"Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence","version":1},"cited_work":{"arxiv_id":"1507.08737","doi":null,"metadata_source":"pith","pith_arxiv_id":"1507.08737","snapshot_observed_at":"2026-07-08T09:14:46.839537Z","title":"Vorticity, Shocks and Magnetic Fields in Subsonic, ICM-like Turbulence","venue":"astro-ph.CO","work_id":"ad1cd9cd-06bd-4ef4-b990-634dedd3fd02","year":2015},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1507.08737","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:21ceb246ec5f19e52bbfa21df4a91d8df00b3cd4e743972fff43647c69d5e12b","observation_id":"bca77d02-e3e1-4d8c-8fa0-f1eb3431a24a","resolution":{"observed_at":"2026-07-08T09:14:46.841030Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1410.6485","last_updated":"2014-10-23T20:00:07Z","snapshot_observed_at":"2026-07-06T03:58:18.329666Z","submitted_at":"2014-10-23T20:00:07Z","title":"Turbulent Heating in Galaxy Clusters Brightest in X-rays","version":1},"cited_work":{"arxiv_id":"1410.6485","doi":null,"metadata_source":"pith","pith_arxiv_id":"1410.6485","snapshot_observed_at":"2026-07-10T22:17:37.642993Z","title":"Turbulent Heating in Galaxy Clusters Brightest in X-rays","venue":"astro-ph.HE","work_id":"d09b2386-bd28-40dc-93fb-4506ad09f81a","year":2014},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1410.6485","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:2c0786a7ea703bd406eccfce212400e02ad624038b64ea0bd682d55868f41f5c","observation_id":"7c2d7230-e984-4f96-85e0-c5827e0c7c36","resolution":{"observed_at":"2026-07-08T09:14:46.829375Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.06564","last_updated":"2018-02-09T22:13:40Z","snapshot_observed_at":"2026-07-06T06:00:20.967053Z","submitted_at":"2017-09-19T18:00:00Z","title":"Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters","version":3},"cited_work":{"arxiv_id":"1709.06564","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.06564","snapshot_observed_at":"2026-07-08T09:14:46.875712Z","title":"Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters","venue":"astro-ph.GA","work_id":"0584bb5c-6170-4e74-b610-c50caf3408a4","year":2017},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1709.06564","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:923586c139cdeca6ccda59f3d5a1cc272b0985f650af6db0b59dbbf3a303e51c","observation_id":"60d41de0-7927-4f23-9e9d-bb4740325dab","resolution":{"observed_at":"2026-07-08T09:14:46.877103Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0608433","last_updated":"2006-08-21T17:01:29Z","snapshot_observed_at":"2026-07-07T01:02:21.117146Z","submitted_at":"2006-08-21T17:01:29Z","title":"The intracluster magnetic field power spectrum in Abell 2255","version":1},"cited_work":{"arxiv_id":"astro-ph/0608433","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0608433","snapshot_observed_at":"2026-07-10T17:37:25.182758Z","title":"The intracluster magnetic field power spectrum in Abell 2255","venue":"astro-ph","work_id":"6c06a10d-9838-485c-a02c-0f3f90140d41","year":2006},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0608433","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:3b009b078059a85691bd99e76102540775332dd2c214d69310d17d7ba0d5ff25","observation_id":"333e8010-d141-4911-8530-8a72a8dbbe55","resolution":{"observed_at":"2026-07-08T09:14:46.918893Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1712.05407","last_updated":"2017-12-14T19:00:00Z","snapshot_observed_at":"2026-08-07T04:53:55.431575Z","submitted_at":"2017-12-14T19:00:00Z","title":"Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi","version":1},"cited_work":{"arxiv_id":"1712.05407","doi":"10.1093/pasj/psx156","metadata_source":"pith","pith_arxiv_id":"1712.05407","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Atomic data and spectral modeling constraints from high-resolution X-ray observations of the Perseus cluster with Hitomi","venue":"astro-ph.HE","work_id":"1f2c5c42-a10d-4c7d-afa8-8f7aaf789be2","year":2017},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1712.05407","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:1315b80f59f81d6f4acff68fe2f316c138c5caef87c940fc5cb36999388387e8","observation_id":"ca60c768-d8cd-44d8-82af-f3450fcc6c49","resolution":{"observed_at":"2026-07-08T09:14:46.948045Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-09T19:18:35.618151+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T19:18:35.618151+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20928","last_updated":"2025-04-29T16:47:34Z","snapshot_observed_at":"2026-08-07T15:58:08.343541Z","submitted_at":"2025-04-29T16:47:34Z","title":"XRISM forecast for the Coma cluster: stormy, with a steep power spectrum","version":1},"cited_work":{"arxiv_id":"2504.20928","doi":null,"metadata_source":"pith","pith_arxiv_id":"2504.20928","snapshot_observed_at":"2026-07-08T09:14:46.898658Z","title":"XRISM forecast for the Coma cluster: stormy, with a steep power spectrum","venue":"astro-ph.HE","work_id":"b6200308-a3dd-49fb-90cf-48f8a8a23bec","year":2025},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2504.20928","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:aed0fe667996897899ff38045fa889dd0b5a9d581a40bd938ff96c1c4b4e13ba","observation_id":"a02ded75-3d59-4d1e-8e88-dc4d26fc9d4a","resolution":{"observed_at":"2026-07-08T09:14:46.900481Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/bfb0106425","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Radio Galaxy Messier 87 , year = 1999, editor =","venue":"Lecture notes in physics","work_id":"61c368fa-7779-48e6-8ed6-58996d13d636","year":1999},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:e139aae1107f2b0e1877354513f9c6cc0c8e6c563ae76a0a951eec529229728f","observation_id":"2dd12ed8-db21-4fb1-bb31-be191fdc0151","resolution":{"observed_at":"2026-07-08T09:14:46.885343Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:54.188199+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:54.188199+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.0801","last_updated":"2007-10-03T14:48:59Z","snapshot_observed_at":"2026-07-06T01:30:44.394035Z","submitted_at":"2007-10-03T14:48:59Z","title":"Cosmic rays and Radio Halos in galaxy clusters : new constraints from radio observations","version":1},"cited_work":{"arxiv_id":"0710.0801","doi":"10.1086/524037","metadata_source":"pith","pith_arxiv_id":"0710.0801","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Cosmic rays and Radio Halos in galaxy clusters : new constraints from radio observations","venue":"astro-ph","work_id":"abc95f42-bfdc-4097-ba8d-d4f26c747953","year":2007},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0710.0801","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:d398ea18b39489888a85ea8e2e36c3cb6906d62c500de8fd4f782212658c87c8","observation_id":"68bb1b84-6a33-4540-af85-d19f83a540fb","resolution":{"observed_at":"2026-07-08T09:14:46.881605Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:54.44655+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:54.44655+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1705.02341","last_updated":"2017-05-05T18:00:01Z","snapshot_observed_at":"2026-08-02T02:17:58.452249Z","submitted_at":"2017-05-05T18:00:01Z","title":"On the connection between turbulent motions and particle acceleration in galaxy clusters","version":1},"cited_work":{"arxiv_id":"1705.02341","doi":null,"metadata_source":"pith","pith_arxiv_id":"1705.02341","snapshot_observed_at":"2026-07-10T17:37:25.836178Z","title":"On the connection between turbulent motions and particle acceleration in galaxy clusters","venue":"astro-ph.HE","work_id":"319569a9-79de-4d92-9bc7-c7e3a8344236","year":2017},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1705.02341","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:5855da79b6331d6af21bbce742ed7a714643f276caef446ed0903708a10ff4f9","observation_id":"2f73a27f-8aa9-4cf6-9f98-1edc08fd522a","resolution":{"observed_at":"2026-07-08T09:14:46.802019Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.04727","doi":"10.48550/arxiv.2507.04727","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"9bd76a86-e184-4c8d-a7f7-afd0588a0d86","year":null},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:f49dad91f22ca3470f3f9498166e1ec28c43064e58ac60fa6daf667cdb10b05f","observation_id":"1edc8a6e-b81d-4ef3-a7f1-03f331040a72","resolution":{"observed_at":"2026-07-08T09:14:46.818925Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:54.693194+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:54.693194+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"0401.093852","doi":"10.1146/annurev.astro.40.060401.093852","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"eprint =","venue":"Annual Review of Astronomy and Astrophysics","work_id":"6892523c-47c0-4992-a175-329935bfef35","year":2002},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:9d5d7bcf03e9d4e7d5ab0da7bae83f629a50cd5df903f9dc8f80a226a0ade91f","observation_id":"430b38e4-d86b-4e3e-99f7-5dc99870f3d5","resolution":{"observed_at":"2026-07-08T09:14:46.926294Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:54.990734+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:54.990734+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1401.7519","last_updated":"2014-01-29T14:05:45Z","snapshot_observed_at":"2026-07-06T03:34:38.396340Z","submitted_at":"2014-01-29T14:05:45Z","title":"Cosmic rays in galaxy clusters and their non-thermal emission","version":1},"cited_work":{"arxiv_id":"1401.7519","doi":null,"metadata_source":"pith","pith_arxiv_id":"1401.7519","snapshot_observed_at":"2026-07-10T19:37:33.018000Z","title":"Cosmic rays in galaxy clusters and their non-thermal emission","venue":"astro-ph.CO","work_id":"7bef5f52-fb72-460d-bb9f-a4d7ae42cd91","year":2014},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1401.7519","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:a3f6def29ef9e460192e584d9e291e2c0c1e9978b35bb1f3cbf67f13134540fc","observation_id":"a5b55b93-7ea0-4e6c-9964-2177c88efccf","resolution":{"observed_at":"2026-07-08T09:14:46.778601Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0011281","last_updated":"2000-11-14T23:00:32Z","snapshot_observed_at":"2026-07-07T00:14:04.045755Z","submitted_at":"2000-11-14T23:00:32Z","title":"A New Radio - X-Ray Probe of Galaxy Cluster Magnetic Fields","version":1},"cited_work":{"arxiv_id":"astro-ph/0011281","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0011281","snapshot_observed_at":"2026-07-08T09:14:46.930021Z","title":"A New Radio - X-Ray Probe of Galaxy Cluster Magnetic Fields","venue":"astro-ph","work_id":"21971a12-4833-48e2-aa2f-e57f5cea2cfe","year":2000},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0011281","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:0d35ac0d861360222244ec854328de8c8e6ac94c254db27cccb430407d64880a","observation_id":"7847675e-3265-4c36-b86e-fb7940ec7f45","resolution":{"observed_at":"2026-07-08T09:14:46.931452Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1007.5207","last_updated":"2010-07-29T12:50:21Z","snapshot_observed_at":"2026-08-04T02:51:42.135979Z","submitted_at":"2010-07-29T12:50:21Z","title":"Rotation Measures of Radio Sources in Hot Galaxy Clusters","version":1},"cited_work":{"arxiv_id":"1007.5207","doi":null,"metadata_source":"pith","pith_arxiv_id":"1007.5207","snapshot_observed_at":"2026-07-08T09:14:46.893688Z","title":"Rotation Measures of Radio Sources in Hot Galaxy Clusters","venue":"astro-ph.CO","work_id":"294a2cf8-7ed9-4312-a391-ac23173def2b","year":2010},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1007.5207","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:6279b4dabd36870f29589df3e1f71c470594a6b0d00e438ab9b00d9629769e37","observation_id":"e30c7fff-04fe-4b4e-b84d-fcc38fd6695b","resolution":{"observed_at":"2026-07-08T09:14:46.894896Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2203.04336","last_updated":"2022-03-28T14:11:17Z","snapshot_observed_at":"2026-08-01T10:02:22.639530Z","submitted_at":"2022-03-08T19:00:14Z","title":"Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs","version":2},"cited_work":{"arxiv_id":"2203.04336","doi":"10.1093/mnras/stac516","metadata_source":"pith","pith_arxiv_id":"2203.04336","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs","venue":"astro-ph.GA","work_id":"9be3d2b7-f19d-483a-bff2-570add075c55","year":2022},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2203.04336","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:661da5c9ec8e6aefb3b4b8d69a8d67c44be2c0b173430724a8a3309e76859e46","observation_id":"8ac6047d-31a3-4855-b0bd-1e27e2044976","resolution":{"observed_at":"2026-07-08T09:14:46.724265Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:56.198868+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:56.198868+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507349","last_updated":"2005-11-02T12:09:47Z","snapshot_observed_at":"2026-07-07T00:52:14.864740Z","submitted_at":"2005-07-14T14:54:16Z","title":"Faraday Rotation Measure Synthesis","version":2},"cited_work":{"arxiv_id":"astro-ph/0507349","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0507349","snapshot_observed_at":"2026-07-10T17:37:25.745364Z","title":"Faraday Rotation Measure Synthesis","venue":"astro-ph","work_id":"d0596453-81c5-434a-a3d4-c106aee73774","year":2005},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0507349","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:5c0266764907c15d333190631f2e90ad365f40c86fb0bbe6fb10282d676eea4c","observation_id":"610784d6-5fd5-4dee-9549-96506f4f914f","resolution":{"observed_at":"2026-07-08T09:14:46.755701Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2303.07741","last_updated":"2023-03-14T09:39:23Z","snapshot_observed_at":"2026-07-06T15:03:04.324080Z","submitted_at":"2023-03-14T09:39:23Z","title":"Introduction to Faraday tomography and its future prospects","version":1},"cited_work":{"arxiv_id":"2303.07741","doi":"10.1093/pasj/psac111","metadata_source":"pith","pith_arxiv_id":"2303.07741","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Introduction to Faraday tomography and its future prospects","venue":"astro-ph.GA","work_id":"8b7fdec2-8dca-4ed5-a60c-b1b2a6dafe66","year":2023},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2303.07741","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:9ad9bd872a4b36318ace4919cfc3619899792eb468bec16eefa5434963eabb60","observation_id":"f363e160-edb6-4999-bc02-bb2bdeb84c4e","resolution":{"observed_at":"2026-07-08T09:14:46.826710Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:56.75898+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:56.75898+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.20325","last_updated":"2024-07-29T18:00:01Z","snapshot_observed_at":"2026-08-03T22:49:00.064920Z","submitted_at":"2024-07-29T18:00:01Z","title":"Probing the Magnetised Gas Distribution in Galaxy Groups and the Cosmic Web with POSSUM Faraday Rotation Measures","version":1},"cited_work":{"arxiv_id":"2407.20325","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.20325","snapshot_observed_at":"2026-07-10T23:57:45.974540Z","title":"Probing the Magnetised Gas Distribution in Galaxy Groups and the Cosmic Web with POSSUM Faraday Rotation Measures","venue":"astro-ph.GA","work_id":"a373b6e3-8935-4da6-9eb8-bcf1458dc60a","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2407.20325","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:5f2ab81e99084b1130224d683c52306de9e6f6d541d08a6146c97a0f0c5d4346","observation_id":"c0307fcc-5106-4b3c-9e1f-96dddaeb9811","resolution":{"observed_at":"2026-07-08T09:14:46.930388Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.00699","last_updated":"2022-07-19T22:41:46Z","snapshot_observed_at":"2026-08-02T02:43:32.123194Z","submitted_at":"2020-10-01T21:52:34Z","title":"MHD Turbulence: A Biased Review","version":3},"cited_work":{"arxiv_id":"2010.00699","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.00699","snapshot_observed_at":"2026-07-10T01:36:44.433513Z","title":"MHD Turbulence: A Biased Review","venue":"physics.plasm-ph","work_id":"3fcd64a5-4ef1-411b-a1d0-cb29797da7a7","year":2020},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2010.00699","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:58754f437992bfa0c54fcfc50c601cc1007e96562863cd64385c0c555de5e7a8","observation_id":"27f776cc-b076-4418-b55d-8c9ca902e455","resolution":{"observed_at":"2026-07-08T09:14:46.853169Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.12151","last_updated":"2024-09-18T17:15:10Z","snapshot_observed_at":"2026-08-09T23:48:24.183483Z","submitted_at":"2024-09-18T17:15:10Z","title":"AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasma","version":1},"cited_work":{"arxiv_id":"2409.12151","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.12151","snapshot_observed_at":"2026-07-08T09:14:46.874123Z","title":"AHKASH: a new Hybrid particle-in-cell code for simulations of astrophysical collisionless plasma","venue":"astro-ph.IM","work_id":"a505fa5d-8f4d-4642-8f79-ff4fa4312d30","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2409.12151","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:42848457fe763aead23a768bf671fbfa5f5c37920acc726c02cdbaf9bd2247c7","observation_id":"0e3e5a87-5c28-4e98-ab45-812b1131824b","resolution":{"observed_at":"2026-07-08T09:14:46.875686Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1002.0594","last_updated":"2010-02-02T21:37:25Z","snapshot_observed_at":"2026-07-06T02:02:48.994726Z","submitted_at":"2010-02-02T21:37:25Z","title":"The Coma cluster magnetic field from Faraday rotation measures","version":1},"cited_work":{"arxiv_id":"1002.0594","doi":null,"metadata_source":"pith","pith_arxiv_id":"1002.0594","snapshot_observed_at":"2026-07-08T09:14:46.826882Z","title":"The Coma cluster magnetic field from Faraday rotation measures","venue":"astro-ph.CO","work_id":"f37b3d0d-d61c-497c-9ca9-b23921b21ee3","year":2010},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1002.0594","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:76a003bcf839c0ceebdb21d604b99affb5f4f1add351f4220140a271444e96af","observation_id":"574f66b5-630a-4e9f-afe3-5ba1a86ee1f0","resolution":{"observed_at":"2026-07-08T09:14:46.828220Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.08688","last_updated":"2017-03-25T13:03:17Z","snapshot_observed_at":"2026-08-07T16:59:02.824752Z","submitted_at":"2017-03-25T13:03:17Z","title":"Sardinia Radio Telescope observations of Abell 194 - the intra-cluster magnetic field power spectrum","version":1},"cited_work":{"arxiv_id":"1703.08688","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.08688","snapshot_observed_at":"2026-07-08T09:14:46.907339Z","title":"Sardinia Radio Telescope observations of Abell 194 - the intra-cluster magnetic field power spectrum","venue":"astro-ph.CO","work_id":"e4f6a29a-bbb5-42c7-8ba8-c3728a9f0467","year":2017},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1703.08688","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:4a7ae6cc56a0084a3f7cb3ec30b105ed6a0e9726088032ab79372c888b132272","observation_id":"a6207488-05dd-46c7-883a-d02a6e7b4f78","resolution":{"observed_at":"2026-07-08T09:14:46.908584Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.06346","last_updated":"2019-06-14T18:00:24Z","snapshot_observed_at":"2026-08-04T02:14:20.561849Z","submitted_at":"2019-06-14T18:00:24Z","title":"Suppressed effective viscosity in the bulk intergalactic plasma","version":1},"cited_work":{"arxiv_id":"1906.06346","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.06346","snapshot_observed_at":"2026-07-08T09:14:46.870476Z","title":"Suppressed effective viscosity in the bulk intergalactic plasma","venue":"astro-ph.HE","work_id":"37fccac0-5393-474a-8498-1a369210f268","year":2019},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1906.06346","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:b7d7bc7efc996fd496d66935534c996758f101e5ccedc3d8ff4b5a925bbbd446","observation_id":"c3202bed-046c-4535-941d-6aa7d44e3126","resolution":{"observed_at":"2026-07-08T09:14:46.871850Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.08445","last_updated":"2015-10-28T20:03:21Z","snapshot_observed_at":"2026-08-07T08:21:38.531631Z","submitted_at":"2015-10-28T20:03:21Z","title":"Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed with Chandra ACIS","version":1},"cited_work":{"arxiv_id":"1510.08445","doi":"10.1051/0004-6361/201526925","metadata_source":"pith","pith_arxiv_id":"1510.08445","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Thermodynamic perturbations in the X-ray halo of 33 clusters of galaxies observed with Chandra ACIS","venue":"astro-ph.CO","work_id":"4346dc4e-6fe6-4ea1-8aa5-102e7a861f67","year":2015},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1510.08445","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:fa9495533404a43fe4549d6f39c8b4f102e1f56961b1af53e75f7382ef5a59b5","observation_id":"3f158738-3862-482f-a92f-f86ee6868c63","resolution":{"observed_at":"2026-07-08T09:14:46.842744Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:18:58.95838+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:18:58.95838+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23634","last_updated":"2025-03-31T00:18:00Z","snapshot_observed_at":"2026-08-07T16:26:51.290702Z","submitted_at":"2025-03-31T00:18:00Z","title":"Magnetic fields in the multiphase interstellar medium of the Milky Way: turbulent kinetic and magnetic energy density relation","version":1},"cited_work":{"arxiv_id":"2503.23634","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.23634","snapshot_observed_at":"2026-07-08T09:14:46.876928Z","title":"Magnetic fields in the multiphase interstellar medium of the Milky Way: turbulent kinetic and magnetic energy density relation","venue":"astro-ph.GA","work_id":"15e9f5bb-4ab4-4288-8485-bcabb09f1060","year":2025},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2503.23634","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:c5df880952be5ecad6db1cbe17e4aebd855487e69be98c0196ca6ae81e9af9b1","observation_id":"c9a68e65-d1da-41ce-8647-1b1d611d29e6","resolution":{"observed_at":"2026-07-08T09:14:46.878482Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.05690","last_updated":"2021-08-23T15:53:06Z","snapshot_observed_at":"2026-08-03T18:50:30.409346Z","submitted_at":"2021-04-12T17:51:48Z","title":"Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis","version":2},"cited_work":{"arxiv_id":"2104.05690","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.05690","snapshot_observed_at":"2026-07-10T19:37:33.577863Z","title":"Dissecting nonthermal emission in the complex multiple-merger galaxy cluster Abell 2744: Radio and X-ray analysis","venue":"astro-ph.CO","work_id":"02308dd5-4642-43b6-85e1-4a96c9a0a9d7","year":2021},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2104.05690","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:cab24c5cd796c4d53f146a6c7352cbf0a3c72c9caecdbdc285e6027e61270ab9","observation_id":"ac2b2d77-2f62-4f66-98b1-5bb9bc5aca12","resolution":{"observed_at":"2026-07-08T09:14:46.894387Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.06940","last_updated":"2022-02-22T08:11:16Z","snapshot_observed_at":"2026-07-06T12:08:04.130427Z","submitted_at":"2021-11-12T20:53:48Z","title":"MeerKAT view of the diffuse radio sources in Abell 3667 and their interactions with the thermal plasma","version":2},"cited_work":{"arxiv_id":"2111.06940","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.06940","snapshot_observed_at":"2026-07-10T19:37:33.254286Z","title":"de Gasperin, L","venue":"astro-ph.CO","work_id":"715a6aa8-1b15-4c2e-a731-4327fee075a5","year":2021},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2111.06940","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:769e652d264db307598efc382c60c23262da241801ae92ff4726ca0f0323cbd3","observation_id":"fba22877-3191-48f8-88de-e289c1950ace","resolution":{"observed_at":"2026-07-08T09:14:46.869111Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2209.13617","last_updated":"2022-09-27T18:21:26Z","snapshot_observed_at":"2026-08-10T11:00:04.325079Z","submitted_at":"2022-09-27T18:21:26Z","title":"Galaxy clusters enveloped by vast volumes of relativistic electrons","version":1},"cited_work":{"arxiv_id":"2209.13617","doi":null,"metadata_source":"pith","pith_arxiv_id":"2209.13617","snapshot_observed_at":"2026-07-10T19:37:33.320274Z","title":"Galaxy clusters enveloped by vast volumes of relativistic electrons","venue":"astro-ph.CO","work_id":"11976399-9263-45b6-a958-ddd95d493ea2","year":2022},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2209.13617","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:f8fba6710b4d6de41639ab50c08b312623c8bcccac5a96249665ff8f00c71a98","observation_id":"90602f5f-7663-4373-9bf5-582a2073edc9","resolution":{"observed_at":"2026-07-08T09:14:46.797872Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.07584","last_updated":"2019-06-18T13:52:30Z","snapshot_observed_at":"2026-08-10T10:59:46.980026Z","submitted_at":"2019-06-18T13:52:30Z","title":"A radio ridge connecting two galaxy clusters in a filament of the cosmic web","version":1},"cited_work":{"arxiv_id":"1906.07584","doi":null,"metadata_source":"pith","pith_arxiv_id":"1906.07584","snapshot_observed_at":"2026-07-10T19:37:33.477348Z","title":"A radio ridge connecting two galaxy clusters in a filament of the cosmic web","venue":"astro-ph.GA","work_id":"b5d45aa7-6584-4149-8603-9c33f4a22be0","year":2019},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1906.07584","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:bf61b387758e99a53e2ab1bd22e57035f4d4eb50d3326a03a46307b76c0b4a0d","observation_id":"104c1e25-cc72-4273-a2a7-2548b999ffae","resolution":{"observed_at":"2026-07-08T09:14:46.874468Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.10285","last_updated":"2019-07-02T01:56:03Z","snapshot_observed_at":"2026-08-08T02:50:03.020949Z","submitted_at":"2019-06-25T00:55:31Z","title":"Observations of a Pre-Merger Shock in Colliding Clusters of Galaxies","version":2},"cited_work":{"arxiv_id":"1906.10285","doi":"10.1038/s41550-019-0798-8","metadata_source":"pith","pith_arxiv_id":"1906.10285","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Observations of a Pre-Merger Shock in Colliding Clusters of Galaxies","venue":"astro-ph.HE","work_id":"830a53c4-db33-47a0-9dea-b76ee93a7c57","year":2019},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1906.10285","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:064f39dd56f4595ac54bde1febfb35da30abc8a82b84f10d85373190b41a7c1b","observation_id":"9f44d36e-552c-49ac-b943-6f8361de0d46","resolution":{"observed_at":"2026-07-08T09:14:46.856241Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:00.83872+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:00.83872+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.04750","last_updated":"2022-11-24T02:34:27Z","snapshot_observed_at":"2026-08-06T05:53:18.843698Z","submitted_at":"2022-08-09T12:38:04Z","title":"Diffuse radio source candidate in CIZA J1358.9-4750","version":3},"cited_work":{"arxiv_id":"2208.04750","doi":null,"metadata_source":"pith","pith_arxiv_id":"2208.04750","snapshot_observed_at":"2026-07-08T09:14:46.919243Z","title":"Diffuse radio source candidate in CIZA J1358.9-4750","venue":"astro-ph.HE","work_id":"415d1446-3cf8-4d5e-b8c8-d3f26a6fe6c3","year":2022},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2208.04750","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:54d83eb0d116f8e892afbba310720b3469e7ee0006daaef92e424b5435b1bf36","observation_id":"30a03f72-293e-4883-ba86-99e1c0f82010","resolution":{"observed_at":"2026-07-08T09:14:46.920404Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.07718","last_updated":"2020-01-21T19:00:00Z","snapshot_observed_at":"2026-07-06T08:51:52.563800Z","submitted_at":"2020-01-21T19:00:00Z","title":"Second order Fermi reacceleration mechanisms and large scale synchrotron radio emission in intra-cluster bridges","version":1},"cited_work":{"arxiv_id":"2001.07718","doi":null,"metadata_source":"pith","pith_arxiv_id":"2001.07718","snapshot_observed_at":"2026-07-10T19:37:33.572112Z","title":"Second order Fermi reacceleration mechanisms and large scale synchrotron radio emission in intra-cluster bridges","venue":"astro-ph.HE","work_id":"f69ebe61-3fd8-4539-95c5-c9766768598b","year":2020},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2001.07718","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:00a2f85dfcd532a267d52685a9d377084d622e226dff65df8ce8167a03803263","observation_id":"069d2dfd-3dec-4844-87b2-f02cfcc77a7d","resolution":{"observed_at":"2026-07-08T09:14:46.940010Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.03172","last_updated":"2020-06-05T00:01:19Z","snapshot_observed_at":"2026-07-06T09:26:14.466190Z","submitted_at":"2020-06-05T00:01:19Z","title":"Magnetism Science with the Square Kilometre Array","version":1},"cited_work":{"arxiv_id":"2006.03172","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.03172","snapshot_observed_at":"2026-07-08T09:14:46.914593Z","title":"Magnetism Science with the Square Kilometre Array","venue":"astro-ph.GA","work_id":"188ad074-1b04-424e-8b75-c472d4101147","year":2020},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2006.03172","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:56b5ebe98062d1c26ea01de8df66ac51ebe435c48ce5cf6f23f6bd95ab4ad2ae","observation_id":"3ba6ca66-da9d-44ef-93ce-a5fd7f9b13d2","resolution":{"observed_at":"2026-07-08T09:14:46.916339Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.13798","last_updated":"2022-10-13T23:27:34Z","snapshot_observed_at":"2026-08-06T04:41:14.248691Z","submitted_at":"2022-06-28T07:27:39Z","title":"Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds","version":2},"cited_work":{"arxiv_id":"2206.13798","doi":null,"metadata_source":"pith","pith_arxiv_id":"2206.13798","snapshot_observed_at":"2026-07-08T09:14:46.895818Z","title":"Rotation measure structure functions with higher-order stencils as a probe of small-scale magnetic fluctuations and its application to the Small and Large Magellanic Clouds","venue":"astro-ph.GA","work_id":"c12f3bec-396d-4467-b125-c44191df3af2","year":2022},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2206.13798","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:2031c3b58ad7f7fc79b2a93741be3755d557a878360ce867737b59eef77e06df","observation_id":"5807c596-3865-4326-9254-7bbd9bd8fb53","resolution":{"observed_at":"2026-07-08T09:14:46.897443Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.04156","last_updated":"2024-08-08T01:51:41Z","snapshot_observed_at":"2026-08-06T05:21:13.028232Z","submitted_at":"2024-08-08T01:51:41Z","title":"Structure functions with higher-order stencils as a probe to separate small- and large-scale magnetic fields","version":1},"cited_work":{"arxiv_id":"2408.04156","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.04156","snapshot_observed_at":"2026-07-08T09:14:46.881434Z","title":"Structure functions with higher-order stencils as a probe to separate small- and large-scale magnetic fields","venue":"astro-ph.GA","work_id":"ce53dd43-ff07-4f23-8a91-3bc63a1f0af4","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2408.04156","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:cacfd2a78349659a8d86e28785656225f6c2718ed945a78bb0d2ce02f5ea3a30","observation_id":"5941c1fd-dc49-4c95-bcaa-8d8dea4885c7","resolution":{"observed_at":"2026-07-08T09:14:46.882938Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.04487","last_updated":"2016-07-15T12:50:06Z","snapshot_observed_at":"2026-07-06T05:03:43.188549Z","submitted_at":"2016-07-15T12:50:06Z","title":"The Quiescent Intracluster Medium in the Core of the Perseus Cluster","version":1},"cited_work":{"arxiv_id":"1607.04487","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.04487","snapshot_observed_at":"2026-07-08T09:14:46.886782Z","title":"The Quiescent Intracluster Medium in the Core of the Perseus Cluster","venue":"astro-ph.GA","work_id":"a21fd116-d69b-4294-80e6-6294d199b593","year":2016},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1607.04487","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:b48acc4c61e5a8808f8a3c4b0947a651a8dc420b09f137fa17840fdd4b1bb05e","observation_id":"68582521-72b8-424f-ad4a-7e019b0fcce3","resolution":{"observed_at":"2026-07-08T09:14:46.888618Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07829","last_updated":"2019-08-29T09:19:42Z","snapshot_observed_at":"2026-08-04T11:08:53.435910Z","submitted_at":"2019-03-15T21:04:42Z","title":"Dynamo theories","version":2},"cited_work":{"arxiv_id":"1903.07829","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.07829","snapshot_observed_at":"2026-07-10T01:36:44.380967Z","title":"Dynamo theories","venue":"physics.plasm-ph","work_id":"0115ca55-61ad-45e9-ad69-173f396263af","year":2019},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1903.07829","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:0f66f3a910474ebb09677b0999a997b886292f7b449d1f36420ceebbd63b8094","observation_id":"ec9ab4b4-3c58-456c-92d7-30917436f1cf","resolution":{"observed_at":"2026-07-08T09:14:46.911007Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ae2a28","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal Letters","work_id":"812f614c-5187-43ce-aed6-c1e5c4f30a29","year":2041},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:30fa17446cdd1921fed2ecb30038a5485954622ad182ea9c5d11c19d02d71572","observation_id":"5c46680d-44d8-4570-8992-3c966bbcbe4d","resolution":{"observed_at":"2026-07-08T09:14:46.920678Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:06.643599+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:06.643599+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.10150","last_updated":"2024-06-26T08:48:34Z","snapshot_observed_at":"2026-08-04T06:18:18.426928Z","submitted_at":"2024-03-15T09:50:00Z","title":"Indications of an offset merger in Abell 3667","version":2},"cited_work":{"arxiv_id":"2403.10150","doi":"10.1051/0004-6361/202449992","metadata_source":"pith","pith_arxiv_id":"2403.10150","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Omiya, K","venue":"astro-ph.HE","work_id":"babfc0fe-264c-47e9-b3d7-75c9c7f9f91f","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2403.10150","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:adc6b7f5d195adbe570693069c4bc077e895db4a0cc6fa6db6e336c1513dc978","observation_id":"62249a82-c1b1-4ce8-af7b-1ae92dd694ea","resolution":{"observed_at":"2026-07-08T09:14:46.769083Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:06.966021+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:06.966021+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ae100c","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"keywords =","venue":"The Astrophysical Journal Letters","work_id":"df173e9a-f035-49e6-81ff-df62383d996e","year":2041},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:e33e82bd0b183298f81631e0eacd9fce56b72546dab255dda771877ff6936d14","observation_id":"214e17c2-bf47-408f-81a0-93ddc1c65fec","resolution":{"observed_at":"2026-07-08T09:14:46.838206Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-09T19:18:48.637414+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T19:18:48.637414+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202556070","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2026, A&A, 705, A129, doi: 10.1051/0004-6361/202556070","venue":"Astronomy and Astrophysics","work_id":"d3ff7f47-e84b-449e-9118-e8dec3278a9c","year":2026},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:4fee7306b06de0612bd2eeaff30292d3298cfc32ad19223e075c3875c567b0b4","observation_id":"cfd1ff4b-b0c9-4f34-a358-fd1df7998803","resolution":{"observed_at":"2026-07-08T09:14:46.933995Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:07.270933+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:07.270933+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.08722","last_updated":"2025-08-24T05:37:24Z","snapshot_observed_at":"2026-08-09T17:37:40.187040Z","submitted_at":"2025-02-12T19:00:11Z","title":"The bulk motion of gas in the core of the Centaurus galaxy cluster","version":2},"cited_work":{"arxiv_id":"2502.08722","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.08722","snapshot_observed_at":"2026-07-09T00:45:48.966599Z","title":"The bulk motion of gas in the core of the Centaurus galaxy cluster","venue":"astro-ph.HE","work_id":"b1e734bf-c0a9-4230-8cc5-7111dee18945","year":2025},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2502.08722","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:203b4aac06600edf477d3816d4103cfc79503a5934f404cc3b18c40a29a9c3bf","observation_id":"d536ad25-6b22-43ad-903d-638d1316a429","resolution":{"observed_at":"2026-07-08T09:14:46.937012Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ae2c5c","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"The Astrophysical Journal","work_id":"b00325d7-d5df-4cbe-98be-47cf128ff540","year":null},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:4642f1b15dba9fbb842caf3b32ccf839637ad8f5a5f2efd643d8419814ccd733","observation_id":"91eeee5c-ca18-465c-a847-570707beb252","resolution":{"observed_at":"2026-07-08T09:14:46.913253Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-09T19:18:47.392025+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-09T19:18:47.392025+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.5302","last_updated":"2014-07-07T21:10:53Z","snapshot_observed_at":"2026-07-06T03:41:42.300617Z","submitted_at":"2014-04-21T20:00:01Z","title":"The relation between gas density and velocity power spectra in galaxy clusters: high-resolution hydrodynamic simulations and the role of conduction","version":2},"cited_work":{"arxiv_id":"1404.5302","doi":"10.1051/0004-6361/201424043","metadata_source":"pith","pith_arxiv_id":"1404.5302","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The relation between gas density and velocity power spectra in galaxy clusters: high-resolution hydrodynamic simulations and the role of conduction","venue":"astro-ph.CO","work_id":"70ffda93-5581-41ea-a2b7-e6e72b695d99","year":2014},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1404.5302","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:a7ca9f6447389dd8746fbd9c1594675fcc715ce22d4e243022e4642568db0bbc","observation_id":"8f5a2090-bdc0-46de-9895-fb0ac289ac85","resolution":{"observed_at":"2026-07-08T09:14:46.906926Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:07.630612+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:07.630612+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.08680","last_updated":"2025-03-11T17:57:07Z","snapshot_observed_at":"2026-08-07T17:12:11.486845Z","submitted_at":"2025-03-11T17:57:07Z","title":"Gas Perturbations in Hot Smooth Atmospheres X-ray Surface Brightness Fluctuations in Smooth Galaxy Cluster Atmospheres","version":1},"cited_work":{"arxiv_id":"2503.08680","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.08680","snapshot_observed_at":"2026-07-08T09:14:46.817906Z","title":"Gas Perturbations in Hot Smooth Atmospheres X-ray Surface Brightness Fluctuations in Smooth Galaxy Cluster Atmospheres","venue":"astro-ph.GA","work_id":"8041bf2a-29c9-4b89-8822-4ced6f9595d1","year":2025},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2503.08680","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:2f6a3c346d6669a1f302660adbbfc3fa002065341585f2674ce3597f9139fc85","observation_id":"030a6949-1b2e-49b1-bed0-a9f7b1240105","resolution":{"observed_at":"2026-07-08T09:14:46.820158Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2011","doi":"10.1111/j.1365-2966.2011","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A., et al., 2011, @doi [ ] 10.1111/j.1365-2966.2011.18706.x , http://adsabs.harvard.edu/abs/2011MNRAS.417.1621D 417","venue":null,"work_id":"d145e33f-f528-4886-b1e5-0963b1b5c030","year":2011},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:94b04d371cbe286eb279a45906fe0ab15fae68fd4a5f97823c488a571f1ce700","observation_id":"594b8e04-cdf5-415d-a5a5-5b83b5a2146d","resolution":{"observed_at":"2026-07-08T09:14:46.816658Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.14805","last_updated":"2020-11-30T06:21:39Z","snapshot_observed_at":"2026-07-06T09:32:58.317099Z","submitted_at":"2020-06-26T05:44:47Z","title":"Unexpected Circular Radio Objects at High Galactic Latitude","version":2},"cited_work":{"arxiv_id":"2006.14805","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.14805","snapshot_observed_at":"2026-07-08T09:14:46.836187Z","title":"Unexpected Circular Radio Objects at High Galactic Latitude","venue":"astro-ph.GA","work_id":"c0c07375-280e-42c2-b11a-24d0f3ff75c9","year":2020},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2006.14805","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:9f0af504bdb558e9775b0a5f5361ae23bafa696e2733449f951b08d36292609d","observation_id":"c75522a0-974e-4463-8866-15058ba0c775","resolution":{"observed_at":"2026-07-08T09:14:46.837438Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2602.18294","last_updated":"2026-04-01T09:13:55Z","snapshot_observed_at":"2026-08-02T14:55:42.328842Z","submitted_at":"2026-02-20T15:42:37Z","title":"Single- and double-headed odd radio circles in the LOFAR surveys","version":2},"cited_work":{"arxiv_id":"2602.18294","doi":"10.1051/0004-6361/202658988","metadata_source":"pith","pith_arxiv_id":"2602.18294","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"2020, A&A, 643, A111 De Gasperin, F., Brüggen, M., Pasini, T., et al","venue":"astro-ph.GA","work_id":"843edaff-db34-44a3-8b71-beddc2358c84","year":2026},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"cited_paper":"/paper/2602.18294","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:7ac95ba6c6a74efcc2668d471ea8f7ad2939db2a5d51313501e675ab882720e2","observation_id":"3f73953e-7c63-4b6d-9d65-7cedc0dcb449","resolution":{"observed_at":"2026-07-08T09:14:46.862164Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08693","last_updated":"2023-11-15T04:44:38Z","snapshot_observed_at":"2026-08-02T16:57:38.508785Z","submitted_at":"2023-11-15T04:44:38Z","title":"Discovery of Diffuse Radio Source in Abell 1060","version":1},"cited_work":{"arxiv_id":"2311.08693","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.08693","snapshot_observed_at":"2026-07-08T09:14:46.849384Z","title":"Discovery of Diffuse Radio Source in Abell 1060","venue":"astro-ph.HE","work_id":"02b7b8c5-c886-4046-81f4-128f8be46f6f","year":2023},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2311.08693","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:5b48937cb2122e8e0a3701816fd84b56913d675a3d62843402d0eef8960e90fa","observation_id":"8637c636-cc4b-4e36-917e-2df9446ca35e","resolution":{"observed_at":"2026-07-08T09:14:46.850613Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/138.1.1","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"year = 1968, month = jan, volume =","venue":"Monthly Notices of the Royal Astronomical Society","work_id":"2978ea45-3568-4c02-aabd-5aa57a4df6e0","year":1968},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:c0f8909701c878ed7728c3a49e1586324bc63746d262dd5b3365a6e51800a468","observation_id":"a8480530-8b34-44ef-8990-5f836fb59286","resolution":{"observed_at":"2026-07-08T09:14:46.896865Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-06T20:38:04.590037+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-06T20:38:04.590037+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/pasj/psaf128","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":", keywords =","venue":"Publications of the Astronomical Society of Japan","work_id":"0beef31f-c31f-4c0a-a657-beff03041e50","year":null},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:9437575e02b15c78fb4d70d67a6080a0bcc9fb1206b29d95c0ec1f565177962c","observation_id":"9f32c2a3-2dc3-4f1b-8455-a396fb7b5fbf","resolution":{"observed_at":"2026-07-08T09:14:46.922932Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:09.59122+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:09.59122+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.15179","last_updated":"2024-01-26T19:56:18Z","snapshot_observed_at":"2026-08-08T03:27:05.323467Z","submitted_at":"2024-01-26T19:56:18Z","title":"Merger-driven multi-scale ICM density perturbations: testing cosmological simulations and constraining plasma physics","version":1},"cited_work":{"arxiv_id":"2401.15179","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.15179","snapshot_observed_at":"2026-07-08T09:14:46.820583Z","title":"Merger-driven multi-scale ICM density perturbations: testing cosmological simulations and constraining plasma physics","venue":"astro-ph.HE","work_id":"170c453f-3000-4d8b-8d84-89a5f548894e","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2401.15179","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:bd076e4d83a6184337f88968e485f5f9fecc78cfa933ec0e7cd4811df44f0627","observation_id":"b9240cbc-1d73-4f35-b6fe-eb1924ba9b97","resolution":{"observed_at":"2026-07-08T09:14:46.822147Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.01493","last_updated":"2022-11-02T21:44:48Z","snapshot_observed_at":"2026-07-06T14:13:46.912823Z","submitted_at":"2022-11-02T21:44:48Z","title":"Magnetic fields and relativistic electrons fill entire galaxy cluster","version":1},"cited_work":{"arxiv_id":"2211.01493","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.01493","snapshot_observed_at":"2026-07-10T17:37:25.302374Z","title":"Magnetic fields and relativistic electrons fill entire galaxy cluster","venue":"astro-ph.CO","work_id":"64df328f-b0b3-49ae-8b0e-e412ce4c6809","year":2022},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2211.01493","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:2d629547417416c7b461544c4e3afe774349ccf6a1172d3094bb89038bcfcecf","observation_id":"48c3d0e0-0314-4666-8148-cbc0f383320e","resolution":{"observed_at":"2026-07-08T09:14:46.754387Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1603.00458","last_updated":"2016-03-01T09:26:30Z","snapshot_observed_at":"2026-07-06T04:47:57.060551Z","submitted_at":"2016-03-01T09:26:30Z","title":"Stochastic reacceleration of relativistic electrons by turbulent reconnection: a mechanism for cluster-scale radio emission ?","version":1},"cited_work":{"arxiv_id":"1603.00458","doi":"10.1093/mnras/stw496","metadata_source":"pith","pith_arxiv_id":"1603.00458","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"doi:10.1093/mnras/stw496, https://arxiv.org/abs/1603.00458 arXiv:1603.00458 [astro-ph.HE]","venue":"astro-ph.HE","work_id":"6a0bb631-fcd1-4c0c-bc2e-c6ef1b75bce7","year":2016},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1603.00458","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:bd4c1aa565418eaee2a312eec4c94a4b11a4e4a08ac0410e3a9e585fe8e09f6d","observation_id":"8407dbaf-eb1f-4606-9fed-c40a114828ef","resolution":{"observed_at":"2026-07-08T09:14:46.950577Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:10.62256+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:10.62256+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0210147","last_updated":"2002-11-05T15:42:00Z","snapshot_observed_at":"2026-08-03T14:34:56.331254Z","submitted_at":"2002-10-07T13:49:30Z","title":"The diffuse radio emission from the Coma cluster at 2.675 GHz and 4.85 GHz","version":3},"cited_work":{"arxiv_id":"astro-ph/0210147","doi":"10.1051/0004-6361:20021474","metadata_source":"pith","pith_arxiv_id":"astro-ph/0210147","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The diffuse radio emission from the Coma cluster at 2.675 GHz and 4.85 GHz","venue":"astro-ph","work_id":"8305217e-6341-4a77-9b04-0b29a00da5dc","year":2002},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0210147","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:586859eb1ebc0c4bcedae943899c3b53529a7a09978637cc0c4f9ec9109bdfc8","observation_id":"7c436aac-74f3-4c6d-9db6-a14f6015c767","resolution":{"observed_at":"2026-07-08T09:14:46.934229Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:10.878908+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:10.878908+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2466","last_updated":"2008-05-16T07:54:58Z","snapshot_observed_at":"2026-07-06T01:39:37.564263Z","submitted_at":"2008-05-16T07:54:58Z","title":"Turbulence and Magnetic Fields in the Large Scale Structure of the Universe","version":1},"cited_work":{"arxiv_id":"0805.2466","doi":null,"metadata_source":"pith","pith_arxiv_id":"0805.2466","snapshot_observed_at":"2026-07-10T19:37:33.121045Z","title":"Turbulence and Magnetic Fields in the Large Scale Structure of the Universe","venue":"astro-ph","work_id":"87584388-04c7-4f55-89fc-43271e43ec23","year":2008},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0805.2466","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:42806b121d65672f01a34593305bdea56ce9a7c78f5a48409564b12da4daf151","observation_id":"0e9268a2-714c-4b7c-9f08-727df5d5b74a","resolution":{"observed_at":"2026-07-08T09:14:46.902722Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1009.0570","last_updated":"2010-09-03T02:41:41Z","snapshot_observed_at":"2026-07-06T02:14:57.171269Z","submitted_at":"2010-09-03T02:41:41Z","title":"Faraday Rotation Measure due to the Intergalactic Magnetic Field","version":1},"cited_work":{"arxiv_id":"1009.0570","doi":"10.1088/0004-637x/723/1/476","metadata_source":"pith","pith_arxiv_id":"1009.0570","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Akahori and D","venue":"astro-ph.CO","work_id":"c78c7d23-753e-442c-b4e8-3c4988943fcd","year":2010},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1009.0570","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:26eab08a514044bbfda85db7f8c9e1a62302e725532cd546020d15e036debaf6","observation_id":"b2bb3ae5-95e5-4199-afd3-81d6f28b14ad","resolution":{"observed_at":"2026-07-08T09:14:46.769937Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:11.392286+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:11.392286+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.18580","last_updated":"2024-09-27T09:36:42Z","snapshot_observed_at":"2026-08-07T03:30:17.971848Z","submitted_at":"2024-09-27T09:36:42Z","title":"Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters","version":1},"cited_work":{"arxiv_id":"2409.18580","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.18580","snapshot_observed_at":"2026-07-08T09:14:46.935372Z","title":"Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters","venue":"astro-ph.CO","work_id":"8a6748e3-4056-43f2-871f-81bbbb6f4980","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2409.18580","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:a6fafcd0d1b9fd8533046b2ea034401679202d78956b4b7756ee74f2e13a6568","observation_id":"8a52c9c5-d3ec-487b-8cfc-49818c1a0e27","resolution":{"observed_at":"2026-07-08T09:14:46.936765Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1017/9781139046657","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Shukurov and K","venue":null,"work_id":"db715495-aed6-4c3d-b737-5fbbcb30f5f8","year":2021},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:15303776d4de6ce02b150399f4c53cdb0bd0af0fa9d1a30ebb9818b825d1d567","observation_id":"9266e3a4-95c5-48d4-b6be-7f0f83b65f7d","resolution":{"observed_at":"2026-07-08T09:14:46.864627Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:11.921947+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:11.921947+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.04496","last_updated":"2019-01-14T19:00:01Z","snapshot_observed_at":"2026-07-06T07:26:40.803102Z","submitted_at":"2019-01-14T19:00:01Z","title":"Diffuse Radio Emission from Galaxy Clusters","version":1},"cited_work":{"arxiv_id":"1901.04496","doi":null,"metadata_source":"pith","pith_arxiv_id":"1901.04496","snapshot_observed_at":"2026-07-10T19:37:32.962157Z","title":"Diffuse Radio Emission from Galaxy Clusters","venue":"astro-ph.HE","work_id":"62b82037-10e8-4f50-93e8-912eef2e01a1","year":2019},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1901.04496","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:144ee3cd7a5c2cefd8be909c0ebe08da9a796199e065cb4337d2aaabe0118a90","observation_id":"96bbaf95-56da-49f6-b997-474c79f4a962","resolution":{"observed_at":"2026-07-08T09:14:46.736052Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0404132","last_updated":"2004-07-26T07:31:36Z","snapshot_observed_at":"2026-07-07T00:41:50.878525Z","submitted_at":"2004-04-06T14:25:51Z","title":"Probing Turbulence in the Coma Galaxy Cluster","version":2},"cited_work":{"arxiv_id":"astro-ph/0404132","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0404132","snapshot_observed_at":"2026-07-08T09:14:46.941372Z","title":"Probing Turbulence in the Coma Galaxy Cluster","venue":"astro-ph","work_id":"2f6d2d98-6896-4662-ab06-8b5fbc7be438","year":2004},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0404132","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:72adefaafe2064600a6fc6223d754515f35726c6d2568704ae32dc3f9f54d794","observation_id":"9bc46739-7759-4e84-8c7d-919e53e76bfd","resolution":{"observed_at":"2026-07-08T09:14:46.942770Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0507686","last_updated":"2007-05-14T21:22:11Z","snapshot_observed_at":"2026-08-09T22:26:37.565109Z","submitted_at":"2005-07-29T02:10:04Z","title":"Turbulence and Magnetic Fields in Astrophysical Plasmas","version":3},"cited_work":{"arxiv_id":"astro-ph/0507686","doi":"10.48550/arxiv.astro-ph/0507686","metadata_source":"pith","pith_arxiv_id":"astro-ph/0507686","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Turbulence and Magnetic Fields in Astrophysical Plasmas","venue":"astro-ph","work_id":"4a7f54c0-234a-4daa-a5ac-ad81b0a9466f","year":2005},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"cited_paper":"/paper/astro-ph/0507686","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:782349d9b5bd01f7f37efedb372f7a3cf280a555fd5573a8d7f05bc7da52c9d0","observation_id":"24f77766-cd29-410b-a9be-c546caf8a335","resolution":{"observed_at":"2026-07-08T09:14:46.810391Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:12.961374+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:12.961374+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.02109","last_updated":"2021-12-08T09:09:12Z","snapshot_observed_at":"2026-07-06T12:04:57.395375Z","submitted_at":"2021-11-03T10:06:44Z","title":"Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences","version":2},"cited_work":{"arxiv_id":"2111.02109","doi":null,"metadata_source":"pith","pith_arxiv_id":"2111.02109","snapshot_observed_at":"2026-07-08T09:14:46.843980Z","title":"Effects of Forcing on Shocks and Energy Dissipation in Interstellar and Intracluster Turbulences","venue":"astro-ph.GA","work_id":"b0ba388b-9286-424e-a334-d01230d8d6a5","year":2021},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2111.02109","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:327cf86b33093f5318635b6a92c839ae290a428b4a79f1ce2a962c14b367807d","observation_id":"b43d6007-e817-4c60-bfd5-63e9ca306e8a","resolution":{"observed_at":"2026-07-08T09:14:46.845275Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0402281","last_updated":"2004-10-26T10:41:53Z","snapshot_observed_at":"2026-07-07T00:40:26.527671Z","submitted_at":"2004-02-12T17:33:46Z","title":"Suppression of small scale dynamo action by an imposed magnetic field","version":3},"cited_work":{"arxiv_id":"astro-ph/0402281","doi":"10.1103/physreve.70.036408","metadata_source":"pith","pith_arxiv_id":"astro-ph/0402281","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Suppression of small scale dynamo action by an imposed magnetic field","venue":"astro-ph","work_id":"dcec07d2-ebf8-4a2c-937f-e3dd3e4bd882","year":2004},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0402281","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:948086f789f22d6180a10511994fb14b58902a3b216e0d63183174c8176e2635","observation_id":"a5e36f83-4a27-446d-9679-792cd6827efb","resolution":{"observed_at":"2026-07-08T09:14:46.953143Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:13.524932+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:13.524932+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0312046","last_updated":"2005-01-16T16:14:56Z","snapshot_observed_at":"2026-07-07T00:38:42.432535Z","submitted_at":"2003-12-01T22:27:01Z","title":"Simulations of small-scale turbulent dynamo","version":3},"cited_work":{"arxiv_id":"astro-ph/0312046","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0312046","snapshot_observed_at":"2026-07-09T22:06:34.982560Z","title":"Simulations of small-scale turbulent dynamo","venue":"astro-ph","work_id":"a606cc6c-e3e8-4ba0-b457-85f536037e9c","year":2003},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/astro-ph/0312046","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:6ac3ab7341d53fb6628872dfe13845c72cb15c2102a1ac74b7f9c1de9c19e98d","observation_id":"df6c1d1d-07eb-4d1d-b755-510a179f2f9e","resolution":{"observed_at":"2026-07-08T09:14:46.955921Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2006","doi":"10.1111/j.1365-2966.2006","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"and Yang , J","venue":null,"work_id":"7ef6cf0d-0877-424d-9dec-97ef68ca2212","year":2006},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:2c5e496fff87b3f58a8a6f13dade000c527f7982727b436b3bc141c3b146acfa","observation_id":"280626f2-989f-46b6-9db7-1a53f2c95a7b","resolution":{"observed_at":"2026-07-08T09:14:46.840020Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2009.12024","last_updated":"2020-09-25T04:09:30Z","snapshot_observed_at":"2026-08-05T15:10:27.310205Z","submitted_at":"2020-09-25T04:09:30Z","title":"Seed magnetic fields in turbulent small-scale dynamos","version":1},"cited_work":{"arxiv_id":"2009.12024","doi":null,"metadata_source":"pith","pith_arxiv_id":"2009.12024","snapshot_observed_at":"2026-07-08T09:14:46.924214Z","title":"Seed magnetic fields in turbulent small-scale dynamos","venue":"astro-ph.GA","work_id":"8f3e0991-e001-402e-973a-fafd55687c35","year":2020},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2009.12024","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:26d57a42b51a34ec971a3d66236b950893d0e0f67c6037f29a5e83dd4385c61d","observation_id":"2a05ffb0-1e2b-408b-a345-10167d54750f","resolution":{"observed_at":"2026-07-08T09:14:46.925561Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1504.02311","last_updated":"2016-04-24T10:25:52Z","snapshot_observed_at":"2026-08-06T15:31:35.682302Z","submitted_at":"2015-04-09T13:57:37Z","title":"The origin, evolution and signatures of primordial magnetic fields","version":2},"cited_work":{"arxiv_id":"1504.02311","doi":null,"metadata_source":"pith","pith_arxiv_id":"1504.02311","snapshot_observed_at":"2026-07-10T19:37:33.315170Z","title":"The origin, evolution and signatures of primordial magnetic fields","venue":"astro-ph.CO","work_id":"bd2f1768-4449-43ff-b851-ec016f0a5aff","year":2015},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1504.02311","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:ac40d9d7b6eb55eb5b3fb4e7812ce691cab8430a26a056f29a619ccf541c5c3c","observation_id":"b61c9d18-42d9-462f-99ea-5fbe3e5e7c74","resolution":{"observed_at":"2026-07-08T09:14:46.909612Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.07997","last_updated":"2020-03-18T00:46:53Z","snapshot_observed_at":"2026-08-08T05:43:18.715579Z","submitted_at":"2020-03-18T00:46:53Z","title":"On the saturation mechanism of the fluctuation dynamo at ${\\text{Pr}_\\mathrm{M}} \\ge 1$","version":1},"cited_work":{"arxiv_id":"2003.07997","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.07997","snapshot_observed_at":"2026-07-09T22:06:35.105505Z","title":"On the saturation mechanism of the fluctuation dynamo at ${\\text{Pr}_\\mathrm{M}} \\ge 1$","venue":"astro-ph.GA","work_id":"bc896c6c-7e53-4a7b-9a54-4a1fe62203d7","year":2020},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2003.07997","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:d8404165817e373898891c8c7f4165cf45f6f52e08d56a73d1aac42fa8bcc12d","observation_id":"ba41c5f0-9be9-46dd-9b24-1682a98f9964","resolution":{"observed_at":"2026-07-08T09:14:46.928540Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1507.00342","last_updated":"2015-07-01T20:00:32Z","snapshot_observed_at":"2026-08-07T16:59:37.473305Z","submitted_at":"2015-07-01T20:00:32Z","title":"Turbulent Amplification and Structure of the Intracluster Magnetic Field","version":1},"cited_work":{"arxiv_id":"1507.00342","doi":null,"metadata_source":"pith","pith_arxiv_id":"1507.00342","snapshot_observed_at":"2026-07-08T09:14:46.783739Z","title":"Turbulent Amplification and Structure of the Intracluster Magnetic Field","venue":"astro-ph.CO","work_id":"1a1e287b-0964-4958-94f5-4a6b16cd33ce","year":2015},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1507.00342","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:d36562a2c7cc9aa0c276aed936dcf4b97454aa449cac87d778056f2fd4936c7e","observation_id":"761194ac-4206-4abf-8e42-ba255513bd3f","resolution":{"observed_at":"2026-07-08T09:14:46.785091Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2109.11698","last_updated":"2021-09-24T00:38:45Z","snapshot_observed_at":"2026-08-07T11:31:08.614684Z","submitted_at":"2021-09-24T00:38:45Z","title":"Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas","version":1},"cited_work":{"arxiv_id":"2109.11698","doi":null,"metadata_source":"pith","pith_arxiv_id":"2109.11698","snapshot_observed_at":"2026-07-09T22:06:35.024559Z","title":"Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas","venue":"astro-ph.GA","work_id":"bbe89026-9aac-4414-8612-78802cce8565","year":2021},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2109.11698","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:0b0ec59cae6e0fa1872969eb060a5d7a0bdafe53c0500f32247858cd4be10318","observation_id":"694f4c73-cf14-4ef5-b22c-bd48502a7893","resolution":{"observed_at":"2026-07-08T09:14:46.945402Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1210.3243","last_updated":"2012-11-28T12:22:19Z","snapshot_observed_at":"2026-07-06T02:57:28.205397Z","submitted_at":"2012-10-11T14:11:59Z","title":"Fluctuation dynamos and their Faraday rotation signatures","version":2},"cited_work":{"arxiv_id":"1210.3243","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.3243","snapshot_observed_at":"2026-07-08T09:14:46.789707Z","title":"Fluctuation dynamos and their Faraday rotation signatures","venue":"astro-ph.CO","work_id":"b127288f-83e8-415d-b92e-e5638c46fc42","year":2012},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1210.3243","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:41270fe6d5cf4531200323ac8b33829e497f9709ec7bf2f2eda45a41ac5ccb33","observation_id":"bb12b2d2-9b2b-4f7c-a1d8-6afa4a4b2f35","resolution":{"observed_at":"2026-07-08T09:14:46.791222Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07178","last_updated":"2025-01-06T15:33:57Z","snapshot_observed_at":"2026-08-06T08:24:52.233644Z","submitted_at":"2024-08-13T19:40:23Z","title":"Probing cluster magnetism with embedded and background radio sources in Planck clusters","version":2},"cited_work":{"arxiv_id":"2408.07178","doi":null,"metadata_source":"pith","pith_arxiv_id":"2408.07178","snapshot_observed_at":"2026-07-08T09:14:46.913818Z","title":"Probing cluster magnetism with embedded and background radio sources in Planck clusters","venue":"astro-ph.CO","work_id":"6cd69d12-cbbe-4ad7-8d17-6c6149484f0a","year":2024},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2408.07178","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:81a763ab4ccd5a03724df0ac1bedeae4ee86e458e39eb88b1d7826052a5731c6","observation_id":"b5380196-d083-499a-a64e-848fad2d12b9","resolution":{"observed_at":"2026-07-08T09:14:46.915557Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2604.18338","last_updated":"2026-04-20T14:39:15Z","snapshot_observed_at":"2026-08-10T22:46:08.439996Z","submitted_at":"2026-04-20T14:39:15Z","title":"The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems","version":1},"cited_work":{"arxiv_id":"2604.18338","doi":"10.48550/arxiv.2604.18338","metadata_source":"pith","pith_arxiv_id":"2604.18338","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems","venue":"astro-ph.CO","work_id":"36ad30e1-edf7-4e4e-b9e1-ea2629736dc8","year":2026},"citing_paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-07-08T09:12:09.993795Z"},"links":{"cited_paper":"/paper/2604.18338","citing_paper":"/paper/2607.06346"},"observation_digest":"sha256:0fe8e670222c20bc37eb8bee4c5c4605a15288ffdf094a370d914541a4b65579","observation_id":"dc37bba7-e6a1-4206-b56d-f8fd1a9b01f9","resolution":{"observed_at":"2026-07-08T09:14:46.731161Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-07-10T22:19:16.371804+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-10T22:19:16.371804+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2607.06346","last_updated":"2026-07-07T14:45:29Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-07T08:11:08.873389Z","submitted_at":"2026-07-07T14:45:29Z","title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM"},"reference_resolution":{"displayed":81,"state_counts":{"malformed_identifier":0,"metadata_mismatch":18,"parse_uncertain":0,"unresolved":0,"verified_exact":63,"verified_fuzzy":0},"total_outbound_references":81},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 81 of 81 outbound references and 0 inbound Pith citation observations for arXiv:2607.06346."}