{"as_of":"2026-08-16T05:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4620abf1915edf281ed0141cb7c7b5767a03472ff6210cc0eaedadabcc5f529e","coverage":[{"denominator":75,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":75,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:47:46.870318Z","state":"measured"},{"denominator":75,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":75,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+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/1908.08808/citation-record","integrity":"/paper/1908.08808/integrity","json":"/paper/1908.08808/citation-record.json","paper":"/paper/1908.08808"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.785757Z","title":"& Kravtsov , A","venue":null,"work_id":"690074ec-de0a-4ba9-aa47-1719368972bc","year":2016},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.559069Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:5a0a48ee7b8370777c85fca4b66a6fe89e7a5b0e7617bfd8f7e1ee9980293179","observation_id":"01553ca1-1334-4423-8416-4dad807accc7","resolution":{"observed_at":"2026-08-14T11:47:47.790272Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.564192Z","title":"E., Springel , V., White , S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.564192Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:0b4e359daeb2b4dccf50230156605e829c26ec904a77d9a8593bb962117dfecb","observation_id":"1e930e20-c0fa-49ca-8c2d-56916da10e28","resolution":{"observed_at":"2026-08-14T11:47:46.564192Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.758878Z","title":"S., Wechsler , R","venue":null,"work_id":"3dc4463a-7c08-4c88-999d-62e50d4b25a6","year":2013},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.568794Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:97bd1c99ca72047621804f71cf846480c7004e9216b414e2c4909c2815e5e92f","observation_id":"58946a17-dfde-4ad1-87b2-c7da734ee397","resolution":{"observed_at":"2026-08-14T11:47:47.763227Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.745449Z","title":"2014, , 443, 874","venue":null,"work_id":"3fa17ef7-1846-4010-bf40-5945bddb61d4","year":2014},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.573001Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:8a1859be4775aff1b1be65a93d19aae5aaf5a0a1707366797f25b3098fef1f40","observation_id":"4a42c043-d2de-4bdf-93ad-82fcc117787e","resolution":{"observed_at":"2026-08-14T11:47:47.750391Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.729696Z","title":null,"venue":null,"work_id":"7f2f723f-2c1a-4508-9f62-002ac21031cc","year":2011},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.577074Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:020f9fc2ef1e03e8222dc6d8dff8a133531070933098b21529ed10831932924b","observation_id":"e0bb4b74-be9b-4fd1-8f47-dc68c777fc96","resolution":{"observed_at":"2026-08-14T11:47:47.735423Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.581105Z","title":"B., et al","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.581105Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:46b9bec006a33f738742bd9c26cc5f92eb69f9158c8a6394297d15e0df43f1d2","observation_id":"1f9acd80-e121-41af-88b4-eaba07debbcb","resolution":{"observed_at":"2026-08-14T11:47:46.581105Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.585183Z","title":"R., Faber , S","venue":null,"work_id":null,"year":1984},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.585183Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:f9b15e4b18389fc072a188f1aa87b1f309f59b5ac61542f336c9ac6f37d915be","observation_id":"61ea3c0e-e149-4b18-a41c-d899563fc955","resolution":{"observed_at":"2026-08-14T11:47:46.585183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.588941Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.588941Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:69b434b9260e7996102ffbfc43af4e80c7a99b48f4c918fc13a8458321355cfb","observation_id":"acc7cb37-d165-4616-a1ef-68840d135215","resolution":{"observed_at":"2026-08-14T11:47:46.588941Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.691415Z","title":"2000, PhD thesis, Astronomy Department, Padova University, Vicolo Osservatorio 2, 35122 Padova, Italy","venue":null,"work_id":"cf0ab281-0580-419b-83e7-325fb89e4534","year":2000},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.592617Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1e69ef2de972052d63a0386be083fc328d492619bbbaa1e691a2e150cde2727a","observation_id":"90cb1cb7-fe27-4061-b94d-1c204bf90113","resolution":{"observed_at":"2026-08-14T11:47:47.696792Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.596342Z","title":"1997, , 114, 1365","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.596342Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:382d89ce198f7671bfb2e4b2f4c48c47aa6054783ca4a2de0e1b29077f9f9051","observation_id":"ac86c8f6-1f3f-4c2d-b259-eb1c75665085","resolution":{"observed_at":"2026-08-14T11:47:46.596342Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.663561Z","title":"B., Grillo , C., Rosati , P., et al","venue":null,"work_id":"1fd9c7e6-be3e-4921-92e1-31e928ab1328","year":2017},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.601826Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:2ddc51c74ccf27574bc5fff8cb2a21796cd4fe0c4a6eec4e966f01c11da78794","observation_id":"ec64d9f8-b92e-4a4d-aba6-aefdac15b277","resolution":{"observed_at":"2026-08-14T11:47:47.670553Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.606021Z","title":"2018, , 609, A133","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.606021Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1d9a128f1da0eb08970cde137f8d75e76e8ddfadc07a222e47ac8e39f25f5540","observation_id":"50800969-0fe0-4ba3-837d-8216e14a1c40","resolution":{"observed_at":"2026-08-14T11:47:46.606021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.609563Z","title":"M., et al","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.609563Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:785e069eb4f8983353ba3946f31e8d1d5d3c4c2adf3f46546b1bfe036792e6ec","observation_id":"27ce1ab5-7580-4923-a9f2-c8187fe2465b","resolution":{"observed_at":"2026-08-14T11:47:46.609563Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.622293Z","title":"& Carraro , G","venue":null,"work_id":"b855627c-9cdd-4e74-b919-b4f9e733effa","year":2002},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.613180Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:95b0831b4ce7ac4ceb7e066062acad32b82c7fa46e599dbdac682f797dec4224","observation_id":"b183715b-7b85-4c95-a9e1-307c44dc1e53","resolution":{"observed_at":"2026-08-14T11:47:47.629810Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1206.2532","last_updated":"2012-08-21T11:37:40Z","snapshot_observed_at":"2026-08-15T00:57:09.389644Z","submitted_at":"2012-06-12T13:46:48Z","title":"The Origin of the Mass-Radius Relation of Early-Type Galaxies","version":4},"cited_work":{"arxiv_id":"1206.2532","doi":null,"metadata_source":"pith","pith_arxiv_id":"1206.2532","snapshot_observed_at":"2026-08-14T11:47:47.029302Z","title":"The Origin of the Mass-Radius Relation of Early-Type Galaxies","venue":"astro-ph.CO","work_id":"e733eae6-c530-4c73-bc33-2fbf0e536b1d","year":2012},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.618078Z"},"links":{"cited_paper":"/paper/1206.2532","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1e12f75c9ff57b77c93295c962f4f4dc94364617dc23b1d3ed9b9e503628e364","observation_id":"fc11b9c8-25e4-4126-b1c4-c861ae33d9dd","resolution":{"observed_at":"2026-08-14T11:47:47.034191Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.608635Z","title":"G., Buta , R","venue":null,"work_id":"5098282a-9004-4b60-bf14-c6bdbd687401","year":1994},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.622349Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:b4c73dab76d6f94e16da5b0399db9a5eb3337a3a297318554294a0c352592a32","observation_id":"63b7e604-220a-47a3-9476-1e42aa1eca45","resolution":{"observed_at":"2026-08-14T11:47:47.613004Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.626742Z","title":"G., et al","venue":null,"work_id":null,"year":1991},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.626742Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:df1429eb74e649056644e8b878b7214c2b705dfe0ecb75c4d2cfba8a07bf2232","observation_id":"73573e6b-7d37-4714-82f4-eb95a78bd912","resolution":{"observed_at":"2026-08-14T11:47:46.626742Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.631019Z","title":"2014, , 572, A87","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.631019Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:c776e777097e914903db522b1fbdd2cc789e20f0bf991149aaeac86cf8074a38","observation_id":"c300251f-c232-4c18-a9e5-c3cdf5725e5e","resolution":{"observed_at":"2026-08-14T11:47:46.631019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.579954Z","title":"2019 a , , submitted","venue":null,"work_id":"afe7aafe-43a9-4050-8646-888b92d7bef1","year":2019},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.635366Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:124287005f5bb63b7e066c8855a132a86951590ce13577b810eeaa6a31b5c943","observation_id":"741d3f9b-f419-40d7-810a-621a34588029","resolution":{"observed_at":"2026-08-14T11:47:47.584204Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.565970Z","title":"2019 b , , 875, 103","venue":null,"work_id":"d07d654e-683e-48c1-ba38-d829f107822a","year":2019},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.639284Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1f39d66bd6881c52610d87a0300f2a44ef35b45c78f9631e57f3793aa3212759","observation_id":"22ea28ef-4e97-4812-bab8-3eb573db7c97","resolution":{"observed_at":"2026-08-14T11:47:47.571114Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.11119","last_updated":"2022-02-04T13:59:54Z","snapshot_observed_at":"2026-08-12T23:43:21.825693Z","submitted_at":"2020-02-25T19:00:00Z","title":"The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations","version":4},"cited_work":{"arxiv_id":"2002.11119","doi":null,"metadata_source":"pith","pith_arxiv_id":"2002.11119","snapshot_observed_at":"2026-08-14T11:47:47.009414Z","title":"The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations","venue":"astro-ph.GA","work_id":"8550a95d-4dec-4674-9412-9a1b96cd8ba9","year":2020},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.643506Z"},"links":{"cited_paper":"/paper/2002.11119","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:113cfedec1413c0c1b4410e163dfc1ba807f258c4bb7ce64dc0f90ed77068e77","observation_id":"8c1f52aa-a440-4a5c-a338-27c1b4c3176d","resolution":{"observed_at":"2026-08-14T11:47:47.014951Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.553695Z","title":null,"venue":null,"work_id":"b0b88b96-a895-4a7e-8f74-7f1946dffc0b","year":1984},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.648016Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:4e17778d1144117442a05bafde982d170df642bf93269f453e82cff33c49d520","observation_id":"61b3a267-8706-4a06-9bb8-0aa524b5ebba","resolution":{"observed_at":"2026-08-14T11:47:47.557467Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.652321Z","title":"2010, , 718, 1460","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.652321Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:5b9c9336954b70f56293002a778de465dfd97f0c28b3c99828a7ded7986b15fb","observation_id":"783a696c-aa30-45f6-a371-5fbc9d879153","resolution":{"observed_at":"2026-08-14T11:47:46.652321Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.656654Z","title":"2006, , 445, 805","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.656654Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:77734e68f7018ffa999d091cca317be7d836265492fb52141a7760eaa531c859","observation_id":"3308d2cd-2055-4cc8-92c7-9ce939ebec1c","resolution":{"observed_at":"2026-08-14T11:47:46.656654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.660635Z","title":"2012, , 420, 926","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.660635Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:5ded089a9e1e8b456625be6d53e8a3a7227a58de8e7566f9726fff4f7f332f67","observation_id":"be47e4c1-c44a-4bae-9b4e-26ebc416ec90","resolution":{"observed_at":"2026-08-14T11:47:46.660635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.664896Z","title":"M., Bettoni , D., et al","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.664896Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:23a63d27da2dbf50863f54bdd74da3fde9c1333af22072948bc10a8f2a9be5bd","observation_id":"e70b1769-b384-4fae-b96d-dd967bee7dfb","resolution":{"observed_at":"2026-08-14T11:47:46.664896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.504362Z","title":"M., Cava , A., et al","venue":null,"work_id":"f91f64d6-bab8-4a6d-a3b2-88fb0da16f99","year":2011},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.669599Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:bd46a70e50307af4c6a339ba15805310941e4c0496c05e7680587b4cb3fb3ec5","observation_id":"b9aefcd6-0262-4d6f-9612-69e640497a0a","resolution":{"observed_at":"2026-08-14T11:47:47.509061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.489668Z","title":"R., Masjedi , M., & West , A","venue":null,"work_id":"de0f30aa-47db-4a2e-9d03-14a1cdd44825","year":2006},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.673560Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:d839d23d54516161a34baa91b89ee9ac5d6c61f1863e72e953669127eba91a25","observation_id":"84c80158-e0f9-46e1-9956-3a63e235256a","resolution":{"observed_at":"2026-08-14T11:47:47.493824Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.476041Z","title":"2018, , 474, 3976","venue":null,"work_id":"9fed1c13-0d07-43dd-8bea-354a77b18437","year":2018},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.678059Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:dd34e9f8493cc6f2cbe3638569126bf1d2dd2e4e0d1b11833855229bd8f91b76","observation_id":"0b3e1ad5-fef8-4ecc-977a-6a9e9e0af79c","resolution":{"observed_at":"2026-08-14T11:47:47.481068Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.461442Z","title":"2014, , 445, 175","venue":null,"work_id":"125cf5cc-ad48-418a-a819-fc2df86bba48","year":2014},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.682035Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:9c30056b87e12974ec9dc10fb85cdc73c514a4b857fd142633b20062958f54d5","observation_id":"e7cccc5c-81cb-4a64-b175-970471267194","resolution":{"observed_at":"2026-08-14T11:47:47.465970Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2001.02230","last_updated":"2020-01-16T09:05:54Z","snapshot_observed_at":"2026-08-10T06:30:42.140594Z","submitted_at":"2020-01-07T19:00:00Z","title":"The stellar-to-halo mass relation over the past 12 Gyr","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.02230","snapshot_observed_at":"2026-08-14T11:47:46.686598Z","title":"2020, arXiv e-prints, arXiv:2001.02230","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.686598Z"},"links":{"cited_paper":"/paper/2001.02230","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:626126ed33c1e606b32126fe1c0d7310b782b8502cb9d1a47ffbe3a2a4e136fa","observation_id":"d383fb87-7518-4da3-9056-64221483bf2b","resolution":{"observed_at":"2026-08-14T11:47:46.686598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.448016Z","title":null,"venue":null,"work_id":"3813a5d9-69c8-45d8-b71b-5819259cbf93","year":1975},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.690679Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:6733195f109f6258a0700e0d870df4142fdc54442c2c312af1d4f3281c1de152","observation_id":"8d79b237-6137-4a9b-9e4d-3becbe5c178c","resolution":{"observed_at":"2026-08-14T11:47:47.452249Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1108.0997","last_updated":"2011-08-04T06:13:58Z","snapshot_observed_at":"2026-08-15T04:39:06.021057Z","submitted_at":"2011-08-04T06:13:58Z","title":"A review of elliptical and disc galaxy structure, and modern scaling laws","version":1},"cited_work":{"arxiv_id":"1108.0997","doi":null,"metadata_source":"pith","pith_arxiv_id":"1108.0997","snapshot_observed_at":"2026-08-14T11:47:46.970471Z","title":"A review of elliptical and disc galaxy structure, and modern scaling laws","venue":"astro-ph.CO","work_id":"71cb5fc7-81d3-4d5f-a019-511a5e7a91d1","year":2011},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.694194Z"},"links":{"cited_paper":"/paper/1108.0997","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:64db1a8335fb22fbb456667c3aa466d8420bbaf16b81626ea217d03403314c83","observation_id":"95653d91-4f0c-487d-9994-361ad776c5f6","resolution":{"observed_at":"2026-08-14T11:47:46.976096Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.434036Z","title":null,"venue":null,"work_id":"928d67ff-8c33-4a38-92b8-250a48749033","year":2013},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.698812Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:9cc89dc632db68f49494122846d4aa860161166a93254e07a1d4d2c61a779125","observation_id":"b2e98bf8-ce38-417c-b168-9e0fcf17cc9e","resolution":{"observed_at":"2026-08-14T11:47:47.438386Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.702542Z","title":"2015, , 581, A41","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.702542Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:cfa5d36e2a6de2655527071677bb77a7fb6931ae739a6301bb6f4cd0a5696ef0","observation_id":"51552a83-939f-4fb5-90ff-555bcf509668","resolution":{"observed_at":"2026-08-14T11:47:46.702542Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.413948Z","title":"H., Mo , H","venue":null,"work_id":"622e5f08-9152-4251-802f-b9b795af51de","year":2009},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.706187Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:c18050f72f853c647df67da98e57d2bd9dd0363bd433caa21422f61ddcfa02af","observation_id":"7fe4c727-01c1-4ad3-a26d-92147de5d7f2","resolution":{"observed_at":"2026-08-14T11:47:47.417894Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.401733Z","title":"F., Khosroshahi , H","venue":null,"work_id":"cd60a6a0-507a-465e-a922-53c624b6a9ea","year":2019},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.710355Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:821c71429d9b7cf7d70b50b49479e318e9132826175e6ba6cbc80b155a335119","observation_id":"d73e707a-6432-4203-8ae2-2b7a80683521","resolution":{"observed_at":"2026-08-14T11:47:47.405629Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.389125Z","title":"1992, , 400, 460","venue":null,"work_id":"b4067bf9-100a-43ae-b9cf-8a59a111731f","year":1992},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.714718Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:cdead0cd6aef83b714a991c0ba84047795dd2f0677cfe97d74670d5487546d61","observation_id":"ff265a75-762b-4369-9d35-2cd6201108fe","resolution":{"observed_at":"2026-08-14T11:47:47.393235Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.375562Z","title":"1993, , 409, 548","venue":null,"work_id":"1109a655-0e40-4258-98d1-13eecdc9e39f","year":1993},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.718716Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:c7355f935b807d064fa7dbc99742bd19666ebeea4464b5f8894b4d7d737b0864","observation_id":"0bea69c5-76a0-40c2-bdb2-73bf8a2c2fa0","resolution":{"observed_at":"2026-08-14T11:47:47.380201Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.723326Z","title":"2013, , 208, 19","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.723326Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1360fd7b4bc8394ffde49a4cb719398dda830743b5e3c0cbbf46e919d0710763","observation_id":"f9e43cad-1ec2-4919-88fc-d1ff77689e86","resolution":{"observed_at":"2026-08-14T11:47:46.723326Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.727325Z","title":"M., Ferguson , H","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.727325Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:006024eb4f527bb1fa31bc015fb4e0aa60d71c79b43c2f8a834223130e0d8462","observation_id":"fcdc6b65-76b0-4a74-8d80-3aac8ea81195","resolution":{"observed_at":"2026-08-14T11:47:46.727325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.347137Z","title":"M., Gebhardt , K., et al","venue":null,"work_id":"48324e3c-7236-4705-b4a9-bae8d19baf50","year":2001},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.731149Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:b11a61139eb0788774c575ae4363330202e6dec63f2e7cec6131e4df0e3db444","observation_id":"02e0a033-051c-4bb5-aebd-78aec0ef4f51","resolution":{"observed_at":"2026-08-14T11:47:47.351224Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.334203Z","title":"2011, , 730, 61","venue":null,"work_id":"05d0e368-6ccd-41e0-aec6-0390ac4b3ac3","year":2011},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.735263Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:c38edcdc1eca11179740a9ae61ae47321e264f3278d5fc415c95425af5980864","observation_id":"a806ba22-64c5-451a-ae23-ce18333a2167","resolution":{"observed_at":"2026-08-14T11:47:47.338506Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.321127Z","title":"2006, , 448, 1031","venue":null,"work_id":"37187f50-23b2-409e-aafc-89fcfcd31b15","year":2006},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.739157Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:3f8069b5d176806ecc365bb023578c0b9da6ca357827a26d9aa04aa2c14c9cc2","observation_id":"63a9077a-f297-406d-9b66-a130720fd4df","resolution":{"observed_at":"2026-08-14T11:47:47.324852Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.310312Z","title":null,"venue":null,"work_id":"abba9a5d-0176-4389-ad5b-0e3b0ef9799a","year":2007},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.743313Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:4422884ba674ff17fbb40cba2767f4c09b16b246741e7b3ca17ad972d7c96db5","observation_id":"e2627fba-1dd7-42fa-838a-0874591f6d68","resolution":{"observed_at":"2026-08-14T11:47:47.313824Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.298503Z","title":"2017, , 604, A54","venue":null,"work_id":"1b1f18fe-e176-44d3-bab3-22666ea401cb","year":2017},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.747282Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:e06af3a4183e1384c0945696a47568ba6d07401a1e3f3bfc4472fd0ba1d692ed","observation_id":"8579ce55-c4f2-42e5-8971-3692eb52ea55","resolution":{"observed_at":"2026-08-14T11:47:47.302464Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.285553Z","title":null,"venue":null,"work_id":"2cc56385-15b0-430e-8a3a-a5438cf9eee0","year":2003},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.751132Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:91b8da7b50731008ff86e3de8c5f06bc765b177fc4bd2981cb56d6d0faa0cf3c","observation_id":"fa5f94d0-182a-47f2-bf0d-6c78951343fd","resolution":{"observed_at":"2026-08-14T11:47:47.290063Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.755640Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.755640Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:a80702a9c3f797f07a27fe59d3cfa9cbb69553abdb1eb49db62ea8f6b749b42b","observation_id":"62f8db6d-ec7d-4d81-baba-537d5ff8cd81","resolution":{"observed_at":"2026-08-14T11:47:46.755640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.266218Z","title":"2009, , 500, 705","venue":null,"work_id":"770d69b9-6711-4657-aed0-2b825c96f50e","year":2009},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.759672Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:fa631f3dafacfa27d1cefc7f003812bb8903e656824a18ffbe60383fa063c4fe","observation_id":"290c788a-3887-4370-9422-d53a53841d97","resolution":{"observed_at":"2026-08-14T11:47:47.270276Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.254347Z","title":"2010, , 513, A36","venue":null,"work_id":"489a932a-8db5-4bc4-98fa-09fee2dc6960","year":2010},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.763706Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:6dba2605fe0e1649ed9426c3e0f625ca019d85a2ac342802742a10335ef9f94f","observation_id":"28899bbb-e28a-4120-9ba3-7c3685631b09","resolution":{"observed_at":"2026-08-14T11:47:47.258187Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.242715Z","title":"& Chiosi , C","venue":null,"work_id":"4faeaef9-371b-465c-8264-dd4d798d2c1f","year":2006},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.767663Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:3d5d506e004e643c0f8743eabaa1bd5092cb9be1f9bd6d8ebc4235391bde6135","observation_id":"5200558f-3b5c-4e00-90f9-574a3a2970f1","resolution":{"observed_at":"2026-08-14T11:47:47.246676Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.230926Z","title":"& Chiosi , C","venue":null,"work_id":"20f3cedf-b022-4393-9c66-1b20b0e839db","year":2007},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.771627Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:a0e10a5260bdd48cc66019cf9c34a2e5a820e38050cb217bee583347b9ee9209","observation_id":"0c35b048-d85d-4d50-bc46-b8cd271127f1","resolution":{"observed_at":"2026-08-14T11:47:47.234774Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.5118","last_updated":"2012-08-17T14:38:54Z","snapshot_observed_at":"2026-08-15T04:12:12.707307Z","submitted_at":"2012-04-23T17:21:06Z","title":"Formation and Evolution of Early-Type Galaxies. III Star formation history as a function of mass and over-density","version":2},"cited_work":{"arxiv_id":"1204.5118","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.5118","snapshot_observed_at":"2026-08-14T11:47:46.948715Z","title":"Formation and Evolution of Early-Type Galaxies. III Star formation history as a function of mass and over-density","venue":"astro-ph.CO","work_id":"f4c08e0e-2033-4255-9eff-31be2a5c962c","year":2012},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.775923Z"},"links":{"cited_paper":"/paper/1204.5118","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:4e448478a01ba2fbf916d23cb8f5a81897dfcfcddcef44523ae9871393f6fa4c","observation_id":"1d4fab60-3a97-4341-97a5-673a51e2dc64","resolution":{"observed_at":"2026-08-14T11:47:46.953952Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.780107Z","title":"2017, , 599, A81","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.780107Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:0d1270e41d850dc59789a43a0fa49ced676a35104e7d237e21527f224c50018d","observation_id":"61372e84-00af-4880-9e33-4a60642de226","resolution":{"observed_at":"2026-08-14T11:47:46.780107Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.784037Z","title":"M., Fasano , G., et al","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.784037Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:3425f06718caec8bd93961c782a8ac2abe793f59b88664351b4854bed235da49","observation_id":"fa31a3f6-798c-4878-b1a8-123e59f8ff72","resolution":{"observed_at":"2026-08-14T11:47:46.784037Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.788620Z","title":"2015, Astronomy and Computing, 13, 12","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.788620Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:9d56cac3884222a1082123d31ef375c93177d3cd4f48f9efc3c0e2bff1a524bb","observation_id":"c65cd083-808f-47d6-80b3-3d88e0734e71","resolution":{"observed_at":"2026-08-14T11:47:46.788620Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.196795Z","title":"& Bertin , G","venue":null,"work_id":"b6d5f980-8373-421e-aa69-a96fd183e17a","year":2008},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.792361Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:b50860ce417e94d97f9a85ff89b462d827e21d88ce6553fb8dfd43ed1515126f","observation_id":"32f51329-c1c0-4d0a-ab11-765825e5a078","resolution":{"observed_at":"2026-08-14T11:47:47.200776Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.796839Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.796839Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:eae8e82c0dfd75de445b6b1922dad05339bcbdeeda480ffe8cdc5cb8092e71ca","observation_id":"9e623990-2504-48b8-bb9b-cbf92b00fc0f","resolution":{"observed_at":"2026-08-14T11:47:46.796839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.177113Z","title":"2019, , 870, 70","venue":null,"work_id":"1d031524-2e32-420e-92df-c539ef380fef","year":2019},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.801237Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:2346d5e655c8a07d4793b04469ef36fcf336a63ade5455223a2ecec4e8f9cbba","observation_id":"aa426889-441b-4f3e-9f6f-8f04a89708a2","resolution":{"observed_at":"2026-08-14T11:47:47.181037Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.805313Z","title":"2006, , 643, 14","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.805313Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:a28013b015df6256e8a12b3d37af1939a33380ca7232e9389102923170917ded","observation_id":"18102097-07ed-4415-b177-8f3888e54b9b","resolution":{"observed_at":"2026-08-14T11:47:46.805313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.6043","last_updated":"2012-09-15T08:21:24Z","snapshot_observed_at":"2026-08-15T04:45:15.224740Z","submitted_at":"2011-05-30T17:13:23Z","title":"Size Evolution of Spheroids in a Hierarchical Universe","version":2},"cited_work":{"arxiv_id":"1105.6043","doi":null,"metadata_source":"pith","pith_arxiv_id":"1105.6043","snapshot_observed_at":"2026-08-14T11:47:46.927795Z","title":"Size Evolution of Spheroids in a Hierarchical Universe","venue":"astro-ph.CO","work_id":"ead99506-be06-4a5a-9738-46a5a0082af8","year":2011},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.808907Z"},"links":{"cited_paper":"/paper/1105.6043","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:974b9352195ecd1598f16c68fcc0ed23d72387823d5f449b326fb0ad19b000f7","observation_id":"97ff80db-a11e-4b52-a2ce-d51f9e4322dd","resolution":{"observed_at":"2026-08-14T11:47:46.934437Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.813810Z","title":"J., White , S","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.813810Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1ea0b1b4133c885c4abaa5394a7e37c8977639323f6e174cc51389d722031a94","observation_id":"f440f574-5759-4717-ae76-431b8cbd5ee4","resolution":{"observed_at":"2026-08-14T11:47:46.813810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.817295Z","title":"S., Behroozi , P., Pandya , V., et al","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.817295Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:2a78049ad0a3f83f57fdcfe7542d2b872b1b54c17c8080f58472583c2bfebf29","observation_id":"a6a43275-594c-4d22-8051-fc7602c73160","resolution":{"observed_at":"2026-08-14T11:47:46.817295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.821014Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.821014Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:1f9e9b4ba85c1a00a32154b20385ac57293484fa33a0477bf91462accbbab769","observation_id":"6ffc0a25-6a88-473c-9527-6e9f17762223","resolution":{"observed_at":"2026-08-14T11:47:46.821014Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.02747","last_updated":"2019-06-06T18:00:00Z","snapshot_observed_at":"2026-08-14T16:19:39.270489Z","submitted_at":"2019-06-06T18:00:00Z","title":"The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.02747","snapshot_observed_at":"2026-08-14T11:47:46.824763Z","title":"A., Bell , E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.824763Z"},"links":{"cited_paper":"/paper/1906.02747","citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:a048fd4e8c853a340e36082e48b92229b282cc266f2054606862396e2c5029d6","observation_id":"2e90a550-a70f-4099-8e48-df0176c5bc6d","resolution":{"observed_at":"2026-08-14T11:47:46.824763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.132299Z","title":"M., et al","venue":null,"work_id":"9947078a-9966-4c87-81dd-b8cb2a74af94","year":2010},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.828490Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:cf12fefbb8ab014eb0e06010ea1132d0cfba38945ede2ff37a78f0c4af6cdac7","observation_id":"9d3ab4f9-8cff-4a7b-a883-cd02b8018dc3","resolution":{"observed_at":"2026-08-14T11:47:47.137072Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.119353Z","title":"M., Fasano , G., et al","venue":null,"work_id":"8fbbb122-de0d-45e2-8f5f-d4708ffa129b","year":2011},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.832387Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:28bd9a0e68d69cd8b5f1f36952ad803d5c7b1ccd6c1699cbf50a1ca1e9adddd3","observation_id":"b166fd4d-101c-41e9-8bb4-4dc36bbf4259","resolution":{"observed_at":"2026-08-14T11:47:47.124260Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.835958Z","title":"G., Whitaker , K","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.835958Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:91f54201a97fe2be7961c4a26522cd2f975680771b2c8281170b385272fc24a2","observation_id":"b3a1a2f8-e94e-4724-a511-e642b8f6ccd2","resolution":{"observed_at":"2026-08-14T11:47:46.835958Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.842030Z","title":"2009, , 497, 667","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.842030Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:6b5058ce247496303c31aff3477c458c3b06890edd8153f78be2fe3e12e55e96","observation_id":"ad47346b-5e55-4a15-92c0-a1594623712d","resolution":{"observed_at":"2026-08-14T11:47:46.842030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.846022Z","title":"2014 a , , 509, 177","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.846022Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:bd7ef2b5b26716d4fd6fdd7ff6042d9ed5b3553685078f721e35933b6d667949","observation_id":"41fde255-7a3f-4de7-a1dc-10e0ea29e226","resolution":{"observed_at":"2026-08-14T11:47:46.846022Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.850207Z","title":"2014 b , , 444, 1518","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.850207Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:7958b08f0ac0710f569e1d92dc515caa4021f59350db2393fadd32b1f8a8e8c3","observation_id":"c6510666-89f7-4013-b253-0ab6247df669","resolution":{"observed_at":"2026-08-14T11:47:46.850207Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.072799Z","title":"2006, The Messenger, 126, 7","venue":null,"work_id":"f33e3dd7-7059-4236-873e-d10078f42868","year":2006},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.854758Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:e8669d2770980ef0245ee203ec7e8b7401a9337e1c29a1cbea08572cba3266a9","observation_id":"6fb7303a-60d9-4182-b278-a8f6cdbeb9ac","resolution":{"observed_at":"2026-08-14T11:47:47.076687Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:47.059499Z","title":"2008, , 390, 1453","venue":null,"work_id":"49772fc5-d693-4111-838b-864e18cc445e","year":2008},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.858984Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:49cf8df241155a96c7173d56b7b322705c088cd1fffda01791be139b501e878e","observation_id":"93f6b65b-7f2c-487a-bc7f-2fc0bd304a89","resolution":{"observed_at":"2026-08-14T11:47:47.063504Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.864980Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.864980Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:ddba0ea059b3b957297d75f4b876954d3341d066f287f00b48c7b8d802903c25","observation_id":"46b478df-9bab-47f7-9abd-94eb1d253af9","resolution":{"observed_at":"2026-08-14T11:47:46.864980Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:47:46.870318Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship","version":2},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-14T11:47:46.870318Z"},"links":{"citing_paper":"/paper/1908.08808"},"observation_digest":"sha256:969c6ee5132d141c11350387f97a40e10db272b4d797f9c3665230cf2ad89f34","observation_id":"eae4a505-d783-4043-b429-aee0c52b6eae","resolution":{"observed_at":"2026-08-14T11:47:46.870318Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"1908.08808","last_updated":"2020-06-27T10:27:09Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-16T03:36:17.209922Z","submitted_at":"2019-08-22T13:05:31Z","title":"The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship"},"reference_resolution":{"displayed":75,"state_counts":{"malformed_identifier":0,"metadata_mismatch":3,"parse_uncertain":0,"unresolved":39,"verified_exact":2,"verified_fuzzy":31},"total_outbound_references":75},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 75 of 75 outbound references and 0 inbound Pith citation observations for arXiv:1908.08808."}