{"as_of":"2026-08-15T13:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:da45cf500e1246e99c9414111aa3d94541a0b973c2a0b48d2e49203c1b0315e0","coverage":[{"denominator":139,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T18:01:50.961206Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"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/2412.08336/citation-record","integrity":"/paper/2412.08336/integrity","json":"/paper/2412.08336/citation-record.json","paper":"/paper/2412.08336"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.433401Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.433401Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:3d45d3dfb845a3d73433a291eb850593a2ba020bc26d6adff7f6a94121a22486","observation_id":"ce53d354-317e-4d46-a233-691151930f06","resolution":{"observed_at":"2026-08-11T18:01:50.433401Z","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":"2026-08-11T18:01:50.443668Z","title":"V., et al., 2023, @doi [ ] 10.1051/0004-6361/202244634 , https://ui.adsabs.harvard.edu/abs/2023A&A...670A..95A 670, A95","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.443668Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:55e95aa20e46f5b7061b30cd36aa1f8f6b61d35de4cc7ff5145343c72b54932a","observation_id":"bedc9b54-9f81-48fe-a474-e8ffb03872ce","resolution":{"observed_at":"2026-08-11T18:01:50.443668Z","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":"2026-08-11T18:01:50.452872Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.452872Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:6a4dde8d66e73670e833030cd536ff37e27483c9b5f7d7640501aecdf0f10437","observation_id":"c8c5b895-8ed8-4e29-bfc4-e5aa97d487dc","resolution":{"observed_at":"2026-08-11T18:01:50.452872Z","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":"2026-08-11T18:01:50.460115Z","title":"X., et al., 2014, @doi [ ] 10.1088/0004-637X/784/2/152 , https://ui.adsabs.harvard.edu/abs/2014ApJ...784..152A 784, 152","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.460115Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:70b236ce80664e2d72cba12d2a2b98b3edb67bcc2173d24fcb8fa673e97fe67e","observation_id":"a620892e-7516-4f23-87b6-eb17be979a1b","resolution":{"observed_at":"2026-08-11T18:01:50.460115Z","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":"2026-08-11T18:01:50.466179Z","title":"J., Cowie L","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.466179Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:06e20bad54b35bd735a43ba121689bf2d6418977141eba2d5b9a076e484ff58a","observation_id":"28358100-732e-42a0-8844-6f27c4309d5b","resolution":{"observed_at":"2026-08-11T18:01:50.466179Z","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":"2026-08-11T18:01:50.472092Z","title":"C., Flynn K., Gebhardt K., 1990, @doi [ ] 10.1086/115487 , https://ui.adsabs.harvard.edu/abs/1990AJ....100...32B 100, 32","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.472092Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:d4ea0e7a0ba6471033b2037b3cd6d31cdc330e8c09b66010cfaaeebfa7a59248","observation_id":"4febada5-c17f-47ef-b5c7-85340db12cef","resolution":{"observed_at":"2026-08-11T18:01:50.472092Z","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":"2026-08-11T18:01:50.479256Z","title":"F., McIntosh D","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.479256Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:621c7aee8f0c240a137be11f9962467c5cc9a774bc7838417cf4555c89de1382","observation_id":"da536c4e-402e-4936-beb8-913d6a27747d","resolution":{"observed_at":"2026-08-11T18:01:50.479256Z","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":"2026-08-11T18:01:50.485308Z","title":"R., Kofman L., Pogosyan D., 1996, @doi [ ] 10.1038/380603a0 , https://ui.adsabs.harvard.edu/abs/1996Natur.380..603B 380, 603","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.485308Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:37163bbdb934fd11ce9efa04c783d41696736aad5a4e1f73630d42d4897fde04","observation_id":"7ae23796-5cf4-4e4e-8a5b-8bc7987944c5","resolution":{"observed_at":"2026-08-11T18:01:50.485308Z","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":"2026-08-11T18:01:50.490411Z","title":"L., Storchi-Bergmann T., 1994, @doi [ ] 10.1086/174346 , https://ui.adsabs.harvard.edu/abs/1994ApJ...429..582C 429, 582","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.490411Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:bcda415301ef1f56fd4c4a78a9ad5738cc60cddbe983c7bc54e68884d5d73d8f","observation_id":"cb2b26f4-f3b6-4c55-992c-e119172cae25","resolution":{"observed_at":"2026-08-11T18:01:50.490411Z","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":"2026-08-11T18:01:50.495733Z","title":"M., 2016, @doi [ ] 10.3847/0004-637X/824/1/36 , https://ui.adsabs.harvard.edu/abs/2016ApJ...824...36C 824, 36","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.495733Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:a8736005436a1425faccd3ae9dae8c257bb6e24d65fecdfc0426f6b77f990fc3","observation_id":"a6efd9ca-9c36-44d0-9cd2-f646b1e99c58","resolution":{"observed_at":"2026-08-11T18:01:50.495733Z","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":"2026-08-11T18:01:50.500758Z","title":"M., et al., 2015, @doi [ ] 10.1088/2041-8205/808/2/L33 , https://ui.adsabs.harvard.edu/abs/2015ApJ...808L..33C 808, L33","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.500758Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:fd8aebe09ebcc32efc748506d099d88b1043f8b8857cdd94704fc0ac7acb9fd6","observation_id":"2022d358-cca0-4de4-a1ef-a7ddceabb504","resolution":{"observed_at":"2026-08-11T18:01:50.500758Z","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":"2026-08-11T18:01:50.507244Z","title":"M., 2000, @doi [ ] 10.1086/309250 , https://ui.adsabs.harvard.edu/abs/2000ApJ...539..718C 539, 718","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.507244Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:245824195dfad2516f167987b98d0ad78c211584315a8cc9f7479843e2c0a5e0","observation_id":"b0e655a9-6137-4654-8962-4c5ce847c063","resolution":{"observed_at":"2026-08-11T18:01:50.507244Z","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":"2026-08-11T18:01:50.513227Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.513227Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:c895ca8921c8a764641ebe1bba4d9fdf0c1848000da47745ae987046e388e244","observation_id":"2ece6654-4b80-4543-abed-d91e1e9d14ab","resolution":{"observed_at":"2026-08-11T18:01:50.513227Z","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":"2026-08-11T18:01:50.518934Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.518934Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:abb9f928ba0ed421769393fb61511302f4b0665926a31f856bc06d3b8539c77b","observation_id":"9c28f81a-7205-48ca-91da-c2a02084269b","resolution":{"observed_at":"2026-08-11T18:01:50.518934Z","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":"2026-08-11T18:01:50.523958Z","title":"L., et al., 2011, @doi [ ] 10.1088/0004-637X/741/1/8 , https://ui.adsabs.harvard.edu/abs/2011ApJ...741....8C 741, 8","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.523958Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:c79699398ce779d57c68000a0fe1c8322dbd1a190e034db0f07b0736ee779bed","observation_id":"18610ad0-a6d9-4c90-b20e-ff40b72d56f0","resolution":{"observed_at":"2026-08-11T18:01:50.523958Z","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":"2026-08-11T18:01:50.529174Z","title":"G., Baugh C","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.529174Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:296badeedc0fd96e21b25cb069fd50eb700e8c861afca7ba392cfed1bab2738d","observation_id":"6ce97407-41e4-40af-91b2-d0f7adbe02fa","resolution":{"observed_at":"2026-08-11T18:01:50.529174Z","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":"2026-08-11T18:01:50.534986Z","title":"T., et al., 2018, @doi [ ] 10.1093/mnras/sty1446 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.479..703C 479, 703","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.534986Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:97aa0a504547020211a59d87e4b62fbc56556fcdacaa8d013e4e4158fa6830c3","observation_id":"d3a75fbe-77b5-4815-a14c-41883696642f","resolution":{"observed_at":"2026-08-11T18:01:50.534986Z","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":"2026-08-11T18:01:50.540583Z","title":"J., et al., 2013, @doi [ ] 10.1088/0004-637X/767/2/118 , https://ui.adsabs.harvard.edu/abs/2013ApJ...767..118C 767, 118","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.540583Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:f47c36b4b8c55ea5d49fa32d0b7e4cb6bf625c6a7f96088506d1bf0d92c30cf8","observation_id":"ef0dc35a-7819-4c7b-9296-0e1c1e4b633d","resolution":{"observed_at":"2026-08-11T18:01:50.540583Z","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":"2026-08-11T18:01:50.545924Z","title":"A., van de Voort F., 2023, @doi [ ] 10.1146/annurev-astro-041923-043618 , https://ui.adsabs.harvard.edu/abs/2023ARA&A..61..473C 61, 473","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.545924Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:140105deebba3cfed6da0121ca8a9da43faa053a47ab0e816c17add8eb5634d1","observation_id":"86362039-fb9b-4924-96fd-58cb2719d5c5","resolution":{"observed_at":"2026-08-11T18:01:50.545924Z","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":"2026-08-11T18:01:50.550905Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.550905Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:e81e6fb8d1334d05943dbfba133ab181404cd957a42e5c6a56a34fe6a05f2b1d","observation_id":"51892215-f869-4633-bee8-ae7c687878a1","resolution":{"observed_at":"2026-08-11T18:01:50.550905Z","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":"2026-08-11T18:01:50.555968Z","title":"J., Khochfar S., Dunlop J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.555968Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:87baa16ce1cb4f2136298c0a030009b9fc7c9a0da3f2745762760c435a664762","observation_id":"6bc2a0b5-dec2-452b-b54d-3449e6e733e0","resolution":{"observed_at":"2026-08-11T18:01:50.555968Z","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":"2026-08-11T18:01:50.561331Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.561331Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:b4cc2ea9e1f6cf36ae0273c4a23717c82a24bd9ab7f28cbd59614de1454eaad7","observation_id":"b43718dc-c4cf-441f-86a9-d4ac944a2335","resolution":{"observed_at":"2026-08-11T18:01:50.561331Z","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":"2026-08-11T18:01:50.566083Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.566083Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:52f3c5bf91ef1da85d836a945082318fdc497268d9107b9fdced5268c3bc243f","observation_id":"d89fc1ed-0393-4d28-a953-04b597f58d7b","resolution":{"observed_at":"2026-08-11T18:01:50.566083Z","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":"2026-08-11T18:01:50.571030Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.571030Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:21b2d31a175c73ae0df709c00ed65072d8ffedca296b9835c518e43c4283987f","observation_id":"8cdbcfe5-9f59-4340-92b5-dd1b32d5f4bd","resolution":{"observed_at":"2026-08-11T18:01:50.571030Z","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":"2026-08-11T18:01:50.576017Z","title":"D., 2007, @doi [ ] 10.1111/j.1365-2966.2006.11177.x , https://ui.adsabs.harvard.edu/abs/2007MNRAS.374..427D 374, 427","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.576017Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:772793f0aecf911717df1c4c8113f0db279f737ec2c2d155e8729ad55ce05321","observation_id":"2ba69025-c4fe-4ab8-a7e4-67226bd601db","resolution":{"observed_at":"2026-08-11T18:01:50.576017Z","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":"2026-08-11T18:01:50.580726Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.580726Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:044059f4ba21fb1646fc46cb9d095e3a8c670e60c9259bd1bb25f6ec9fc33898","observation_id":"4003e864-41e6-47cc-894c-0fc7868fe7e3","resolution":{"observed_at":"2026-08-11T18:01:50.580726Z","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":"2026-08-11T18:01:50.585943Z","title":null,"venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.585943Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:c7327969d18730d7caac9ad461160513a381a5511eeb4b2e8739df0cdd77c06f","observation_id":"c4685f3e-60b0-4c47-884c-7e42c758abd8","resolution":{"observed_at":"2026-08-11T18:01:50.585943Z","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":"2026-08-11T18:01:50.590922Z","title":"G., et al., 2017, @doi [ ] 10.3847/1538-4357/aa756a , https://ui.adsabs.harvard.edu/abs/2017ApJ...843..126D 843, 126","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.590922Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:be040c0b7e8a8231e1cce08275c9bd8ed10b3d108763d5e7f08ddc03e40ad396","observation_id":"3c948715-a0cb-45e3-abb0-75366834f34e","resolution":{"observed_at":"2026-08-11T18:01:50.590922Z","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":"2026-08-11T18:01:50.595934Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.595934Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:b87ec482b6a3fa1eeb89d5373f166508e52a14dd8b2987cfae4d877e51ecb6bd","observation_id":"d781e74e-b15a-416b-aa12-a843a07902dc","resolution":{"observed_at":"2026-08-11T18:01:50.595934Z","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":"2026-08-11T18:01:50.601127Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.601127Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:f6782072e6fa938cf31b262e596578d1d269cef47f15bd72b1ab5664d21967ba","observation_id":"997f1c43-3911-4e4b-b138-7db166ad1ca3","resolution":{"observed_at":"2026-08-11T18:01:50.601127Z","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":"2026-08-11T18:01:50.606394Z","title":null,"venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.606394Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:81457595e1ef9441742e2a7be0b80f16c5c33eee822c39d413532c29fcf30e32","observation_id":"9a8bd060-d66d-47b8-8102-dccda8bbc17d","resolution":{"observed_at":"2026-08-11T18:01:50.606394Z","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":"2026-08-11T18:01:50.611639Z","title":"M., 2022, @doi [ ] 10.1016/j.physrep.2022.04.005 , https://ui.adsabs.harvard.edu/abs/2022PhR...973....1D 973, 1","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.611639Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:10c6ec041c636bba22c1870392a97609a93f5f62dbe7e055bb45564ca7d0bf6b","observation_id":"4e3eef90-de70-41e7-b86a-fd1ca4286144","resolution":{"observed_at":"2026-08-11T18:01:50.611639Z","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":"2026-08-11T18:01:50.616568Z","title":"M., Wuyts S., 2020, @doi [ ] 10.1146/annurev-astro-032620-021910 , https://ui.adsabs.harvard.edu/abs/2020ARA&A..58..661F 58, 661","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.616568Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:05da1251751df7185b8d0341214b1ffc8933191886e6d75c9eb48e92b54774cd","observation_id":"d9f98ea2-74a7-465d-a426-486729032be8","resolution":{"observed_at":"2026-08-11T18:01:50.616568Z","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":"2026-08-11T18:01:50.621261Z","title":"S., White S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.621261Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:2ba3f207ea1f0b6394e371341312850e5d2089c29c87eec0e70fdef7917931b9","observation_id":"e6e7d0b8-fec1-48d7-8c65-6c9945b0a036","resolution":{"observed_at":"2026-08-11T18:01:50.621261Z","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":"10.1093/mnras/stad3404","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:03:31.685978Z","title":null,"venue":null,"work_id":"a909efc8-8a60-44da-bcc3-5cd666ce50fc","year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.626481Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:ddd3fcf41a3c76b42d61733546800b828c682e3d1574d652241051f5354a2e75","observation_id":"7eb2f4c1-b49b-4d3c-bc6c-1e4a342f5ab8","resolution":{"observed_at":"2026-08-11T18:03:31.689805Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.631220Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.631220Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:26aeb772f7c1b72849cecda992359903c42de4154fb49f2776d7adfd11b6b4ad","observation_id":"07f65ae8-e3c2-4902-a811-b5c4d4221e0f","resolution":{"observed_at":"2026-08-11T18:01:50.631220Z","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":"2026-08-11T18:01:50.636033Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.636033Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:ddeaf57e8f47e6a5c3b812edabe7f49687775c5a66862b8e737f245b9b679b88","observation_id":"48f0ed95-d04e-430a-bc09-4f1c5961cc5d","resolution":{"observed_at":"2026-08-11T18:01:50.636033Z","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":"10.1093/mnras/stz388","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:03:31.661055Z","title":null,"venue":null,"work_id":"2584dfac-3cdd-4816-9e0e-fa7fc21323c5","year":2019},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.641040Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:091540fbb4526dd661113b657efc62b6907f9ed0fe7359287b3f078b17ae5fd9","observation_id":"c9f9b712-7983-4da9-9f39-8fac0a5d42a9","resolution":{"observed_at":"2026-08-11T18:03:31.664183Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.646297Z","title":"K., Geach J","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.646297Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:f468c6d9cd7bf794f959c2ffcda497e330c40d4a3071c266eedfdd559cfbe92b","observation_id":"41bee321-038d-4b3c-96fe-914a18ae688c","resolution":{"observed_at":"2026-08-11T18:01:50.646297Z","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":"2026-08-11T18:01:50.651083Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.651083Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:2ef50ade41465f1948361e644a84e674e3abd4a80d10cacc060e1ee80facd3d6","observation_id":"c33a00e2-07e7-4b8c-b793-8d7f57538030","resolution":{"observed_at":"2026-08-11T18:01:50.651083Z","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":"2026-08-11T18:01:50.655793Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.655793Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:6727c44d4b0b0572bb40491c2bb09fc7e6fe5eb4e8599f2edfbcb8a4f5c95aee","observation_id":"2ff8df9d-9a15-4b7b-84ce-186a0767f2a8","resolution":{"observed_at":"2026-08-11T18:01:50.655793Z","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":"2026-08-11T18:01:50.660603Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.660603Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:1666159f49ceac55221c160c3e832dcb36fc9ae7adca021bfd6302748fec85ae","observation_id":"9bd6b9c3-618f-4a2d-9dfe-d47bb5408444","resolution":{"observed_at":"2026-08-11T18:01:50.660603Z","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":"2026-08-11T18:01:50.665644Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.665644Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:48a42b88d19df796c36e17a45a57da5f72477901d020d22c505f2412486f5a68","observation_id":"4f413f45-e8b7-4c80-9a6d-013e5f4ca20a","resolution":{"observed_at":"2026-08-11T18:01:50.665644Z","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":"10.3847/1538-4357/abe876","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:03:31.616535Z","title":"F., et al., 2021, @doi [ ] 10.3847/1538-4357/abe876 , https://ui.adsabs.harvard.edu/abs/2021ApJ...910..106J 910, 106","venue":null,"work_id":"2a8efe79-843f-441e-b130-4e83fe16bad6","year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.670715Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:fdcef10306126d8e581912c99693dd499ed3d71dfc5ef5953023622fc938faf3","observation_id":"f28d5d3b-15c7-4aff-9961-6fd43f0a7e64","resolution":{"observed_at":"2026-08-11T18:03:31.621765Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.675627Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.675627Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:9a7f2648beec35502598d502fe7102931ae63a4ca58284360650d39659f5dcc4","observation_id":"32cd8407-7dac-40b9-8db7-faee236aa688","resolution":{"observed_at":"2026-08-11T18:01:50.675627Z","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":"2026-08-11T18:01:50.680491Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.680491Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:30aa33fdfb55eca2ad3dfb4c7bacb3e482894b757017464bf1b6242aa4e4d0ff","observation_id":"8ae7cd65-501e-4375-a17b-a9fd795fe9d5","resolution":{"observed_at":"2026-08-11T18:01:50.680491Z","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":"2026-08-11T18:01:50.685296Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.685296Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:37fd19507a30a679d68e1fa9650f0272c11b4909d42364bb209319a551e480eb","observation_id":"08e3b627-18d2-4ecf-906f-be289e121e4c","resolution":{"observed_at":"2026-08-11T18:01:50.685296Z","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":"10.1088/0004-637x/736/1/38","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:03:31.584598Z","title":"D., et al., 2011, @doi [ ] 10.1088/0004-637X/736/1/38 , https://ui.adsabs.harvard.edu/abs/2011ApJ...736...38K 736, 38","venue":null,"work_id":"4b5dc330-a90e-419b-8502-f8a898d3a498","year":2011},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.689790Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:61babd81302557a88da9e487aa371b807e86e04a9e973ddf33ae847aafb03b58","observation_id":"a7c6ce20-f2b5-47d3-8679-77055b27138b","resolution":{"observed_at":"2026-08-11T18:03:31.590103Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.695413Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.695413Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:de3afede07364e1d07a4aa0d4aa98adc877a689efd045977e130057f7d7d05b6","observation_id":"3892484c-9872-431f-ac73-acdc8f47e5ac","resolution":{"observed_at":"2026-08-11T18:01:50.695413Z","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":"2026-08-11T18:01:50.700450Z","title":null,"venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.700450Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:107988dea7d93129d0521598de726ecc4dcf1a238a2cc0926ee37b5b1cad7292","observation_id":"99921852-9b45-48a3-9af6-82932c8acbc3","resolution":{"observed_at":"2026-08-11T18:01:50.700450Z","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":"10.1093/mnras/staa2243","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:03:31.545395Z","title":null,"venue":null,"work_id":"5254400d-9a71-4378-b95c-bb4e55a0dad9","year":2020},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.705465Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:148254518356023a0e825440ee67705b081869103ef91e2cdbb3e5f243903cad","observation_id":"8a2313df-2609-4193-b86b-11da6e0b7237","resolution":{"observed_at":"2026-08-11T18:03:31.552757Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.710368Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.710368Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:b5f724b42a37b094e7f9f70810f95135bf356e87dbff0994b01ff2528d262049","observation_id":"24ae7510-9146-46e1-b857-4bd5c0878296","resolution":{"observed_at":"2026-08-11T18:01:50.710368Z","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":"2026-08-11T18:01:50.715197Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.715197Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:79e3b9c468ca5570e32a0028c0e3571435719b893f9925013ad97ee655a69144","observation_id":"36dba59c-742b-431c-8048-8c5a120bfe65","resolution":{"observed_at":"2026-08-11T18:01:50.715197Z","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":"2026-08-11T18:01:50.720408Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.720408Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:a9fa413c6828a433eb925c5b056e2f1d7cef9d6694cb617aa7623ed2b942042a","observation_id":"41a2f164-806a-4b8b-93a7-010bbdc23492","resolution":{"observed_at":"2026-08-11T18:01:50.720408Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005058","last_updated":"2000-05-03T12:35:12Z","snapshot_observed_at":"2026-08-15T10:58:15.153628Z","submitted_at":"2000-05-03T12:35:12Z","title":"Search for clusters at high redshift - I. Candidate Lya emitters near 1138-262 at z=2.2","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005058","snapshot_observed_at":"2026-08-11T18:01:50.725243Z","title":"D., et al., 2000, @doi [ ] 10.48550/arXiv.astro-ph/0005058 , https://ui.adsabs.harvard.edu/abs/2000A&A...358L...1K 358, L1","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.725243Z"},"links":{"cited_paper":"/paper/astro-ph/0005058","citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:0099e848265b73f40ad0ba358dad0f0d83cc8b0b4eecb50ddbbea5b9ffb8461a","observation_id":"91f46074-f988-40a7-a63d-3b4da1eb1f9a","resolution":{"observed_at":"2026-08-11T18:01:50.725243Z","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":"2026-08-11T18:01:50.730470Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.730470Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:50be6147833e4d6fe3e60052717bc0334b7ed776e480e979dd87589cae36bd5b","observation_id":"7560c1f3-35f8-414a-b002-d6d71fd33e92","resolution":{"observed_at":"2026-08-11T18:01:50.730470Z","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":"2026-08-11T18:01:50.735245Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.735245Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:12b136aba14f808f23b30a205b4dfc84db9c8e426bae63812fe9af0c3f9ccc0e","observation_id":"177341cd-bdd4-47aa-90e6-4a63825218aa","resolution":{"observed_at":"2026-08-11T18:01:50.735245Z","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":"2026-08-11T18:01:50.740967Z","title":"I., Boquien M., Andrews B","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.740967Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:1097657f229956122c6af83879000e15b403a2d568634ba8eb5023406ea4aa36","observation_id":"972dfa80-14b1-4a56-9bd1-a0f046eff678","resolution":{"observed_at":"2026-08-11T18:01:50.740967Z","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":"2026-08-11T18:01:50.746223Z","title":"J., et al., 2007, @doi [ ] 10.1086/516589 , https://ui.adsabs.harvard.edu/abs/2007ApJS..172...70L 172, 70","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.746223Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:bfc13beef5eb33193564ec8b0dfdff4ca851369151d7f3b09d9003a7106d51ba","observation_id":"a10a7909-4b4a-41ac-ab5e-5241106a54ef","resolution":{"observed_at":"2026-08-11T18:01:50.746223Z","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":"2026-08-11T18:01:50.751202Z","title":"J., et al., 2009, @doi [ ] 10.1088/0067-0049/184/2/218 , https://ui.adsabs.harvard.edu/abs/2009ApJS..184..218L 184, 218","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.751202Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:453572d644de6def3c600be5ca4ce7f209692a269c2683560e429734f5d6c04a","observation_id":"901efa91-3a99-43a7-925a-d4cf1ea35154","resolution":{"observed_at":"2026-08-11T18:01:50.751202Z","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":"2026-08-11T18:01:50.756034Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.756034Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:9adff2dad36f16ee580be82253ceba6a5f96c64d093ceab24f852f520b7ba23e","observation_id":"53c167e4-19e1-4081-8f15-53e68a402753","resolution":{"observed_at":"2026-08-11T18:01:50.756034Z","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":"2026-08-11T18:01:50.760997Z","title":"M., et al., 2013, @doi [ ] 10.1088/0004-637X/773/2/154 , https://ui.adsabs.harvard.edu/abs/2013ApJ...773..154L 773, 154","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.760997Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:02fbe883e5cea47bc2901f24e11b0eda8fa11a35f62c7365617e7f364de25eba","observation_id":"e6fbdc9b-9eaf-4c7e-96fc-7b4072080d4e","resolution":{"observed_at":"2026-08-11T18:01:50.760997Z","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":"2026-08-11T18:01:50.766125Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.766125Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:21fd280cb7b68813e732bfdde8dd18a3acf4b31347ad76954c96caf9cf5d0a48","observation_id":"404bbefc-4791-4959-a2a6-0184deb3ff60","resolution":{"observed_at":"2026-08-11T18:01:50.766125Z","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":"2026-08-11T18:01:50.771179Z","title":"S., et al., 2016, @doi [ ] 10.3847/2041-8205/827/2/L25 , https://ui.adsabs.harvard.edu/abs/2016ApJ...827L..25M 827, L25","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.771179Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:a79f3bfdfb1e89771347ec386237b980ffcd0ea3939917a7cfc9f8c2cd1bea1c","observation_id":"123c4b29-0ea2-4aac-b225-3dac1ffc66d5","resolution":{"observed_at":"2026-08-11T18:01:50.771179Z","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":"2026-08-11T18:01:50.776591Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.776591Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:e95dd738421bde1b2bd8a5558585a904f91e1d4d15c2bc44201242fdb83dceaf","observation_id":"bd92ffda-3366-4745-85fc-be84e8df44b9","resolution":{"observed_at":"2026-08-11T18:01:50.776591Z","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":"10.3847/1538-3881/acb707","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:52.020930Z","title":null,"venue":null,"work_id":"86e46290-a5bb-414c-ad1a-3d882dd8f6dc","year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.781611Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:da9b58689186f449632d50f69cacd8be2c0d0626ac5ac4ed1024a8bd34f41460","observation_id":"525406f7-4b3a-44c4-864c-62cc40def954","resolution":{"observed_at":"2026-08-11T18:01:52.025562Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.793932Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.793932Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:a1a25ddcbce646e66ef9675143adf543abe487c890d5ea038f1ee2ffa973bc5b","observation_id":"6b7b2ae0-80b2-4795-bf12-a10c63f256e4","resolution":{"observed_at":"2026-08-11T18:01:50.793932Z","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":"2026-08-11T18:01:50.800009Z","title":"C., White S., 2010, Galaxy Formation and Evolution","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.800009Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:36c5456d774472aad4a781cfc636f1fd88fd7ff1367e650acc60a4237d52612a","observation_id":"350e109b-7b8a-49c6-8e46-f7cee5c51e6f","resolution":{"observed_at":"2026-08-11T18:01:50.800009Z","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":"2026-08-11T18:01:50.806526Z","title":"B., et al., 2021, @doi [ ] 10.3847/1538-4357/ac0f84 , https://ui.adsabs.harvard.edu/abs/2021ApJ...919...51M 919, 51","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.806526Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:abecd45fc8e376cd2bf413b62a1e97b8fa85b23c5b1eda2524c2a8c6e1c81fab","observation_id":"ca33396a-5a8b-47b4-a181-4f3e62337ff3","resolution":{"observed_at":"2026-08-11T18:01:50.806526Z","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":"2026-08-11T18:01:50.811264Z","title":"B., et al., 2023, @doi [ ] 10.3847/1538-4357/acd449 , https://ui.adsabs.harvard.edu/abs/2023ApJ...951...15M 951, 15","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.811264Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:98c599c077e9d945aae64977d6a09d9abebdfc245c7e6528e290bb0914507f74","observation_id":"7718f4de-8bda-448e-bb93-60aff5af2c08","resolution":{"observed_at":"2026-08-11T18:01:50.811264Z","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":"2026-08-11T18:01:50.815912Z","title":"A., et al., 2022, @doi [ ] 10.3847/1538-4357/ac71af , https://ui.adsabs.harvard.edu/abs/2022ApJ...933..129M 933, 129","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.815912Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:7e0be7939344e480c2c3d661a4936855a9abe6a582562e7f2593833a77b40db6","observation_id":"5198d0d1-5909-45c1-9b19-32a2034bc6a7","resolution":{"observed_at":"2026-08-11T18:01:50.815912Z","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":"2026-08-11T18:01:50.820308Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.820308Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:66d325690317a38e3b6dcc7ef173a3c037afd04c6713bdf3c0f0760265455060","observation_id":"e982274d-e483-46dd-aca5-380f3a0c7f9a","resolution":{"observed_at":"2026-08-11T18:01:50.820308Z","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":"2026-08-11T18:01:50.824720Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.824720Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:30862bc438ecd6d5eafa2082cd6e1857fb49e0199a6d4940a628b45adedeb868","observation_id":"a4b7e0ec-8522-42ba-9154-f58ec93ab235","resolution":{"observed_at":"2026-08-11T18:01:50.824720Z","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":"10.1088/0004-637x/765/1/47","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:51.936698Z","title":"B., Shapley A","venue":null,"work_id":"40b54aa0-0499-4188-a7a0-fe2d33419231","year":2013},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.829489Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:600742c2f395c78ef5d14cb184a0e3fc6a87d7268338ed4cf2c3f80411527e5b","observation_id":"5c0e294a-ccbf-4bdd-a67b-4ba0931df9e4","resolution":{"observed_at":"2026-08-11T18:01:51.946946Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.833962Z","title":"B., Ellis R","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.833962Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:989b9190ac9f5fb3d5a51ccf9803bf69f1721c5e822e5e02b40f2160443ff7f6","observation_id":"b0314770-c266-46f4-bb76-e982fcb28dbe","resolution":{"observed_at":"2026-08-11T18:01:50.833962Z","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":"2026-08-11T18:01:50.838524Z","title":"A., Moster B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.838524Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:e008a9998f28a6ab5c15d11936a837b5db18ebaf0d5ee2d2ae504b0250267110","observation_id":"b4eb208e-932d-4a86-b843-745038e8aac7","resolution":{"observed_at":"2026-08-11T18:01:50.838524Z","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":"2026-08-11T18:01:50.843092Z","title":null,"venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.843092Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:796715ae89859199d36392e14d11d3a0dc991cb45df2a2fba33fa61cb77fec29","observation_id":"e3097eef-526e-49fe-929a-5ccf72900e1d","resolution":{"observed_at":"2026-08-11T18:01:50.843092Z","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":"2026-08-11T18:01:50.847642Z","title":"A., 2016, @doi [ ] 10.1007/s00159-016-0100-3 , https://ui.adsabs.harvard.edu/abs/2016A&ARv..24...14O 24, 14","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.847642Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:67db6d2120dfca4055b05ccf5c37283accef106eff53016080393d126a15a41d","observation_id":"1edc74be-5ac8-4e69-a8c9-4c5735a5112f","resolution":{"observed_at":"2026-08-11T18:01:50.847642Z","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":"2026-08-11T18:01:50.852713Z","title":"A., et al., 2001, @doi [ ] 10.1038/35065528 , https://ui.adsabs.harvard.edu/abs/2001Natur.410..169P 410, 169","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.852713Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:de09928475e799aabe86d7a318adbd1e295cbeb902d6adb5815681fa0fa65c30","observation_id":"c12a5410-5dd2-4641-9358-e1b3413c2133","resolution":{"observed_at":"2026-08-11T18:01:50.852713Z","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":"2026-08-11T18:01:50.857449Z","title":"Y., Ho L","venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.857449Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:a84247efbd9afe6e6eca4c7e2f905730b6f7998a18ee62bb83ca081069219048","observation_id":"729b5edd-ac6b-48f6-b400-51361abf4e3d","resolution":{"observed_at":"2026-08-11T18:01:50.857449Z","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":"2026-08-11T18:01:50.862319Z","title":"Y., Ho L","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.862319Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:9508975e06758c5b08e394bffb4c5460257f8a5e32accd122d55f85917c57bf6","observation_id":"19a85c4d-be38-4dc1-9355-1a3e307d0066","resolution":{"observed_at":"2026-08-11T18:01:50.862319Z","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":"2026-08-11T18:01:50.868086Z","title":"M., et al., 2023, @doi [ ] 10.1093/mnras/stac2784 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.1707P 518, 1707","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.868086Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:55ed59d420a5dd3b12ac884a2d0b4d936b801315564b0c645bd4cd10751a6b7c","observation_id":"08032927-5504-4a61-9efe-15e67320697c","resolution":{"observed_at":"2026-08-11T18:01:50.868086Z","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":"10.1051/0004-6361/201118169","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:51.848862Z","title":null,"venue":null,"work_id":"670dbf51-214e-4011-b956-f89181562e57","year":2012},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.872661Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:c5af8ea2486e1a3bd36ff9a8b0a2a067002db11a949b2faa3db2db6d3dc6b8ac","observation_id":"872b5074-90ca-481f-8bea-dc11b0ef2cdc","resolution":{"observed_at":"2026-08-11T18:01:51.853903Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.877347Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.877347Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:076e4088ed610b72aaf35b8cccf47dc4fa32932d4ddd3ab31d0671297b0c971e","observation_id":"d9b1867e-a367-48ff-b9f9-1291336870ab","resolution":{"observed_at":"2026-08-11T18:01:50.877347Z","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":"2026-08-11T18:01:50.882118Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.882118Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:99f8d8ecc72ce1375724486c5ba527463f67c4c247b1cf63711eed68fe299430","observation_id":"db64a68d-e1c6-4baf-bee5-348841a52f4b","resolution":{"observed_at":"2026-08-11T18:01:50.882118Z","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":"2026-08-11T18:01:50.886951Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.886951Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:744465d038bf05c7bc3c62eb27b780c45372b84b7c2c66f2371bc17f51801ef6","observation_id":"d786d298-1261-49ff-9fb7-7d34c37e20f2","resolution":{"observed_at":"2026-08-11T18:01:50.886951Z","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":"2026-08-11T18:01:50.892324Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.892324Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:5fea94fe0436b07f13268fbb564b964a3a9a31135f09c01c73127eb7d3aa7f56","observation_id":"260a9035-968b-47d0-8678-6f98c0d0857c","resolution":{"observed_at":"2026-08-11T18:01:50.892324Z","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":"2026-08-11T18:01:50.897151Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.897151Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:b3133b668cece910aa0e598ed7f511d4b1ca6e8fc43ff876b5999d44be177809","observation_id":"38d3f103-e22f-4c73-b77f-0dc8f1abe812","resolution":{"observed_at":"2026-08-11T18:01:50.897151Z","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":"2026-08-11T18:01:50.902116Z","title":"C., Bottrell C., Hani M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.902116Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:35da2491fbc79372d8903fb7e3f01e6157585f15bae2a9029c2d4a26740b0ce7","observation_id":"7b9c7b7b-2782-4736-b24b-cb5c07bf712d","resolution":{"observed_at":"2026-08-11T18:01:50.902116Z","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":"2026-08-11T18:01:50.907428Z","title":"B., Caputi K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.907428Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:7d5cfc0ede49605a5593351ffa14e5cc3ea455a50d71dba9fbba8fa06d938fa2","observation_id":"e0f3fa4e-e850-444e-bf6f-14463400e7fb","resolution":{"observed_at":"2026-08-11T18:01:50.907428Z","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":"2026-08-11T18:01:50.915373Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.915373Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:c799e0f54f33a757e0850077d1bb5602a6547871fc8a06222526ba0f86de7975","observation_id":"31a5b6fc-9a56-4861-b309-f1ae2e841832","resolution":{"observed_at":"2026-08-11T18:01:50.915373Z","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":"10.1093/mnras/stv747","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:51.747639Z","title":null,"venue":null,"work_id":"4bccceec-cd0e-4813-a7da-20515111b7d6","year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.920750Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:279ff1ea7ba3f8f22988e2d2d36067050aaa0f841b7705c6d8664f1c8f1144e3","observation_id":"89fcfca9-51bd-4353-b5f2-1ec1a8dce4df","resolution":{"observed_at":"2026-08-11T18:01:51.752541Z","resolver_source":"doi","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":"10.1088/0067-0049/202/1/8","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:51.731733Z","title":"K., Ree C","venue":null,"work_id":"4cbd0230-9407-49d1-bfd5-8a03fd70c820","year":2012},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.925885Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:a2364c070a14c06cd447b1b7735e2c81a27ed42da56b63bf6c5ba84ab5491845","observation_id":"b2326f59-e74e-4fb8-a9ef-baa65638d694","resolution":{"observed_at":"2026-08-11T18:01:51.736948Z","resolver_source":"doi","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":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T18:01:50.931071Z","title":"D., Cai Z., Fan X., Zheng X","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.931071Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:4eba0ec3a7b61b3ec06afbe5d54647f322a855a09afdaca8297dc3a0c1b520e3","observation_id":"de3b2e7b-ec19-4c22-bcfa-4ee97789a5d6","resolution":{"observed_at":"2026-08-11T18:01:50.931071Z","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":"2026-08-11T18:01:50.935996Z","title":"D., Wang X., Zheng X","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.935996Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:f010ff4cb71399d0589eba4d396b221786bcf81d87b1cd2c31bcbe49beca371f","observation_id":"a2fe5ef5-26b3-4e52-b764-69f71f9d25cb","resolution":{"observed_at":"2026-08-11T18:01:50.935996Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2403.06729","last_updated":"2024-11-27T13:58:06Z","snapshot_observed_at":"2026-08-15T10:58:05.898988Z","submitted_at":"2024-03-11T13:47:51Z","title":"Galaxy Morphologies Revealed with Subaru HSC and Super-Resolution Techniques II: Environmental Dependence of Galaxy Mergers at z~2-5","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2403.06729","snapshot_observed_at":"2026-08-11T18:01:50.940894Z","title":"arXiv:2403.06729","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.940894Z"},"links":{"cited_paper":"/paper/2403.06729","citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:1dee56c436caa71f72625656ddff78eb961d8b83ef586522e499a88601ba44aa","observation_id":"3e928af7-9b56-49f9-922d-956e83f132e8","resolution":{"observed_at":"2026-08-11T18:01:50.940894Z","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":"2026-08-11T18:01:50.946013Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.946013Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:ce8ccd7c82a17f14f43b94956ca3d09c5d791b52d9a2c1b9a215a1a007859250","observation_id":"98b46d01-8449-4dbf-b70b-9fa11351300b","resolution":{"observed_at":"2026-08-11T18:01:50.946013Z","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":"2026-08-11T18:01:50.951194Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.951194Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:e39a5bbe30860dff24461e8deafffc58020f970fd16c6fedd2371f7bc8e8bb2e","observation_id":"a35c9258-6313-437f-8771-0611ba596ca3","resolution":{"observed_at":"2026-08-11T18:01:50.951194Z","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":"2026-08-11T18:01:50.956267Z","title":"D., et al., 2015, @doi [ ] 10.1088/0067-0049/220/1/12 , https://ui.adsabs.harvard.edu/abs/2015ApJS..220...12S 220, 12","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.956267Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:e3d308b8324087b1ef2fe981077e7412081a6c0f8a714f0c8d075931e0435b64","observation_id":"317b5803-e061-4164-889f-4611138fa129","resolution":{"observed_at":"2026-08-11T18:01:50.956267Z","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":"2026-08-11T18:01:50.961206Z","title":"N., Geach J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon","version":1},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-11T18:01:50.961206Z"},"links":{"citing_paper":"/paper/2412.08336"},"observation_digest":"sha256:e11f6f816853795005cd169f380ca09155f2a163117a53d0b5dee49bbaccf149","observation_id":"9b3a43cf-6058-471e-a47e-146193bd9799","resolution":{"observed_at":"2026-08-11T18:01:50.961206Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.08336","last_updated":"2024-12-11T12:23:55Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-15T08:06:44.277275Z","submitted_at":"2024-12-11T12:23:55Z","title":"A first measurement of galaxy merger rate increasing in dynamically colder protoclusters at cosmic noon"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":90,"verified_exact":10,"verified_fuzzy":0},"total_outbound_references":139},"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 15 August 2026, this Paper Citation Record lists 100 of 139 outbound references and 0 inbound Pith citation observations for arXiv:2412.08336."}