{"as_of":"2026-08-19T08:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:217fa108d50751bed8c769ab861e084cf3c156a4b472aa8bf31d7f36ecd6e8b8","coverage":[{"denominator":71,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":71,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T23:25:58.411799Z","state":"measured"},{"denominator":71,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":71,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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/2505.04990/citation-record","integrity":"/paper/2505.04990/integrity","json":"/paper/2505.04990/citation-record.json","paper":"/paper/2505.04990"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.185478Z","title":"M., et al","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.185478Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:f2a799ab11cf8c53ebb6c1e6d89a5a9f77998239270a2941671236830d35654a","observation_id":"25af527a-7f33-44e0-9a68-b51db343bfce","resolution":{"observed_at":"2026-08-15T23:25:58.185478Z","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":"2026-08-15T23:25:58.189620Z","title":"1973, Information Theory and an Extension of the Maximum Likelihood Principle (New York, NY: Springer New York), 199--213","venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.189620Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:74550d0eeb16d08cfe6e23325ae7e7f3d8b8b8824ca23b5812f98024713f9b53","observation_id":"7b3d9bac-68e8-4d28-ab96-2a95e5d4fa96","resolution":{"observed_at":"2026-08-15T23:25:58.189620Z","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":"2026-08-15T23:25:58.193093Z","title":"M., Lim , P","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.193093Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:9de709490002750cb26091944065cb14ee70c8532eefee69a69feb9500a6be02","observation_id":"1f78521c-e40c-4f69-a54d-2e6e0efc95f9","resolution":{"observed_at":"2026-08-15T23:25:58.193093Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:59.040028Z","title":"A., Lorimer , D","venue":null,"work_id":"8fc81c8e-d907-4336-8417-5d06a4cf23b3","year":1994},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.197017Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:aa11263fe7fa4d7801535f495c726247ead23ea0b014b63fc08f241dd2b4ec37","observation_id":"9b885e87-240c-4f7e-b480-6a3c32bbc44a","resolution":{"observed_at":"2026-08-15T23:25:59.043654Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:59.029358Z","title":"F., et al","venue":null,"work_id":"cd549b4c-19dd-4c9e-b408-2b9b21080ed2","year":1997},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.200485Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:44f96b7b5023479ddab52a9cb9f6e8393c2ceaa8b61f5e030e4ec1fc4f8a9222","observation_id":"dcaa24e6-06a9-44cf-b8c6-ff35064da434","resolution":{"observed_at":"2026-08-15T23:25:59.032722Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:59.019207Z","title":"R., Salter , C","venue":null,"work_id":"d69186fc-8fde-41dc-b288-b562a8046953","year":1973},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.204060Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:5c47edd379019faa18e10fd9f71d86f34b7a838a332acf18c84c374c2347c6a1","observation_id":"33460585-c6fb-49f4-a1e6-4a754199d65d","resolution":{"observed_at":"2026-08-15T23:25:59.022536Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:59.009263Z","title":null,"venue":null,"work_id":"0186d674-d6e0-4957-80aa-8dd19f2250e6","year":2000},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.207750Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:8364c05aab4fecb3f1441f4df5697a6770ddac8b1d72397dea549bcbe74d7340","observation_id":"1447ead9-dedb-4db5-9a12-b398f86c3c8d","resolution":{"observed_at":"2026-08-15T23:25:59.012643Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.999025Z","title":"J., Shrauner , J","venue":null,"work_id":"da58f150-4f2d-48d9-8317-fb69d6ecedf6","year":1996},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.210832Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:5788d55cdc68a9c6fdf9a53ed6b2f42433a736c398c22af05bffd3c837651397","observation_id":"6ee19608-fa44-4515-9f6c-7b097f45fc65","resolution":{"observed_at":"2026-08-15T23:25:59.002495Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.213814Z","title":"2022, , 509, 5538","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.213814Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:741bd0fa5c82e12722c3f292eff53b86b022086a4e6412bb786a7dc8a46ec106","observation_id":"e805009e-0665-4471-abac-02d302d7f360","resolution":{"observed_at":"2026-08-15T23:25:58.213814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.981922Z","title":"2013, in SF2A-2013: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, ed","venue":null,"work_id":"ac33ddbf-f5b0-47bf-8e83-c694224e82c1","year":2013},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.216868Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:952676823d6f22eb76e0c8ffc7c5aba200e87f9f0e1457452bf6069ff07e2916","observation_id":"b92d99eb-816c-4688-9f68-5d99d0411102","resolution":{"observed_at":"2026-08-15T23:25:58.985432Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.971425Z","title":"D., Lovelace , R","venue":null,"work_id":"3aeaed6d-a0fd-4239-9c39-21ded755f48a","year":1968},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.219896Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:3517ab73cb4c32d93da069f2141ac7da037fef11b2f684f8f0392547dee02aec","observation_id":"67f9a78b-9049-432d-af66-91d58f0dc7dd","resolution":{"observed_at":"2026-08-15T23:25:58.975061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.962032Z","title":"H., & Hulse , R","venue":null,"work_id":"bbd72dcb-de1e-4145-a1d5-3a9aa12f4860","year":1978},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.223210Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:87b1a4e4e7aa4aeb6365e29c7df15915fe456c5f45ccd00a8bf041d50f3b183e","observation_id":"b6ee52a0-5b5a-4e21-abb0-cb47c9bb78ef","resolution":{"observed_at":"2026-08-15T23:25:58.965210Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.952491Z","title":null,"venue":null,"work_id":"1159d388-133f-44df-8299-ec074f44bf6d","year":1970},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.226219Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:19190bc375a8ded643d652393efa9504322a2769f48a666f87c3f270295d9fcf","observation_id":"d9bebf31-1c5c-435f-8175-adb6b34ada49","resolution":{"observed_at":"2026-08-15T23:25:58.955686Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.942539Z","title":"C., Cognard , I., Lespagnol , P., & Theureau , G","venue":null,"work_id":"4048ff57-5033-431d-94ab-e4dadac18e41","year":2011},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.229135Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:2a7acb10e7d3935bd96a7424bba8d9e59d0f0adcfdc5c608d85c4bdf2f00c528","observation_id":"694fef5c-1797-4916-9dbe-f51341f25023","resolution":{"observed_at":"2026-08-15T23:25:58.945918Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13463","last_updated":"2024-10-28T17:43:47Z","snapshot_observed_at":"2026-08-18T09:53:02.153364Z","submitted_at":"2024-06-19T11:40:08Z","title":"Exploring pulsar timing precision: A comparative study of polarization calibration methods for NANOGrav data from the Green Bank Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13463","snapshot_observed_at":"2026-08-15T23:25:58.232327Z","title":"A., Wahl , H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.232327Z"},"links":{"cited_paper":"/paper/2406.13463","citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:26c5f1270854e674e9f91f1fd1a33c187ad40ea22e310f34f05f0aba4f7b5bda","observation_id":"804dc861-3457-4f55-881f-05cc331c621e","resolution":{"observed_at":"2026-08-15T23:25:58.232327Z","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":"2026-08-15T23:25:58.235776Z","title":"& van Haasteren, R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.235776Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:e617701df5b1aad66f396a1a3a4ee8a73093476e14987d7fedd386220c0bdf4d","observation_id":"adc1ecde-2f09-441e-85c7-40f95de31f00","resolution":{"observed_at":"2026-08-15T23:25:58.235776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.926894Z","title":"A., Vallisneri , M., Taylor , S","venue":null,"work_id":"f265c2ef-f915-4936-a5a1-9da151e5ae94","year":2020},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.238752Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:e0246eff3cc79015d0d0dfea0b352cdf137b77efa62cf23b33cd8bd01f3fd65f","observation_id":"8d32cdbe-e7e6-49ab-aa83-b79c538394bb","resolution":{"observed_at":"2026-08-15T23:25:58.930193Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.241847Z","title":"2023 a , , 678, A48","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.241847Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:7a2b022b790218ce6bdff6dc06afe6ea219f74a8d7b2457e50b0db413d36abfa","observation_id":"c28e6f60-7372-4f7c-92f2-0f792098447c","resolution":{"observed_at":"2026-08-15T23:25:58.241847Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.910541Z","title":"2023 b , , 678, A50","venue":null,"work_id":"7c8d42e6-5a85-4227-a2a1-5f32f43b9d23","year":2023},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.244916Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:2993982a4bdb19ad990152acd5f5a3ac395b6bdafb4039f8ff73fb605673dd3d","observation_id":"b6900fb5-be7a-4a20-89eb-b907f7dcedf3","resolution":{"observed_at":"2026-08-15T23:25:58.913709Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.900153Z","title":"B., et al","venue":null,"work_id":"82bf6ec3-2cdf-45ec-b43b-e044da14b1ee","year":2022},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.248021Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:5feefa15430af28c712d07ae407415b3d31a9e3c07bb1f90d34468d69dcba33c","observation_id":"bcc19bf8-287b-4909-b276-518331ea57c6","resolution":{"observed_at":"2026-08-15T23:25:58.904263Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.890620Z","title":"2015, , 453, 1489","venue":null,"work_id":"5440a547-4941-4c8f-b107-8300befa6d5d","year":2015},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.251135Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:5bc121029714da4c4b2b5f041d574469a651fb7e88d4fff1d014e5ec4ac32615","observation_id":"6af12b24-3af6-415c-a43c-fac16b7cfa88","resolution":{"observed_at":"2026-08-15T23:25:58.893839Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.880764Z","title":"S., Wolszczan , A., & Camilo , F","venue":null,"work_id":"887e84c4-04fa-47e2-a948-fc17c21d3c89","year":1993},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.254186Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:f4138c68c1800090472c47a23e0b0dd9a563e1092d1fa695cf50ae50a46b3f7c","observation_id":"8f3732e7-7a72-42e4-ba0b-3d83c4bcc8b8","resolution":{"observed_at":"2026-08-15T23:25:58.884342Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.870569Z","title":"2023, , 678, A79","venue":null,"work_id":"fc84a613-73c4-45c5-b539-8dab091a13a9","year":2023},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.257296Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:95fa578e13f3b7bf6fc3db05e9a7ac0ba65a67c06eb72e57b10e096c29da63cd","observation_id":"9f54a7d2-fbd9-4f32-ae24-9231bc0e0aa3","resolution":{"observed_at":"2026-08-15T23:25:58.874002Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.260433Z","title":"R., Millman, K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.260433Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:7959b21e8ed4228855d92f5ab6095536d8ad71257f8f61b306c6b51c1810b5d1","observation_id":"4919ef1a-f5ee-46e3-a77a-c1813d82cd53","resolution":{"observed_at":"2026-08-15T23:25:58.260433Z","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":"2026-08-15T23:25:58.263674Z","title":"B., Edwards , R","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.263674Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:3c9edd0e102c53127470399789905e70ed1588062008a56d623fc61df91637b2","observation_id":"2eb6c887-50ca-4455-8bb9-dcac54633f7c","resolution":{"observed_at":"2026-08-15T23:25:58.263674Z","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":"2026-08-15T23:25:58.266713Z","title":"W., van Straten , W., & Manchester , R","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.266713Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:26a83956389d032416e1ae6b34f1b2a08ee511caad70121c3f4287dc82201661","observation_id":"fbf858f3-8563-4f95-82ec-6c83d92a4cda","resolution":{"observed_at":"2026-08-15T23:25:58.266713Z","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":"2026-08-15T23:25:58.269718Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.269718Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:10dbb3e7fc463bea7b3bac6d285070c4f5f9b029e3922ad9491df25d1445f6cd","observation_id":"7933a8b6-6ac8-4e6e-bd1c-84f806d2f002","resolution":{"observed_at":"2026-08-15T23:25:58.269718Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.836061Z","title":"A., Bailes , M., Ord , S","venue":null,"work_id":"fe16f548-da05-42af-acdc-b5233c22adc4","year":2007},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.273124Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:6b75b0c5a2688b8978f15c96ce76faa1d6b9b0047466f765d81f0e882dd4fc4a","observation_id":"c7750d17-a23c-4f8a-87f0-0477f98aee03","resolution":{"observed_at":"2026-08-15T23:25:58.840269Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.826477Z","title":"A., Bailes , M., van Kerkwijk , M","venue":null,"work_id":"97043e1e-c0a9-401b-b6a9-fc10476658dd","year":2003},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.276247Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:127e3b10d8be2323b8f9ab577d50fe75397bc666a3e080fa914956e713619587","observation_id":"a691a15c-916d-4c69-a552-6cc2ee9d41f0","resolution":{"observed_at":"2026-08-15T23:25:58.829712Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.816801Z","title":"F., et al","venue":null,"work_id":"9aa50fff-e33d-40d4-91b3-bf70a300ce69","year":2018},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.279388Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:9c6c41874e28e3ea76ea4639abb9a7a021e0159acc2274707d932c14286181f4","observation_id":"8d05c6c6-3297-48c1-9348-87b35e169937","resolution":{"observed_at":"2026-08-15T23:25:58.820273Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.12266","last_updated":"2024-01-31T18:59:08Z","snapshot_observed_at":"2026-08-16T16:22:06.009813Z","submitted_at":"2022-10-21T21:45:24Z","title":"An unusual pulse shape change event in PSR J1713+0747 observed with the Green Bank Telescope and CHIME","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.12266","snapshot_observed_at":"2026-08-15T23:25:58.282312Z","title":"J., Cordes , J","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.282312Z"},"links":{"cited_paper":"/paper/2210.12266","citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:0e44448ee82d043629f81f93a0a71ce31abe77455f962e9b47ba4971d109cab2","observation_id":"62ee374d-36d4-403d-b87c-06bf206b58c5","resolution":{"observed_at":"2026-08-15T23:25:58.282312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.807003Z","title":"2002, , 19, 277","venue":null,"work_id":"fc3b69a1-e4c1-4939-be1d-534660547ce3","year":2002},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.285934Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:ee8f89cad107499b3d872d83beea6518385305302b3f686886b3a81f3fc72d8f","observation_id":"95abf09c-9b2e-40e9-8de9-9284fe24c219","resolution":{"observed_at":"2026-08-15T23:25:58.810300Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.797313Z","title":"1998, International Journal of Computer Vision, 26, 171","venue":null,"work_id":"0bc65914-fcef-45fe-bb5b-b92dc671a1bc","year":1998},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.289093Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:cd96fae7e85b05588e6556f28f47d8309b32664ba48ebb86a77b6c2b60abcb87","observation_id":"9adf544a-226b-4b43-b12a-8c94d9ecda1b","resolution":{"observed_at":"2026-08-15T23:25:58.800717Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.787615Z","title":"H., Manchester , R","venue":null,"work_id":"839054b1-68ab-48a2-aaae-028f5e60e1c2","year":2021},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.292317Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:6fbc291013ce011cdb71d7e5d6fecd71d1c5f6172a94f6fb5fcdf6af8e8baae2","observation_id":"89ca9422-c146-4737-8093-9a6ddd780870","resolution":{"observed_at":"2026-08-15T23:25:58.790802Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.777797Z","title":null,"venue":null,"work_id":"73c42f1c-f010-42b2-b0c6-3035c9e392a1","year":1960},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.295370Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:67208c7529c7be95285d3b5dc4896c4fc7b5da20d6fc8b40695b03e657f61440","observation_id":"582852c9-b050-4f39-9ed0-979d61b637d5","resolution":{"observed_at":"2026-08-15T23:25:58.780900Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.768053Z","title":null,"venue":null,"work_id":"0916637e-f72b-412e-807c-595f261146cf","year":1966},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.298645Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:bf2bd4afc24a220fd33b21158a5e8a2e2e6f11b8758d778f7557327db134e3a6","observation_id":"d65c2c1c-7470-4ea8-b75e-bf7c4dafb8c4","resolution":{"observed_at":"2026-08-15T23:25:58.771464Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.757753Z","title":null,"venue":null,"work_id":"eaf2f743-34c6-4cff-8373-810e8da31e9e","year":1969},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.301612Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:b3da6b6b06a12009756874847e92a24d0b76b4921ce6cbaf25b0191022979ddc","observation_id":"233c7e4b-f2ba-43c0-bf2b-d3bc85233854","resolution":{"observed_at":"2026-08-15T23:25:58.761168Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.748159Z","title":"2016, , 458, 868","venue":null,"work_id":"fcfe4b46-80e9-46b1-bbe3-5aefef163a9f","year":2016},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.304789Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:619598b9a44260693efc7957f3ed761604146fac8942a2fd1d79a321cf3af340","observation_id":"9ad4407d-84c1-4176-a99b-41d75c8a4f47","resolution":{"observed_at":"2026-08-15T23:25:58.751393Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.738468Z","title":"M., Coles , W","venue":null,"work_id":"9597b6d8-78ae-4bd9-947f-9a1b2eabd917","year":2016},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.307739Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:acedd530f44adb7f5d80683878cebc166e5fe4ca58db4a9e8327617220ee29b8","observation_id":"29b17a9a-39a4-46f2-b641-d1f9368fc1be","resolution":{"observed_at":"2026-08-15T23:25:58.741865Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.728100Z","title":null,"venue":null,"work_id":"d9f3d1e4-4bfc-4411-97fd-5a9a38362aac","year":2004},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.310780Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:0ebdb6896fbb009436510f2c0af612afed43e6daf72242b8af1ea59c60ab7b13","observation_id":"627e77a5-2732-46cc-9c98-c7c5251cd4a8","resolution":{"observed_at":"2026-08-15T23:25:58.731421Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.718283Z","title":"R., Nicastro , L., Lyne , A","venue":null,"work_id":"2630a1cb-25ce-400b-9402-e27d526828f1","year":1995},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.313915Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:c1da09006ef83f483cb3747b521e88b7e55f9280e031502a125e7f192b4b3058","observation_id":"21f2aaec-47b0-4019-be4a-41b1287a88e1","resolution":{"observed_at":"2026-08-15T23:25:58.721736Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.317022Z","title":"N., Hobbs , G., Bailes , M., et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.317022Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:87f38f85d733ef714bd08ab48859abf14e178fa2ed0970da63f4a5880863b1d1","observation_id":"78937063-e7c5-4d5b-a99c-6e7b7c166a85","resolution":{"observed_at":"2026-08-15T23:25:58.317022Z","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":"2026-08-15T23:25:58.320148Z","title":"N., Hobbs , G","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.320148Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:b7f4146ae358cc13353146f0ca9e8ec5d3d4bbf65ca095aed8220794f3f9ea38","observation_id":"c0d06117-dd3b-44f3-923e-a01e6d1c5f31","resolution":{"observed_at":"2026-08-15T23:25:58.320148Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.695928Z","title":"N., Lyne , A","venue":null,"work_id":"a018beae-e438-4167-af24-ea3f2100da7e","year":1978},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.323491Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:0db4fd69286eb7c11175cc347db39d4088b1912a760db62b0e942192ceda0da1","observation_id":"5275c219-8c85-4c95-bf62-d834ff9642e4","resolution":{"observed_at":"2026-08-15T23:25:58.699561Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.685328Z","title":"N., Taylor , J","venue":null,"work_id":"aa2d31bf-582a-4b2d-9257-5463810980bb","year":1972},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.326453Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:18099e5149788d92b15ff6a9b35e7ae9c4d23cd7d071de6eda8e451bfac5fd06","observation_id":"c92d377e-b9d7-4db1-94e1-f126dbb53d66","resolution":{"observed_at":"2026-08-15T23:25:58.688971Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.675394Z","title":null,"venue":null,"work_id":"836aabe8-a58d-4c7e-9dae-8c67b1982056","year":2017},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.329338Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:637069c79d83fd3befa22f8c8f1b0e25c9c8830e47f1d92eefaa465d4dd64ffc","observation_id":"09d3160d-6f26-4eaf-b8fb-1f9e46607f6a","resolution":{"observed_at":"2026-08-15T23:25:58.678620Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.665254Z","title":"2018, RMextract: Ionospheric Faraday Rotation calculator , Astrophysics Source Code Library, record ascl:1806.024","venue":null,"work_id":"7af6bb0c-e3da-4baf-91c6-93e6635d2b01","year":2018},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.332336Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:67c2cd7df944ebad25d541d85fc77e1cb0b8f3556626646e50ff7a5d140414b3","observation_id":"4aaa4ac7-e732-4f26-a34e-4a7b69fca8ca","resolution":{"observed_at":"2026-08-15T23:25:58.668634Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.655065Z","title":"D., Cooper , S., et al","venue":null,"work_id":"4069fb6e-7083-4d79-92d5-7424f0600314","year":2019},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.335534Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:383fb7919569eb1e1c162628954ee989e0937da7f1f58dbdf1f22a51d6cbb6ba","observation_id":"7bc00afb-a4de-4bd2-90c7-d6606e3cba76","resolution":{"observed_at":"2026-08-15T23:25:58.658389Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.645051Z","title":"C., Keith , M","venue":null,"work_id":"1423d0b7-2026-4d3a-852c-2ed50aa9eb7f","year":2024},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.338516Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:1c646b0f3b3dedd3f3f58dd8236fc9b5fda47b12c729da999c3abac390857de1","observation_id":"d106bffc-a389-49a0-9e35-8a853739e946","resolution":{"observed_at":"2026-08-15T23:25:58.648490Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.341539Z","title":"& Freire , P","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.341539Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:b5f4ec32741624904ce57dd98eb20768509cd920e572ca8d2f085b97016922ed","observation_id":"c4ca8ac3-aa16-4853-933c-87c8806aa2fa","resolution":{"observed_at":"2026-08-15T23:25:58.341539Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.629047Z","title":"V., Barr , E","venue":null,"work_id":"edfa8a4b-d4c0-483a-9554-5fb3e5094da7","year":2021},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.344471Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:3a5cb481e950697710151e22ba13cb2ebf2a8707044f897bedb64c9a7d2f1921","observation_id":"f482d839-c255-4dd4-b23e-6e005c6bc97c","resolution":{"observed_at":"2026-08-15T23:25:58.632379Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.619200Z","title":"S., Folkner , W","venue":null,"work_id":"77fd9868-d002-4a8c-a18d-ca6a9427b7b1","year":2021},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.350335Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:1766ada82bd65b1de4b7766b4dd52bdd7b06f6bdaae408426f6bfddc01860469","observation_id":"3ae26d20-9fc0-41ad-9fb0-ecb5cd0df8cd","resolution":{"observed_at":"2026-08-15T23:25:58.622598Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.608145Z","title":"T., Demorest , P","venue":null,"work_id":"0a4ea49b-289a-4167-a64f-4114006c48f5","year":2014},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.353632Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:2e5808568c031e2d52f8aaceec4cfa614c2e262bad6b81da48b1d42bb1b71f65","observation_id":"27e06134-eeb4-4784-8b54-e62366d9720e","resolution":{"observed_at":"2026-08-15T23:25:58.612615Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.356797Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.356797Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:1be69d45df628d359adc85389d2e5e5d532161cbd34c47be999d5cbc88f4ca64","observation_id":"af17a26b-ea2c-4f56-b4f0-74551bbbc3d7","resolution":{"observed_at":"2026-08-15T23:25:58.356797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.592333Z","title":null,"venue":null,"work_id":"6ef5db1c-5d7e-4915-a164-b8fe674a83fe","year":1968},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.360053Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:33b75ec595ef1bf68f03315c5a414ce52faefdf0d6cd8cde7b75df3a19e8ac21","observation_id":"ce030265-e503-4a64-a422-7e7e83b557f0","resolution":{"observed_at":"2026-08-15T23:25:58.595754Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.363175Z","title":"J., Zic , A., Shannon , R","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.363175Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:47aba3f69822b3e87f3753b15d1156c3fe1923b62b4202f24c8e6c79a7408e3b","observation_id":"2c9f75c4-bf87-4b17-8663-f761c6631aae","resolution":{"observed_at":"2026-08-15T23:25:58.363175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.575433Z","title":"1989, Stochastic Complexity in Statistical Inquiry, Computer Science Series (World Scientific Publishing Company Pte Limited)","venue":null,"work_id":"dde0f450-2b7a-4324-84ff-c085adb111f4","year":1989},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.366438Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:007f3944981d1b0daff967d13fbf5b469a2a07af860c71b9c0c4d398343ffc56","observation_id":"f51f3ff6-4d06-4693-8607-56f0aa0b40c2","resolution":{"observed_at":"2026-08-15T23:25:58.579244Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.565465Z","title":"F., van Straten , W., Gulyaev , S., et al","venue":null,"work_id":"5b79f73a-eaea-41bd-b7a6-72908ae1f0ab","year":2024},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.369608Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:4a6a888f43b8f205bcc64a0c1b03e87205eff242d55107a108d95fde3b1b560d","observation_id":"86b8907a-3623-4a17-a3b0-41d51e8a8558","resolution":{"observed_at":"2026-08-15T23:25:58.569015Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.372749Z","title":"1978, The Annals of Statistics, 6, 461","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.372749Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:e18164bc9a744657b52ab54c3c91105f77eaeff8bca04b184ac296a4779b7225","observation_id":"d27ca01d-e3ce-4ceb-a8d9-0c03f8446156","resolution":{"observed_at":"2026-08-15T23:25:58.372749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.549747Z","title":"J., Rawley , L","venue":null,"work_id":"437f1913-bf5f-42b5-9bac-a68462248ca7","year":1986},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.376189Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:b7a3593dc4689b2a1e21d5473a065e21379c52907b5d8cd1495006a243cacf14","observation_id":"5eae5926-8323-4ac2-91a6-a99389bc28c8","resolution":{"observed_at":"2026-08-15T23:25:58.553126Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.379285Z","title":"P., Joshi , B","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.379285Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:b0820dddd79b55ac871935dd02bd6a85242e811c68b2afee8d5ad03b7ecaa8c2","observation_id":"3c341006-b59b-4476-ab38-086ba0ce06e8","resolution":{"observed_at":"2026-08-15T23:25:58.379285Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.533686Z","title":"R., Cordes , J","venue":null,"work_id":"b67ea321-f705-46a9-8daf-d06a1f0e024f","year":1984},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.382463Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:c77e5e909292d69c12e414cbff1bae7f851ad300861f19233d28d7480607bc70","observation_id":"53afba2f-c526-4a0f-98b3-1787f147180e","resolution":{"observed_at":"2026-08-15T23:25:58.537278Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.523724Z","title":"2005, , 430, 373","venue":null,"work_id":"7624233c-79e8-4372-948d-230a104d26b4","year":2005},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.385764Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:cc8c1549e7c729fd0c0e94790388191616d5bfdfae82f5e3d72b7724ec6caaf5","observation_id":"5548de8c-7884-4ab5-a41c-9b162a5282b4","resolution":{"observed_at":"2026-08-15T23:25:58.527011Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.513640Z","title":"2004, , 152, 129","venue":null,"work_id":"640a6b81-157c-46e8-b103-0fa69fd92b34","year":2004},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.389005Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:0c1e2a31f76377b59a7eb34ab53c1be0fd1d6220dff13bba9edac8a28aa79d07","observation_id":"1e3b1c84-dd3a-4c99-8ee5-eecaebfb8c57","resolution":{"observed_at":"2026-08-15T23:25:58.517000Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.392249Z","title":"2006, , 642, 1004","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.392249Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:fb823d735c0d747062c15d9734d2c8cd42d95ca4262a36b2d1cfbcdbaa50182c","observation_id":"eb14ce22-ffe7-46fe-af6c-4a85e6b9dcd7","resolution":{"observed_at":"2026-08-15T23:25:58.392249Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.497289Z","title":"2013, , 204, 13","venue":null,"work_id":"daf53083-a8f6-45e3-b624-73969c879321","year":2013},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.395514Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:9740d06d868e616f7f453b9cc74a8541c62e5fe24751d06acad1371bb3340a28","observation_id":"16fb4947-4cb9-479c-b85b-347f8c0f9680","resolution":{"observed_at":"2026-08-15T23:25:58.501096Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.398750Z","title":"E., et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.398750Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:c3cc695dc5632d96d0d11646b52d8c5a480b87319b3654af6e357f1d45e6efc5","observation_id":"649007f7-b5b4-461c-9100-2542b7c3fec9","resolution":{"observed_at":"2026-08-15T23:25:58.398750Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.482031Z","title":"2025, , 693, A143","venue":null,"work_id":"3c3b1d3d-5fad-4008-88c9-54fae773fcff","year":2025},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.402161Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:e9c85743faf2be0a2db940521f9c6db2dfcc5a24f2d880309326157359fb9977","observation_id":"85306ffc-3657-48f3-9071-bc2dce62e773","resolution":{"observed_at":"2026-08-15T23:25:58.485177Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.470580Z","title":"X., Burgay , M., et al","venue":null,"work_id":"3d620f4b-334b-4863-a3ad-2d8cc9b32b63","year":2021},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.405165Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:83be4ece3916f6587d6b080cabbf197bfcd46ce11a4444bd8cc6af0bbbebdf48","observation_id":"01a20910-d319-4540-b011-daabeeb13f9e","resolution":{"observed_at":"2026-08-15T23:25:58.474861Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-15T23:25:58.408141Z","title":", \" * write output.state after.block = add.period write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.408141Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:84394cdeed42c1d7bbfc063fba6200a689a8cb4450c7a8136850475811221976","observation_id":"b558d959-4ed3-43de-be07-b65b4223c626","resolution":{"observed_at":"2026-08-15T23:25:58.408141Z","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":"2026-08-15T23:25:58.411799Z","title":"write newline","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing","version":2},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-15T23:25:58.411799Z"},"links":{"citing_paper":"/paper/2505.04990"},"observation_digest":"sha256:7686a6cd30ef3191860b4ea09926cfa39956d36c9abefe1accfeec9c90986c2b","observation_id":"5e9e0d7a-f6c7-4536-ba7c-a6283869fce7","resolution":{"observed_at":"2026-08-15T23:25:58.411799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.04990","last_updated":"2025-05-23T08:25:01Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-17T18:47:42.620577Z","submitted_at":"2025-05-08T06:53:20Z","title":"The polarimetric response of the Nan\\c{c}ay Radio Telescope and its impact on precision pulsar timing"},"reference_resolution":{"displayed":71,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":31,"verified_exact":0,"verified_fuzzy":40},"total_outbound_references":71},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 71 of 71 outbound references and 0 inbound Pith citation observations for arXiv:2505.04990."}