{"as_of":"2026-07-29T09:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:40584e69f4e581cf8f9b9d44071305c78b9aee6d476bb678e2098b6923c488a2","coverage":[{"denominator":32,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":32,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-27T11:03:01.530146Z","state":"measured"},{"denominator":32,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":32,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-29T08:13:00.99439+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/2606.10686/citation-record","integrity":"/paper/2606.10686/integrity","json":"/paper/2606.10686/citation-record.json","paper":"/paper/2606.10686"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2024.116805","doi":"10.1016/j.cma.2024.116805","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Computer Methods in Applied Mechanics and Engineering 421, 116805","venue":null,"work_id":"09db11ae-f36f-4d58-bfdb-4ea8ee5edced","year":2024},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:6de2d9e9a33b54c71269ae72707191bfab9357e2365e3a9d0ea836722c484f23","observation_id":"e828a02e-c3a9-4391-8cf1-9232fbcf6d15","resolution":{"observed_at":"2026-06-27T11:10:51.827388Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/2041-8213/ad0556","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T08:51:48.354323Z","title":"M., & Levin, Y","venue":null,"work_id":"4a7eda7a-8221-4d70-8bd2-d342fb12066c","year":2023},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:5ebfd9fdd8cadd20ffa4fb7ce0aa162f30b829ee5a9a8fe7591ff9b0aeecee9c","observation_id":"1a5fc839-c196-4705-a77f-70577bb7eb93","resolution":{"observed_at":"2026-06-27T11:10:51.810368Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-05-24T15:25:33.666378+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-24T15:25:33.666378+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stv042","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T04:23:06.225479Z","title":"Particle acceleration in axisymmetric pulsar current sheets,","venue":null,"work_id":"ebd4516a-b029-42a3-9f6d-0e6070fe8fd3","year":2015},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:c21d3238d286f1982345f95085ba64c1c3aa62f6104265ab6561a7bb6fd4a6e9","observation_id":"a289a16e-9f37-4eba-afde-b9d2acf870eb","resolution":{"observed_at":"2026-06-27T11:10:51.837608Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/306652","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-01T06:15:27.899919Z","title":"1999, ApJ, 511, 351, doi: 10.1086/306652","venue":null,"work_id":"17f5ebe9-6708-407a-bad4-e3df8501f94a","year":1999},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:4ba358b480d8ef6b3d2dbee09a79715bf6a41b8f38cc91bd20c17bd8ea286abe","observation_id":"e194725a-2c94-46a9-a354-2e2c5162d8fe","resolution":{"observed_at":"2026-06-27T11:10:51.839437Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-13T20:49:51.531898+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T20:49:51.531898+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202554175","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.807453Z","title":"Astronomy & Astrophysics 705, A140","venue":null,"work_id":"1fc66dbd-f2d9-4fd0-a7e6-488c19492904","year":2024},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:1166679923f8e660b2665bde55aae70476c80249bce183a8164cb77bd481a188","observation_id":"593cf6ff-002c-48ad-9b18-bbd2be987f8e","resolution":{"observed_at":"2026-06-27T11:10:51.808657Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/152639","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.810886Z","title":"Astrophysical Journal 187, 359–360","venue":null,"work_id":"74d40c55-9124-41dd-8dbf-ae240a10d310","year":null},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:29626975e6dd1dfde57f2c8c3f24e3cd09fddcecc8e90524e3b2b54e60e7fda8","observation_id":"fdfee7b3-a019-4612-bfb9-4cd48508d894","resolution":{"observed_at":"2026-06-27T11:10:51.812030Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.camwa.2026.05.003","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.840019Z","title":null,"venue":null,"work_id":"c38976a6-3806-493b-8660-ccbc818c4a83","year":2026},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:23d9cf9d3801972bf8502759b8b789a83532d715413f1c1f8f8828373243a09b","observation_id":"efa5263e-5a97-46a3-a5f9-aa20c7505453","resolution":{"observed_at":"2026-06-27T11:10:51.841081Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/150119","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-03T19:38:51.918633Z","title":"year = 1969, month = aug, volume =","venue":"The Astrophysical Journal","work_id":"2690565e-a870-4cba-97a9-c781988b2d49","year":1969},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:5a26e353764b4679eec12f66711801b3b62204fd45aafd55c724268963b871c0","observation_id":"c7c33274-7f7b-4565-95f2-d5fa29674712","resolution":{"observed_at":"2026-06-27T11:10:51.835674Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-13T20:49:56.387438+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T20:49:56.387438+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1038/217709a0","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T13:07:05.384001Z","title":"J., Pilkington , J","venue":null,"work_id":"f27b36bd-4b96-4f1b-8c18-4ac0c9e95b9c","year":1968},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:75a1af514d4fda0f8b84a05ecdda2c31d51c31c9e7be06e0b538da3cc64483f2","observation_id":"f4f6d744-d89d-489b-bdb6-e29a1efcb4ef","resolution":{"observed_at":"2026-06-27T11:10:51.804996Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-13T10:49:45.06418+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T10:49:45.06418+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2022.111402","doi":"10.1016/j.jcp.2022.111402","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"8580–8589","venue":null,"work_id":"5b460e6f-96eb-489e-9c8f-514503c77529","year":2022},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:47b5a2296f54dcecc276ce9ad50966ecfa5a8296f0e5f2c948edcc7232dedee1","observation_id":"e875a803-7a22-404b-b582-4e3b588f4214","resolution":{"observed_at":"2026-06-27T11:10:51.824750Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aab550","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.821426Z","title":"K., & Kazanas, D","venue":null,"work_id":"7b53173e-5068-4213-bc23-b9708c94d8e8","year":2009},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:6a7224d380237bd56698c5415b7c84361e014236beeeff7d847ea10443b08971","observation_id":"b277e97c-8e7a-4a68-8680-d73c3f3d8f71","resolution":{"observed_at":"2026-06-27T11:10:51.822448Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-13T20:49:58.874515+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T20:49:58.874515+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2966.2005","doi":"10.1111/j.1365-2966.2005","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A., okas E","venue":null,"work_id":"fbe25bd0-9403-4539-b873-fcf6743fba70","year":2005},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:184f21e6db356245ef6bdbb38a150f5102f857003702a91482fba5bf2b74bb7b","observation_id":"16256614-f9be-44be-8855-4394376fff2d","resolution":{"observed_at":"2026-06-27T11:10:51.803188Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.neunet.2020.12.028","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.805605Z","title":"Neural Networks 136, 112–125","venue":null,"work_id":"0f3b6a50-98ac-4904-b884-4e66606d648f","year":2020},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:91f3489de78db50660875dd16868822b375bc64091bf5399e941d904713d2a28","observation_id":"556d584c-35d2-4175-8d37-040f3e4a028f","resolution":{"observed_at":"2026-06-27T11:10:51.806887Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.107.064025","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.812578Z","title":"Physical Review D 107, 064025","venue":null,"work_id":"f8ac3e00-faee-4024-b741-d004d1f9d0ba","year":null},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:49338c7dd4864631a0241673b72b2a74c1c37f9c3aaa794c3e4e4735ec238400","observation_id":"5b0e3ff6-0c6d-4b23-b616-faca2d429730","resolution":{"observed_at":"2026-06-27T11:10:51.813626Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+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":"2026-06-27T11:03:01.530146Z","title":"Mémoires of the Société Royale des Sciences de Leège 8, 79–91","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:dfbf5494830fd4917f4c5f6c51c06b999f68ad7fbe4a4a72177d60e4e7f8a21f","observation_id":"6db6a497-d67f-419c-98c9-5b7fe43e1c00","resolution":{"observed_at":"2026-06-27T11:03:01.530146Z","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/692/","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.819825Z","title":"Philippov,A.A.,Spitkovsky,A.,2018","venue":null,"work_id":"9707db9b-9a63-4519-801e-10e52de32d5f","year":2018},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:df02901852c8615eb9e008fff9ba9f3b500a39fc1bde110ad12c4725bba748de","observation_id":"bf8b3c13-c45b-493c-b5b5-339fbf2dd020","resolution":{"observed_at":"2026-06-27T11:10:51.820895Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aaabbc","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T23:34:03.905321Z","title":"A., & Spitkovsky, A","venue":null,"work_id":"9a3ae5ba-de5d-47de-bdb1-89e46faf953e","year":2018},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:8447400a167f2cfcf168b6f424209973d60d895c69c4178cb03cd4e747986b41","observation_id":"2742bcd1-07c9-49d5-a2fa-4bdc991a4c52","resolution":{"observed_at":"2026-06-27T11:10:51.798689Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-12T18:20:51.908693+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-12T18:20:51.908693+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.jcp.2018.10","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T08:11:49.497807Z","title":"Journal of Computational Physics,378, 686–707.http://dx.doi.org/10.1016/j.jcp.2018.10","venue":null,"work_id":"05312348-b5e5-41e2-80f2-2434f0346039","year":2019},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:3237ea55536fa720e1d17dbb98a79e11050299d5daeffed5c58ea8e00c4292fa","observation_id":"c1f2814d-7081-45e6-9f6d-cb02a98b95e0","resolution":{"observed_at":"2026-06-27T11:10:51.819235Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-05-19T15:22:33.049688+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-19T15:22:33.049688+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevfluids.6.073301","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.814168Z","title":"Physical Review Fluids 6, 073301","venue":null,"work_id":"638612de-ff4c-4dbf-a58f-c31682667255","year":2026},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:747505e011ccd6b039709bb2db5df38679207920747b785b6973080b98351e0b","observation_id":"02e4b2e7-50e9-47a3-9cb3-9e491b09b727","resolution":{"observed_at":"2026-06-27T11:10:51.815253Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.21105/joss.07830","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.794103Z","title":"Rigas,S.,Papachristou,M.,Papadopoulos,T.,Anagnostopoulos,F.,Alexandridis,G.,2024","venue":null,"work_id":"2191cc50-656f-4645-80e9-104862021f42","year":2024},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:8ce690f181c54aafe64ef889fbbc26614eb2c1d75b1f3c07b6cf5ddfd35d0021","observation_id":"8f99e3f2-0127-46cf-b285-13b65a11d462","resolution":{"observed_at":"2026-06-27T11:10:51.795424Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.neunet.2023.03.014","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T21:32:38.073085Z","title":"Deep learning-accelerated computational framework based on physics informed neural network for the solution of linear elasticity","venue":null,"work_id":"014e6963-f210-4b37-b8a5-e63fae43439c","year":2023},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:a038f40d557867bf8c8fc1fa3baf4dc341f903671173bb28065ab486c8a53c13","observation_id":"8695ff55-88d1-4e23-96b9-cd0575c14ca4","resolution":{"observed_at":"2026-06-27T11:10:51.797071Z","resolver_source":"doi","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2024.117290","doi":"10.1016/j.cma.2024.117290","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A comprehensive and fair comparison between mlp and kan representations for differential equations and operator networks","venue":null,"work_id":"88afb0f1-f6ac-49ac-8526-ddd9e4540d03","year":2024},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:dc033b85702e5dacfce9c562f603de49ff0cb3626eb56a90dcdbaeb4f08df3e1","observation_id":"7a087f29-268e-4810-8886-1594eda982b7","resolution":{"observed_at":"2026-06-27T11:10:51.829905Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-05-25T15:54:15.875918+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-25T15:54:15.875918+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361/202450238","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.830419Z","title":"Astronomy & Astrophysics 690, A170","venue":null,"work_id":"677a1f5d-58b6-4d49-9907-3179f0afbea1","year":2006},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:e5ac730e9146eafbe710795b7c12ecb3d5637438247b8628132f64088dccb71f","observation_id":"77466582-9bc1-4c7e-ae16-118574daaa52","resolution":{"observed_at":"2026-06-27T11:10:51.831442Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/stad2840","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.790483Z","title":"Monthly Notices of the Royal Astronomical Society 526, 1504–1511","venue":null,"work_id":"d5c04425-f3af-42c6-9491-ae2cf9a14cbb","year":null},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:79c65a9e74db96993815b63e6dc1bd8961d6790ab7f938147f27bbb76988c913","observation_id":"3192f506-38a4-4260-a566-9a4d06b56262","resolution":{"observed_at":"2026-06-27T11:10:51.791911Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnrasl/slt076","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.815821Z","title":"Monthly Notices of the Royal Astronomical Society: Letters 435, L1–L5","venue":null,"work_id":"cac1d25c-111a-4767-95f2-fecdb63846b4","year":2006},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:414cdcdd97010d7e9a9e84d92384e65410d97f43e799bb7052a1c7fba8298766","observation_id":"ae26c8e1-4939-4bfc-b648-f598fcfe7c3b","resolution":{"observed_at":"2026-06-27T11:10:51.817064Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2025.107831","doi":"10.1016/j.neunet.2025.107831","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Toscano, J.D., Wang, L.L., Karniadakis, G.E., 2025b","venue":null,"work_id":"1cd2f359-70b8-4c5a-abad-36c5373fe3ee","year":2025},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:acfaaad9e0fa3bbd7b33551a5608adbd3f8b12099219a44d61a549a3d709c75e","observation_id":"274a2b50-87a3-4d76-9140-82f6b90fe2a0","resolution":{"observed_at":"2026-06-27T11:10:51.833873Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjc/s10052-025-14942-z","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.788817Z","title":null,"venue":null,"work_id":"3b2a388a-5c62-493d-aef2-d8af9b1d3f20","year":2023},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:880cf3cb939b7aca7f1444b5b424aaf97a696e7ee91a680313d6bdd369d68c4e","observation_id":"610e4077-a9b6-49cc-bad3-c6eb2155eca1","resolution":{"observed_at":"2026-06-27T11:10:51.789927Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1086/378849","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T11:10:51.792427Z","title":"Wang, S., Li, B., Chen, Y., Perdikaris, P.,","venue":null,"work_id":"4106def3-22fa-43af-a9ab-1cdf0e791c34","year":null},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:021e622f59a3a0dfb6423960e7ff84e8dd2c842754791937ba6d5365d59422a7","observation_id":"30d16964-8345-414e-9c67-738c3c8740f1","resolution":{"observed_at":"2026-06-27T11:10:51.793577Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1137/20m1318043","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T19:15:30.321168Z","title":"Understanding and Mitigating Gradient Flow Pathologies in Physics-Informed Neural Networks.SIAM Journal on Scientific Computing, 43(5):A3055–A3081","venue":null,"work_id":"53d02581-afe6-4c86-a4f6-3cf42b260d77","year":2021},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:9e1c531eea7d0981c00b0694b23809069da90d543fe8714acc5908d75516befe","observation_id":"75d755cb-14c0-4a88-9fde-bcd96ae173f0","resolution":{"observed_at":"2026-06-27T11:10:51.800541Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-11T04:49:03.759395+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T04:49:03.759395+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2021.110768","doi":"10.1016/j.jcp.2021.110768","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"When and why pinns fail to train: A neural tangent kernel perspective","venue":null,"work_id":"bbe79eb6-d9a2-408e-a4c5-d783ed773ff0","year":2022},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:a64d7970dd726b614155cfb3ecfbb058251fdd7e1ada0d7db5b25838adbc9be1","observation_id":"4b5c595d-d637-491e-9202-5bacf5eaaca1","resolution":{"observed_at":"2026-06-27T11:10:51.785697Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-11T01:19:05.793563+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T01:19:05.793563+00:00","source":"openalex_status_cache"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2021.114124","doi":"10.1016/j.cma.2021.114124","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"URL:https://openreview.net/forum?id=ydlDRUuGm9","venue":null,"work_id":"34cba0ec-23f3-43cf-b2b3-59f5c852a63e","year":2021},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:25ee9a7fc78b1e3134604b53871515d961a6655c4157e7e35cda6d103e597c79","observation_id":"f6c5e448-80f6-4f66-8648-4cdfce2a1ff5","resolution":{"observed_at":"2026-06-27T11:10:51.788173Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-29T08:13:00.99439+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+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":"2026-06-27T11:03:01.530146Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-06-27T11:03:01.530146Z"},"links":{"citing_paper":"/paper/2606.10686"},"observation_digest":"sha256:adb698c4f20ef7011e72c56c27649beeecca4f6f5f0728d2f7c158efd6124cba","observation_id":"9cb1becc-e9cc-4fd8-ba7d-554965c30312","resolution":{"observed_at":"2026-06-27T11:03:01.530146Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2606.10686","last_updated":"2026-06-18T15:50:35Z","latest_version":2,"primary_category":"physics.comp-ph","snapshot_observed_at":"2026-07-06T23:49:51.672382Z","submitted_at":"2026-06-09T10:44:10Z","title":"An adaptive framework for the axisymmetric pulsar magnetosphere using physics-informed Kolmogorov-Arnold networks"},"reference_resolution":{"displayed":32,"state_counts":{"malformed_identifier":1,"metadata_mismatch":8,"parse_uncertain":0,"unresolved":2,"verified_exact":21,"verified_fuzzy":0},"total_outbound_references":32},"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":"2026-07-29T08:13:00.99439+00:00","source":"crossref"},{"observed_at":"2026-07-29T08:12:51.666926+00:00","source":"retraction_watch"}],"thesis":"As of 29 July 2026, this Paper Citation Record lists 32 of 32 outbound references and 0 inbound Pith citation observations for arXiv:2606.10686."}