{"as_of":"2026-08-19T21:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bfacb97933c361f0fe974442b24467301a8b573e5a6f1d706a9667b36c57bc62","coverage":[{"denominator":137,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T01:02:50.872004Z","state":"measured"},{"denominator":100,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":100,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+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/2508.04744/citation-record","integrity":"/paper/2508.04744/integrity","json":"/paper/2508.04744/citation-record.json","paper":"/paper/2508.04744"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T01:02:41.600818Z","title":"Perlmutter et al","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:41.600818Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:36e7da509f9eef5d237a7cd6a19f8e88a36f2e251eb6f783f296b29cf8d30348","observation_id":"d83b6e36-7c05-499c-8ede-7d6021990391","resolution":{"observed_at":"2026-08-06T01:02:41.600818Z","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":"2026-08-06T01:02:41.676588Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":2,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:41.676588Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:512305aebeacf2998bd35d3924ea1bba404ddb7f390a1bf95f15df03d89d9a1e","observation_id":"0772c918-2b6d-40aa-b05c-309c42e9b0f6","resolution":{"observed_at":"2026-08-06T01:02:41.676588Z","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":"2026-08-06T01:02:41.757479Z","title":"Collaboration, Astronomy & Astrophysics (2020)","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:41.757479Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:0d8b2acace57c5a479aff7cff2a77a1dfd28fca97b7d0fb54c9b869ebbeda1d4","observation_id":"761359dc-2c62-4975-bcb8-c386d812675b","resolution":{"observed_at":"2026-08-06T01:02:41.757479Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1093/mnras/staa3914","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Monthly Notices of the Royal Astronomical Society","work_id":"bace311b-7b93-4682-aeb5-bac45d2b4d27","year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":4,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:41.852552Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:89cd4bca9494d1ffa2a788abdae2d480325a25124a207f3d22f700e57f6471d9","observation_id":"056f16d0-4f9c-47e5-bcfe-81d5af7881c8","resolution":{"observed_at":"2026-08-06T01:02:58.295996Z","resolver_source":"doi","status":"verified_exact"},"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":"10.1103/physrevd.65.063001","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Huterer, Physical Review D 65 , 063001 (2001), doi:10.1103/PhysRevD.65.063001","venue":"Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields","work_id":"48a1522d-a589-45e7-b293-d3d1d6a2f16b","year":2001},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:41.952349Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:3d71ff1a76299bf2998e118049e10c6607aeb00682552ceed2bcdc8e41256219","observation_id":"9b303d3a-6e61-4df5-a685-b5fa1160b96d","resolution":{"observed_at":"2026-08-06T01:02:58.084216Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:02:42.052429Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.052429Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:0be91df88ff6c3fe541977f547211d1db52d282aa6630472b08ea9e7dd252244","observation_id":"671394d1-b33a-4937-9c6d-5099f3bf6cec","resolution":{"observed_at":"2026-08-06T01:02:42.052429Z","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":"2026-08-06T01:02:42.147525Z","title":"Del Popolo and M","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.147525Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:e0bd6d4e6ad92781a1a321a48491c7f068af8dc248231e564b925481cc7907c4","observation_id":"3f61db52-3683-4915-bbd2-155c98a7b3f9","resolution":{"observed_at":"2026-08-06T01:02:42.147525Z","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":"2026-08-06T01:02:42.231785Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.231785Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:359203fbe6035b92f56ae37132de87ff22808ee4aa268739214cbb75893c2000","observation_id":"477f6b63-0876-4e3f-81d4-baada010bb1b","resolution":{"observed_at":"2026-08-06T01:02:42.231785Z","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":"2026-08-06T01:02:42.327584Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":9,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.327584Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:247076a3449d6a6019c0bfe650f50a95f70ae535fdbad12dbe68be3a8fd4e060","observation_id":"c3c35d6e-624e-41e7-8d8f-d4a9d4f73ef6","resolution":{"observed_at":"2026-08-06T01:02:42.327584Z","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":"2026-08-06T01:02:42.446884Z","title":"Armendariz-Picon, V","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.446884Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:64b5bc7b3bcbdfe9b68a29bbf69c6c091faa19c2a83091cebd5a6903adf63b24","observation_id":"025e3454-40d3-4652-9b98-29aa7a8f8005","resolution":{"observed_at":"2026-08-06T01:02:42.446884Z","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":"2026-08-06T01:02:42.577389Z","title":"Khoury and A","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.577389Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:87e970ef234f23ce17c1f157f61eba937268dc86346a2e49c9a704916b4871f3","observation_id":"b38b1583-32bc-4170-942d-8a8b679efead","resolution":{"observed_at":"2026-08-06T01:02:42.577389Z","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":"2026-08-06T01:02:42.651873Z","title":"Khoury, Classical and Quantum Gravity 30 , 214004 (2013)","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.651873Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:69e95acb7171a23a4a919b9d64b16d6985f045181e610a4e7d50a5282aee6c5d","observation_id":"40e4abe3-bb1e-4872-b211-17033cf7988d","resolution":{"observed_at":"2026-08-06T01:02:42.651873Z","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":"10.1103/physrevd.104.084017","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical review. D/Physical review. D.","work_id":"c17db63b-9799-419a-851b-237b1166dc49","year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":13,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.717970Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:d359b92d3206612722f1ba1536a92fcd83b3f165fb9756b1f31d57686b383387","observation_id":"7895b580-5b5a-42d9-a46d-1a15e7db1501","resolution":{"observed_at":"2026-08-06T01:02:57.798595Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:02:42.849376Z","title":"Brax, A.-C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":14,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.849376Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:304b328fdb3b130fe83abc54a6741230cc03590565cf7504c680bd4eb0a28ace","observation_id":"5a9a0d62-e800-41fe-b658-e08226b21b67","resolution":{"observed_at":"2026-08-06T01:02:42.849376Z","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":"2026-08-06T01:02:42.953713Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":15,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:42.953713Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:0c17b67a8250552985879901f726bcad1fd91139e235f5b50b5752058c5a6c80","observation_id":"d210cab1-0507-4b51-8bb5-811164e70b90","resolution":{"observed_at":"2026-08-06T01:02:42.953713Z","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":"10.1103/physrevd.103.044042","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Vlachos, E","venue":"Physical review. D/Physical review. D.","work_id":"3308ad9c-4314-450b-995f-82ce5f0557e1","year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.083715Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:2deacf62e8bcae964223cd754ba77082aa9574ae74eef14a99b30be144f0ba26","observation_id":"a2541599-04d0-40b7-a28d-c9ee2dc54c11","resolution":{"observed_at":"2026-08-06T01:02:57.621364Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:02:43.191063Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":17,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.191063Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:172abeeb3bb544fbbace62def30c06a85787f196c1e3e52bd265f187c0291011","observation_id":"e2a1b349-37f5-4135-9097-0b8d4e1550c8","resolution":{"observed_at":"2026-08-06T01:02:43.191063Z","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":"10.1088/1361-6382/abf97f","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Cañate, J","venue":"Classical and Quantum Gravity","work_id":"5e0d9af6-87d5-4d1c-8e36-7f6068e2af72","year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.283521Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:203498f5b5706b7f3c4a7fd2d931fa8502062a23c460087dea8a9bb6a8572887","observation_id":"d19687f2-b5a7-4a49-99fd-67b45bd77681","resolution":{"observed_at":"2026-08-06T01:02:57.406137Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:02:43.400076Z","title":"de Cesare and R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":19,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.400076Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:f79e4d3636d116a05f7e823e41c59054efd2eac3bcd499e1772127d7fd8263d7","observation_id":"4e84bb43-d215-4393-b714-2b45734a3098","resolution":{"observed_at":"2026-08-06T01:02:43.400076Z","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":"2026-08-06T01:02:43.531381Z","title":"Davis, R","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.531381Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:98267e9f11618160f959bdb5dc17b41374195e4f8b4898c1b3efdd35a14d78b7","observation_id":"7b29b90b-e64c-4530-b8cb-cb542dbca0e1","resolution":{"observed_at":"2026-08-06T01:02:43.531381Z","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":"2026-08-06T01:02:43.661067Z","title":"Ottoni, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":21,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.661067Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:943acaa4a69fe63e6cf1bdc6cd7996b6492afc39d92d1820d450c1a6844b8a4a","observation_id":"ef772449-5b07-4623-bec7-ebc5f4a67905","resolution":{"observed_at":"2026-08-06T01:02:43.661067Z","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":"2026-08-06T01:02:43.787763Z","title":"Maurya, K","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":22,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.787763Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:721fea6776333af09d0b3f8a8121b823ec533780c3f06cb8510e7e5c9e04bb94","observation_id":"d52f4043-4ff4-40d6-bb43-2579bf436796","resolution":{"observed_at":"2026-08-06T01:02:43.787763Z","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":"2026-08-06T01:02:43.919586Z","title":"Barausse, C","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":23,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:43.919586Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:d4db21d798f59770271dec6532792edfd961013a77b0454d6d75891939920d1b","observation_id":"c83c94a2-1b03-4937-8d4e-c19c5497f20a","resolution":{"observed_at":"2026-08-06T01:02:43.919586Z","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":"10.1103/physrevlett.126.011103","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Herdeiro, E","venue":"Physical Review Letters","work_id":"e78c5fd5-356d-4b97-84e2-0564baa0fdb2","year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":24,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.041682Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:1064fc26866bbb4ca450105cbd4bbe3b2aa123350ead0bd1adcda2c2721d1ba8","observation_id":"8b7d9d97-0b5f-4471-a723-95b785fdceb2","resolution":{"observed_at":"2026-08-06T01:02:57.271046Z","resolver_source":"doi","status":"verified_exact"},"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":"10.1103/physrevd.100.024010","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Physical review. D/Physical review. D.","work_id":"951f248f-1035-4890-98b6-cbdd41e47805","year":2019},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":25,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.195249Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a5ab740086550e7540ff468fdc018c7f513023027ee391da2982196b8cacdbec","observation_id":"48ce7499-985d-4afa-bcb0-30b6939aa473","resolution":{"observed_at":"2026-08-06T01:02:57.075398Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:02:44.299930Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":26,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.299930Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:63d698b6bf2bd5e51c130d6293925fbda2591f97e84ee19f8a9f00cceebdb665","observation_id":"3bf429d7-509c-411c-a981-fd7838d863d3","resolution":{"observed_at":"2026-08-06T01:02:44.299930Z","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":"2026-08-06T01:02:44.422253Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":27,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.422253Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:6cacc1b218a3bf5961d144d27cb9cfbfea2e3410d5e3a90e1e29d3293ad088ce","observation_id":"a7898c20-8bcd-4f41-b2b4-b9a725512197","resolution":{"observed_at":"2026-08-06T01:02:44.422253Z","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":"10.1088/0305-4470/8/4/012","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":null,"venue":"Journal of Physics A Mathematical and General","work_id":"8c4bdc89-4e4e-4ed6-b5cd-8a544c38c813","year":1975},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":28,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.513746Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:10726335821f265ac4b029c2144ffa269f0e8694971bdacb57007af7f7fea471","observation_id":"34471148-ed2b-43eb-af2b-d1c1dc044ae4","resolution":{"observed_at":"2026-08-06T01:02:56.721227Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:02:44.574738Z","title":"Abbas, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":29,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.574738Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:aaf4f5c16e5a98ca0b778231b2879bdceb299a853caa181b1e244009d38be6d8","observation_id":"ed6e8f74-b53b-4f1a-9917-34638954b36c","resolution":{"observed_at":"2026-08-06T01:02:44.574738Z","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":"2026-08-06T01:02:44.620740Z","title":"Abbas, S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.620740Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:4a381e5265a1475c1bfe08c74a1fc3e1602b996f68cb5034be38a498565df1a2","observation_id":"a2d503ca-bd0a-41fe-8507-324b21a11faf","resolution":{"observed_at":"2026-08-06T01:02:44.620740Z","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":"2026-08-06T01:02:44.696016Z","title":"Abbas, D","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":31,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.696016Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:1e41f71ea074e5a1554bb87ab63d1c056e04f3db196d4f9b562a16abf2a6c347","observation_id":"a84391a1-230d-40ec-ac0e-61eb2dbcd01d","resolution":{"observed_at":"2026-08-06T01:02:44.696016Z","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":"2026-08-06T01:02:44.769304Z","title":"Zubair, G","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":32,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.769304Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a6e56531fef6dc311ebaf8d2f45672b46fff3a50bb8b5fa68f3b91e65fa96f67","observation_id":"11f5e1b8-89cc-4dd6-870d-bee658a16017","resolution":{"observed_at":"2026-08-06T01:02:44.769304Z","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":"2026-08-06T01:02:44.838853Z","title":"Abbas, M","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":33,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.838853Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:2a49db46e7923b7594dec3df649726445106a5430b065ffe0bd009bc45f7dd32","observation_id":"4e061897-aa4c-4743-b438-64d64a520a01","resolution":{"observed_at":"2026-08-06T01:02:44.838853Z","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":"2026-08-06T01:02:44.919647Z","title":"Wyman, Physical Review D 24 , 839 (1981)","venue":null,"work_id":null,"year":1981},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":34,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:44.919647Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:55c1e0e5f1516d2ba1ea6cc06509945b2f8d004c59f0310cc05c1cdf5a5ce740","observation_id":"72261b15-8253-4500-84a4-11327ded58e7","resolution":{"observed_at":"2026-08-06T01:02:44.919647Z","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":"2026-08-06T01:02:45.014813Z","title":"Jetzer and D","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":35,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.014813Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:1120a1823815af9d29816e31e0831905d828ea99717cf5d1bd6494104c7b7151","observation_id":"87672200-1020-4dee-9f9b-0f85858bb0cf","resolution":{"observed_at":"2026-08-06T01:02:45.014813Z","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":"2026-08-06T01:02:45.120883Z","title":"Kodama, Physical Review D 18 , 3529 (1978)","venue":null,"work_id":null,"year":1978},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.120883Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:e0ce03d6ba80276b9b24e8789cf046143bcaba352a6029d7932f33187f9f2ec2","observation_id":"54c9f9c0-5dcf-4cf8-ab9f-40b3134f850e","resolution":{"observed_at":"2026-08-06T01:02:45.120883Z","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":"2026-08-06T01:02:45.232526Z","title":"Kodama, L","venue":null,"work_id":null,"year":1979},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":37,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.232526Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:49b4c4d5d684de9c6c60e1845560b37fbbc35c85b485acc5385cf1ee525ae687","observation_id":"4c8c5ae5-58c4-4e99-8687-9feed6479688","resolution":{"observed_at":"2026-08-06T01:02:45.232526Z","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":"2026-08-06T01:02:45.325050Z","title":"Antoniadis, P","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.325050Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:e0f9b7999dc9a25cce32de26c072543073b5838878981339026187097f806d59","observation_id":"cc6e99f3-e0e7-424f-8c84-b947489798c9","resolution":{"observed_at":"2026-08-06T01:02:45.325050Z","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":"2026-08-06T01:02:45.422761Z","title":"Torii, K","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.422761Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:e1d201bd2c3dcaf87e44f262e1282ad846d24e55675d41a7319ef432b9e3f910","observation_id":"2cd090b8-74af-4f99-8519-dff3b0faf85c","resolution":{"observed_at":"2026-08-06T01:02:45.422761Z","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":"2026-08-06T01:02:45.521447Z","title":"Nazar, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":40,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.521447Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:8c3560760cc698ab69f41e15ea1b784eeaaf0e5113652c004ea041ae45ee2c2a","observation_id":"e2e361cb-5d3f-4729-8b74-699337d7f3d2","resolution":{"observed_at":"2026-08-06T01:02:45.521447Z","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":"2026-08-06T01:02:45.603795Z","title":"Sakstein, Physical Review D—Particles, Fields, Gravitation, and Cosmology 88 , 124013 (2013)","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":41,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.603795Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:7d260eab035d027c4f4e6d7a0f05d22912c41fe75e7082e9341eb2c6f40164f7","observation_id":"a44660f3-1871-44fd-ae93-bc573d269f80","resolution":{"observed_at":"2026-08-06T01:02:45.603795Z","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":"2026-08-06T01:02:45.710168Z","title":"Sakstein, B","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":42,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.710168Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:db9901fa9aa6630c7b6d209c38217fdb6b3cede0117acf4a082ffbfad4824f79","observation_id":"ec51bcef-8736-4351-950c-abb22c8063b1","resolution":{"observed_at":"2026-08-06T01:02:45.710168Z","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":"2026-08-06T01:02:45.801210Z","title":"Sakstein, Physical Review D 92 , 124045 (2015)","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":43,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.801210Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:513f3d5ed6016ea3f18a4c53e055ba3a5a003cfd5f9a517431181e31c026a0fa","observation_id":"d5e0bdf8-d6e6-45b4-a830-2a45998c3b5b","resolution":{"observed_at":"2026-08-06T01:02:45.801210Z","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":"2026-08-06T01:02:45.880710Z","title":null,"venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":44,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.880710Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:b023365f47cf7bcd8d56015c8a19c99b092ee4333ba8090727f69e621e4aca58","observation_id":"a6d0bb90-9dc1-41b6-a77d-94996fa1fe36","resolution":{"observed_at":"2026-08-06T01:02:45.880710Z","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":"2026-08-06T01:02:45.979661Z","title":"Galeev, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":45,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:45.979661Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a9e85070210e3348db9f430d7961e22e6a113c8a38095e7d77dedd2579ed90b7","observation_id":"35d1d4ea-0000-45b1-8c9a-4a7595780c7f","resolution":{"observed_at":"2026-08-06T01:02:45.979661Z","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":"2026-08-06T01:02:46.068520Z","title":"Kennedy, L","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.068520Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:7c6f81a99af5d21a11a4b54d9e98c63ca9718c9ef914ad77cac1bcd27d294ee1","observation_id":"cdf85156-29c9-4588-8067-191d840a5f95","resolution":{"observed_at":"2026-08-06T01:02:46.068520Z","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":"2026-08-06T01:02:46.116216Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":47,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.116216Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:057426505fa9e28add2deb90bf2351b84d9ab06026f43c5aaf0bd31df54ddd71","observation_id":"9b581357-39eb-4f9a-bd0c-15b506fdd5fa","resolution":{"observed_at":"2026-08-06T01:02:46.116216Z","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":"2026-08-06T01:02:46.184862Z","title":null,"venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.184862Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:9b85b91674acc6a42fb2a91183492547ddf77c3f33fd6837e820d984926db6ff","observation_id":"9bdbba14-fd29-44d9-8004-498e23e227d9","resolution":{"observed_at":"2026-08-06T01:02:46.184862Z","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":"2026-08-06T01:02:46.270745Z","title":"Kulkarni, E","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.270745Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:8d64408299d53ea401b46766a613fc3296f341c71f2960deb545df3f3a8cd456","observation_id":"1689d5ef-491f-4e57-82bc-a70fde5c830d","resolution":{"observed_at":"2026-08-06T01:02:46.270745Z","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":"2026-08-06T01:02:46.341233Z","title":"Ventagli, P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":50,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.341233Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:15f68e7be0dbcc3f6760533a8ee007fff445e183b2e947478b7fcc653d5c5594","observation_id":"8a4bf93f-d3aa-416f-94ae-e7b1769d900c","resolution":{"observed_at":"2026-08-06T01:02:46.341233Z","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":"2026-08-06T01:02:46.430001Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":51,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.430001Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:68617a3e2bec3920e72517727090cd3c19ea3d60da2c84d0908ac4180b2fb2f8","observation_id":"3216fc1d-9c60-469a-8262-9941c6976a1c","resolution":{"observed_at":"2026-08-06T01:02:46.430001Z","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":"2026-08-06T01:02:46.502665Z","title":"Heydarzade and F","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.502665Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:fbe36312d58b7aa3839bc6e39f8c29f3aca5b764100ea52b5c33f864cfccb9ba","observation_id":"5ea15530-c2e0-40d8-86eb-2319b2b61bea","resolution":{"observed_at":"2026-08-06T01:02:46.502665Z","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":"2026-08-06T01:02:46.558143Z","title":"Konoplya, Physics Letters B 795 , 1 (2019)","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.558143Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a08391e49ae87cab881400d8942eb80b4a5fbb86e9102f1499086e973f9ad380","observation_id":"b5f9771a-0967-49cc-9d06-b24df1999d41","resolution":{"observed_at":"2026-08-06T01:02:46.558143Z","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":"2026-08-06T01:02:46.628763Z","title":"Zeng, H.-Q","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":54,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.628763Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:2b2ccac3e4cfd8de11d02d5c2d6a68d72c2be20e74a25a611518ea0c65b995c0","observation_id":"1cfa9352-1511-460c-9910-feecc2bb9179","resolution":{"observed_at":"2026-08-06T01:02:46.628763Z","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":"2026-08-06T01:02:46.703387Z","title":"Abdujabbarov, B","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.703387Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:ffb8fd3377b9e01c2f81fc6dc47cdb74d5a552249db234967153ded987fb8b14","observation_id":"90a60b8e-94a6-4608-8eef-e4d89c481fae","resolution":{"observed_at":"2026-08-06T01:02:46.703387Z","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":"2026-08-06T01:02:46.783490Z","title":"Chen and J","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":56,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.783490Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:89a70a86ceaaf1286f01e2a7bda7e5a3b8528ae1b5788cc1d85f91646f60d65f","observation_id":"b926b5eb-6bcb-43cb-814c-d996c6dd42b3","resolution":{"observed_at":"2026-08-06T01:02:46.783490Z","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":"2026-08-06T01:02:46.860918Z","title":"Zhang and Y","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":57,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.860918Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:56282e8fdb7a09da3947ec30752ed2c7fbb4a780d533fec067442eb2b47dfc05","observation_id":"0741be1c-bb80-42b2-919e-4d37bb3c717a","resolution":{"observed_at":"2026-08-06T01:02:46.860918Z","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":"2026-08-06T01:02:46.930160Z","title":null,"venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":58,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:46.930160Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:d892a2dae7cdc3dccceb488fb82d149abf66642f117ccd857c7156b64bd45557","observation_id":"04529dcd-97c8-499b-8c7d-075bc55dc7a5","resolution":{"observed_at":"2026-08-06T01:02:46.930160Z","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":"2026-08-06T01:02:47.033491Z","title":"Saleh, B","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":59,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.033491Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:288ab1b846642a0e9d32fd9f957ae74e04ba04e8836298cf7da2fad7c97c55a9","observation_id":"8dfe6d5b-ad22-4602-aa0a-fdda08dc122e","resolution":{"observed_at":"2026-08-06T01:02:47.033491Z","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":"2026-08-06T01:02:47.088937Z","title":"Toledo and V","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":60,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.088937Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a3d7d34a581e4283c965a07e1934f760c8a9ab43be58a4fb4f45d245153f85d8","observation_id":"e28cbbb2-5e31-4821-9248-f754bc183124","resolution":{"observed_at":"2026-08-06T01:02:47.088937Z","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":"2026-08-06T01:02:47.159241Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":61,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.159241Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:d4a4ef837a700eed550709e6651075d8143317499346b94c15e29ea68ce34587","observation_id":"8e15557e-66a4-45a3-81ed-af4cd3a87b8b","resolution":{"observed_at":"2026-08-06T01:02:47.159241Z","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":"2026-08-06T01:02:47.235978Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":62,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.235978Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:c1e0936539d3b64d362780b15a7237a953539a4f3129aadac01920b3d214dea9","observation_id":"e705b509-b7de-4d3e-8fdf-8aac27ebaef1","resolution":{"observed_at":"2026-08-06T01:02:47.235978Z","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":"2026-08-06T01:02:47.321032Z","title":"Santos, F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.321032Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:445dd14d83ae546de20c866a876be099907d8adb836ca1d99b9a2960dc995591","observation_id":"51c716c1-59f1-4974-af44-e1352e83060c","resolution":{"observed_at":"2026-08-06T01:02:47.321032Z","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":"2026-08-06T01:02:47.422815Z","title":"Saadati and F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":64,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.422815Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:b30c47d75c090a832e6c75a46d65bf43642eac087d28fdd01d54fa03b6fd1047","observation_id":"ef4e07fa-6c0c-4be7-bae8-02a111a69871","resolution":{"observed_at":"2026-08-06T01:02:47.422815Z","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":"2026-08-06T01:02:47.494583Z","title":"Javed and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.494583Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:04bd0272b3dcc8a3c5304808f3a7e761f10abc14371bd49054949ba3bdd410e1","observation_id":"0e6c066b-87ce-4523-90ab-538aba62c1c9","resolution":{"observed_at":"2026-08-06T01:02:47.494583Z","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":"2026-08-06T01:02:47.568966Z","title":"Dzhunushaliev, V","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.568966Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:fe05cdf44faeea336a7a3a211283af6c31c0e62ac8d1e31405c994952cfa10c8","observation_id":"d5a9dba0-4c57-4feb-9ad4-204219f128dd","resolution":{"observed_at":"2026-08-06T01:02:47.568966Z","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":"10.1103/physrevd.101.024022","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Boonserm, T","venue":"Physical review. D/Physical review. D.","work_id":"c852c8e5-61bf-44b3-811f-5355b7cefa63","year":2019},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.658140Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:4a508ace1a8ebd2fe13004d2f9831c23d1352e63cf9c3d01e7db71b62358e68b","observation_id":"bc9dec9b-2001-4a1b-8653-72f00908fcd7","resolution":{"observed_at":"2026-08-06T01:02:56.424976Z","resolver_source":"doi","status":"verified_exact"},"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":"2403.18752","last_updated":"2024-03-27T16:52:53Z","snapshot_observed_at":"2026-08-17T07:37:40.168538Z","submitted_at":"2024-03-27T16:52:53Z","title":"Neutron Stars Mass-Radius relations analysis in the Quintessence scenario","version":1},"cited_work":{"arxiv_id":"2403.18752","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.18752","snapshot_observed_at":"2026-08-06T01:02:58.716188Z","title":"Neutron Stars Mass-Radius relations analysis in the Quintessence scenario","venue":"gr-qc","work_id":"0dbd0c3a-c0cf-4e5c-95ac-d6c57bf6c42c","year":2024},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.723459Z"},"links":{"cited_paper":"/paper/2403.18752","citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:e8ec9c84fd61c7a48c5e7e3f40003d5ff990b2c954aaa790d7e8f834d0dac3cd","observation_id":"daf15ecf-d3b8-449c-be0b-5e97ddbdec85","resolution":{"observed_at":"2026-08-06T01:02:58.809374Z","resolver_source":"local_arxiv","status":"verified_exact"},"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":"2026-08-06T01:02:47.803242Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":69,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.803242Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:eb35f73900d85976a4036ea964a4821cffdca76bdac12e3ce71042437e3d02dc","observation_id":"cd115014-f9f8-443b-82f9-8ceaa84e21c0","resolution":{"observed_at":"2026-08-06T01:02:47.803242Z","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":"2026-08-06T01:02:47.901006Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":70,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:47.901006Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:f99f9890b991fc8c9780aacceea3e61853e8d463c35e1c7ef2576d9dde8ec8cc","observation_id":"b8c8d106-db14-48b7-a27a-f109af1d369e","resolution":{"observed_at":"2026-08-06T01:02:47.901006Z","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":"2026-08-06T01:03:11.999811Z","title":null,"venue":null,"work_id":"2dd9f0a4-835b-4f1f-9f91-98d555349dd7","year":2018},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.152389Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:ed112d9e771c488b23659bab2622469d7d73729d26657c3ad21380c4c5fe9a7e","observation_id":"8238454c-ac39-4b1c-9daf-7562dac60e34","resolution":{"observed_at":"2026-08-06T01:03:12.070895Z","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":"2026-08-06T01:03:11.751553Z","title":null,"venue":null,"work_id":"36bec375-afa8-4d45-a6a7-37c8531f0c8a","year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":72,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.331713Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:7afdc7c1ddb2672c4fe817edc29ded0e7f92af0c47392abe381221227d288fff","observation_id":"1c733e13-5586-4efa-81cf-cf9865079887","resolution":{"observed_at":"2026-08-06T01:03:11.858090Z","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":"2026-08-06T01:03:11.569530Z","title":null,"venue":null,"work_id":"f7724e9c-e757-4eca-a52b-7abaa20a6bfb","year":2006},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":73,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.509285Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:76f2fc1d5fa27f5055c95bf21bfa44a8dd3f8fd0df5fcc6c6c589c22c38b46e7","observation_id":"23e59fbb-6fac-4f0c-9505-123abd1a9edf","resolution":{"observed_at":"2026-08-06T01:03:11.669795Z","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":"2026-08-06T01:03:11.434907Z","title":null,"venue":null,"work_id":"23692dc1-5065-42ba-a441-6d154dc0e379","year":2016},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":74,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.628007Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:3912094b073c86a6fc8063c18cc3342447659c480d5d2c8ffbf57ed3ff22fa8c","observation_id":"7c3d2b63-6e8a-47b2-b411-f37d489199e2","resolution":{"observed_at":"2026-08-06T01:03:11.499559Z","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":"2026-08-06T01:03:11.247089Z","title":"Jamil, S","venue":null,"work_id":"bc948b24-a5ed-48ab-bcd4-2905be02a237","year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":75,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.758712Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:152197fb6834b97cc9f2abf32652aebc70a13fa76ccc648e16a3d4685f49dce9","observation_id":"6163b18f-3698-4ddf-96a8-ddb8e8908f28","resolution":{"observed_at":"2026-08-06T01:03:11.346302Z","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":"2026-08-06T01:03:11.041781Z","title":"Visser, Classical and Quantum Gravity 37 , 045001 (2020)","venue":null,"work_id":"615bbabd-4414-4752-9f32-286ac3c5f328","year":2020},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":76,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.870556Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:c165c4d1b8fd631fbc2ed8ab89e4ade8445775e070ee5fd6502b8793a219ba56","observation_id":"76bab56d-a31f-42d4-9b59-1bbced54ddcd","resolution":{"observed_at":"2026-08-06T01:03:11.134896Z","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":"2026-08-06T01:03:10.634999Z","title":"Caldwell and E","venue":null,"work_id":"ee7ad368-a0a6-452e-81a2-03c3c8adfd85","year":2005},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":77,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:48.938260Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a65f202836867a035721855eb647432ab9f73b4813ecce4f87a136b437494b3a","observation_id":"e84bbe62-80cf-43c2-8f4a-ef46ddf89ff6","resolution":{"observed_at":"2026-08-06T01:03:10.927408Z","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":"2026-08-06T01:03:10.228543Z","title":null,"venue":null,"work_id":"849dab6c-1cfb-4cb9-9291-c1a8b1b91744","year":2000},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.037684Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:85a5540a9f944a130f67abc2c1d2add906faf104dfd2a9c8cad50ae7a961905b","observation_id":"1b6249d8-67da-450e-9f0b-7eba8d4af49b","resolution":{"observed_at":"2026-08-06T01:03:10.325211Z","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":"2026-08-06T01:03:10.059194Z","title":"Amendola, C","venue":null,"work_id":"a6296830-b0ac-4fcd-a897-ba9b706250df","year":2005},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.084647Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:69ae4d5a88dc225ae23f64043664602d5bb0484bd9fcbf000b8f91e37b068148","observation_id":"b87d2439-0a4d-49f3-8e6b-feff68cca658","resolution":{"observed_at":"2026-08-06T01:03:10.119874Z","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":"2026-08-06T01:03:09.898572Z","title":"Babichev, V","venue":null,"work_id":"75c2af8b-b86c-4869-9f4e-fc9a6cd65147","year":2005},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":80,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.143127Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a6490b517f0ae5a439074bceaee98cf266f80a026c8f861298277c743d270ad0","observation_id":"c3546303-77be-4b52-96f0-7b081ad98863","resolution":{"observed_at":"2026-08-06T01:03:09.959740Z","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":"2026-08-06T01:03:09.656955Z","title":null,"venue":null,"work_id":"4de92900-08f8-4a34-aed9-ec885e403c2a","year":2013},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":81,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.215742Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:521ac01c27145539c57d15d86625379c4be2d285133e69c31830dd5c677e054c","observation_id":"efc6f136-ec65-4425-a1d9-7c3352fdb9b2","resolution":{"observed_at":"2026-08-06T01:03:09.779233Z","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":"2026-08-06T01:03:09.449796Z","title":"Zlatev, L","venue":null,"work_id":"b56183a5-aa5e-4e9d-aa97-4e39c9a21b83","year":1999},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":82,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.303092Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:87777f921b1c83a7a32035616e614487a1c3d5255b5e3c6f9966c915f867309e","observation_id":"cfcb31d6-15f9-4c84-a592-6d548469a06e","resolution":{"observed_at":"2026-08-06T01:03:09.565875Z","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":"2026-08-06T01:03:09.279844Z","title":null,"venue":null,"work_id":"2a5be3b1-263e-46a3-a157-d1b282170c4e","year":1988},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.392563Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:0ff9c9304a3a22a0b34036bad4383bfd38ce19612b88e9fad5667da6eea8c38e","observation_id":"21951bac-43d7-4803-abb3-e75b4b3f9beb","resolution":{"observed_at":"2026-08-06T01:03:09.339776Z","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":"2026-08-06T01:03:09.064926Z","title":null,"venue":null,"work_id":"25a2506e-4b0d-4061-84d0-1177f6651644","year":1998},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":84,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.465258Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:115a9fd3bb42e87294716d5a4920f523ad68df1d82de6da9eb89e2cb21e8a08c","observation_id":"b4b70065-dd9e-4f03-9836-007345f7a002","resolution":{"observed_at":"2026-08-06T01:03:09.153549Z","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":"2026-08-06T01:03:08.877269Z","title":null,"venue":null,"work_id":"b60cfcc4-1787-4ba2-b860-ef5f0d2e7e99","year":2000},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.545973Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:45f27b243236e055c35e83b84ae6f6b140ce00ae79d6eeec9fdba87c03dbf96a","observation_id":"89beb749-cb76-4e15-9ec8-cf72803b82a0","resolution":{"observed_at":"2026-08-06T01:03:08.952124Z","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":"10.1103/physrevd.97.064016","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Sagunski, J","venue":"Physical review. D/Physical review. D.","work_id":"638b3efa-14e4-4347-8604-1f729efd7f4e","year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.651571Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:d93d5e7bf40d65605093bf4eca947fa8fcb473b8ad62eda484c9fc1f92f2f773","observation_id":"92b6af9e-8855-455a-869b-75692158dc2b","resolution":{"observed_at":"2026-08-06T01:02:56.131278Z","resolver_source":"doi","status":"verified_exact"},"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":"10.1103/physrevd.91.123522","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Barreira, P","venue":"Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology","work_id":"18f5d6ba-34ea-46dc-8307-00e19665c4b1","year":2015},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":87,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.755314Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:7cedd98a0fbd5c2646d41b22f9954838875777d4be3d04f6ed257de4343420a5","observation_id":"93c78f0f-048d-4102-9d7c-04066f276d56","resolution":{"observed_at":"2026-08-06T01:02:55.854819Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:03:08.610768Z","title":null,"venue":null,"work_id":"1d15d045-5cb0-4414-abe4-491c95b524da","year":1974},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.834133Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:6bbe76a18bdad799f9f3649e50729b4b4f42bb20cfd09894286c5050c38685fb","observation_id":"f6b6b484-28b6-4de9-a07b-090741914e0b","resolution":{"observed_at":"2026-08-06T01:03:08.734594Z","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":"2026-08-06T01:03:08.371167Z","title":null,"venue":null,"work_id":"583d5bfb-27a1-4f1c-919e-d760dd75aa8f","year":2001},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":89,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:49.913343Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:5dd89465c5e3f59ecf532609ca8ca10b7a99ba1146bc102ef03235c5250546ff","observation_id":"62c9d427-a0b1-4222-9850-61ad00603642","resolution":{"observed_at":"2026-08-06T01:03:08.459607Z","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":"2026-08-06T01:03:08.147609Z","title":null,"venue":null,"work_id":"d26b9761-5b78-4f07-beaa-df8787f4ad95","year":2006},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":90,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.061373Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:7cdd44ad8cf8b1a7095b6c5c9a2dad42fe292587aee0a82acef9d3c096d6466a","observation_id":"d2b9ca26-6137-45a7-9c6e-c78e9e147f85","resolution":{"observed_at":"2026-08-06T01:03:08.239807Z","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":"2026-08-06T01:03:07.929150Z","title":"Jetzer, Physics Reports 220 , 163 (1992)","venue":null,"work_id":"2b82842a-db7f-456d-b9fb-86721edac242","year":1992},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":91,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.122939Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:1a097723d04f34fcfbee259adbb9898e2b429b16e0ba77f8119c43a7a0d9e973","observation_id":"0cefe681-6be0-42a8-ab73-86af4c437a92","resolution":{"observed_at":"2026-08-06T01:03:08.030888Z","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":"2026-08-06T01:02:50.183771Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":92,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.183771Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a29367c9d98ce4b4559d50713e1fde878e036aa49761c94a93c7d20014d0defc","observation_id":"fb3ed954-1cb8-4aa0-a067-fd4a41ecebc2","resolution":{"observed_at":"2026-08-06T01:02:50.183771Z","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":"10.1103/physrevd.85.122005","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Berti, L","venue":"Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology","work_id":"38d05085-8648-4cf3-9f2d-a4672d82271f","year":2012},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.296933Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a55c92438cee26edf26e0659fd28527e04c762acbbb6461b349955896661ef97","observation_id":"9070ea5d-8574-45a7-aa9b-442976a8c401","resolution":{"observed_at":"2026-08-06T01:02:55.664817Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:03:07.690656Z","title":"Sennett, T","venue":null,"work_id":"542691cc-4c9d-4312-8b13-cc039486bf7f","year":2017},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":94,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.376419Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:3366da3390c7c5c00b741f03e8c95cfc97c5ff1ef58325d703b226361d428aee","observation_id":"7fb2ca58-456b-4c4f-b77c-7c4a7de57ae3","resolution":{"observed_at":"2026-08-06T01:03:07.823838Z","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":"10.1103/physrevlett.109.041301","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-10T05:30:23.456663Z","title":"Upadhye, W","venue":"Physical Review Letters","work_id":"f3d47831-acbd-49bf-b6b0-2263affb67a2","year":2012},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":95,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.447774Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:a922dc6bc26d2e99a30f42440f84216f434e5a2cd027604f2fd2cd1055c94b4c","observation_id":"156ff542-c664-40a3-92b0-a796f8d5d53a","resolution":{"observed_at":"2026-08-06T01:02:55.479646Z","resolver_source":"doi","status":"verified_exact"},"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":"2026-08-06T01:03:07.568074Z","title":null,"venue":null,"work_id":"beec5689-3f71-43b8-bc23-05bab0b6c45c","year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":96,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.511482Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:29ac6ee1b62ce461e0041adc40ec20aba0c8f597e276b38da47b4e4242a73da2","observation_id":"233989b5-6184-40c7-95a1-a10a041c8d36","resolution":{"observed_at":"2026-08-06T01:03:07.622377Z","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":"2026-08-06T01:03:07.331763Z","title":null,"venue":null,"work_id":"031c8ee3-f117-4dcb-98d9-f1376bfdef73","year":2022},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":97,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.607996Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:8d11635380d600ca0873eb7f56f9b482d00ba10a22132b5587bac0c3278ab82e","observation_id":"da128aba-1534-4e6f-b8a1-5a3a8b74518a","resolution":{"observed_at":"2026-08-06T01:03:07.405310Z","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":"2026-08-06T01:03:07.109380Z","title":null,"venue":null,"work_id":"f78f83f1-1b2b-45eb-b43a-d4dab0893ec6","year":2000},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":98,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.683089Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:b873fb434556aeffdb90a0e24bf84ec83583dde36c5d8f0541e4a8bdd0a9278b","observation_id":"43b44fe6-49a7-4b50-8faf-ef2375533385","resolution":{"observed_at":"2026-08-06T01:03:07.212946Z","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":"2026-08-06T01:03:06.727128Z","title":null,"venue":null,"work_id":"44052438-f8c3-426f-a4a4-bf3cbbf054e9","year":1988},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":99,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.767668Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:4d7999c4aacab467d0e74846978086cd5f16b0e161bfb7a49a596ecae2fe7679","observation_id":"e9a57014-a3ff-448d-a5db-b3a0e82079f6","resolution":{"observed_at":"2026-08-06T01:03:06.899547Z","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":"2026-08-06T01:03:06.475271Z","title":"Douchin and P","venue":null,"work_id":"a4b4fe1b-54b2-4212-9257-e1c80706df48","year":2001},"citing_paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars","version":1},"reference_index":100,"source":"arxiv_source","source_observed_at":"2026-08-06T01:02:50.872004Z"},"links":{"citing_paper":"/paper/2508.04744"},"observation_digest":"sha256:e57050f4fd276950f16e81689d6aa69bf3d90fa91202c91ff5b0fcde15f75b6f","observation_id":"a736ab90-c414-4f9d-845e-86748b3aa0e1","resolution":{"observed_at":"2026-08-06T01:03:06.575268Z","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"}}],"paper":{"arxiv_id":"2508.04744","last_updated":"2025-08-06T05:37:33Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-17T18:40:53.310728Z","submitted_at":"2025-08-06T05:37:33Z","title":"Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":77,"verified_exact":14,"verified_fuzzy":9},"total_outbound_references":137},"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 100 of 137 outbound references and 0 inbound Pith citation observations for arXiv:2508.04744."}