{"as_of":"2026-08-06T22:43:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:681fc31460cc404db51bf21d94f05bcd9f2aa27805b0a8bc55b0c024a39f4663","coverage":[{"denominator":34,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":34,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-25T04:15:35.829969Z","state":"measured"},{"denominator":34,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":34,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+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/2605.23317/citation-record","integrity":"/paper/2605.23317/integrity","json":"/paper/2605.23317/citation-record.json","paper":"/paper/2605.23317"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-10T17:57:26.267924Z","title":"Jaeckel and A","venue":null,"work_id":"f0c4f913-8727-4dd7-b793-6bb95183a789","year":2010},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:12a904a372c63685e4888fa7e689b24403ff1cccd79e19a710b439d60661e666","observation_id":"a1e59048-d26a-43f3-bd67-2f0985dae444","resolution":{"observed_at":"2026-05-25T04:16:36.301711Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Ringwald, Exploring the Role of Axions and Other WISPs in the Dark Universe, Phys","venue":null,"work_id":"0b009873-6766-4dc3-8fad-1deae79a8551","year":2012},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:1d5239818a81d3b277495e0b020432ed897ec22078e9669c6bb98e1f077b0250","observation_id":"43bf3f5f-2815-4c65-aee4-cfebc3b677f0","resolution":{"observed_at":"2026-05-25T04:16:36.322613Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Antelet al., Feebly-interacting particles: FIPs 2022 Workshop Report, Eur","venue":null,"work_id":"4fe1a656-9f88-47b7-a703-4ae8887f4db2","year":2022},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:714c5217f5817eaec028033c39160c493380fe5db0cf269ad564acf915d99385","observation_id":"edbe909c-bb85-4fe2-8032-a12fbc57d55c","resolution":{"observed_at":"2026-05-25T04:16:36.311337Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Agrawalet al., Feebly-interacting particles: FIPs 2020 workshop report, Eur","venue":null,"work_id":"71cd0f11-d290-47a1-82e4-06672524581b","year":2020},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:6c0549841a401aa773869f5f28913f8b189db9d4c0183860663b811dd1402ee6","observation_id":"ff928ed7-7837-4476-bae3-ab7988fb5e31","resolution":{"observed_at":"2026-05-25T04:16:36.316906Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2603.03433","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T15:06:18.281015Z","title":"Arzaet al., The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles, arXiv:2603.03433 [hep-ph] (2026)","venue":null,"work_id":"5f290f7d-534d-4961-bf15-b7ece7172dd8","year":2026},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:f4f5a818bfdf9c74e01f3db7bed5d1d8cfa3963293c52c7f04b700bd45df8d72","observation_id":"0b6ac864-c9c8-41dc-8dee-f27a0502ce30","resolution":{"observed_at":"2026-05-25T04:16:36.028225Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"d9309493-b612-4d32-8b76-ec86c9b8c3af","year":1996},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:3da8cfac3279e960161a08f0d4c9a9cf049fd5782825f14dceee2eb587d74b5d","observation_id":"c9f6d65c-459b-4aa3-993d-6e24c6980a15","resolution":{"observed_at":"2026-05-25T04:16:36.295686Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.02492","last_updated":"2025-02-26T20:20:46Z","snapshot_observed_at":"2026-08-04T16:22:06.374881Z","submitted_at":"2024-11-04T19:00:01Z","title":"Axion Astrophysics","version":2},"cited_work":{"arxiv_id":"2411.02492","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.02492","snapshot_observed_at":"2026-07-09T15:06:18.258900Z","title":"Carenza, M","venue":"hep-ph","work_id":"e291397f-aea2-477f-9c1a-ff0d7b6d0ae1","year":2024},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/2411.02492","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:e41a8bcc44993adf7e1d81250c39a3e8ae4a64b413620346ce5c64cd0ba001bd","observation_id":"ed7d7c73-cfde-4fc1-8c40-fb77c3681f13","resolution":{"observed_at":"2026-05-25T04:16:36.038079Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Andriamonjeet al., Search for solar axion emission from 7LiandD(p, γ) 3Henuclear decays with the CAST γ-ray calorimeter, JCAP03, 032","venue":null,"work_id":"ac707500-3e14-41e7-b729-19341cbf96a7","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:933907c363fbf7fe492afb65dcbe0efb0e1acd6cc4c330902269f1a08a9b622b","observation_id":"0927c74d-dcca-4d46-924b-421d077a2c0c","resolution":{"observed_at":"2026-05-25T04:16:36.292917Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Belliniet al., Search for Solar Axions Produced in p(d, 3He)A Reaction with Borexino Detector, Phys","venue":null,"work_id":"07e3e710-8977-4300-ba8e-f6766f945e33","year":2012},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:30f2e722eae492081ab9849ece56461845a0de115c2f29866c50121d7b5d9f2f","observation_id":"fa726ab1-fe98-4a60-808c-d0d8f1e4dc0d","resolution":{"observed_at":"2026-05-25T04:16:36.315332Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Bhusal, N","venue":null,"work_id":"fd1baa2e-faf5-48e2-bd05-4e9548344229","year":2021},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:b61a4d0a9366609a11e85819b85d3179ff840c47bc0524cfd4da92c2f1476b92","observation_id":"de5fe072-f8c0-41a4-b70a-ef2ac147a4af","resolution":{"observed_at":"2026-05-25T04:16:36.279327Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"D’Eramo, G","venue":null,"work_id":"2215df50-092d-430f-9e7e-4b35f320d23e","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:dfe00bfad8a4be717b83e826e0ad68eb00de79ffa96608597d1020755ca9f63f","observation_id":"64f5882e-da6d-48c5-b766-6f3b27b47df6","resolution":{"observed_at":"2026-05-25T04:16:36.312427Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"026b8935-9842-4462-b73d-f419094bbc0b","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:3c769567278c82c40bd8321b6a1123b1dce1af644554cadb22f06be608e7524f","observation_id":"dcb406ac-66c8-42ff-8f08-58b78dec5b69","resolution":{"observed_at":"2026-05-25T04:16:36.309749Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-07-07T18:34:04.705513Z","title":"Holdom, Two U(1)’s and Epsilon Charge Shifts, Phys","venue":null,"work_id":"afaab59b-8ee7-43a9-9987-4fa05c43cd58","year":1986},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:30fe196d692523c99b12df587016c66d39ea2194b80e059e3d7603f89cfa4aa1","observation_id":"bb6b9c5e-7e0d-4982-b748-874db624d5d6","resolution":{"observed_at":"2026-05-25T04:16:36.302061Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Fabbrichesi, E","venue":null,"work_id":"1af599dd-235d-453a-9579-afdb6ab88eb4","year":2020},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:05834e5fe0d20ed3521fa754904eeac959c43a244407ff4c11617b9da566396a","observation_id":"7c33ee1e-8179-4b1e-908c-a117d1bf3e83","resolution":{"observed_at":"2026-05-25T04:16:36.307026Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"f0190a20-602e-480e-90bc-bd8adfbcdf02","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:d8f5740462e07dd27f6740e1bb21fcfe6b305dfefd4eea0dedcfc36de850d300","observation_id":"005bd016-6ad9-4d77-b5b3-2995289412a6","resolution":{"observed_at":"2026-05-25T04:16:36.299270Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1305.6059","last_updated":"2013-05-26T19:26:47Z","snapshot_observed_at":"2026-07-06T03:14:21.137747Z","submitted_at":"2013-05-26T19:26:47Z","title":"Covariant Compton Scattering Kernel in General Relativistic Radiative Transfer","version":1},"cited_work":{"arxiv_id":"1305.6059","doi":null,"metadata_source":"pith","pith_arxiv_id":"1305.6059","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Covariant Compton Scattering Kernel in General Relativistic Radiative Transfer","venue":"astro-ph.HE","work_id":"4858b252-ad67-47d1-8b87-ecf49a9b3c80","year":2013},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/1305.6059","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:57763da9d248b522bf65af38860f12f5732c08849c9eafc0b7feffe29e8633a2","observation_id":"a2dc9b73-0da2-458b-ac48-bddcc02c124f","resolution":{"observed_at":"2026-05-25T04:16:36.052370Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"plasma conditions or specific couplings related to the WISP considered","venue":null,"work_id":"a731c31b-2ac6-4cc8-8a31-dc956e2ea78f","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:839871a2a101062d1da0316ec1d6e224da965c5bed7521af05dfb583a9afa13a","observation_id":"cdbafe26-091c-4309-b62c-daaba019fac8","resolution":{"observed_at":"2026-05-25T04:16:36.269120Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"203891ad-3722-437c-bd1c-09b8370db477","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:1decd3b3ce900dde5b317c5519e62042252ce09cf86e7449a7578de7bf6e5554","observation_id":"18790869-b321-426f-a490-7eba0d76d9ec","resolution":{"observed_at":"2026-05-25T04:16:36.276397Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"fa152633-26f5-4b3c-a145-6753dfc218c5","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:d9f26f3e2d858212f70cd014fc610ccc31adfafbd7ead218a29d6b3ce9413900","observation_id":"7122ba0a-ed0e-401d-bcbd-8a696feb6a77","resolution":{"observed_at":"2026-05-25T04:16:36.279039Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"e5204923-0787-431f-bf2a-2a1aad4fecac","year":2013},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:0645fe897e4e8ed5e97ed3cff8bce92d8b75484274709d10ebefaafddfb132a8","observation_id":"d2516725-5bb7-41b2-9925-59fc99a02b7b","resolution":{"observed_at":"2026-05-25T04:16:36.286438Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Redondo and G","venue":null,"work_id":"cefd2f1a-299d-4e79-96ca-b2cc3beb9a50","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:dfdd7862b92544ec74e99b7711246ab3ad9deae42172915e471c363d78629d79","observation_id":"92dbd547-7ee1-46c3-990c-f797aab7f452","resolution":{"observed_at":"2026-05-25T04:16:36.261955Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Hardy and R","venue":null,"work_id":"572362eb-a4e6-4f1f-b974-9cfe70fb15df","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:cb8c67d24bc97172741fbdf6bb13559ef025dfcc7301b8822f54b87424238de9","observation_id":"ad999d64-a257-468d-b28b-c95772bcacfd","resolution":{"observed_at":"2026-05-25T04:16:36.271083Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Redondo, Helioscope Bounds on Hidden Sector Pho- tons, JCAP07, 008","venue":null,"work_id":"8b06a3ae-bfca-43ac-a664-e3ef9be51334","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:0d501117e8b500a5d792d0f65fd79a636dc5db391ce56ddb74c2e517834b768c","observation_id":"01e5f3ad-f234-404d-8778-b00664fd301a","resolution":{"observed_at":"2026-05-25T04:16:36.289508Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.10446","last_updated":"2025-08-13T08:19:01Z","snapshot_observed_at":"2026-07-06T17:31:00.274878Z","submitted_at":"2024-02-16T04:38:30Z","title":"The XENONnT Dark Matter Experiment","version":2},"cited_work":{"arxiv_id":"2402.10446","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2402.10446","snapshot_observed_at":"2026-07-04T14:49:54.556209Z","title":"Aprileet al.(XENON), The XENONnT dark mat- ter experiment, Eur","venue":null,"work_id":"7043e06d-3b1a-4772-acf6-c1de186a9f3a","year":2025},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/2402.10446","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:e95c0684007503983bf61d5322770fd4a130a0b95b7650011e20094975f29add","observation_id":"e3ba0872-d729-4eb9-90fa-2b90e15c8e74","resolution":{"observed_at":"2026-05-25T04:16:36.055893Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2511.01655","last_updated":"2026-05-25T08:29:50Z","snapshot_observed_at":"2026-08-06T16:46:47.451372Z","submitted_at":"2025-11-03T15:17:25Z","title":"Direct detection of solar chameleons with electron recoil data from XENONnT","version":2},"cited_work":{"arxiv_id":"2511.01655","doi":null,"metadata_source":"pith","pith_arxiv_id":"2511.01655","snapshot_observed_at":"2026-07-04T22:30:10.393070Z","title":"Yuan, A.-C","venue":"hep-ph","work_id":"d35a9d63-3c1d-491e-9f84-2e25d755f1d0","year":2025},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/2511.01655","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:089116ddd947f176f0bbb7b80c181b3b5b24d4b3d85a9e67b7be813c1b1eefc3","observation_id":"9d88aab6-e759-47a5-b67b-5b1f9ce55ca2","resolution":{"observed_at":"2026-05-26T03:04:07.320045Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.09155","last_updated":"2019-06-06T14:16:33Z","snapshot_observed_at":"2026-07-06T07:47:12.240477Z","submitted_at":"2019-04-19T11:52:06Z","title":"Physics potential of the International Axion Observatory (IAXO)","version":3},"cited_work":{"arxiv_id":"1904.09155","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.09155","snapshot_observed_at":"2026-07-02T19:07:18.472500Z","title":"Physics potential of the International Axion Observatory (IAXO)","venue":"hep-ph","work_id":"a9861fd1-f512-40ea-9d8b-50636336388d","year":2019},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/1904.09155","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:ebe280866f1420e46e919007a32977a36558024047eed1d95cac0895265b855e","observation_id":"1de44e91-81a0-498f-875c-9821285f764a","resolution":{"observed_at":"2026-05-25T04:16:36.058864Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.12076","last_updated":"2021-03-04T10:07:27Z","snapshot_observed_at":"2026-08-05T03:41:37.910680Z","submitted_at":"2020-10-22T21:32:03Z","title":"Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory","version":3},"cited_work":{"arxiv_id":"2010.12076","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2010.12076","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Abelnet al.(IAXO), Conceptual design of BabyI- AXO, the intermediate stage towards the International Axion Observatory, JHEP05, 137, arXiv:2010.12076 [physics.ins-det]","venue":null,"work_id":"167a227e-58c2-4f1c-a285-b0e1664d8b59","year":2010},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/2010.12076","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:e407798b3ec7fa3d57d8d717f7c6d7c20f15020e1856388add32a7961bf9b632","observation_id":"87aba9d7-57fe-41e9-ae7e-289a1dbbc1aa","resolution":{"observed_at":"2026-05-25T04:16:36.044485Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.13915","last_updated":"2024-11-29T10:54:56Z","snapshot_observed_at":"2026-07-06T19:53:34.670694Z","submitted_at":"2024-11-21T07:58:29Z","title":"An accurate solar axions ray-tracing response of BabyIAXO","version":2},"cited_work":{"arxiv_id":"2411.13915","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.13915","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ahyouneet al.(IAXO), An accurate solar axions ray-tracing response of BabyIAXO, JHEP02, 159, arXiv:2411.13915 [hep-ex]","venue":null,"work_id":"970f0e30-1359-42b3-9e78-128001578aae","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/2411.13915","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:4c7148ea462c218f0e6947f1ee7927213f4e7f3f4845fb165a61d25526fc56f1","observation_id":"cf7edbbf-77de-45ac-9d4d-66bb3a79840d","resolution":{"observed_at":"2026-05-25T04:16:36.035131Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Herrera and A","venue":null,"work_id":"42e65087-b169-4324-930b-3593a22d45c4","year":2023},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:1c7a3401151621cfac87639d5b271ba3a83b801585e4be33cc89af4359a6dc2b","observation_id":"9f65c17e-55a4-44b6-bc1d-d96e297c09c7","resolution":{"observed_at":"2026-05-25T04:16:36.319451Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"number per second","venue":null,"work_id":"c5c3939f-ed0f-4b91-81b3-b1d2c68c7f26","year":null},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:cf3bd22e80b96b6dfae1e1a58cc011197db5b158b3225ff68ba69ea0171ecc48","observation_id":"a1d0ebc8-5879-4b85-8303-5047e6113a1b","resolution":{"observed_at":"2026-05-25T04:16:36.313868Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1009.4620","last_updated":"2010-09-23T14:13:01Z","snapshot_observed_at":"2026-07-06T02:15:50.341412Z","submitted_at":"2010-09-23T14:13:01Z","title":"The 511 keV emission from positron annihilation in the Galaxy","version":1},"cited_work":{"arxiv_id":"1009.4620","doi":null,"metadata_source":"pith","pith_arxiv_id":"1009.4620","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The 511 keV emission from positron annihilation in the Galaxy","venue":"astro-ph.HE","work_id":"c93adf37-cfd3-4fec-907c-340f3243df29","year":2010},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"cited_paper":"/paper/1009.4620","citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:992b6b23eb6f67a2c54f6b7b79101d91b6c0375229f60f33fb43222afcfd6fd5","observation_id":"cb6eaf3e-5c1f-4ad7-b651-b2fcc64c4f07","resolution":{"observed_at":"2026-05-25T04:16:36.041145Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"Agostinelliet al.(GEANT4), GEANT4 - A Simulation Toolkit, Nucl","venue":null,"work_id":"4ac33e74-6e74-47cc-bbf0-ff641016a80a","year":2003},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:77f8f4f0e03f082ffef389501e07b95de1ea94de54db8fdd8218ff4c473b6307","observation_id":"8823cbef-509b-4491-b99f-b80151f23e08","resolution":{"observed_at":"2026-05-25T04:16:36.304671Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":"[34]K th denotes the thermalization energy scale in the Sun, of the order of the solar-core thermal energy","venue":null,"work_id":"cc537f00-b712-45dd-aa6a-3dd35f72f021","year":2024},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:938658466ddcf1038bfc879f9d42187724ab713ec4e41fe3a7d0a85d7b58811e","observation_id":"8d362ef9-2a3c-4a60-b032-16dee609ebcd","resolution":{"observed_at":"2026-05-25T04:16:36.318118Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+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":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"39051ef3-17b1-463a-804e-df6bd04c68fe","year":1979},"citing_paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-25T04:15:35.829969Z"},"links":{"citing_paper":"/paper/2605.23317"},"observation_digest":"sha256:4bcd55dc8009e5386d24c5597fcee6b860d363ab3e241c9a97b9916d583a9cbf","observation_id":"c890f9fa-c792-4269-89c0-0a5ac2e9bcc8","resolution":{"observed_at":"2026-05-25T04:16:36.307705Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2605.23317","last_updated":"2026-05-22T07:36:05Z","latest_version":1,"primary_category":"hep-ph","snapshot_observed_at":"2026-07-06T23:33:34.409634Z","submitted_at":"2026-05-22T07:36:05Z","title":"Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades"},"reference_resolution":{"displayed":34,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":7,"verified_exact":9,"verified_fuzzy":18},"total_outbound_references":34},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 34 of 34 outbound references and 0 inbound Pith citation observations for arXiv:2605.23317."}