{"as_of":"2026-08-19T13:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bc0d3065dccff4fc73a5cbc9104d99340c377c015578c4e93a29edbddd8847ff","coverage":[{"denominator":73,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":73,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T05:04:59.572341Z","state":"measured"},{"denominator":73,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":73,"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/2607.05606/citation-record","integrity":"/paper/2607.05606/integrity","json":"/paper/2607.05606/citation-record.json","paper":"/paper/2607.05606"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T05:04:59.572341Z","title":"Cosmic ray spectrum from 250 TeV to 10 PeV using IceTop","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f6e08f01662dd89cd61e6207ae8fc50a2f6d76e04a339713c9611314f6910246","observation_id":"dbc2a927-8422-40a4-9fdb-05f3ba59fd65","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Measurement of Separate Cosmic-Ray Electron and Positron Spectra with the Fermi Large Area Telescope","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f86c9a0fae6b2b70f08e83400cd627653a06a7ebec568d719bb338337e579150","observation_id":"e50dc0bb-9458-4d04-b780-33dde65fccf3","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-07-11T05:04:59.572341Z","title":"An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:b19cbd640f09eba6377228a4d47ac5357abc5ec9486e61e19b3e6dad4d04c449","observation_id":"4a517d13-31ef-4771-83c3-165523f44c65","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:3c4731ad770520fbc59d7cbc52711b612f72f91050bef118dac1bcc3e7c6a12b","observation_id":"f5f65202-a625-4e99-8257-5ff653ddb877","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/0004-637x/791/2/93","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Measurement of Boron and Carbon Fluxes in Cosmic Rays with the PAMELA Experiment","venue":"The Astrophysical Journal","work_id":"c8f7e54d-2722-4ce5-8e9f-b12ece519752","year":2014},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f1031581340dc3e8f0f3d0a8d85011cbb8a4b8389b3108b01fa46795558a5501","observation_id":"dbe3aed0-b188-4ac0-b192-a3f740b69708","resolution":{"observed_at":"2026-07-11T05:07:46.404415Z","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":"2026-07-11T13:49:26.311229+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:26.311229+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Direct Measurement of the Cosmic-Ray Carbon and Oxygen Spectra from 10 GeV/nto 2.2 TeV/nwith the Calorimetric Electron Telescope on the International Space Station","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:7adc70a03f2417d10b935562a122fe39b7d8e693b58a57d3d4a7b9f1fadf01c0","observation_id":"08422bec-a7f7-4778-8ff5-45edb2c8c8b0","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Measurement of the Iron Spectrum in Cosmic Rays from 10 GeV/nto 2.0 TeV/n with the Calorimetric Electron Telescope on the International Space Station","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:fbb9c76b7cfdec90f3c404a7955a7c640ed1d4106d64e546f1f55bcb8b4a6d3a","observation_id":"4f7fb782-35d7-4faf-888b-dd60a8670bba","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Cosmic-Ray Boron Flux Measured from 8.4 GeV/nto 3.8 TeV/nwith the Calorimetric Electron Telescope on the International Space Station","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:9d31b7a5195b2c20c6ab54951996f6550713b9ed1c2b09b2de2aa5c42566f381","observation_id":"466ab424-365a-4d1b-8ad8-03ffd99720ff","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Observation of Spectral Structures in the Flux of Cosmic-Ray Protons from 50 GeV to 60 TeV with the Calorimetric Electron Telescope on the International Space Station","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:0bbe1b69fc06301e16efc8d3d479c64c63bca431258d34d3ee872b1a5358b337","observation_id":"b44312d0-4577-4943-aea2-b26603c600f5","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Direct Measurement of the Cosmic-Ray Helium Spectrum from 40 GeV to 250 TeV with the Calorimetric Electron Telescope on the International Space Station","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:1e3f08c5334a060fea2787db30660a20a5981a09abdf2c634000b349c7ee9fd3","observation_id":"4d03918b-044d-4fad-bd4b-c01617d6cf15","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:e1ec7ae2c5deac4b16643168566d63d56467de8d77126824dc067a76f916118e","observation_id":"9c6ab6b8-a305-4ffd-b87f-1694ff9228c3","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:2fc15913e0cc70977186148b7c52f6a1dfc6690de091e7d5c30b4c596b075925","observation_id":"742e0bac-c926-40f6-bb4a-a12fe180076c","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:8fd9db96f0877196fdca467b1b965129bcf0c37f8b138ac425c956bee70d1fbc","observation_id":"a372302c-1d8e-4d7a-9522-940d34403501","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:0a45fbffc568268db5168b623b37697a10ed703379c9d8d60d7e2feb7c8b74b3","observation_id":"3dce033c-55d6-4a9b-b285-c7d113cba1c7","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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.122.101101","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Towards Understanding the Origin of Cosmic-Ray Electrons","venue":"Physical Review Letters","work_id":"e716a804-9755-49bd-abba-d861c857cef4","year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:2a4661d23762c95f9084a64131e7be6263823f430b8f70d37f19357d57a9fa31","observation_id":"e50998d2-c260-48a5-936f-15cf27cc587e","resolution":{"observed_at":"2026-07-11T05:07:46.649179Z","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":"2026-07-11T13:49:29.707956+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:29.707956+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Towards Understanding the Origin of Cosmic-Ray Positrons","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:df37b45c0f7d8d091c18aaad25741c00966c36c05cf541a80f0f41e5c0e873a9","observation_id":"c0413d6a-175f-4da7-8e78-3d4e42e975a1","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:3ee1c14bcfc2a16e84775674deeba66332b38503223215d57a8aa5fd9f7f1ba3","observation_id":"661300b0-19c7-4311-962e-db939075ff74","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-07-11T05:04:59.572341Z","title":"Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:abc4f51db86de0f768187adc0551c8eb0a6cb67dfc757c69113a38c553db2dbc","observation_id":"22afce0b-78dc-4439-b869-342d89aaf5c8","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:2961723a96758668fb10d819a4b31e922add1cb14c806a6f2c8415864f6d395d","observation_id":"3932bfb8-6b54-464b-81e3-bb1c1419a5b3","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II – Results from the first seven years","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:501b614ed38eb191e917f3d3f42f165117cdaa4c7b27948df839cf897f7d8a2a","observation_id":"75396a4a-b369-425f-8b3f-3fee30bbabcb","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-07-11T05:04:59.572341Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:4e1dd904c5f81c338054273646b22d11b4a015cb460bf6aa3b0c5f12c0264aa9","observation_id":"f7335977-1777-4c09-902b-ccece6674c12","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Energy Spectra of Cosmic-ray Nuclei at High Energies","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:ee1b476ec2b112ace713dcd5fe011b6ed709970c7c80b9f3c69c5112e1217cad","observation_id":"bc490c00-d884-4f20-9c67-a3c592bf1ac7","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Discrepant Hardening Observed in Cosmic-ray Elemental Spectra","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:e3e1bd0e8ce21d3cfd8aaa4536498a2afdff6fbdf872d91e84ef98edd9643287","observation_id":"2ac9de73-7720-4d2b-a3e4-564d80272f93","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Measurement of the Cosmic Ray Helium Energy Spectrum from 70 GeV to 80 TeV with the DAMPE Space Mission","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f0c7105daa5d5c1a779fef042a31947affcc98c11cbd1d582ff906c4ca8519ef","observation_id":"2be47956-347e-46db-9377-977a8edd047b","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-07-11T05:04:59.572341Z","title":"The All-Particle Spectrum of Primary Cosmic Rays in the Wide Energy Range from 1014 to 1017 eV Observed with the Tibet-III Air-Shower Array","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:e966cd028cf0c86d93a8fefcb2652a4479f5bad79868d785205e4b41af195e6f","observation_id":"7a062f31-098d-41d9-a68b-b36849da4b96","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:372b744f8fc18cb403c0439e2ec4e7408de130b6bef02fe1e9f2ecdd2e8c9c02","observation_id":"36b90896-c084-487a-85d0-0f2a6cb8efcb","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9908202","last_updated":"1999-08-18T14:56:58Z","snapshot_observed_at":"2026-08-06T15:24:47.286794Z","submitted_at":"1999-08-18T14:56:58Z","title":"Energy Spectrum and Chemical Composition of Cosmic Rays between 0.3 and 10 PeV determined from the Cherenkov-Light and Charged-Particle distributions in Air Showers","version":1},"cited_work":{"arxiv_id":"astro-ph/9908202","doi":"10.48550/arxiv.astro-ph/9908202","metadata_source":"pith","pith_arxiv_id":"astro-ph/9908202","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Energy Spectrum and Chemical Composition of Cosmic Rays between 0.3 and 10 PeV determined from the Cherenkov-Light and Charged-Particle distributions in Air Showers","venue":"astro-ph","work_id":"de9be683-4158-4158-bb6d-b81ec8267375","year":1999},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"cited_paper":"/paper/astro-ph/9908202","citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:9cc386299076558148d6059a999fae1ce58672b576c5fac7831e631693e86368","observation_id":"b41e11ee-5c52-456a-a5d1-793c0c45b1c6","resolution":{"observed_at":"2026-07-11T05:07:46.428403Z","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":"2026-07-11T13:49:32.514163+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:32.514163+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":null,"venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:5e5fc645b5843e7c1bbfab5890eb1a189dd40e415a16214722a0af3a838003e6","observation_id":"ad78a939-f0bc-41fe-a0ed-bc9537fe5b20","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1086/308545","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The Cosmic-Ray Electron and Positron Spectra Measured at 1 AU during Solar Minimum Activity","venue":"The Astrophysical Journal","work_id":"b98b98d2-aaed-4558-98db-8deb6f66d3af","year":2000},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:0a0c52081a6d806d70285df9f884c4b4799e9b9859243527e145ff8b42ec10a4","observation_id":"f0be65c0-d9e3-41b1-bfd7-bac8fcf54e90","resolution":{"observed_at":"2026-07-11T05:07:46.618921Z","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":"2026-07-11T13:49:32.757523+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:32.757523+00:00","source":"openalex_status_cache"},{"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":"10.3847/1538-4357/ab64f1","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Deciphering the Local Interstellar Spectra of Secondary Nuclei with the Gal- prop/Helmod Framework and a Hint for Primary Lithium in Cosmic Rays","venue":"The Astrophysical Journal","work_id":"90816734-9930-4ad3-b065-78a1db2c1bed","year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:63a5df960555febde461c7cdc025958a44deea780e06070c816d9f83041e9f2e","observation_id":"8ecc1783-f7df-4b46-b661-00695fe3b420","resolution":{"observed_at":"2026-07-11T05:07:46.444915Z","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":"2026-07-11T13:49:33.060535+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:33.060535+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z≤28 with the GALPROP-HELMOD Framework","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f5caf73e5a989dcaf77c077b58cd3b99f7541d942d81103956d01ec294547217","observation_id":"eb694289-dc5c-4b45-a700-07fdadd474d4","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1016/j.asr.2017.04.017","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Propagation of cosmic rays in heliosphere: The HelMod model","venue":"Advances in Space Research","work_id":"2cabc243-5692-4260-b67f-c3ce41cad2db","year":2018},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f7422b65f06586a61fb212db1ac3708f0017b691b7b284170b19b5211395380a","observation_id":"51342fbf-1277-44b7-a32b-000ef59b2ea3","resolution":{"observed_at":"2026-07-11T05:07:46.457934Z","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":"2026-07-11T13:49:33.443969+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:33.443969+00:00","source":"openalex_status_cache"},{"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/physrevresearch.2.023022","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"AMS-02 antiprotons’ consistency with a secondary astrophysical origin","venue":"Physical Review Research","work_id":"3598eff4-1c37-4a6c-8d7d-c1fb29dd1b01","year":2020},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:72fb4c3ab66026ee9483d1af657310d3f12f802b36e62071ed28e7e47d76b527","observation_id":"a8a9f024-22a2-4513-b617-428143b79fd1","resolution":{"observed_at":"2026-07-11T05:07:46.506276Z","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":"2026-07-11T13:49:33.690278+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:33.690278+00:00","source":"openalex_status_cache"},{"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":"10.1016/j.asr.2022.07.037","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Investigating cosmic ray elemental spectra and the at- mospheric muon neutrino flux","venue":"Advances in Space Research","work_id":"5a49917b-88bc-456c-9382-f2dba2f9d788","year":2022},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:bb69b22a3ae02bc27e81a9a369931b2b5236607c3de101d551228b0a3daa82d2","observation_id":"fe1e78fb-b992-4837-b0b3-16085853dff2","resolution":{"observed_at":"2026-07-11T05:07:46.501389Z","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":"2026-07-11T13:49:33.97733+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:33.97733+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Measurements of All-Particle Energy Spectrum and Mean Logarithmic Mass of Cosmic Rays from 0.3 to 30 PeV with LHAASO-KM2A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:eab1c2a3f2267417d03b9f4c99d5cd3a921099c2628bbd1091ead1e8537bb49d","observation_id":"296d3d20-ce20-4046-a5cd-08d93a1a601a","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1038/nature07477","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"An excess of cosmic ray electrons at energies of 300-800 GeV","venue":"Nature","work_id":"bdd40926-37dd-4acf-8d1d-8f05e2093a74","year":2008},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:b78f58a7589fa835782efe8857b76b9a6c7374015a75cf91eb303c0c58778de4","observation_id":"0cf7c05c-a9b3-4345-86c2-2f0dbf590974","resolution":{"observed_at":"2026-07-11T05:07:46.613568Z","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":"2026-07-11T13:49:34.64599+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:34.64599+00:00","source":"openalex_status_cache"},{"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":"10.22323/1.444.0069","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Studies of Cosmic-Ray Propagation Using GALPROP","venue":null,"work_id":"4cf2c133-fb98-4614-b23a-7c238290d748","year":2023},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:17843c994d1d2d4e067b61946aea124697a8f681a017db9e039d8da13314ef4c","observation_id":"f5b36e32-9e2c-4aa5-bc09-16361a87a06e","resolution":{"observed_at":"2026-07-11T05:07:46.434586Z","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":"2026-07-11T13:49:34.865442+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:34.865442+00:00","source":"openalex_status_cache"},{"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":"10.3847/1538-4357/ac9d2c","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Measurement of High-energy Cosmic-Ray Proton Spectrum from the ISS-CREAM Experiment","venue":"The Astrophysical Journal","work_id":"c7496ae3-1646-4594-b601-1b3d900d7088","year":2022},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:4a427e6dd977a9b1f65bb0af827005d5f61e08e8d54a23e7a83b1b26ecf5b85d","observation_id":"765eb98e-6652-484a-8fb0-1d64af1123e2","resolution":{"observed_at":"2026-07-11T05:07:46.553402Z","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":"2026-07-11T13:49:35.179177+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:35.179177+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Galactic Cosmic Rays in the Local Interstellar Medium: Voyager 1 Observa- tions and Model Results","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f89e9b9160fb0216f1e71d15c2c60f80616388c20573776390581bde29f80053","observation_id":"6b75c06c-63cf-42fc-8335-6f3d28226fe8","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Fitting B/C cosmic-ray data in the AMS-02 era: a cookbook. Model numerical pre- cision, data covariance matrix of errors, cross-section nuisance parameters, and mock data","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:415ef59236e609a5f7232007ebd954ccfe325baacbd4c63e1191382a033699b1","observation_id":"8e8d493c-41fc-49f3-9724-f811e7180dad","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1086/322324","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Cosmic-Ray Electrons and Positrons from 1 to 100 GeV: Measurements with HEAT and Their Interpretation","venue":"The Astrophysical Journal","work_id":"45487a61-f654-47ec-858b-5fb0f8495c5f","year":2001},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f598b77c4bf7c91220ea4bf29c95f0dc675f8929905f38e8e23cbcbe9c93da45","observation_id":"bfaffc2b-3ab7-45fc-b499-cde3e7b408be","resolution":{"observed_at":"2026-07-11T05:07:46.691346Z","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":"2026-07-11T13:49:35.969948+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:35.969948+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to Ni - Results from HEAO-3-C2","venue":null,"work_id":null,"year":1990},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:1c289cfb64da83b4b922422f1ea9f773f09310925ffea8e4c9124d18cf10c0ed","observation_id":"6e73b65c-cd41-47a4-bcee-7f106715e780","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Cosmic ray energy spectrum from measurements of air showers","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:40f132b5b563939a16d8018ea9354e06b500d2d7bf5f2fda67300d73027b5bc6","observation_id":"da44ebce-6e4f-4d3f-9666-24b11478e42e","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"The cosmic ray energy spectrum between 10 14 and 1016 eV","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:2259298e1fe00b0ef828fb892556968aa9d02675246cfaa4c2701324badbafdd","observation_id":"d6b36499-c978-4158-ae00-df4ba781d681","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1086/149822","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Solar Modulation of Galactic Cosmic Rays","venue":"The Astrophysical Journal","work_id":"d317b2db-9a2c-491a-aded-e48b099480ad","year":1968},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:fd8fa98fc503b0c226cb7a0075ddeeabec378b2eb13fd48c255280f116f8dbb5","observation_id":"7a8c876c-07dd-4075-8a72-796cf70a1509","resolution":{"observed_at":"2026-07-11T05:07:46.697264Z","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":"2026-07-11T13:49:36.754542+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:36.754542+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Energy spectra of abundant cosmic-ray nuclei in the NUCLEON experiment","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:b457b683730f56903d737ae7d0eb25ebd3e65f99749f4eb02b28fcc27d74dfc0","observation_id":"bb8ae925-b5f1-4f19-aa55-8d3ede1a60ba","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1051/0004-6361:20020845","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Measurements of the absolute energy spectra of cosmic-ray positrons and electrons above 7 GeV","venue":"Astronomy and Astrophysics","work_id":"6a759265-a67d-4c1a-8c9f-ce78c830ff5d","year":2002},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:8dac5abb71a7d2102cb907c45642c58b4cf687e7e1036c6a179e4a1ad8551233","observation_id":"1896734d-cf05-424c-a8fd-aa2f883212fd","resolution":{"observed_at":"2026-07-11T05:07:46.580805Z","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":"2026-07-11T13:49:37.323938+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:37.323938+00:00","source":"openalex_status_cache"},{"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.48.1949","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Observation of heavy cosmic-ray primaries over the wide energy range from ∼100 GeV/particle to∼100 TeV/particle: Is the celebrated","venue":"Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields","work_id":"346ce6ec-b91a-426d-a5dc-64243d16cacf","year":1993},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:debb7df297a13ada8b4e46c571b9ce3bcc8dfbbf34106eb17c8e1b7fdf7a51f0","observation_id":"0f9d123c-62f0-413b-a461-4fe3c58bf1df","resolution":{"observed_at":"2026-07-11T05:07:46.516402Z","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":"2026-07-11T13:49:37.572389+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:37.572389+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"(1998).MINUIT – Function Minimization and Error Analysis: Reference Manual Version 94.1","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:62b123e2e27b2c06d1b1bd3264a12c46955de41c56bea620e02b9edc119976ea","observation_id":"ff2cd1b6-e1be-4b60-881a-b1ebbc8fa9ff","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Minuit - a system for function minimization and analysis of the parameter errors and correlations","venue":null,"work_id":null,"year":1975},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:66d6d4dd62455bc43aafe48514cc698a8ac4092ce069345842cf41a7dfde8ee2","observation_id":"9489c130-538a-4d3f-bb1f-a84befef06ba","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-07-11T05:04:59.572341Z","title":"Azimuthally controlled observation of heavy cosmic-ray primaries by means of the balloon-borne emulsion chamber","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:794cf4917f3b8cad3a1fe1eba14cb65f083d12332a1de264f4992582d0bc2f46","observation_id":"580b796b-12a7-4832-b2ef-b64e7dcf2523","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/ac7049","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"On the Origin of Observed Cosmic-Ray Spectrum Below 100 TV","venue":"The Astrophysical Journal","work_id":"4727ab7e-c892-4076-bf3c-56d94cb565df","year":2022},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:d2d679995e733b7ba5371bb32937b3312aaba91c9b33376c4f67d70c6e23c59b","observation_id":"2539426d-1217-4766-a17e-0d17ac2b2534","resolution":{"observed_at":"2026-07-11T05:07:46.409913Z","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":"2026-07-11T13:49:37.879916+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:37.879916+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"(2018).USINE Documentation: Section 5.4","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:55a4171cc7e2d02d91d8029fa471649137c001a2a576e9f053fb31bbc2f8f8a8","observation_id":"d571338a-5d27-400b-90e5-46f2273e5d5c","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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.104.103029","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Explaining cosmic ray antimatter with secondaries from old supernova remnants","venue":"Physical review. D/Physical review. D.","work_id":"e7540916-62b3-452b-bba5-3ba8fd0726d7","year":2021},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:07dbfd64400b3522e1c7edf72d5ab43ce4c08a3ab48d36e12e4cfc73b6bbd8de","observation_id":"7bc3151f-6d0a-4e80-bc1f-23915f0299f2","resolution":{"observed_at":"2026-07-11T05:07:46.530826Z","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":"2026-07-11T13:49:38.129226+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:38.129226+00:00","source":"openalex_status_cache"},{"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":"10.22323/1.395.0330","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"The all-particle cosmic ray energy spectrum measured with HAWC","venue":"Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)","work_id":"aead1a5b-3fa3-4ea9-b3e7-f842cbbedd20","year":2022},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:a517351772163e4f08ac5e1ef4c4ec96473e0c4b00cfb5418d61d1c27e54964c","observation_id":"fb55ae4a-90cf-4e20-9a73-3ddb68899a0b","resolution":{"observed_at":"2026-07-11T05:07:46.624142Z","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":"2026-07-11T13:49:38.451936+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:38.451936+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Production and Propagation of Cosmic-Ray Positrons and Electrons","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:ff890e725a9a08c798bb37b6676702f10e93129051a3f7bce704147a2f240ed2","observation_id":"747862c7-daa4-4060-805a-dd4d1bc95a4c","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1086/170125","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Energy Spectra and Composition of Primary Cosmic Rays","venue":"The Astrophysical Journal","work_id":"4bb09183-a658-4e68-8608-1ef128759208","year":1991},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:8de2cc216b7cb67fb42143d2d3a3c9ed92725c9a7d4b3ee0605d19949fba4c6a","observation_id":"34469a77-c439-44ef-8911-a7456d983f32","resolution":{"observed_at":"2026-07-11T05:07:46.439795Z","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":"2026-07-11T13:49:38.956569+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:38.956569+00:00","source":"openalex_status_cache"},{"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":"10.1088/0004-637x/742/1/14","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Energy Spectra of Primary and Secondary Cosmic-Ray Nuclei Measured with TRACER","venue":"The Astrophysical Journal","work_id":"6f8aa16f-2e89-4d12-8fa9-3644edc004f6","year":2011},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:47f4e3aa2e58a54ba36c5af4ae0c06818b93745fd8e444ffaca7feeaf4a890f6","observation_id":"1cacf8a0-3c31-4170-91de-3701966b4d75","resolution":{"observed_at":"2026-07-11T05:07:46.463438Z","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":"2026-07-11T13:49:39.203026+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:39.203026+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0707.4415","last_updated":"2007-07-30T13:46:39Z","snapshot_observed_at":"2026-08-15T10:35:09.686676Z","submitted_at":"2007-07-30T13:46:39Z","title":"Relative abundances of cosmic ray nuclei B-C-N-O in the energy region from 10 GeV/n to 300 GeV/n. Results from ATIC-2 (the science flight of ATIC)","version":1},"cited_work":{"arxiv_id":"0707.4415","doi":"10.48550/arxiv.0707.4415","metadata_source":"pith","pith_arxiv_id":"0707.4415","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"Relative abundances of cosmic ray nuclei B-C-N-O in the energy region from 10 GeV/n to 300 GeV/n. Results from ATIC-2 (the science flight of ATIC)","venue":"astro-ph","work_id":"d0475c54-c089-4efe-81f6-f3cd0759ed4e","year":2007},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"cited_paper":"/paper/0707.4415","citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:0a4f77afdd1127426a3614415e5cb2f1c8c15907e684f1098836b615569262c7","observation_id":"7b2beaaf-8135-4a38-be82-6555e201091a","resolution":{"observed_at":"2026-07-11T05:07:46.525357Z","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":"2026-07-11T13:49:39.426104+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:39.426104+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Energy spectra of abundant nuclei of primary cosmic rays from the data of ATIC-2 experiment: Final results","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:4eb855bcf8ad0c936ccda7c659267408230995b0876ce9e950c26a50c8e4315d","observation_id":"913db912-613e-4d56-b795-853097496986","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"The GALPROP Cosmic-ray Propagation and Nonthermal Emissions Framework: Release v57","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:e59deef12e2eded1f7a7395b360dfc99ebc4ce081588c20def8f7e45965d5d89","observation_id":"b5c3132b-7011-4f32-9d20-742019edf435","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1016/j.nima.2013.09.018","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Tunka-133: Results of 3 year operation","venue":"Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment","work_id":"f063e078-bafe-450b-9a1a-9f2355bbb4d0","year":2014},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:7ff66cbcae737b00adfe89581647e908ca7bf2e2b285d3a89a739634c9024987","observation_id":"62453ffa-0200-42ac-8505-1849aeddc240","resolution":{"observed_at":"2026-07-11T05:07:46.490134Z","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":"2026-07-11T13:49:40.285712+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:40.285712+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Stochastic Reacceleration of Cosmic Rays in the Interstellar Medium","venue":null,"work_id":null,"year":1994},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:0592093507be30439f265a0df2934bef7a2b1c1155e7decea4e5d076af77fb79","observation_id":"990b55b2-131f-4f02-9572-769d52ead4dc","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"10.1007/s40042-021-00081-7","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Advances in direct measurements of cosmic rays","venue":"Journal of the Korean Physical Society","work_id":"e90ef764-b352-4713-852d-beab9468454a","year":2021},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:47c544539a3257065f636bab5ad793831926858c2c80c73765a4c583b32e4c42","observation_id":"963dd92b-0c5e-4b79-a381-7b8677389b03","resolution":{"observed_at":"2026-07-11T05:07:46.588709Z","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":"2026-07-11T13:49:40.829633+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:40.829633+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Measurements of 0.2-20 GeV/n cosmic-ray proton and helium spectra from 1997 through 2002 with the BESS spectrometer","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:00a5066093b042500847b43d6ed9022f3132dec27bc1d796831345888b1cc1b3","observation_id":"af7c254d-00fd-47a0-8b77-8fbfd9a9b2af","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-07-11T05:04:59.572341Z","title":"Updated Partial Cross Sections of Proton-Nucleus Reactions","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:4cdd95ab594462b652348eb777d66142ad6d03f413d4824e4514cadb6ad4398c","observation_id":"08d00bb3-c93a-406e-8f23-6352327906e5","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Voyager 1 Observes Low-Energy Galactic Cosmic Rays in a Region Depleted of Heliospheric Ions","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f521e92980fa6bb3cce36c706ff388303fa5baf13b7c7f3dd8b0d8bdd8816a53","observation_id":"ad45f188-5a1c-4372-bddc-c483a850f835","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Cosmic ray measurements from Voyager 2 as it crossed into interstellar space","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:7769f6e8e6ba5b75b7c4b3d76df7af3f0288db4a71f610682a6941e723f2d51a","observation_id":"44884435-f6aa-450c-aecf-c5768c99c5f8","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Propagation of Cosmic-Ray Nucleons in the Galaxy","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:eb32d77126cdf4c5de0a9bc973a07f8e25f7bbb7114059ffa8775ab043d22cf2","observation_id":"c0b78f3a-6b4c-4f6a-9fa7-dde0afe9499e","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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.89.123003","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Sharp knee phenomenon of primary cosmic ray energy spectrum","venue":"Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology","work_id":"df61708a-6372-4bf3-980a-4d297a03907a","year":2014},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:1e5ecfc54468ddac4cd3f669172eea0deb57677b0794020b3d273734dd863d82","observation_id":"bb80bc92-2947-477b-a5fd-312635ee3e93","resolution":{"observed_at":"2026-07-11T05:07:46.495819Z","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":"2026-07-11T13:49:42.022898+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:42.022898+00:00","source":"openalex_status_cache"},{"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":"10.22323/1.395.0155","metadata_source":"openalex","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Study Of Cosmic Ray Spectral Hardening Using GALPROP","venue":"Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)","work_id":"89231114-79b3-45d9-ae22-62333e6e1237","year":2021},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:f2b8848c6a0d4fccba15780490aadd9b185eba53b171b4f83a5566049b798079","observation_id":"2a61d12a-7efa-4cfd-9c75-a4d6f662b427","resolution":{"observed_at":"2026-07-11T05:07:46.566861Z","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":"2026-07-11T13:49:42.270657+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-11T13:49:42.270657+00:00","source":"openalex_status_cache"},{"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":"2026-07-11T05:04:59.572341Z","title":"Cosmic-ray Proton and Helium Spectra from the First CREAM Flight","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:ec9eac72e85dd97de1d024c5bb9f717a6c4f0cd0bb529ecc98910a6e618f5118","observation_id":"83676d0c-4f5c-470c-832e-81ba6e4ee91f","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","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":"2026-07-11T05:04:59.572341Z","title":"Proton and Helium Spectra from the CREAM-III Flight","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-11T05:04:59.572341Z"},"links":{"citing_paper":"/paper/2607.05606"},"observation_digest":"sha256:0a63daee7dcef3dc9739840011a53c5ffbcb54fb0be7105d7e1af58c8318c1e1","observation_id":"23c04034-2294-417a-a306-f408244cebe5","resolution":{"observed_at":"2026-07-11T05:04:59.572341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2607.05606","last_updated":"2026-07-06T20:04:06Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-18T09:17:49.229831Z","submitted_at":"2026-07-06T20:04:06Z","title":"Analyzing Cosmic Ray Spectral Features: A Numerical Investigation"},"reference_resolution":{"displayed":73,"state_counts":{"malformed_identifier":8,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":40,"verified_exact":25,"verified_fuzzy":0},"total_outbound_references":73},"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 73 of 73 outbound references and 0 inbound Pith citation observations for arXiv:2607.05606."}