{"as_of":"2026-08-23T12:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:caee430ffb57e1d02a1ac6db189c3c4a18d692b66b08d1e4c407646fca3dc64e","coverage":[{"denominator":25,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":25,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T11:51:54.140487Z","state":"measured"},{"denominator":25,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":25,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+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/1908.08139/citation-record","integrity":"/paper/1908.08139/integrity","json":"/paper/1908.08139/citation-record.json","paper":"/paper/1908.08139"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.414001Z","title":"Aartsen et al., J","venue":null,"work_id":"22889fc7-a72f-42d1-82ed-7a0e8422f6d9","year":2017},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.052474Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:526ffdd372d8952ebc89ddaae2dc5b9c5a05c30f58443b41d1c789c9e16e08cd","observation_id":"a3b08bc8-3970-49dc-bfc7-5e243a1b32bd","resolution":{"observed_at":"2026-08-14T11:51:54.417363Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.403425Z","title":"Abbasi et al., Nucl","venue":null,"work_id":"2f998446-23da-4bcc-a4f5-999b1b055172","year":2013},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.057065Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:64d38f49668db6cf43218b23c36b041f402d90e20f922fddf7e43780edf9bed0","observation_id":"a78c5c12-db2c-4b76-9d66-00504189fe7b","resolution":{"observed_at":"2026-08-14T11:51:54.407599Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.393187Z","title":"Kampert and M","venue":null,"work_id":"f5125da8-8c62-4812-99f0-67cccbae7b91","year":2012},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.061316Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:c6488c68998504a66026cfb1c32365d73d492ce0da0fddf5326d1151b0370cc2","observation_id":"4439c7c8-c0a1-4b6f-bb99-593d48ead3ca","resolution":{"observed_at":"2026-08-14T11:51:54.397077Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.384075Z","title":"Abbasi et al., Nucl","venue":null,"work_id":"7a8a3684-cc14-4bb2-b902-b731ce7a5aae","year":2009},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.065393Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:d88b46371e5706e4d9eef427de2ef937e1370a82b151db71f2dc3c4c28b4306f","observation_id":"6fda41f3-fed9-4c42-88d9-fa212f7d4fcb","resolution":{"observed_at":"2026-08-14T11:51:54.387375Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.374436Z","title":"Abbasi et al., Nucl","venue":null,"work_id":"337d4872-716a-44ae-ac2b-6ec0cf95b8ff","year":2008},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.069961Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:533f23d9bd01d01cf992f7c98522790ce2429ba4de76deb970db18fbdacda94d","observation_id":"9c28a01a-4891-4f1e-b3c8-1ae937f83106","resolution":{"observed_at":"2026-08-14T11:51:54.377648Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.365094Z","title":"Andeen and M","venue":null,"work_id":"609ef2c0-e381-4f61-b484-71898e1e76cb","year":2019},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.074025Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:1df323cfc82906d771d983bf8174843d640e83641a9588e33afe41f5a44fccfc","observation_id":"c522db26-45a4-458c-8a79-825455d74d79","resolution":{"observed_at":"2026-08-14T11:51:54.368475Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.354355Z","title":null,"venue":null,"work_id":"d34eeecf-02f7-47a7-a163-8fb36bbfc431","year":2014},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.077892Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:4efa92ef62651fab3f7a18b172141b47652457595291b64d91c4e5191f2ea585","observation_id":"64cb2b6c-9406-4a4a-9a44-55700e268c2c","resolution":{"observed_at":"2026-08-14T11:51:54.358823Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.344166Z","title":"Aartsen et al., Physical Review D 88 (Aug, 2013) 042004","venue":null,"work_id":"75bb07ee-4418-47b3-a5a1-74d01484c7a4","year":2013},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.081354Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:c626006f4935b0cd1c9eb80fcf592a3139edbc49c8d897a131a6cd4eccd2d3d6","observation_id":"52e5a4be-a28c-4a2c-9245-34acc485e67e","resolution":{"observed_at":"2026-08-14T11:51:54.347542Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.333431Z","title":"Heck et al., CORSIKA: A Monte Carlo code to simulate extensive air showers, Report FZKA 6019, F orschungszentrum Karlsruhe, 1998","venue":null,"work_id":"85e19d8f-030f-4a7e-a123-3657df5b7925","year":1998},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.084981Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:f125160076b1771a49da78032cfa10158c6b20321eec18888d1a84372fa4318d","observation_id":"57ac9daf-26b8-43f2-aedd-b4e492198157","resolution":{"observed_at":"2026-08-14T11:51:54.337308Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.322823Z","title":"Heck and T","venue":null,"work_id":"3ff23ac0-dbf8-4acb-8875-a1fc8101e238","year":null},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.088399Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:9ffe5218100307980f49b32dff8caae4fcf3655cc9c0194136058a578131c37f","observation_id":"eec27e84-3413-47a9-9dc3-1c2ebfdde72f","resolution":{"observed_at":"2026-08-14T11:51:54.326932Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.312062Z","title":"Battistoni et al., AIP Conference Proceedings 896 (2007) 31–49","venue":null,"work_id":"308128de-2a0b-4df4-829c-3bf1191321b0","year":2007},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.092013Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:aae5b0dee084d4343e5f6ae643b65f279310d528eb8a3b1fbdf86866082104a6","observation_id":"fedbfa44-0a02-4e9e-8567-3483434b5e70","resolution":{"observed_at":"2026-08-14T11:51:54.315799Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.302140Z","title":null,"venue":null,"work_id":"3bc6ce1f-da23-42d1-8ea2-31348082ac23","year":2009},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.095514Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:c141ab5fed42aadabe96bc0d1c10eafdf51a81a401a130f93400d37a12e6d13d","observation_id":"97ae0aea-f837-4d75-a00f-b34d0a57f832","resolution":{"observed_at":"2026-08-14T11:51:54.305569Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.291795Z","title":"Agostinelli et al., Nucl","venue":null,"work_id":"32d453a2-d84b-452f-9de3-8187393f71a2","year":2003},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.099187Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:d509e40a6ffbfee458b4a88d080a3dc7f621f274ff0c91eca1448a51d4b82fd9","observation_id":"fc2419be-8ed6-4cca-9074-fff921cbfd3c","resolution":{"observed_at":"2026-08-14T11:51:54.295115Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.281683Z","title":"Allison et al., IEEE Transactions on Nuclear Science 53 (2006) 270–278","venue":null,"work_id":"1461fa82-d6fe-4835-8caa-212f8a002005","year":2006},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.102520Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:4dcaa09ca65b15b44a4dd2f71241f1e03b7a11702ccc87ae681aae8ef9487b17","observation_id":"5e9c4bf9-450b-4697-9448-82baef83f855","resolution":{"observed_at":"2026-08-14T11:51:54.285514Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.271612Z","title":null,"venue":null,"work_id":"990c87f6-7d09-4ac7-b64c-2c4ab0d611c7","year":2012},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.105850Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:47901ddf31e74152fd32069feac6056aa0acf171de1a1840153c80a538b28621","observation_id":"112131ef-747f-46b1-a43d-541af0f5a967","resolution":{"observed_at":"2026-08-14T11:51:54.275254Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.260162Z","title":null,"venue":null,"work_id":"29773694-9d4a-4e71-9bc9-868745b45e3a","year":2014},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.109093Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:d0bfec0e1bf33985f2b624c3ed843d6303baacd39536115be83f2211a0b3881f","observation_id":"2add5329-885e-45d9-b529-5d704cdde6a8","resolution":{"observed_at":"2026-08-14T11:51:54.263723Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.248965Z","title":"De Ridder","venue":null,"work_id":"b69d1f2d-ce6c-404f-9be0-3df9b95ff56d","year":2019},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.112264Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:f455c6e11746a5a893ef6b71a94c37c2f16eeef9f72fa6679061291c8d37f00e","observation_id":"37891517-9b9f-4ad9-86d2-8157d5bff5ed","resolution":{"observed_at":"2026-08-14T11:51:54.253046Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.238525Z","title":"Abbasi et al., Astroparticle Physics 42 (2013) 33","venue":null,"work_id":"5d966c99-23b7-4bbf-acb3-ff92c681e4e1","year":2013},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.115747Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:c064044b3993142314bb15f473c53d59f609f9b6fa0088396bb666f210f957a2","observation_id":"baedd1a6-2678-4d13-9543-bc7acb217425","resolution":{"observed_at":"2026-08-14T11:51:54.242346Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.227885Z","title":"Cranmer, Computer Physics Communications 136 (2001) 198 – 207","venue":null,"work_id":"ac15ca9f-ce7c-40e0-a508-7a145dea658f","year":2001},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.119191Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:e19ce37170bc3510a3574d326221cd33367374892428fd9e8de7cc92304c86a0","observation_id":"3786f7d6-769b-480a-80c1-07625f10817d","resolution":{"observed_at":"2026-08-14T11:51:54.231635Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.217555Z","title":"Pierog, I","venue":null,"work_id":"d31714d0-4c89-4e24-9504-bc0c0e53ce67","year":2015},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.122407Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:9056d1be41a0743b5d1a88ca3581b87e4ee33bfb845772aad759967ed6c1749e","observation_id":"08321cd1-488a-4446-964c-650bd6cf965d","resolution":{"observed_at":"2026-08-14T11:51:54.221047Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.126058Z","title":"Riehn, R","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.126058Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:c961e027db17ab93933a65db9f441bc252480381b60ca9e8f0e74a0f2cb5f781","observation_id":"b3d5dee7-d7e1-40a5-8695-67464b89b34e","resolution":{"observed_at":"2026-08-14T11:51:54.126058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.201538Z","title":"Ostapchenko, Phys","venue":null,"work_id":"ec04d5ba-32a4-492c-8a18-3a9f9efd0ed0","year":2011},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.129374Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:ebb48f1a35eee278a5ccd93a15b4b73ddf998459e48b7c4f3a96213a2849d2b3","observation_id":"34f8befd-b636-4a4f-8757-0b496dbd5aed","resolution":{"observed_at":"2026-08-14T11:51:54.205172Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1906.04317","last_updated":"2019-11-12T19:06:25Z","snapshot_observed_at":"2026-08-18T05:20:26.520818Z","submitted_at":"2019-06-10T23:13:25Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV Using 3 Years of Data From IceTop and IceCube","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.04317","snapshot_observed_at":"2026-08-14T11:51:54.133112Z","title":null,"venue":null,"work_id":null,"year":1906},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.133112Z"},"links":{"cited_paper":"/paper/1906.04317","citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:c627219fbdea28d9bcc974c9ac9ee4c1fd51a6505bc6e8fa8b86fe148ea21966","observation_id":"c0495ab8-6638-4fca-a76c-b144d460fa67","resolution":{"observed_at":"2026-08-14T11:51:54.133112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.190499Z","title":null,"venue":null,"work_id":"63645e00-d9ac-418d-b26d-e31e7218e21f","year":2013},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.136931Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:b4e7084cbc21bb24168dcc9deba25e18efd69aa2ef6fca3a26a8df4c66fd707d","observation_id":"e996140f-ee17-414d-8f87-550f00376260","resolution":{"observed_at":"2026-08-14T11:51:54.194504Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-14T11:51:54.177836Z","title":null,"venue":null,"work_id":"31063a67-1cde-45fb-a9b7-84083fdbad64","year":2018},"citing_paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-14T11:51:54.140487Z"},"links":{"citing_paper":"/paper/1908.08139"},"observation_digest":"sha256:4f9b09547fd07e1dcb8a8240de42b7adf864aa47b82718c51529529e98d92bee","observation_id":"5cc23954-2f63-4962-aca7-4df5fce5e55c","resolution":{"observed_at":"2026-08-14T11:51:54.182932Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"1908.08139","last_updated":"2019-08-21T23:20:41Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-22T10:51:46.727146Z","submitted_at":"2019-08-21T23:20:41Z","title":"Cosmic Ray Spectrum and Composition from PeV to EeV from the IceCube Neutrino Observatory"},"reference_resolution":{"displayed":25,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":8,"verified_exact":0,"verified_fuzzy":17},"total_outbound_references":25},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 25 of 25 outbound references and 0 inbound Pith citation observations for arXiv:1908.08139."}