{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:T2GYBN4DJR6AAXV5QEO37ZHMTJ","short_pith_number":"pith:T2GYBN4D","schema_version":"1.0","canonical_sha256":"9e8d80b7834c7c005ebd811dbfe4ec9a62fcfc92ca2b230cb88b306989ac93a8","source":{"kind":"arxiv","id":"1810.10410","version":3},"attestation_state":"computed","paper":{"title":"Cosmic-Ray Extremely Distributed Observatory: status and perspectives","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"A.R. Duffy, D. Alvarez-Castillo, D. G\\'ora, D. Ostrog\\'orski, J. Ja{\\l}ocha, J. Stasielak, J. Zamora-Saa, K. Almeida Cheminant, K. Kopa\\'nski, K. Rzecki, K. Smo{\\l}ek, K. W. Wo\\'zniak, {\\L}. Bratek, M. Kasztelan, M. Nied\\'zwiecki, N. Dhital, O. Sushchov, P. Homola, P. Jagoda, P. Kovacs, V. Nazari","submitted_at":"2018-10-24T14:13:07Z","abstract_excerpt":"The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date cosmic-ray research has been focused on detecting single air showers, while the search for ensembles of cosmic-rays, which may overspread a significant fraction of the Earth, is a scientific terra incognita. Instead of developing and commissioning a completely new global detector infrastructure, CREDO proposes approaching the global cosmic-ray anal"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1810.10410","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2018-10-24T14:13:07Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"4ca6b693fe57cef754255ac663ae882987098d64605123b50f4f299c72b1fdf9","abstract_canon_sha256":"4a90b4595e662bd4ba2ec0b2043902e852c2f832143a71dfc8bfc803db975da2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:02:08.683630Z","signature_b64":"JSEKDp7ItQ1+yqLz1+eImeq3b8pGBS/7LF3H2p3z1irQvJd4IF1vsuRtBJnlpwrFht53IFyvn7wTnc6tFGeVCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e8d80b7834c7c005ebd811dbfe4ec9a62fcfc92ca2b230cb88b306989ac93a8","last_reissued_at":"2026-05-18T00:02:08.683057Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:02:08.683057Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic-Ray Extremely Distributed Observatory: status and perspectives","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.IM","authors_text":"A.R. Duffy, D. Alvarez-Castillo, D. G\\'ora, D. Ostrog\\'orski, J. Ja{\\l}ocha, J. Stasielak, J. Zamora-Saa, K. Almeida Cheminant, K. Kopa\\'nski, K. Rzecki, K. Smo{\\l}ek, K. W. Wo\\'zniak, {\\L}. Bratek, M. Kasztelan, M. Nied\\'zwiecki, N. Dhital, O. Sushchov, P. Homola, P. Jagoda, P. Kovacs, V. Nazari","submitted_at":"2018-10-24T14:13:07Z","abstract_excerpt":"The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date cosmic-ray research has been focused on detecting single air showers, while the search for ensembles of cosmic-rays, which may overspread a significant fraction of the Earth, is a scientific terra incognita. Instead of developing and commissioning a completely new global detector infrastructure, CREDO proposes approaching the global cosmic-ray anal"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.10410","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1810.10410","created_at":"2026-05-18T00:02:08.683149+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.10410v3","created_at":"2026-05-18T00:02:08.683149+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.10410","created_at":"2026-05-18T00:02:08.683149+00:00"},{"alias_kind":"pith_short_12","alias_value":"T2GYBN4DJR6A","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_16","alias_value":"T2GYBN4DJR6AAXV5","created_at":"2026-05-18T12:32:53.628368+00:00"},{"alias_kind":"pith_short_8","alias_value":"T2GYBN4D","created_at":"2026-05-18T12:32:53.628368+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ","json":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ.json","graph_json":"https://pith.science/api/pith-number/T2GYBN4DJR6AAXV5QEO37ZHMTJ/graph.json","events_json":"https://pith.science/api/pith-number/T2GYBN4DJR6AAXV5QEO37ZHMTJ/events.json","paper":"https://pith.science/paper/T2GYBN4D"},"agent_actions":{"view_html":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ","download_json":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ.json","view_paper":"https://pith.science/paper/T2GYBN4D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.10410&json=true","fetch_graph":"https://pith.science/api/pith-number/T2GYBN4DJR6AAXV5QEO37ZHMTJ/graph.json","fetch_events":"https://pith.science/api/pith-number/T2GYBN4DJR6AAXV5QEO37ZHMTJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ/action/storage_attestation","attest_author":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ/action/author_attestation","sign_citation":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ/action/citation_signature","submit_replication":"https://pith.science/pith/T2GYBN4DJR6AAXV5QEO37ZHMTJ/action/replication_record"}},"created_at":"2026-05-18T00:02:08.683149+00:00","updated_at":"2026-05-18T00:02:08.683149+00:00"}