{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:K25JIOS5KHK4ZNNQOYWCJHEVE2","short_pith_number":"pith:K25JIOS5","schema_version":"1.0","canonical_sha256":"56ba943a5d51d5ccb5b0762c249c9526a20ca44f9944d8af13f7cc56a268cb73","source":{"kind":"arxiv","id":"1110.0012","version":1},"attestation_state":"computed","paper":{"title":"Low Energy Neutrino Astronomy in Super-Kamiokande","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ex","authors_text":"Michael Smy","submitted_at":"2011-09-30T20:19:35Z","abstract_excerpt":"Super-Kamiokande is sensitive to neutrino interactions between 4 and 100MeV via elastic scattering and inverse beta decay. I will present Super-Kamiokande's ongoing measurements of solar neutrinos and its searches for supernova neutrinos."},"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":"1110.0012","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ex","submitted_at":"2011-09-30T20:19:35Z","cross_cats_sorted":[],"title_canon_sha256":"55698d8a3d8b6148471b5222ec07a3239ec7cbe8a69168212a7cd96635e75501","abstract_canon_sha256":"ca8c9b84256a9fb3fee7017c8e119778e38f0b51f11e9ed8a06d483d8dab80bf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:11:50.982241Z","signature_b64":"zDCAn/2apegpWqN1eLDcTxh+yicmrT82Kx0ICBMbhzHHJIZDfB605bV+/VYL6YSpkrFdPSNYwY97Q6oA654GCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"56ba943a5d51d5ccb5b0762c249c9526a20ca44f9944d8af13f7cc56a268cb73","last_reissued_at":"2026-05-18T04:11:50.981715Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:11:50.981715Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Low Energy Neutrino Astronomy in Super-Kamiokande","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ex","authors_text":"Michael Smy","submitted_at":"2011-09-30T20:19:35Z","abstract_excerpt":"Super-Kamiokande is sensitive to neutrino interactions between 4 and 100MeV via elastic scattering and inverse beta decay. I will present Super-Kamiokande's ongoing measurements of solar neutrinos and its searches for supernova neutrinos."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1110.0012","kind":"arxiv","version":1},"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":"1110.0012","created_at":"2026-05-18T04:11:50.981808+00:00"},{"alias_kind":"arxiv_version","alias_value":"1110.0012v1","created_at":"2026-05-18T04:11:50.981808+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1110.0012","created_at":"2026-05-18T04:11:50.981808+00:00"},{"alias_kind":"pith_short_12","alias_value":"K25JIOS5KHK4","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"K25JIOS5KHK4ZNNQ","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"K25JIOS5","created_at":"2026-05-18T12:26:32.869790+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/K25JIOS5KHK4ZNNQOYWCJHEVE2","json":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2.json","graph_json":"https://pith.science/api/pith-number/K25JIOS5KHK4ZNNQOYWCJHEVE2/graph.json","events_json":"https://pith.science/api/pith-number/K25JIOS5KHK4ZNNQOYWCJHEVE2/events.json","paper":"https://pith.science/paper/K25JIOS5"},"agent_actions":{"view_html":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2","download_json":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2.json","view_paper":"https://pith.science/paper/K25JIOS5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1110.0012&json=true","fetch_graph":"https://pith.science/api/pith-number/K25JIOS5KHK4ZNNQOYWCJHEVE2/graph.json","fetch_events":"https://pith.science/api/pith-number/K25JIOS5KHK4ZNNQOYWCJHEVE2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2/action/storage_attestation","attest_author":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2/action/author_attestation","sign_citation":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2/action/citation_signature","submit_replication":"https://pith.science/pith/K25JIOS5KHK4ZNNQOYWCJHEVE2/action/replication_record"}},"created_at":"2026-05-18T04:11:50.981808+00:00","updated_at":"2026-05-18T04:11:50.981808+00:00"}