{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:UJEL7CN5HKSRSK5XGOW7CTDDA3","short_pith_number":"pith:UJEL7CN5","canonical_record":{"source":{"id":"1006.0546","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-06-03T03:01:06Z","cross_cats_sorted":["astro-ph.IM","physics.data-an"],"title_canon_sha256":"f98fe52168e803142fbaa5ea4a09193d0af61daf3312930536d74cfb3a3cf493","abstract_canon_sha256":"e469f80832ae895bdcfb65288aa8106721b7e1bba198c1e6b1abbe8a3db69f63"},"schema_version":"1.0"},"canonical_sha256":"a248bf89bd3aa5192bb733adf14c6306cda128f42fb5815b712bc3c04a0993bd","source":{"kind":"arxiv","id":"1006.0546","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.0546","created_at":"2026-05-18T02:33:18Z"},{"alias_kind":"arxiv_version","alias_value":"1006.0546v1","created_at":"2026-05-18T02:33:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.0546","created_at":"2026-05-18T02:33:18Z"},{"alias_kind":"pith_short_12","alias_value":"UJEL7CN5HKSR","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"UJEL7CN5HKSRSK5X","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"UJEL7CN5","created_at":"2026-05-18T12:26:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:UJEL7CN5HKSRSK5XGOW7CTDDA3","target":"record","payload":{"canonical_record":{"source":{"id":"1006.0546","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-06-03T03:01:06Z","cross_cats_sorted":["astro-ph.IM","physics.data-an"],"title_canon_sha256":"f98fe52168e803142fbaa5ea4a09193d0af61daf3312930536d74cfb3a3cf493","abstract_canon_sha256":"e469f80832ae895bdcfb65288aa8106721b7e1bba198c1e6b1abbe8a3db69f63"},"schema_version":"1.0"},"canonical_sha256":"a248bf89bd3aa5192bb733adf14c6306cda128f42fb5815b712bc3c04a0993bd","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:33:18.123499Z","signature_b64":"XFmzGPdJOEnetNLbzamzGCpAqIfsbH3XyBdwRYBrwNv7ssTc1ahQMeJJ20E9HH8zG8c1Y2lOdbALsWJcwqWXCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a248bf89bd3aa5192bb733adf14c6306cda128f42fb5815b712bc3c04a0993bd","last_reissued_at":"2026-05-18T02:33:18.122842Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:33:18.122842Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1006.0546","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:33:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"q9w2ar4I9Sa/lDMdA0eJiOHNK1fafqshY8iAdCEklyTEjmqzE7ojXkDiu7KEzNvbt/k1nNUfmJUabqWbAy9XDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T00:14:08.440233Z"},"content_sha256":"f16a9f745138ea24b3ba66c4f097554915cbb277ea9497570f50ab71ff15d8f5","schema_version":"1.0","event_id":"sha256:f16a9f745138ea24b3ba66c4f097554915cbb277ea9497570f50ab71ff15d8f5"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:UJEL7CN5HKSRSK5XGOW7CTDDA3","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"False-alarm probability in relation to over-sampled power spectra, with application to Super-Kamiokande solar neutrino data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM","physics.data-an"],"primary_cat":"hep-ph","authors_text":"Jeffrey D. Scargle, Peter A. Sturrock","submitted_at":"2010-06-03T03:01:06Z","abstract_excerpt":"The term \"false-alarm probability\" denotes the probability that at least one out of M independent power values in a prescribed search band of a power spectrum computed from a white-noise time series is expected to be as large as or larger than a given value. The usual formula is based on the assumption that powers are distributed exponentially, as one expects for power measurements of normally distributed random noise. However, in practice one typically examines peaks in an over-sampled power spectrum. It is therefore more appropriate to compare the strength of a particular peak with the distr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.0546","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:33:18Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SM2uNBXYrdOM9uKqwg57IyXRQtp/cdGkb4gUz+Vy1FTiqs+GC/iz/mdWKuoRzbczY2GoYoKXd3AJQHknr7ONBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T00:14:08.440868Z"},"content_sha256":"c1df2f8ea9fff6518223fd971788e0614df46aa726934ae77d2bb2afb0b74881","schema_version":"1.0","event_id":"sha256:c1df2f8ea9fff6518223fd971788e0614df46aa726934ae77d2bb2afb0b74881"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3/bundle.json","state_url":"https://pith.science/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-31T00:14:08Z","links":{"resolver":"https://pith.science/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3","bundle":"https://pith.science/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3/bundle.json","state":"https://pith.science/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3/state.json","well_known_bundle":"https://pith.science/.well-known/pith/UJEL7CN5HKSRSK5XGOW7CTDDA3/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:UJEL7CN5HKSRSK5XGOW7CTDDA3","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"e469f80832ae895bdcfb65288aa8106721b7e1bba198c1e6b1abbe8a3db69f63","cross_cats_sorted":["astro-ph.IM","physics.data-an"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-06-03T03:01:06Z","title_canon_sha256":"f98fe52168e803142fbaa5ea4a09193d0af61daf3312930536d74cfb3a3cf493"},"schema_version":"1.0","source":{"id":"1006.0546","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.0546","created_at":"2026-05-18T02:33:18Z"},{"alias_kind":"arxiv_version","alias_value":"1006.0546v1","created_at":"2026-05-18T02:33:18Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.0546","created_at":"2026-05-18T02:33:18Z"},{"alias_kind":"pith_short_12","alias_value":"UJEL7CN5HKSR","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"UJEL7CN5HKSRSK5X","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"UJEL7CN5","created_at":"2026-05-18T12:26:15Z"}],"graph_snapshots":[{"event_id":"sha256:c1df2f8ea9fff6518223fd971788e0614df46aa726934ae77d2bb2afb0b74881","target":"graph","created_at":"2026-05-18T02:33:18Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"The term \"false-alarm probability\" denotes the probability that at least one out of M independent power values in a prescribed search band of a power spectrum computed from a white-noise time series is expected to be as large as or larger than a given value. The usual formula is based on the assumption that powers are distributed exponentially, as one expects for power measurements of normally distributed random noise. However, in practice one typically examines peaks in an over-sampled power spectrum. It is therefore more appropriate to compare the strength of a particular peak with the distr","authors_text":"Jeffrey D. Scargle, Peter A. Sturrock","cross_cats":["astro-ph.IM","physics.data-an"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-06-03T03:01:06Z","title":"False-alarm probability in relation to over-sampled power spectra, with application to Super-Kamiokande solar neutrino data"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.0546","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:f16a9f745138ea24b3ba66c4f097554915cbb277ea9497570f50ab71ff15d8f5","target":"record","created_at":"2026-05-18T02:33:18Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"e469f80832ae895bdcfb65288aa8106721b7e1bba198c1e6b1abbe8a3db69f63","cross_cats_sorted":["astro-ph.IM","physics.data-an"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-06-03T03:01:06Z","title_canon_sha256":"f98fe52168e803142fbaa5ea4a09193d0af61daf3312930536d74cfb3a3cf493"},"schema_version":"1.0","source":{"id":"1006.0546","kind":"arxiv","version":1}},"canonical_sha256":"a248bf89bd3aa5192bb733adf14c6306cda128f42fb5815b712bc3c04a0993bd","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a248bf89bd3aa5192bb733adf14c6306cda128f42fb5815b712bc3c04a0993bd","first_computed_at":"2026-05-18T02:33:18.122842Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:33:18.122842Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"XFmzGPdJOEnetNLbzamzGCpAqIfsbH3XyBdwRYBrwNv7ssTc1ahQMeJJ20E9HH8zG8c1Y2lOdbALsWJcwqWXCw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:33:18.123499Z","signed_message":"canonical_sha256_bytes"},"source_id":"1006.0546","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:f16a9f745138ea24b3ba66c4f097554915cbb277ea9497570f50ab71ff15d8f5","sha256:c1df2f8ea9fff6518223fd971788e0614df46aa726934ae77d2bb2afb0b74881"],"state_sha256":"0b7130f1ebcdcd5c9cc94a18c9683d6f661d425b7b961da15cc6fac28abe67c4"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"cjNZIB4JpoKZyOj7fz6tyNn0iL490WUSCbsffEDY9MXx6ztDOf8plkUSXjTuL7+jbgp7tXadFF8RuxacYlKEAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T00:14:08.444427Z","bundle_sha256":"ed944b34d7e242dfdd53c7b1fc9256e3459a55a993e8adc64436eab223e820f4"}}