{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:ST3MYXZ6EW4OZAVNBQJQSU2K6M","short_pith_number":"pith:ST3MYXZ6","schema_version":"1.0","canonical_sha256":"94f6cc5f3e25b8ec82ad0c1309534af32d7f433cff1ae667d0df89878d8c801e","source":{"kind":"arxiv","id":"1403.4170","version":1},"attestation_state":"computed","paper":{"title":"Detection of significant cm to sub-mm band radio and gamma-ray correlated variability in Fermi bright blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. C. S. Readhead, A. Sievers, E. Angelakis, H. Ungerechts, I. Nestoras, J. A. Zensus, J. Chiang, L. Fuhrmann, S. Larsson, T. J. Pearson, T. P. Krichbaum, V. Pavlidou, W. Max-Moerbeck","submitted_at":"2014-03-17T17:05:08Z","abstract_excerpt":"The exact location of the gamma-ray emitting region in blazars is still controversial. In order to attack this problem we present first results of a cross-correlation analysis between radio (11 cm to 0.8 mm wavelength, F-GAMMA program) and gamma-ray (0.1-300 GeV) ~ 3.5 year light curves of 54 Fermi-bright blazars. We perform a source stacking analysis and estimate significances and chance correlations using mixed source correlations. Our results reveal: (i) the first highly significant multi-band radio and gamma-ray correlations (radio lagging gamma rays) when averaging over the whole sample, "},"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":"1403.4170","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-03-17T17:05:08Z","cross_cats_sorted":[],"title_canon_sha256":"7cc8b587ca525efb5ba80af1d3b283acd67df90a048506c7ce410bf50ac6871b","abstract_canon_sha256":"9cd568f27c44d9437c086c807e628ec17025b4c07fff60b656cef90f1d82f92c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:44:00.417863Z","signature_b64":"To75PSK+LDqVQCuyZJv1CC9l9CHesBBKm3sltIyese2wCy0a89/J0QX7XqoVGrfBHX0b3KxryddT0xE/XxqTDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"94f6cc5f3e25b8ec82ad0c1309534af32d7f433cff1ae667d0df89878d8c801e","last_reissued_at":"2026-05-18T01:44:00.417334Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:44:00.417334Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of significant cm to sub-mm band radio and gamma-ray correlated variability in Fermi bright blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. C. S. Readhead, A. Sievers, E. Angelakis, H. Ungerechts, I. Nestoras, J. A. Zensus, J. Chiang, L. Fuhrmann, S. Larsson, T. J. Pearson, T. P. Krichbaum, V. Pavlidou, W. Max-Moerbeck","submitted_at":"2014-03-17T17:05:08Z","abstract_excerpt":"The exact location of the gamma-ray emitting region in blazars is still controversial. In order to attack this problem we present first results of a cross-correlation analysis between radio (11 cm to 0.8 mm wavelength, F-GAMMA program) and gamma-ray (0.1-300 GeV) ~ 3.5 year light curves of 54 Fermi-bright blazars. We perform a source stacking analysis and estimate significances and chance correlations using mixed source correlations. Our results reveal: (i) the first highly significant multi-band radio and gamma-ray correlations (radio lagging gamma rays) when averaging over the whole sample, "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.4170","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":"1403.4170","created_at":"2026-05-18T01:44:00.417407+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.4170v1","created_at":"2026-05-18T01:44:00.417407+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.4170","created_at":"2026-05-18T01:44:00.417407+00:00"},{"alias_kind":"pith_short_12","alias_value":"ST3MYXZ6EW4O","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_16","alias_value":"ST3MYXZ6EW4OZAVN","created_at":"2026-05-18T12:28:49.207871+00:00"},{"alias_kind":"pith_short_8","alias_value":"ST3MYXZ6","created_at":"2026-05-18T12:28:49.207871+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/ST3MYXZ6EW4OZAVNBQJQSU2K6M","json":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M.json","graph_json":"https://pith.science/api/pith-number/ST3MYXZ6EW4OZAVNBQJQSU2K6M/graph.json","events_json":"https://pith.science/api/pith-number/ST3MYXZ6EW4OZAVNBQJQSU2K6M/events.json","paper":"https://pith.science/paper/ST3MYXZ6"},"agent_actions":{"view_html":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M","download_json":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M.json","view_paper":"https://pith.science/paper/ST3MYXZ6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.4170&json=true","fetch_graph":"https://pith.science/api/pith-number/ST3MYXZ6EW4OZAVNBQJQSU2K6M/graph.json","fetch_events":"https://pith.science/api/pith-number/ST3MYXZ6EW4OZAVNBQJQSU2K6M/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M/action/storage_attestation","attest_author":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M/action/author_attestation","sign_citation":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M/action/citation_signature","submit_replication":"https://pith.science/pith/ST3MYXZ6EW4OZAVNBQJQSU2K6M/action/replication_record"}},"created_at":"2026-05-18T01:44:00.417407+00:00","updated_at":"2026-05-18T01:44:00.417407+00:00"}