{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:BGCEND7DY4LXCHRDWOVCOYGGIL","short_pith_number":"pith:BGCEND7D","schema_version":"1.0","canonical_sha256":"0984468fe3c717711e23b3aa2760c642f6de8a7efce1f038f80265c0c4ab1b5d","source":{"kind":"arxiv","id":"1412.3559","version":1},"attestation_state":"computed","paper":{"title":"On the gamma-ray emission from 3C 120","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Zargaryan, N. Sahakyan, V. Baghmanyan","submitted_at":"2014-12-11T07:25:55Z","abstract_excerpt":"We report the analysis of Fermi Large Area Telescope data from five years of observations of the broad line radio galaxy 3C 120. The accumulation of larger data set results in the detection of high-energy $\\gamma$-rays up to 10 GeV, with a detection significance of about $8.7\\sigma$. A power-law spectrum with a photon index of $2.72\\pm0.1$ and integrated flux of $F_{\\gamma}=(2.35\\pm0.5)\\times10^{-8}\\:\\mathrm{photon\\:cm}^{-2}s^{-1}$ above 100 MeV well describe the data averaged over five year observations. The variability analysis of the light curve with 180-, and 365- day bins reveals flux inc"},"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":"1412.3559","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-12-11T07:25:55Z","cross_cats_sorted":[],"title_canon_sha256":"2a776b93069db03016f71ca87b9f008543b34f6dc51a23a1a47b36c71c6546cc","abstract_canon_sha256":"428448b3affb4c65a7bc5d5b7d2f147fcf9fce120e7b64dfec8e9f89836455ae"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:28:04.863306Z","signature_b64":"6GcD3dykJhmeXlPrjdul046Kvn/dxMRrETngz+vUEvwhDxjw7opmlKy6PccUzlaEywvVMbKf7k/J8CZGt6neCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0984468fe3c717711e23b3aa2760c642f6de8a7efce1f038f80265c0c4ab1b5d","last_reissued_at":"2026-05-18T02:28:04.862920Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:28:04.862920Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the gamma-ray emission from 3C 120","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Zargaryan, N. Sahakyan, V. Baghmanyan","submitted_at":"2014-12-11T07:25:55Z","abstract_excerpt":"We report the analysis of Fermi Large Area Telescope data from five years of observations of the broad line radio galaxy 3C 120. The accumulation of larger data set results in the detection of high-energy $\\gamma$-rays up to 10 GeV, with a detection significance of about $8.7\\sigma$. A power-law spectrum with a photon index of $2.72\\pm0.1$ and integrated flux of $F_{\\gamma}=(2.35\\pm0.5)\\times10^{-8}\\:\\mathrm{photon\\:cm}^{-2}s^{-1}$ above 100 MeV well describe the data averaged over five year observations. The variability analysis of the light curve with 180-, and 365- day bins reveals flux inc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.3559","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":"1412.3559","created_at":"2026-05-18T02:28:04.862975+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.3559v1","created_at":"2026-05-18T02:28:04.862975+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.3559","created_at":"2026-05-18T02:28:04.862975+00:00"},{"alias_kind":"pith_short_12","alias_value":"BGCEND7DY4LX","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"BGCEND7DY4LXCHRD","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"BGCEND7D","created_at":"2026-05-18T12:28:22.404517+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/BGCEND7DY4LXCHRDWOVCOYGGIL","json":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL.json","graph_json":"https://pith.science/api/pith-number/BGCEND7DY4LXCHRDWOVCOYGGIL/graph.json","events_json":"https://pith.science/api/pith-number/BGCEND7DY4LXCHRDWOVCOYGGIL/events.json","paper":"https://pith.science/paper/BGCEND7D"},"agent_actions":{"view_html":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL","download_json":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL.json","view_paper":"https://pith.science/paper/BGCEND7D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.3559&json=true","fetch_graph":"https://pith.science/api/pith-number/BGCEND7DY4LXCHRDWOVCOYGGIL/graph.json","fetch_events":"https://pith.science/api/pith-number/BGCEND7DY4LXCHRDWOVCOYGGIL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL/action/storage_attestation","attest_author":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL/action/author_attestation","sign_citation":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL/action/citation_signature","submit_replication":"https://pith.science/pith/BGCEND7DY4LXCHRDWOVCOYGGIL/action/replication_record"}},"created_at":"2026-05-18T02:28:04.862975+00:00","updated_at":"2026-05-18T02:28:04.862975+00:00"}