{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:QP5L2ZZMDA2VJXWPKVUAXRLCCV","short_pith_number":"pith:QP5L2ZZM","schema_version":"1.0","canonical_sha256":"83fabd672c183554decf55680bc5621571fe75267294ad3c3270f75fe65c5046","source":{"kind":"arxiv","id":"1801.09381","version":1},"attestation_state":"computed","paper":{"title":"Fermi-LAT Observation of Non-Blazar AGNs","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":"2018-01-29T07:34:54Z","abstract_excerpt":"We report on a detailed investigation of the $\\gamma$-ray emission from 26 non-blazar AGNs based on the Fermi LAT data accumulated for 7 years. The photon index of non-blazar AGNs changes in the range of 1.84-2.86 and the flux varies from a few times $10^{-9} photon\\: cm^{-2} s^{-1}$ to $10^{-7} photon\\: cm^{-2}s^{-1}$. Over long time periods, power-law provides an adequate description of the $\\gamma$-ray spectra of almost all sources. Significant curvature is observed in the $\\gamma$-ray spectra of NGC 1275, NGC 6251, SBS 0846+513 and PMN J0948+0022 and their spectra are better described by l"},"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":"1801.09381","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-01-29T07:34:54Z","cross_cats_sorted":[],"title_canon_sha256":"60aaa6294a5178e253309fb1e3c24541d0648903b562622ee6e27d89741a4aed","abstract_canon_sha256":"e62b4cf211fda15079325c165e0398e76932e2e860fb2fc7861a92e4b0bcc92d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:14:08.777145Z","signature_b64":"gfQ+oeqfo8dxSufVpyW2ZlqEEuu8QGpdJujT+AeMATcC7fI7nfjv54j7hOhoKZoSHbEd5g1wH3laBz/KnUisDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"83fabd672c183554decf55680bc5621571fe75267294ad3c3270f75fe65c5046","last_reissued_at":"2026-05-18T00:14:08.776538Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:14:08.776538Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermi-LAT Observation of Non-Blazar AGNs","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":"2018-01-29T07:34:54Z","abstract_excerpt":"We report on a detailed investigation of the $\\gamma$-ray emission from 26 non-blazar AGNs based on the Fermi LAT data accumulated for 7 years. The photon index of non-blazar AGNs changes in the range of 1.84-2.86 and the flux varies from a few times $10^{-9} photon\\: cm^{-2} s^{-1}$ to $10^{-7} photon\\: cm^{-2}s^{-1}$. Over long time periods, power-law provides an adequate description of the $\\gamma$-ray spectra of almost all sources. Significant curvature is observed in the $\\gamma$-ray spectra of NGC 1275, NGC 6251, SBS 0846+513 and PMN J0948+0022 and their spectra are better described by l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.09381","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":"1801.09381","created_at":"2026-05-18T00:14:08.776623+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.09381v1","created_at":"2026-05-18T00:14:08.776623+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.09381","created_at":"2026-05-18T00:14:08.776623+00:00"},{"alias_kind":"pith_short_12","alias_value":"QP5L2ZZMDA2V","created_at":"2026-05-18T12:32:46.962924+00:00"},{"alias_kind":"pith_short_16","alias_value":"QP5L2ZZMDA2VJXWP","created_at":"2026-05-18T12:32:46.962924+00:00"},{"alias_kind":"pith_short_8","alias_value":"QP5L2ZZM","created_at":"2026-05-18T12:32:46.962924+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/QP5L2ZZMDA2VJXWPKVUAXRLCCV","json":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV.json","graph_json":"https://pith.science/api/pith-number/QP5L2ZZMDA2VJXWPKVUAXRLCCV/graph.json","events_json":"https://pith.science/api/pith-number/QP5L2ZZMDA2VJXWPKVUAXRLCCV/events.json","paper":"https://pith.science/paper/QP5L2ZZM"},"agent_actions":{"view_html":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV","download_json":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV.json","view_paper":"https://pith.science/paper/QP5L2ZZM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.09381&json=true","fetch_graph":"https://pith.science/api/pith-number/QP5L2ZZMDA2VJXWPKVUAXRLCCV/graph.json","fetch_events":"https://pith.science/api/pith-number/QP5L2ZZMDA2VJXWPKVUAXRLCCV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV/action/storage_attestation","attest_author":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV/action/author_attestation","sign_citation":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV/action/citation_signature","submit_replication":"https://pith.science/pith/QP5L2ZZMDA2VJXWPKVUAXRLCCV/action/replication_record"}},"created_at":"2026-05-18T00:14:08.776623+00:00","updated_at":"2026-05-18T00:14:08.776623+00:00"}