{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:UU2XDRWSY2OSPBOF6ZA3IAXLPI","short_pith_number":"pith:UU2XDRWS","schema_version":"1.0","canonical_sha256":"a53571c6d2c69d2785c5f641b402eb7a2e7ab79b65011d4f491dfd91c761e82a","source":{"kind":"arxiv","id":"1603.07386","version":1},"attestation_state":"computed","paper":{"title":"Time-Dependent Electron Acceleration in Blazar Transients: X-Ray Time Lags and Spectral Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Justin D. Finke, Peter A. Becker, Tiffany R. Lewis","submitted_at":"2016-03-23T23:04:46Z","abstract_excerpt":"Electromagnetic radiation from blazar jets often displays strong variability, extending from radio to $\\gamma$-ray frequencies. In a few cases, this variability has been characterized using Fourier time lags, such as those detected in the X-rays from Mrk~421 using BeppoSAX. The lack of a theoretical framework to interpret the data has motivated us to develop a new model for the formation of the X-ray spectrum and the time lags in blazar jets based on a transport equation including terms describing stochastic Fermi acceleration, synchrotron losses, shock acceleration, adiabatic expansion, and s"},"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":"1603.07386","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-03-23T23:04:46Z","cross_cats_sorted":[],"title_canon_sha256":"885654ab0ee019b648d1804c874a24049bd3c20a15881553ba5949fade003b2b","abstract_canon_sha256":"18f5c469d07d728d26cf6734213855cb98b5f35f8efac53f4d8d97cd573b0a25"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:11:48.289272Z","signature_b64":"/1+nUE0+CcbLKEZ/6RzhH2iw+c2L1xrMGNgPWeCf2IM8CscYtWJ52T4t52mZtCClfHf/oqV7VPiU2wNuCTqFDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a53571c6d2c69d2785c5f641b402eb7a2e7ab79b65011d4f491dfd91c761e82a","last_reissued_at":"2026-05-18T01:11:48.288904Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:11:48.288904Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Time-Dependent Electron Acceleration in Blazar Transients: X-Ray Time Lags and Spectral Formation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Justin D. Finke, Peter A. Becker, Tiffany R. Lewis","submitted_at":"2016-03-23T23:04:46Z","abstract_excerpt":"Electromagnetic radiation from blazar jets often displays strong variability, extending from radio to $\\gamma$-ray frequencies. In a few cases, this variability has been characterized using Fourier time lags, such as those detected in the X-rays from Mrk~421 using BeppoSAX. The lack of a theoretical framework to interpret the data has motivated us to develop a new model for the formation of the X-ray spectrum and the time lags in blazar jets based on a transport equation including terms describing stochastic Fermi acceleration, synchrotron losses, shock acceleration, adiabatic expansion, and s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.07386","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":"1603.07386","created_at":"2026-05-18T01:11:48.288968+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.07386v1","created_at":"2026-05-18T01:11:48.288968+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.07386","created_at":"2026-05-18T01:11:48.288968+00:00"},{"alias_kind":"pith_short_12","alias_value":"UU2XDRWSY2OS","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"UU2XDRWSY2OSPBOF","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"UU2XDRWS","created_at":"2026-05-18T12:30:46.583412+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.15867","citing_title":"Spectral-Regime Overlap and Transition-like Behavior in the Blazar Population from Multi-Instrument X-ray and TeV Observations","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI","json":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI.json","graph_json":"https://pith.science/api/pith-number/UU2XDRWSY2OSPBOF6ZA3IAXLPI/graph.json","events_json":"https://pith.science/api/pith-number/UU2XDRWSY2OSPBOF6ZA3IAXLPI/events.json","paper":"https://pith.science/paper/UU2XDRWS"},"agent_actions":{"view_html":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI","download_json":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI.json","view_paper":"https://pith.science/paper/UU2XDRWS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.07386&json=true","fetch_graph":"https://pith.science/api/pith-number/UU2XDRWSY2OSPBOF6ZA3IAXLPI/graph.json","fetch_events":"https://pith.science/api/pith-number/UU2XDRWSY2OSPBOF6ZA3IAXLPI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI/action/storage_attestation","attest_author":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI/action/author_attestation","sign_citation":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI/action/citation_signature","submit_replication":"https://pith.science/pith/UU2XDRWSY2OSPBOF6ZA3IAXLPI/action/replication_record"}},"created_at":"2026-05-18T01:11:48.288968+00:00","updated_at":"2026-05-18T01:11:48.288968+00:00"}