{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:3MQFTIFAL6IJUUDL6S4GQ4QAUF","short_pith_number":"pith:3MQFTIFA","schema_version":"1.0","canonical_sha256":"db2059a0a05f909a506bf4b8687200a1494a0fa73237c68e6b0b554152adc8e0","source":{"kind":"arxiv","id":"1502.03261","version":1},"attestation_state":"computed","paper":{"title":"Synchrotron Self-Compton Emission by Relativistic Electrons under Stochastic Acceleration: Application to Mrk 421 and Mrk 501","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fumio Takahara, Jun Kakuwa, Katsuaki Asano, Kenji Toma, Masaaki Kusunose","submitted_at":"2015-02-11T11:00:08Z","abstract_excerpt":"We examine the applicability of the stochastic electron acceleration to two high synchrotron peaked blazars, Mrk 421 and Mrk 501, assuming synchrotron self-Compton emission of gamma-rays. Our model considers an emitting region moving at relativistic speed, where non-thermal electrons are accelerated and attain a steady-state energy spectrum together with the photons they emit. The kinetic equations of the electrons and photons are solved numerically, given a stationary wave number spectrum of the magnetohydrodynamic (MHD) disturbances, which are responsible for the electron acceleration and es"},"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":"1502.03261","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-02-11T11:00:08Z","cross_cats_sorted":[],"title_canon_sha256":"763f1b219fc5e0310c15eb5e5c2c9a737016ec6d44966463f7a807c767faa98b","abstract_canon_sha256":"6954207fcf4c409d43b601c4487541499a777f64a89211ff1ba2e547cec23208"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:03.824517Z","signature_b64":"qwd8V5YtTsj7GRY7dpruA58utbctWeC0TltDVYDIcItoFIygj0qg5EfCpa+TNihlUpsMuovbkN9zBRgDWrshCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db2059a0a05f909a506bf4b8687200a1494a0fa73237c68e6b0b554152adc8e0","last_reissued_at":"2026-05-18T01:41:03.823951Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:03.823951Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Synchrotron Self-Compton Emission by Relativistic Electrons under Stochastic Acceleration: Application to Mrk 421 and Mrk 501","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Fumio Takahara, Jun Kakuwa, Katsuaki Asano, Kenji Toma, Masaaki Kusunose","submitted_at":"2015-02-11T11:00:08Z","abstract_excerpt":"We examine the applicability of the stochastic electron acceleration to two high synchrotron peaked blazars, Mrk 421 and Mrk 501, assuming synchrotron self-Compton emission of gamma-rays. Our model considers an emitting region moving at relativistic speed, where non-thermal electrons are accelerated and attain a steady-state energy spectrum together with the photons they emit. The kinetic equations of the electrons and photons are solved numerically, given a stationary wave number spectrum of the magnetohydrodynamic (MHD) disturbances, which are responsible for the electron acceleration and es"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.03261","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":"1502.03261","created_at":"2026-05-18T01:41:03.824040+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.03261v1","created_at":"2026-05-18T01:41:03.824040+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.03261","created_at":"2026-05-18T01:41:03.824040+00:00"},{"alias_kind":"pith_short_12","alias_value":"3MQFTIFAL6IJ","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_16","alias_value":"3MQFTIFAL6IJUUDL","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_8","alias_value":"3MQFTIFA","created_at":"2026-05-18T12:29:02.477457+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/3MQFTIFAL6IJUUDL6S4GQ4QAUF","json":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF.json","graph_json":"https://pith.science/api/pith-number/3MQFTIFAL6IJUUDL6S4GQ4QAUF/graph.json","events_json":"https://pith.science/api/pith-number/3MQFTIFAL6IJUUDL6S4GQ4QAUF/events.json","paper":"https://pith.science/paper/3MQFTIFA"},"agent_actions":{"view_html":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF","download_json":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF.json","view_paper":"https://pith.science/paper/3MQFTIFA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.03261&json=true","fetch_graph":"https://pith.science/api/pith-number/3MQFTIFAL6IJUUDL6S4GQ4QAUF/graph.json","fetch_events":"https://pith.science/api/pith-number/3MQFTIFAL6IJUUDL6S4GQ4QAUF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF/action/storage_attestation","attest_author":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF/action/author_attestation","sign_citation":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF/action/citation_signature","submit_replication":"https://pith.science/pith/3MQFTIFAL6IJUUDL6S4GQ4QAUF/action/replication_record"}},"created_at":"2026-05-18T01:41:03.824040+00:00","updated_at":"2026-05-18T01:41:03.824040+00:00"}