{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:H7RFG7HH32YWJAY6UL3CEAHKJS","short_pith_number":"pith:H7RFG7HH","schema_version":"1.0","canonical_sha256":"3fe2537ce7deb164831ea2f62200ea4c8f3228f0080c4c9f156f4873de15522e","source":{"kind":"arxiv","id":"1304.0605","version":1},"attestation_state":"computed","paper":{"title":"Leptonic and Hadronic Modeling of Fermi-Detected Blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Prakash (Ohio University), A. Reimer (University of Innsbruck, Austria), K. Sweeney (Ohio University), M. Boettcher (NWU Potchefstroom, South Africa)","submitted_at":"2013-04-02T12:07:29Z","abstract_excerpt":"We describe new implementations of leptonic and hadronic models for the broadband emission from relativistic jets in AGN in a temporary steady state. For the leptonic model, a temporary equilibrium between particle injection/acceleration, radiative cooling, and escape from a spherical emission region is evaluated, and the self-consistent radiative output is calculated. For the hadronic model, a temporary equilibrium between particle injection/acceleration, radiative and adiabatic cooling, and escape is evaluated for both primary electrons and protons. A new, semi-analytical method to evaluate "},"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":"1304.0605","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-04-02T12:07:29Z","cross_cats_sorted":[],"title_canon_sha256":"3d20ede8215996745c1b238c049e83a3d26ae83d02f53e119a7fd77c5158c9e9","abstract_canon_sha256":"a10e1a0a4858e8927b019f1363e708457e47529d9521575d76fb7c2ec790be7b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:50.075340Z","signature_b64":"xXGv36tMfkryRKK25+74V4A0ZBkYa4+mRCyqpzPS+myMvgCfCOTsr6dBp6ilbu6BA1dUaD3CwBJjhPfYWlp5Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3fe2537ce7deb164831ea2f62200ea4c8f3228f0080c4c9f156f4873de15522e","last_reissued_at":"2026-05-18T01:50:50.074666Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:50.074666Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Leptonic and Hadronic Modeling of Fermi-Detected Blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Prakash (Ohio University), A. Reimer (University of Innsbruck, Austria), K. Sweeney (Ohio University), M. Boettcher (NWU Potchefstroom, South Africa)","submitted_at":"2013-04-02T12:07:29Z","abstract_excerpt":"We describe new implementations of leptonic and hadronic models for the broadband emission from relativistic jets in AGN in a temporary steady state. For the leptonic model, a temporary equilibrium between particle injection/acceleration, radiative cooling, and escape from a spherical emission region is evaluated, and the self-consistent radiative output is calculated. For the hadronic model, a temporary equilibrium between particle injection/acceleration, radiative and adiabatic cooling, and escape is evaluated for both primary electrons and protons. A new, semi-analytical method to evaluate "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.0605","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":"1304.0605","created_at":"2026-05-18T01:50:50.074786+00:00"},{"alias_kind":"arxiv_version","alias_value":"1304.0605v1","created_at":"2026-05-18T01:50:50.074786+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.0605","created_at":"2026-05-18T01:50:50.074786+00:00"},{"alias_kind":"pith_short_12","alias_value":"H7RFG7HH32YW","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"H7RFG7HH32YWJAY6","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"H7RFG7HH","created_at":"2026-05-18T12:27:46.883200+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2605.21320","citing_title":"FR0 radio galaxy jets -- I. linking jet dynamics and high-energy emission in LEDA 55267 and LEDA 58287","ref_index":20,"is_internal_anchor":true},{"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":168,"is_internal_anchor":true},{"citing_arxiv_id":"2601.11203","citing_title":"Little Red Dots as Hidden Neutrino Sources","ref_index":88,"is_internal_anchor":true},{"citing_arxiv_id":"2605.12602","citing_title":"Tracking down the broadband polarimetric properties of PG 1553+113","ref_index":182,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS","json":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS.json","graph_json":"https://pith.science/api/pith-number/H7RFG7HH32YWJAY6UL3CEAHKJS/graph.json","events_json":"https://pith.science/api/pith-number/H7RFG7HH32YWJAY6UL3CEAHKJS/events.json","paper":"https://pith.science/paper/H7RFG7HH"},"agent_actions":{"view_html":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS","download_json":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS.json","view_paper":"https://pith.science/paper/H7RFG7HH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1304.0605&json=true","fetch_graph":"https://pith.science/api/pith-number/H7RFG7HH32YWJAY6UL3CEAHKJS/graph.json","fetch_events":"https://pith.science/api/pith-number/H7RFG7HH32YWJAY6UL3CEAHKJS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS/action/storage_attestation","attest_author":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS/action/author_attestation","sign_citation":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS/action/citation_signature","submit_replication":"https://pith.science/pith/H7RFG7HH32YWJAY6UL3CEAHKJS/action/replication_record"}},"created_at":"2026-05-18T01:50:50.074786+00:00","updated_at":"2026-05-18T01:50:50.074786+00:00"}