{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:7H5POTVS66GNKKCAPAXXB3O4D5","short_pith_number":"pith:7H5POTVS","schema_version":"1.0","canonical_sha256":"f9faf74eb2f78cd52840782f70eddc1f50a4a07894309bc8b7e1c39bc7630bd6","source":{"kind":"arxiv","id":"2203.07956","version":1},"attestation_state":"computed","paper":{"title":"ExHaLe-jet: An extended hadro-leptonic jet model for blazars. I. Code description and initial results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Andreas Zech, Anita Reimer, Catherine Boisson, Michael Zacharias","submitted_at":"2022-03-15T14:39:14Z","abstract_excerpt":"The processes operating in blazar jets are still an open question. Modeling the radiation emanating from an extended part of the jet allows one to capture these processes on all scales. Kinetic codes solving the Fokker-Planck equation along the jet flow are well suited to this task, as they can efficiently derive the radiation and particle spectra without the need for computationally demanding plasma-physical simulations. Here, we present a new extended hadro-leptonic jet code -- ExHaLe-jet -- which considers simultaneously the processes of relativistic protons and electrons. Within a pre-set "},"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":"2203.07956","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-03-15T14:39:14Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"3bfc3c160423dfd37c52a6c71dd784444bb1827d3c7aeb6152f236cf4f153ef4","abstract_canon_sha256":"dbc4dda82e234abeefa99c585930fe8e706787b629593a8728c4f242e51b7bc6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:12:39.147873Z","signature_b64":"Cyzu7Hnnd0VAT1/6lDUb9eyTqmu8b1g1Xo3xurDi/R1hoR0+T/uKP8xhyJu7RZ4ut5lGU31XhMsIKaUp1fbjAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f9faf74eb2f78cd52840782f70eddc1f50a4a07894309bc8b7e1c39bc7630bd6","last_reissued_at":"2026-07-05T04:12:39.147488Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:12:39.147488Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ExHaLe-jet: An extended hadro-leptonic jet model for blazars. I. Code description and initial results","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Andreas Zech, Anita Reimer, Catherine Boisson, Michael Zacharias","submitted_at":"2022-03-15T14:39:14Z","abstract_excerpt":"The processes operating in blazar jets are still an open question. Modeling the radiation emanating from an extended part of the jet allows one to capture these processes on all scales. Kinetic codes solving the Fokker-Planck equation along the jet flow are well suited to this task, as they can efficiently derive the radiation and particle spectra without the need for computationally demanding plasma-physical simulations. Here, we present a new extended hadro-leptonic jet code -- ExHaLe-jet -- which considers simultaneously the processes of relativistic protons and electrons. Within a pre-set "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.07956","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2203.07956/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2203.07956","created_at":"2026-07-05T04:12:39.147543+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.07956v1","created_at":"2026-07-05T04:12:39.147543+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.07956","created_at":"2026-07-05T04:12:39.147543+00:00"},{"alias_kind":"pith_short_12","alias_value":"7H5POTVS66GN","created_at":"2026-07-05T04:12:39.147543+00:00"},{"alias_kind":"pith_short_16","alias_value":"7H5POTVS66GNKKCA","created_at":"2026-07-05T04:12:39.147543+00:00"},{"alias_kind":"pith_short_8","alias_value":"7H5POTVS","created_at":"2026-07-05T04:12:39.147543+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.12696","citing_title":"An Evolving Leptonic Jet Model for Delayed Radio Flares in Neutrino Blazars","ref_index":45,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5","json":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5.json","graph_json":"https://pith.science/api/pith-number/7H5POTVS66GNKKCAPAXXB3O4D5/graph.json","events_json":"https://pith.science/api/pith-number/7H5POTVS66GNKKCAPAXXB3O4D5/events.json","paper":"https://pith.science/paper/7H5POTVS"},"agent_actions":{"view_html":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5","download_json":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5.json","view_paper":"https://pith.science/paper/7H5POTVS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.07956&json=true","fetch_graph":"https://pith.science/api/pith-number/7H5POTVS66GNKKCAPAXXB3O4D5/graph.json","fetch_events":"https://pith.science/api/pith-number/7H5POTVS66GNKKCAPAXXB3O4D5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5/action/storage_attestation","attest_author":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5/action/author_attestation","sign_citation":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5/action/citation_signature","submit_replication":"https://pith.science/pith/7H5POTVS66GNKKCAPAXXB3O4D5/action/replication_record"}},"created_at":"2026-07-05T04:12:39.147543+00:00","updated_at":"2026-07-05T04:12:39.147543+00:00"}