{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:3QFW4SCFUJKDPQ5MF6CPEHVG5K","short_pith_number":"pith:3QFW4SCF","schema_version":"1.0","canonical_sha256":"dc0b6e4845a25437c3ac2f84f21ea6eaa5660e2d850313392463e07038c95424","source":{"kind":"arxiv","id":"1311.7647","version":1},"attestation_state":"computed","paper":{"title":"Jet Emission in Young Radio Sources: a Fermi-LAT Gamma-ray View","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Aneta Siemiginowska, Annalisa Celotti, Brandon C. Kelly, Giulia Migliori, Lukasz Stawarz, Mitchell C. Begelman","submitted_at":"2013-11-29T17:56:09Z","abstract_excerpt":"We investigate the contribution of the beamed jet component to the high energy emission in young and compact extragalactic radio sources, focusing for the first time on the gamma-ray band. We derive predictions on the gamma-ray luminosities associated with the relativistic jet assuming a leptonic radiative model. The high energy emission is produced via Compton scattering by the relativistic electrons in a spherical region at the considered scales ($\\lesssim$10 kpc). Simulations show a wide range of gamma-ray luminosities, with intensities up to $\\sim10^{46}-10^{48}$ erg s$^{-1}$ depending on "},"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":"1311.7647","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-11-29T17:56:09Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"1acaa61a28eb0baa22d3cc448cc77a9cffc15860ab6723a78e3e2d759f9b8911","abstract_canon_sha256":"d1069d0777596e8b318a0a4f9c5d394d1e4abc0f420d3e2a00cb64ce6c85529b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:04.732435Z","signature_b64":"rN3QGMUY/mxLpN0cy6ecx6+KHMTwtAHNk/DttcuuqNTV+u68r37bEfJg/g/Vx9jVrgLclpkDteNbPnkTO9KTDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dc0b6e4845a25437c3ac2f84f21ea6eaa5660e2d850313392463e07038c95424","last_reissued_at":"2026-05-18T01:46:04.731904Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:04.731904Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Jet Emission in Young Radio Sources: a Fermi-LAT Gamma-ray View","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Aneta Siemiginowska, Annalisa Celotti, Brandon C. Kelly, Giulia Migliori, Lukasz Stawarz, Mitchell C. Begelman","submitted_at":"2013-11-29T17:56:09Z","abstract_excerpt":"We investigate the contribution of the beamed jet component to the high energy emission in young and compact extragalactic radio sources, focusing for the first time on the gamma-ray band. We derive predictions on the gamma-ray luminosities associated with the relativistic jet assuming a leptonic radiative model. The high energy emission is produced via Compton scattering by the relativistic electrons in a spherical region at the considered scales ($\\lesssim$10 kpc). Simulations show a wide range of gamma-ray luminosities, with intensities up to $\\sim10^{46}-10^{48}$ erg s$^{-1}$ depending on "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1311.7647","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":"1311.7647","created_at":"2026-05-18T01:46:04.731978+00:00"},{"alias_kind":"arxiv_version","alias_value":"1311.7647v1","created_at":"2026-05-18T01:46:04.731978+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1311.7647","created_at":"2026-05-18T01:46:04.731978+00:00"},{"alias_kind":"pith_short_12","alias_value":"3QFW4SCFUJKD","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"3QFW4SCFUJKDPQ5M","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"3QFW4SCF","created_at":"2026-05-18T12:27:32.513160+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/3QFW4SCFUJKDPQ5MF6CPEHVG5K","json":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K.json","graph_json":"https://pith.science/api/pith-number/3QFW4SCFUJKDPQ5MF6CPEHVG5K/graph.json","events_json":"https://pith.science/api/pith-number/3QFW4SCFUJKDPQ5MF6CPEHVG5K/events.json","paper":"https://pith.science/paper/3QFW4SCF"},"agent_actions":{"view_html":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K","download_json":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K.json","view_paper":"https://pith.science/paper/3QFW4SCF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1311.7647&json=true","fetch_graph":"https://pith.science/api/pith-number/3QFW4SCFUJKDPQ5MF6CPEHVG5K/graph.json","fetch_events":"https://pith.science/api/pith-number/3QFW4SCFUJKDPQ5MF6CPEHVG5K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K/action/storage_attestation","attest_author":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K/action/author_attestation","sign_citation":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K/action/citation_signature","submit_replication":"https://pith.science/pith/3QFW4SCFUJKDPQ5MF6CPEHVG5K/action/replication_record"}},"created_at":"2026-05-18T01:46:04.731978+00:00","updated_at":"2026-05-18T01:46:04.731978+00:00"}