{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:WBCL7N2AQXBSCH7OMOOADJ3563","short_pith_number":"pith:WBCL7N2A","schema_version":"1.0","canonical_sha256":"b044bfb74085c3211fee639c01a77df6f11f6c4bc338d4d493dfeeefb0aba761","source":{"kind":"arxiv","id":"1210.8370","version":1},"attestation_state":"computed","paper":{"title":"Non-thermal emission from Pulsar-Wind Nebulae in Starburst Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jim Hinton, Stefan Ohm","submitted_at":"2012-10-31T15:40:31Z","abstract_excerpt":"The recently detected gamma-ray emission from Starburst galaxies is most commonly considered to be diffuse emission arising from strong interactions of accelerated cosmic rays. Mannheim et al. (2012), however, have argued that a population of individual pulsar-wind nebulae (PWNe) could be responsible for the detected TeV emission. Here we show that the Starburst environment plays a critical role in the TeV emission from Starburst PWNe, and perform the first detailed calculations for this scenario. Our approach is based on the measured star-formation rates in the Starburst nuclei of NGC 253 and"},"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":"1210.8370","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-10-31T15:40:31Z","cross_cats_sorted":[],"title_canon_sha256":"8d082ef39b18515ffcca519c48e2d91243fa62b34a710ab9d82b741a7054ff7d","abstract_canon_sha256":"2e5dfdeb9d02ea662f4c6ac6fc4788f6e2e902d5232552614912e17dc023b1f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:53:28.762255Z","signature_b64":"0CPcblHKwANzFgzNX0JcNN22gg8AQcMsN3Myza0eJARZSiD/L5b4vM7EmIYvjsiMLmEXabHsTCuRW4ZGQRQiBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b044bfb74085c3211fee639c01a77df6f11f6c4bc338d4d493dfeeefb0aba761","last_reissued_at":"2026-05-18T01:53:28.761708Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:53:28.761708Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-thermal emission from Pulsar-Wind Nebulae in Starburst Galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Jim Hinton, Stefan Ohm","submitted_at":"2012-10-31T15:40:31Z","abstract_excerpt":"The recently detected gamma-ray emission from Starburst galaxies is most commonly considered to be diffuse emission arising from strong interactions of accelerated cosmic rays. Mannheim et al. (2012), however, have argued that a population of individual pulsar-wind nebulae (PWNe) could be responsible for the detected TeV emission. Here we show that the Starburst environment plays a critical role in the TeV emission from Starburst PWNe, and perform the first detailed calculations for this scenario. Our approach is based on the measured star-formation rates in the Starburst nuclei of NGC 253 and"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.8370","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":"1210.8370","created_at":"2026-05-18T01:53:28.761802+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.8370v1","created_at":"2026-05-18T01:53:28.761802+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.8370","created_at":"2026-05-18T01:53:28.761802+00:00"},{"alias_kind":"pith_short_12","alias_value":"WBCL7N2AQXBS","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_16","alias_value":"WBCL7N2AQXBSCH7O","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_8","alias_value":"WBCL7N2A","created_at":"2026-05-18T12:27:25.539911+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/WBCL7N2AQXBSCH7OMOOADJ3563","json":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563.json","graph_json":"https://pith.science/api/pith-number/WBCL7N2AQXBSCH7OMOOADJ3563/graph.json","events_json":"https://pith.science/api/pith-number/WBCL7N2AQXBSCH7OMOOADJ3563/events.json","paper":"https://pith.science/paper/WBCL7N2A"},"agent_actions":{"view_html":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563","download_json":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563.json","view_paper":"https://pith.science/paper/WBCL7N2A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.8370&json=true","fetch_graph":"https://pith.science/api/pith-number/WBCL7N2AQXBSCH7OMOOADJ3563/graph.json","fetch_events":"https://pith.science/api/pith-number/WBCL7N2AQXBSCH7OMOOADJ3563/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563/action/storage_attestation","attest_author":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563/action/author_attestation","sign_citation":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563/action/citation_signature","submit_replication":"https://pith.science/pith/WBCL7N2AQXBSCH7OMOOADJ3563/action/replication_record"}},"created_at":"2026-05-18T01:53:28.761802+00:00","updated_at":"2026-05-18T01:53:28.761802+00:00"}