{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:KHB4BW5WGRIU4OIPS4ZEFSACTD","short_pith_number":"pith:KHB4BW5W","schema_version":"1.0","canonical_sha256":"51c3c0dbb634514e390f973242c80298fa018e26813b9648b90b9144274372ef","source":{"kind":"arxiv","id":"1804.07341","version":2},"attestation_state":"computed","paper":{"title":"Kinetic \"jets\" from fast moving pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maxim Lyutikov, Maxim V. Barkov, Noel Klingler, Pol Bordas","submitted_at":"2018-04-19T19:13:23Z","abstract_excerpt":"Some fast-moving pulsars, like the Guitar and the Lighthouse, exhibit asymmetric non-thermal emission features that extend well beyond their ram pressure confined pulsar wind nebulae (PWNe). Using 3D relativistic simulations we explain these features as kinetically streaming pulsar wind particles that escaped into the interstellar medium (ISM) due to reconnection between the PWN and ISM magnetic fields. The structure of the reconnecting magnetic fields at the incoming and outgoing regions produce highly asymmetric magnetic bottles, and result in asymmetric extended features. For the features t"},"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":"1804.07341","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-04-19T19:13:23Z","cross_cats_sorted":[],"title_canon_sha256":"e3751c76dc61fbc4f4277dcf311aadb19109624c47af66c0bdbbcb1ed9022788","abstract_canon_sha256":"0d4718796daa5b02d5a4436d50b71978a23e8b68b0daa2c5b8b7c54715299a6d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:07.809058Z","signature_b64":"73vBiF4TMsfZj8ygdQDyKUa5YYdAX/099KASO/R6D0pJSDcV3oZ/uZR9Y5xegaGdDESIJnCymn1DL0Nl6xJVBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"51c3c0dbb634514e390f973242c80298fa018e26813b9648b90b9144274372ef","last_reissued_at":"2026-05-17T23:52:07.808700Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:07.808700Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinetic \"jets\" from fast moving pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Maxim Lyutikov, Maxim V. Barkov, Noel Klingler, Pol Bordas","submitted_at":"2018-04-19T19:13:23Z","abstract_excerpt":"Some fast-moving pulsars, like the Guitar and the Lighthouse, exhibit asymmetric non-thermal emission features that extend well beyond their ram pressure confined pulsar wind nebulae (PWNe). Using 3D relativistic simulations we explain these features as kinetically streaming pulsar wind particles that escaped into the interstellar medium (ISM) due to reconnection between the PWN and ISM magnetic fields. The structure of the reconnecting magnetic fields at the incoming and outgoing regions produce highly asymmetric magnetic bottles, and result in asymmetric extended features. For the features t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.07341","kind":"arxiv","version":2},"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":"1804.07341","created_at":"2026-05-17T23:52:07.808758+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.07341v2","created_at":"2026-05-17T23:52:07.808758+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.07341","created_at":"2026-05-17T23:52:07.808758+00:00"},{"alias_kind":"pith_short_12","alias_value":"KHB4BW5WGRIU","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_16","alias_value":"KHB4BW5WGRIU4OIP","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_8","alias_value":"KHB4BW5W","created_at":"2026-05-18T12:32:33.847187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.13697","citing_title":"Guitar Nebula: extreme accelerator in extreme environment","ref_index":86,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD","json":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD.json","graph_json":"https://pith.science/api/pith-number/KHB4BW5WGRIU4OIPS4ZEFSACTD/graph.json","events_json":"https://pith.science/api/pith-number/KHB4BW5WGRIU4OIPS4ZEFSACTD/events.json","paper":"https://pith.science/paper/KHB4BW5W"},"agent_actions":{"view_html":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD","download_json":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD.json","view_paper":"https://pith.science/paper/KHB4BW5W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.07341&json=true","fetch_graph":"https://pith.science/api/pith-number/KHB4BW5WGRIU4OIPS4ZEFSACTD/graph.json","fetch_events":"https://pith.science/api/pith-number/KHB4BW5WGRIU4OIPS4ZEFSACTD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD/action/storage_attestation","attest_author":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD/action/author_attestation","sign_citation":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD/action/citation_signature","submit_replication":"https://pith.science/pith/KHB4BW5WGRIU4OIPS4ZEFSACTD/action/replication_record"}},"created_at":"2026-05-17T23:52:07.808758+00:00","updated_at":"2026-05-17T23:52:07.808758+00:00"}