{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:LK7OAHNAICDTUKZPZXILQ4T7HZ","short_pith_number":"pith:LK7OAHNA","schema_version":"1.0","canonical_sha256":"5abee01da040873a2b2fcdd0b8727f3e6395e8f80cef354732c9ca4d112f3170","source":{"kind":"arxiv","id":"0906.4803","version":1},"attestation_state":"computed","paper":{"title":"High-energy emission from jet-clump interactions in microquasars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Anabella T. Araudo, Gustavo E. Romero, Valenti Bosch-Ramon","submitted_at":"2009-06-25T21:26:36Z","abstract_excerpt":"High-mass microquasars are binary systems consisting of a massive star and an accreting compact object from which relativistic jets are launched. There is considerable observational evidence that winds of massive stars are clumpy. Individual clumps may interact with the jets in high-mass microquasars to produce outbursts of high-energy emission. Gamma-ray flares have been detected in some high-mass X-ray binaries, such as Cygnus X-1, and probably in LS 5039 and LS I+61 303. We predict the high-energy emission produced by the interaction between a jet and a clump of the stellar wind in a high-m"},"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":"0906.4803","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-06-25T21:26:36Z","cross_cats_sorted":[],"title_canon_sha256":"0148d2a40192ba81cb9b1f5c563ceeee3219ffedfb5783006897737db2bde37d","abstract_canon_sha256":"28cd8cf93200b709754c220d7e5d18d96ca7305a725487739f535365a10cda29"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:12.602994Z","signature_b64":"k+c99STgg/h5Pxx9/bYkWsXbmcGMIWVDILCTS5pzG/xwLZ47eZwltgyTzf+0DZJXlKVYK+MhlpNU0942hQm5Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5abee01da040873a2b2fcdd0b8727f3e6395e8f80cef354732c9ca4d112f3170","last_reissued_at":"2026-05-18T02:13:12.602514Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:12.602514Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"High-energy emission from jet-clump interactions in microquasars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Anabella T. Araudo, Gustavo E. Romero, Valenti Bosch-Ramon","submitted_at":"2009-06-25T21:26:36Z","abstract_excerpt":"High-mass microquasars are binary systems consisting of a massive star and an accreting compact object from which relativistic jets are launched. There is considerable observational evidence that winds of massive stars are clumpy. Individual clumps may interact with the jets in high-mass microquasars to produce outbursts of high-energy emission. Gamma-ray flares have been detected in some high-mass X-ray binaries, such as Cygnus X-1, and probably in LS 5039 and LS I+61 303. We predict the high-energy emission produced by the interaction between a jet and a clump of the stellar wind in a high-m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0906.4803","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":"0906.4803","created_at":"2026-05-18T02:13:12.602588+00:00"},{"alias_kind":"arxiv_version","alias_value":"0906.4803v1","created_at":"2026-05-18T02:13:12.602588+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0906.4803","created_at":"2026-05-18T02:13:12.602588+00:00"},{"alias_kind":"pith_short_12","alias_value":"LK7OAHNAICDT","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_16","alias_value":"LK7OAHNAICDTUKZP","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_8","alias_value":"LK7OAHNA","created_at":"2026-05-18T12:26:00.592388+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/LK7OAHNAICDTUKZPZXILQ4T7HZ","json":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ.json","graph_json":"https://pith.science/api/pith-number/LK7OAHNAICDTUKZPZXILQ4T7HZ/graph.json","events_json":"https://pith.science/api/pith-number/LK7OAHNAICDTUKZPZXILQ4T7HZ/events.json","paper":"https://pith.science/paper/LK7OAHNA"},"agent_actions":{"view_html":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ","download_json":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ.json","view_paper":"https://pith.science/paper/LK7OAHNA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0906.4803&json=true","fetch_graph":"https://pith.science/api/pith-number/LK7OAHNAICDTUKZPZXILQ4T7HZ/graph.json","fetch_events":"https://pith.science/api/pith-number/LK7OAHNAICDTUKZPZXILQ4T7HZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ/action/storage_attestation","attest_author":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ/action/author_attestation","sign_citation":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ/action/citation_signature","submit_replication":"https://pith.science/pith/LK7OAHNAICDTUKZPZXILQ4T7HZ/action/replication_record"}},"created_at":"2026-05-18T02:13:12.602588+00:00","updated_at":"2026-05-18T02:13:12.602588+00:00"}