{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:5HJJA4L6YFQXDDSPGXRIGAWMRJ","short_pith_number":"pith:5HJJA4L6","canonical_record":{"source":{"id":"1701.05028","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-18T12:15:02Z","cross_cats_sorted":[],"title_canon_sha256":"d94e75361d6070dcbe8bd1f570fdae288c46551ba7531459ba2e704e593a94c3","abstract_canon_sha256":"985386821e17922ffe9d6cb740f0564602d8a6417a76659975777bb5b91bcdf1"},"schema_version":"1.0"},"canonical_sha256":"e9d290717ec161718e4f35e28302cc8a68b791e51c5f68485bf4adddbc22e0a5","source":{"kind":"arxiv","id":"1701.05028","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.05028","created_at":"2026-05-18T00:38:30Z"},{"alias_kind":"arxiv_version","alias_value":"1701.05028v1","created_at":"2026-05-18T00:38:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.05028","created_at":"2026-05-18T00:38:30Z"},{"alias_kind":"pith_short_12","alias_value":"5HJJA4L6YFQX","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_16","alias_value":"5HJJA4L6YFQXDDSP","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_8","alias_value":"5HJJA4L6","created_at":"2026-05-18T12:31:00Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:5HJJA4L6YFQXDDSPGXRIGAWMRJ","target":"record","payload":{"canonical_record":{"source":{"id":"1701.05028","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-18T12:15:02Z","cross_cats_sorted":[],"title_canon_sha256":"d94e75361d6070dcbe8bd1f570fdae288c46551ba7531459ba2e704e593a94c3","abstract_canon_sha256":"985386821e17922ffe9d6cb740f0564602d8a6417a76659975777bb5b91bcdf1"},"schema_version":"1.0"},"canonical_sha256":"e9d290717ec161718e4f35e28302cc8a68b791e51c5f68485bf4adddbc22e0a5","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:30.511993Z","signature_b64":"Vc7PTDbDEw8KnwbA+F2hv4hZHlDNX8CtRqc5030oML9Rjb8oBoNWTwp10beLBW3uh9ceDpYF1FONb7FSKcSUBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e9d290717ec161718e4f35e28302cc8a68b791e51c5f68485bf4adddbc22e0a5","last_reissued_at":"2026-05-18T00:38:30.511296Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:30.511296Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1701.05028","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:38:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"zekAUAQMDckajX6wDE01J4GnJxE0XqUbIZW0T6H4eFON0Tvhnxzv/WEI+d538kc9Yq9O6NV8ajE9+Rdcm5KdDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T05:14:26.223409Z"},"content_sha256":"515642f9f27e2cb37cd69bf38243ae0a3bbb6c5293caa142ced3f2c102ee0d38","schema_version":"1.0","event_id":"sha256:515642f9f27e2cb37cd69bf38243ae0a3bbb6c5293caa142ced3f2c102ee0d38"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:5HJJA4L6YFQXDDSPGXRIGAWMRJ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Gamma rays from clumpy wind-jet interactions in high-mass microquasars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D. Khangulyan, G. E. Romero, S. del Palacio, V. Bosch-Ramon, V. M. de la Cita, X. Paredes-Fortuny","submitted_at":"2017-01-18T12:15:02Z","abstract_excerpt":"The stellar winds of the massive stars in high-mass microquasars are thought to be inhomogeneous. The interaction of these inhomogeneities, or clumps, with the jets of these objects may be a major factor in gamma-ray production. Our goal is to characterize a typical scenario of clump-jet interaction, and calculate the contribution of these interactions to the gamma-ray emission from these systems. We use axisymmetric, RHD simulations to model the emitting flow in a typical clump-jet interaction. Using the simulation results we perform a numerical calculation of the high-energy emission from on"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.05028","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:38:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Yh4tDO3YOMNrtwePOU8CZrFoNpw3FWKGu4hW18OR+E+6ui26UXehvAoeCkRxzEmC+q91ohlG/xvwlCeY0HDtCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T05:14:26.223791Z"},"content_sha256":"41d79977cc4fe123ec44aac2ed919210eef4a9c02ff1179bc0fe8f8df8723f3f","schema_version":"1.0","event_id":"sha256:41d79977cc4fe123ec44aac2ed919210eef4a9c02ff1179bc0fe8f8df8723f3f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ/bundle.json","state_url":"https://pith.science/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-26T05:14:26Z","links":{"resolver":"https://pith.science/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ","bundle":"https://pith.science/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ/bundle.json","state":"https://pith.science/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/5HJJA4L6YFQXDDSPGXRIGAWMRJ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:5HJJA4L6YFQXDDSPGXRIGAWMRJ","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"985386821e17922ffe9d6cb740f0564602d8a6417a76659975777bb5b91bcdf1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-18T12:15:02Z","title_canon_sha256":"d94e75361d6070dcbe8bd1f570fdae288c46551ba7531459ba2e704e593a94c3"},"schema_version":"1.0","source":{"id":"1701.05028","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.05028","created_at":"2026-05-18T00:38:30Z"},{"alias_kind":"arxiv_version","alias_value":"1701.05028v1","created_at":"2026-05-18T00:38:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.05028","created_at":"2026-05-18T00:38:30Z"},{"alias_kind":"pith_short_12","alias_value":"5HJJA4L6YFQX","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_16","alias_value":"5HJJA4L6YFQXDDSP","created_at":"2026-05-18T12:31:00Z"},{"alias_kind":"pith_short_8","alias_value":"5HJJA4L6","created_at":"2026-05-18T12:31:00Z"}],"graph_snapshots":[{"event_id":"sha256:41d79977cc4fe123ec44aac2ed919210eef4a9c02ff1179bc0fe8f8df8723f3f","target":"graph","created_at":"2026-05-18T00:38:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"The stellar winds of the massive stars in high-mass microquasars are thought to be inhomogeneous. The interaction of these inhomogeneities, or clumps, with the jets of these objects may be a major factor in gamma-ray production. Our goal is to characterize a typical scenario of clump-jet interaction, and calculate the contribution of these interactions to the gamma-ray emission from these systems. We use axisymmetric, RHD simulations to model the emitting flow in a typical clump-jet interaction. Using the simulation results we perform a numerical calculation of the high-energy emission from on","authors_text":"D. Khangulyan, G. E. Romero, S. del Palacio, V. Bosch-Ramon, V. M. de la Cita, X. Paredes-Fortuny","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-18T12:15:02Z","title":"Gamma rays from clumpy wind-jet interactions in high-mass microquasars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.05028","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:515642f9f27e2cb37cd69bf38243ae0a3bbb6c5293caa142ced3f2c102ee0d38","target":"record","created_at":"2026-05-18T00:38:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"985386821e17922ffe9d6cb740f0564602d8a6417a76659975777bb5b91bcdf1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-18T12:15:02Z","title_canon_sha256":"d94e75361d6070dcbe8bd1f570fdae288c46551ba7531459ba2e704e593a94c3"},"schema_version":"1.0","source":{"id":"1701.05028","kind":"arxiv","version":1}},"canonical_sha256":"e9d290717ec161718e4f35e28302cc8a68b791e51c5f68485bf4adddbc22e0a5","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e9d290717ec161718e4f35e28302cc8a68b791e51c5f68485bf4adddbc22e0a5","first_computed_at":"2026-05-18T00:38:30.511296Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:38:30.511296Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Vc7PTDbDEw8KnwbA+F2hv4hZHlDNX8CtRqc5030oML9Rjb8oBoNWTwp10beLBW3uh9ceDpYF1FONb7FSKcSUBg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:38:30.511993Z","signed_message":"canonical_sha256_bytes"},"source_id":"1701.05028","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:515642f9f27e2cb37cd69bf38243ae0a3bbb6c5293caa142ced3f2c102ee0d38","sha256:41d79977cc4fe123ec44aac2ed919210eef4a9c02ff1179bc0fe8f8df8723f3f"],"state_sha256":"d6463f93012444e8f4d1b00584cd097c8a523370405e9eb0a03369f45af636ce"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Z03NA7+oqK743LOxU81KTh+62g2GCkcQDm0GMSUucEbG5bBBfuYpycDag+08jfxLK3Ezx/Xh8PMLLbfJ5GvrBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T05:14:26.226079Z","bundle_sha256":"da9c6d876bc6c0909956eb77c6f5bb79484358711fbf52f4529baa58b06640a0"}}