{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:PVGEXN4KKH3AHVCUWIQJDCCDJ7","short_pith_number":"pith:PVGEXN4K","schema_version":"1.0","canonical_sha256":"7d4c4bb78a51f603d454b2209188434fdb5c8ba2502a37898ba3e04d5c903894","source":{"kind":"arxiv","id":"1312.2470","version":1},"attestation_state":"computed","paper":{"title":"Dynamical and radiative simulations of $\\gamma$-ray jets in microquasars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"T.S. Kosmas, T. Smponias","submitted_at":"2013-12-09T15:35:57Z","abstract_excerpt":"The emission of $\\gamma$-rays in jets emanating from the vicinity of collapsed stellar remnants, in binary systems known as microquasars, is investigated using a three dimensional relativistic hydrocode (PLUTO), in combination with two in-house radiative transfer codes. Even though a great number of stellar systems may be addressed by such models, we restrict ourselves to the concrete example of the SS433 X-ray binary, the only microquasar with a definite hadronic content in its jets, as verified from spectral line observations. A variety of system configurations have been examined, by employi"},"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":"1312.2470","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-12-09T15:35:57Z","cross_cats_sorted":[],"title_canon_sha256":"80d084b92f2df30a3759d60ca0c17587a529887b406b4a38db5c30c198ea0db4","abstract_canon_sha256":"b3e4b5eaa73000d82384b376f7a769147929547e9b26a9dcc514f535b194d9ef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:45:57.148414Z","signature_b64":"1KxA42GzF53BJA0cisHPDxI3Bh6xsEYZ80cwXwYnxrdyvizyfy2+2HvP6+QuYTMgDf6xeBUMPl+Cvoeqy1p2AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7d4c4bb78a51f603d454b2209188434fdb5c8ba2502a37898ba3e04d5c903894","last_reissued_at":"2026-05-18T01:45:57.147787Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:45:57.147787Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamical and radiative simulations of $\\gamma$-ray jets in microquasars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"T.S. Kosmas, T. Smponias","submitted_at":"2013-12-09T15:35:57Z","abstract_excerpt":"The emission of $\\gamma$-rays in jets emanating from the vicinity of collapsed stellar remnants, in binary systems known as microquasars, is investigated using a three dimensional relativistic hydrocode (PLUTO), in combination with two in-house radiative transfer codes. Even though a great number of stellar systems may be addressed by such models, we restrict ourselves to the concrete example of the SS433 X-ray binary, the only microquasar with a definite hadronic content in its jets, as verified from spectral line observations. A variety of system configurations have been examined, by employi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.2470","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":"1312.2470","created_at":"2026-05-18T01:45:57.147877+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.2470v1","created_at":"2026-05-18T01:45:57.147877+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.2470","created_at":"2026-05-18T01:45:57.147877+00:00"},{"alias_kind":"pith_short_12","alias_value":"PVGEXN4KKH3A","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_16","alias_value":"PVGEXN4KKH3AHVCU","created_at":"2026-05-18T12:27:57.521954+00:00"},{"alias_kind":"pith_short_8","alias_value":"PVGEXN4K","created_at":"2026-05-18T12:27:57.521954+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/PVGEXN4KKH3AHVCUWIQJDCCDJ7","json":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7.json","graph_json":"https://pith.science/api/pith-number/PVGEXN4KKH3AHVCUWIQJDCCDJ7/graph.json","events_json":"https://pith.science/api/pith-number/PVGEXN4KKH3AHVCUWIQJDCCDJ7/events.json","paper":"https://pith.science/paper/PVGEXN4K"},"agent_actions":{"view_html":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7","download_json":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7.json","view_paper":"https://pith.science/paper/PVGEXN4K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.2470&json=true","fetch_graph":"https://pith.science/api/pith-number/PVGEXN4KKH3AHVCUWIQJDCCDJ7/graph.json","fetch_events":"https://pith.science/api/pith-number/PVGEXN4KKH3AHVCUWIQJDCCDJ7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7/action/storage_attestation","attest_author":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7/action/author_attestation","sign_citation":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7/action/citation_signature","submit_replication":"https://pith.science/pith/PVGEXN4KKH3AHVCUWIQJDCCDJ7/action/replication_record"}},"created_at":"2026-05-18T01:45:57.147877+00:00","updated_at":"2026-05-18T01:45:57.147877+00:00"}