{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:JVMSZPNDQOXMI2VKOPGZ3LYH53","short_pith_number":"pith:JVMSZPND","schema_version":"1.0","canonical_sha256":"4d592cbda383aec46aaa73cd9daf07eeddd9fe1739088a1c5985d73db18d7850","source":{"kind":"arxiv","id":"1111.0878","version":2},"attestation_state":"computed","paper":{"title":"The gamma-ray emitting region of the jet in Cyg X-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrzej A. Zdziarski, Anna Ogorzalek, Benoit Cerutti, Feng Yuan, Guillaume Dubus, Marek Sikora","submitted_at":"2011-11-03T15:25:13Z","abstract_excerpt":"We study models of the gamma-ray emission of Cyg X-3 observed by Fermi. We calculate the average X-ray spectrum during the gamma-ray active periods. Then, we calculate spectra from Compton scattering of a photon beam into a given direction by isotropic relativistic electrons with a power-law distribution, both based on the Klein-Nishina cross section and in the Thomson limit. Applying the results to scattering of stellar blackbody radiation in the inner jet of Cyg X-3, we find that a low-energy break in the electron distribution at a Lorentz factor of ~ 300--1000 is required by the shape of th"},"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":"1111.0878","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-11-03T15:25:13Z","cross_cats_sorted":[],"title_canon_sha256":"1995770d2c5614a2d860b0b44d438c96f9235537c398655d7309102029d56e4c","abstract_canon_sha256":"535b600c5bf98fe8f4a7f2ab19a556e04a61255469c54cf11161d088c3cb7f9f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:45.964282Z","signature_b64":"cF8QDZOHCLpn/SdW8z+CgXbSKeJq+t/XXXRhKjNoFk1lSZ4VdBl/g6B6SaAVx8169jvRiEMomE3aJVpWi6diBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4d592cbda383aec46aaa73cd9daf07eeddd9fe1739088a1c5985d73db18d7850","last_reissued_at":"2026-05-18T01:59:45.963529Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:45.963529Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The gamma-ray emitting region of the jet in Cyg X-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrzej A. Zdziarski, Anna Ogorzalek, Benoit Cerutti, Feng Yuan, Guillaume Dubus, Marek Sikora","submitted_at":"2011-11-03T15:25:13Z","abstract_excerpt":"We study models of the gamma-ray emission of Cyg X-3 observed by Fermi. We calculate the average X-ray spectrum during the gamma-ray active periods. Then, we calculate spectra from Compton scattering of a photon beam into a given direction by isotropic relativistic electrons with a power-law distribution, both based on the Klein-Nishina cross section and in the Thomson limit. Applying the results to scattering of stellar blackbody radiation in the inner jet of Cyg X-3, we find that a low-energy break in the electron distribution at a Lorentz factor of ~ 300--1000 is required by the shape of th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1111.0878","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":"1111.0878","created_at":"2026-05-18T01:59:45.963658+00:00"},{"alias_kind":"arxiv_version","alias_value":"1111.0878v2","created_at":"2026-05-18T01:59:45.963658+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1111.0878","created_at":"2026-05-18T01:59:45.963658+00:00"},{"alias_kind":"pith_short_12","alias_value":"JVMSZPNDQOXM","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"JVMSZPNDQOXMI2VK","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"JVMSZPND","created_at":"2026-05-18T12:26:32.869790+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.16638","citing_title":"Cygnus X-3: A variable petaelectronvolt gamma-ray source","ref_index":63,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53","json":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53.json","graph_json":"https://pith.science/api/pith-number/JVMSZPNDQOXMI2VKOPGZ3LYH53/graph.json","events_json":"https://pith.science/api/pith-number/JVMSZPNDQOXMI2VKOPGZ3LYH53/events.json","paper":"https://pith.science/paper/JVMSZPND"},"agent_actions":{"view_html":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53","download_json":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53.json","view_paper":"https://pith.science/paper/JVMSZPND","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1111.0878&json=true","fetch_graph":"https://pith.science/api/pith-number/JVMSZPNDQOXMI2VKOPGZ3LYH53/graph.json","fetch_events":"https://pith.science/api/pith-number/JVMSZPNDQOXMI2VKOPGZ3LYH53/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53/action/storage_attestation","attest_author":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53/action/author_attestation","sign_citation":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53/action/citation_signature","submit_replication":"https://pith.science/pith/JVMSZPNDQOXMI2VKOPGZ3LYH53/action/replication_record"}},"created_at":"2026-05-18T01:59:45.963658+00:00","updated_at":"2026-05-18T01:59:45.963658+00:00"}