{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:RCN2GOXCFPPZKJAZ6V6VALNQGJ","short_pith_number":"pith:RCN2GOXC","canonical_record":{"source":{"id":"1002.1563","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-02-08T10:15:19Z","cross_cats_sorted":[],"title_canon_sha256":"4975e607afb9bfc6caff1b53e96562087cb443591bee987a2e68654b981ef27d","abstract_canon_sha256":"5b68e80abdcca5eee090933e4c259165a4444c6d7f59a3f1d781e5c9f80a1bf9"},"schema_version":"1.0"},"canonical_sha256":"889ba33ae22bdf952419f57d502db03255274dd1471ccc8d81e8db251973b454","source":{"kind":"arxiv","id":"1002.1563","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1002.1563","created_at":"2026-05-18T02:09:11Z"},{"alias_kind":"arxiv_version","alias_value":"1002.1563v2","created_at":"2026-05-18T02:09:11Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.1563","created_at":"2026-05-18T02:09:11Z"},{"alias_kind":"pith_short_12","alias_value":"RCN2GOXCFPPZ","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_16","alias_value":"RCN2GOXCFPPZKJAZ","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_8","alias_value":"RCN2GOXC","created_at":"2026-05-18T12:26:13Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:RCN2GOXCFPPZKJAZ6V6VALNQGJ","target":"record","payload":{"canonical_record":{"source":{"id":"1002.1563","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-02-08T10:15:19Z","cross_cats_sorted":[],"title_canon_sha256":"4975e607afb9bfc6caff1b53e96562087cb443591bee987a2e68654b981ef27d","abstract_canon_sha256":"5b68e80abdcca5eee090933e4c259165a4444c6d7f59a3f1d781e5c9f80a1bf9"},"schema_version":"1.0"},"canonical_sha256":"889ba33ae22bdf952419f57d502db03255274dd1471ccc8d81e8db251973b454","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:09:11.390680Z","signature_b64":"12rxSapM0AKFHvRLC12UvM42/ctuiEPQgeanXYmcqzwTXdl64/WcPny1mKEvahQ9QNHAdtJLLjjwWg4MQYd1Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"889ba33ae22bdf952419f57d502db03255274dd1471ccc8d81e8db251973b454","last_reissued_at":"2026-05-18T02:09:11.390171Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:09:11.390171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1002.1563","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:09:11Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"b10vYfc8GBPmz9Z51Ul2OiUqYIVj9CciAoQedZ+weesu51hK3w8RLDfcNZO2gYbU4UtA4ryRe/1URNOgbtyaAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-09T19:09:24.826455Z"},"content_sha256":"6f96ca8ea1d421d23dd3f9b4c5ed1538b3d7270573553f8ff91e7564d266b10e","schema_version":"1.0","event_id":"sha256:6f96ca8ea1d421d23dd3f9b4c5ed1538b3d7270573553f8ff91e7564d266b10e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:RCN2GOXCFPPZKJAZ6V6VALNQGJ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"On the possibility of sub-TeV Gamma-ray emission from Cyg X-3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"W. Bednarek","submitted_at":"2010-02-08T10:15:19Z","abstract_excerpt":"The compact X-ray binary system Cyg X-3 has been recently discovered as a source of GeV gamma-rays by the AGILE and the {\\it Fermi} satellites. It shows emission features in the GeV gamma-rays similar to other gamma-ray binaries which were also observed in the TeV gamma-rays (LS 5039 and LSI +61 303). The question appears whether Cyg X-3 can be also detected in the TeV gamma-rays by the Cherenkov telescopes.\n  Here we discuss this problem in detail based on the anisotropic inverse Compton (IC) e-p pair cascade model successfully applied to TeV gamma-ray binaries. We calculate the gamma-ray lig"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.1563","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:09:11Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UR9vP4JGHs07iQtEut/UDVlkJGlib8AK4ALx5KrkaKb2ioZkp5YUULPa7TcwUG98zgYaab8UFb91xJSx9KZSCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-09T19:09:24.827110Z"},"content_sha256":"c6b6e8c6b676af090ed2d4f52721fdccc4b1c1853c34091de91be6c7fcc6b5a6","schema_version":"1.0","event_id":"sha256:c6b6e8c6b676af090ed2d4f52721fdccc4b1c1853c34091de91be6c7fcc6b5a6"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ/bundle.json","state_url":"https://pith.science/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ/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":"2026-06-09T19:09:24Z","links":{"resolver":"https://pith.science/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ","bundle":"https://pith.science/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ/bundle.json","state":"https://pith.science/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/RCN2GOXCFPPZKJAZ6V6VALNQGJ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:RCN2GOXCFPPZKJAZ6V6VALNQGJ","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":"5b68e80abdcca5eee090933e4c259165a4444c6d7f59a3f1d781e5c9f80a1bf9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-02-08T10:15:19Z","title_canon_sha256":"4975e607afb9bfc6caff1b53e96562087cb443591bee987a2e68654b981ef27d"},"schema_version":"1.0","source":{"id":"1002.1563","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1002.1563","created_at":"2026-05-18T02:09:11Z"},{"alias_kind":"arxiv_version","alias_value":"1002.1563v2","created_at":"2026-05-18T02:09:11Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1002.1563","created_at":"2026-05-18T02:09:11Z"},{"alias_kind":"pith_short_12","alias_value":"RCN2GOXCFPPZ","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_16","alias_value":"RCN2GOXCFPPZKJAZ","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_8","alias_value":"RCN2GOXC","created_at":"2026-05-18T12:26:13Z"}],"graph_snapshots":[{"event_id":"sha256:c6b6e8c6b676af090ed2d4f52721fdccc4b1c1853c34091de91be6c7fcc6b5a6","target":"graph","created_at":"2026-05-18T02:09:11Z","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 compact X-ray binary system Cyg X-3 has been recently discovered as a source of GeV gamma-rays by the AGILE and the {\\it Fermi} satellites. It shows emission features in the GeV gamma-rays similar to other gamma-ray binaries which were also observed in the TeV gamma-rays (LS 5039 and LSI +61 303). The question appears whether Cyg X-3 can be also detected in the TeV gamma-rays by the Cherenkov telescopes.\n  Here we discuss this problem in detail based on the anisotropic inverse Compton (IC) e-p pair cascade model successfully applied to TeV gamma-ray binaries. We calculate the gamma-ray lig","authors_text":"W. Bednarek","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-02-08T10:15:19Z","title":"On the possibility of sub-TeV Gamma-ray emission from Cyg X-3"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1002.1563","kind":"arxiv","version":2},"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":"sha256:6f96ca8ea1d421d23dd3f9b4c5ed1538b3d7270573553f8ff91e7564d266b10e","target":"record","created_at":"2026-05-18T02:09:11Z","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":"5b68e80abdcca5eee090933e4c259165a4444c6d7f59a3f1d781e5c9f80a1bf9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-02-08T10:15:19Z","title_canon_sha256":"4975e607afb9bfc6caff1b53e96562087cb443591bee987a2e68654b981ef27d"},"schema_version":"1.0","source":{"id":"1002.1563","kind":"arxiv","version":2}},"canonical_sha256":"889ba33ae22bdf952419f57d502db03255274dd1471ccc8d81e8db251973b454","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"889ba33ae22bdf952419f57d502db03255274dd1471ccc8d81e8db251973b454","first_computed_at":"2026-05-18T02:09:11.390171Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:09:11.390171Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"12rxSapM0AKFHvRLC12UvM42/ctuiEPQgeanXYmcqzwTXdl64/WcPny1mKEvahQ9QNHAdtJLLjjwWg4MQYd1Ag==","signature_status":"signed_v1","signed_at":"2026-05-18T02:09:11.390680Z","signed_message":"canonical_sha256_bytes"},"source_id":"1002.1563","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:6f96ca8ea1d421d23dd3f9b4c5ed1538b3d7270573553f8ff91e7564d266b10e","sha256:c6b6e8c6b676af090ed2d4f52721fdccc4b1c1853c34091de91be6c7fcc6b5a6"],"state_sha256":"1ad77fc76e287b8195f517f8a4e32183f398599aa6158348db64e343f78a9275"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DtIZGDTRwiEzvDafBVzYLRFv0CBElGY9fiVpbz4PnPvYHLci9iqUwejdKIiEJ2+XelxHE4v0EA1mGkrsaMceCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-09T19:09:24.831378Z","bundle_sha256":"804b36d9d84632a8143fe71147e3342264694dfa5ae69d4245475752301c65c2"}}