{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:BZOR27VAJ5KAJNC5KMZJ2MFPJO","short_pith_number":"pith:BZOR27VA","canonical_record":{"source":{"id":"1301.6824","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-29T03:25:43Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"f6410dd539a4d59be709ad6b2d0195ed57420da1282bc7a8231f832cef4fb943","abstract_canon_sha256":"888973deafc3992b89b5a7f57f7cddecc7c93fbc43f0d8d4b9cc195243f61c20"},"schema_version":"1.0"},"canonical_sha256":"0e5d1d7ea04f5404b45d53329d30af4bb98ed03c783958fb50f78251f825ca32","source":{"kind":"arxiv","id":"1301.6824","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1301.6824","created_at":"2026-05-18T03:34:47Z"},{"alias_kind":"arxiv_version","alias_value":"1301.6824v2","created_at":"2026-05-18T03:34:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.6824","created_at":"2026-05-18T03:34:47Z"},{"alias_kind":"pith_short_12","alias_value":"BZOR27VAJ5KA","created_at":"2026-05-18T12:27:40Z"},{"alias_kind":"pith_short_16","alias_value":"BZOR27VAJ5KAJNC5","created_at":"2026-05-18T12:27:40Z"},{"alias_kind":"pith_short_8","alias_value":"BZOR27VA","created_at":"2026-05-18T12:27:40Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:BZOR27VAJ5KAJNC5KMZJ2MFPJO","target":"record","payload":{"canonical_record":{"source":{"id":"1301.6824","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-29T03:25:43Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"f6410dd539a4d59be709ad6b2d0195ed57420da1282bc7a8231f832cef4fb943","abstract_canon_sha256":"888973deafc3992b89b5a7f57f7cddecc7c93fbc43f0d8d4b9cc195243f61c20"},"schema_version":"1.0"},"canonical_sha256":"0e5d1d7ea04f5404b45d53329d30af4bb98ed03c783958fb50f78251f825ca32","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:34:47.782814Z","signature_b64":"gMF1y/Cv0EdYI/mbCYxl6BoKActSYHcYOYbwbbxkpzBnisKuv7tgqUhgdE7+AAjPhefscf/vNmEnbtHe/tQLCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0e5d1d7ea04f5404b45d53329d30af4bb98ed03c783958fb50f78251f825ca32","last_reissued_at":"2026-05-18T03:34:47.782107Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:34:47.782107Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1301.6824","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":"2026-05-18T03:34:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"34t/Jd1TRZ2UBoXdAhIEutNvri3ibRXNq/kyB+FR3BdRlBQZQfC+ZTEPkXnu35Dr24diQjuHj1TR7IHuO57cDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T23:32:28.402585Z"},"content_sha256":"a3b0016b2d412fbd39bdd32c50608a004d38b7f1715273632254ae50bb8b444c","schema_version":"1.0","event_id":"sha256:a3b0016b2d412fbd39bdd32c50608a004d38b7f1715273632254ae50bb8b444c"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:BZOR27VAJ5KAJNC5KMZJ2MFPJO","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Exploration of Galactic {\\gamma}-Ray Supernova Remnants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Jianli Zhang, Wenwu Tian","submitted_at":"2013-01-29T03:25:43Z","abstract_excerpt":"New generational very-high-energy telescope arrays have been detecting more than 120 TeV {\\gamma}-ray sources. Multi-wavelength observations on these Gamma-ray sources have proven to be robust in shedding light on their nature. The coming radio telescope arrays like ASKAP and FAST may find more faint (extended) radio sources due to their better sensitivities and resolutions, might identify more previously un-identified {\\gamma}-ray sources and set many new targets for future deep surveys by very-high-energy ground-based telescopes like LHAASO. We in the paper summarize a list of known Galactic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.6824","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":"2026-05-18T03:34:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mD7MRPgeoImSCAXKTmbgotXHLCTMGOE7I6let/vX/hdB052QDgkFqrFGEnT8TU7ufEUYvQSawPo6LSnRD/CLBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T23:32:28.402956Z"},"content_sha256":"6e4ca1d476616e17cdd7d9a3828fe8c3f4bc8a53a5cfabf7432455899b245943","schema_version":"1.0","event_id":"sha256:6e4ca1d476616e17cdd7d9a3828fe8c3f4bc8a53a5cfabf7432455899b245943"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO/bundle.json","state_url":"https://pith.science/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO/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":"2026-06-01T23:32:28Z","links":{"resolver":"https://pith.science/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO","bundle":"https://pith.science/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO/bundle.json","state":"https://pith.science/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO/state.json","well_known_bundle":"https://pith.science/.well-known/pith/BZOR27VAJ5KAJNC5KMZJ2MFPJO/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:BZOR27VAJ5KAJNC5KMZJ2MFPJO","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":"888973deafc3992b89b5a7f57f7cddecc7c93fbc43f0d8d4b9cc195243f61c20","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-29T03:25:43Z","title_canon_sha256":"f6410dd539a4d59be709ad6b2d0195ed57420da1282bc7a8231f832cef4fb943"},"schema_version":"1.0","source":{"id":"1301.6824","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1301.6824","created_at":"2026-05-18T03:34:47Z"},{"alias_kind":"arxiv_version","alias_value":"1301.6824v2","created_at":"2026-05-18T03:34:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.6824","created_at":"2026-05-18T03:34:47Z"},{"alias_kind":"pith_short_12","alias_value":"BZOR27VAJ5KA","created_at":"2026-05-18T12:27:40Z"},{"alias_kind":"pith_short_16","alias_value":"BZOR27VAJ5KAJNC5","created_at":"2026-05-18T12:27:40Z"},{"alias_kind":"pith_short_8","alias_value":"BZOR27VA","created_at":"2026-05-18T12:27:40Z"}],"graph_snapshots":[{"event_id":"sha256:6e4ca1d476616e17cdd7d9a3828fe8c3f4bc8a53a5cfabf7432455899b245943","target":"graph","created_at":"2026-05-18T03:34:47Z","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":"New generational very-high-energy telescope arrays have been detecting more than 120 TeV {\\gamma}-ray sources. Multi-wavelength observations on these Gamma-ray sources have proven to be robust in shedding light on their nature. The coming radio telescope arrays like ASKAP and FAST may find more faint (extended) radio sources due to their better sensitivities and resolutions, might identify more previously un-identified {\\gamma}-ray sources and set many new targets for future deep surveys by very-high-energy ground-based telescopes like LHAASO. We in the paper summarize a list of known Galactic","authors_text":"Jianli Zhang, Wenwu Tian","cross_cats":["astro-ph.GA"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-29T03:25:43Z","title":"Exploration of Galactic {\\gamma}-Ray Supernova Remnants"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.6824","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:a3b0016b2d412fbd39bdd32c50608a004d38b7f1715273632254ae50bb8b444c","target":"record","created_at":"2026-05-18T03:34:47Z","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":"888973deafc3992b89b5a7f57f7cddecc7c93fbc43f0d8d4b9cc195243f61c20","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-29T03:25:43Z","title_canon_sha256":"f6410dd539a4d59be709ad6b2d0195ed57420da1282bc7a8231f832cef4fb943"},"schema_version":"1.0","source":{"id":"1301.6824","kind":"arxiv","version":2}},"canonical_sha256":"0e5d1d7ea04f5404b45d53329d30af4bb98ed03c783958fb50f78251f825ca32","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"0e5d1d7ea04f5404b45d53329d30af4bb98ed03c783958fb50f78251f825ca32","first_computed_at":"2026-05-18T03:34:47.782107Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:34:47.782107Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"gMF1y/Cv0EdYI/mbCYxl6BoKActSYHcYOYbwbbxkpzBnisKuv7tgqUhgdE7+AAjPhefscf/vNmEnbtHe/tQLCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T03:34:47.782814Z","signed_message":"canonical_sha256_bytes"},"source_id":"1301.6824","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:a3b0016b2d412fbd39bdd32c50608a004d38b7f1715273632254ae50bb8b444c","sha256:6e4ca1d476616e17cdd7d9a3828fe8c3f4bc8a53a5cfabf7432455899b245943"],"state_sha256":"c2ceda5a97b6307cf6df6b1b2184d31ba3e2245c5788e86c8df7bb64df652f00"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h99PKyiOFUZRCzi+snjaYR0drlCCgsbDONnfxqu0MXlVdhGQZ6seHbsH+IoahPCw9MZeG214SsnzR6D3S0WbAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T23:32:28.405739Z","bundle_sha256":"528b950128a7a16aad1266363758c1f1077c943b1960169a1ff18f99ac18082b"}}