{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:VXAXESR2QTLZEGXGCVMAGKDJBU","short_pith_number":"pith:VXAXESR2","canonical_record":{"source":{"id":"1701.06173","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-22T15:14:43Z","cross_cats_sorted":[],"title_canon_sha256":"5e2284263e8c63a0402af40fb1c0699cd63173b43182fd444c259db80f51e40f","abstract_canon_sha256":"9eb65b8b45c59614695d8f4c728b58e3b649f2508ff692dd3ed6a47ed4e7013d"},"schema_version":"1.0"},"canonical_sha256":"adc1724a3a84d7921ae615580328690d3af23611b309a253308a9f3a6a98b63a","source":{"kind":"arxiv","id":"1701.06173","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.06173","created_at":"2026-05-18T00:51:11Z"},{"alias_kind":"arxiv_version","alias_value":"1701.06173v1","created_at":"2026-05-18T00:51:11Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.06173","created_at":"2026-05-18T00:51:11Z"},{"alias_kind":"pith_short_12","alias_value":"VXAXESR2QTLZ","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_16","alias_value":"VXAXESR2QTLZEGXG","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_8","alias_value":"VXAXESR2","created_at":"2026-05-18T12:31:49Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:VXAXESR2QTLZEGXGCVMAGKDJBU","target":"record","payload":{"canonical_record":{"source":{"id":"1701.06173","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-22T15:14:43Z","cross_cats_sorted":[],"title_canon_sha256":"5e2284263e8c63a0402af40fb1c0699cd63173b43182fd444c259db80f51e40f","abstract_canon_sha256":"9eb65b8b45c59614695d8f4c728b58e3b649f2508ff692dd3ed6a47ed4e7013d"},"schema_version":"1.0"},"canonical_sha256":"adc1724a3a84d7921ae615580328690d3af23611b309a253308a9f3a6a98b63a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:51:11.710151Z","signature_b64":"AjDmZX/jVdri/hf9E6C1gSetOvKH+1AxV4NfSIAuAoRF7gG8X3xKMPWgvhDBSUBzwsD0AC9c24trwlRl2etDBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"adc1724a3a84d7921ae615580328690d3af23611b309a253308a9f3a6a98b63a","last_reissued_at":"2026-05-18T00:51:11.709565Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:51:11.709565Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1701.06173","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":"2026-05-18T00:51:11Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uQ/TvC9hs5g3vHel8b10zfPNtoJdBHWCFieTys5zDhbwf5DZPdfrmXyUxTW2AztmxgFsXiW3bYv6aT3YYtEtBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T19:23:38.516981Z"},"content_sha256":"8553cd92a494f567d9f18825263b207ceb02a7a317b5ad571fe0f3efe1d30693","schema_version":"1.0","event_id":"sha256:8553cd92a494f567d9f18825263b207ceb02a7a317b5ad571fe0f3efe1d30693"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:VXAXESR2QTLZEGXGCVMAGKDJBU","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Modeling the Spectral Energy Distribution of the radio galaxy IC310","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Galvan-Gamez, A. Marinelli, E. Aguilar-Ruiz, N. Fraija","submitted_at":"2017-01-22T15:14:43Z","abstract_excerpt":"The radio galaxy IC310 located in the Perseus Cluster is one of the brightest objects in the radio and X-ray bands, and one of the closest active galactic nuclei observed in very-high energies. In GeV - TeV $\\gamma$-rays, IC310 was detected in low and high flux states by the MAGIC telescopes from October 2009 to February 2010. Taking into account that the spectral energy distribution (SED) up to a few GeV seems to exhibit a double-peak feature and that a single-zone synchrotron self-Compton (SSC) model can explain all of the multiwavelength emission except for the non-simultaneous MAGIC emissi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.06173","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":"2026-05-18T00:51:11Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"tFbFZG2pHT6e6nizJ8OhrN0OZqxaESIOuEeJmjCBCN/CdwbVP7dV3r2pYitZZOxQNhLIg8wLLZOoyfVfa3v8Dg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T19:23:38.517341Z"},"content_sha256":"419328b13e21380c0f0b059d8df688fe3b55d0a23f8672159e0c67bcc6246f98","schema_version":"1.0","event_id":"sha256:419328b13e21380c0f0b059d8df688fe3b55d0a23f8672159e0c67bcc6246f98"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VXAXESR2QTLZEGXGCVMAGKDJBU/bundle.json","state_url":"https://pith.science/pith/VXAXESR2QTLZEGXGCVMAGKDJBU/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VXAXESR2QTLZEGXGCVMAGKDJBU/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":"2026-05-20T19:23:38Z","links":{"resolver":"https://pith.science/pith/VXAXESR2QTLZEGXGCVMAGKDJBU","bundle":"https://pith.science/pith/VXAXESR2QTLZEGXGCVMAGKDJBU/bundle.json","state":"https://pith.science/pith/VXAXESR2QTLZEGXGCVMAGKDJBU/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VXAXESR2QTLZEGXGCVMAGKDJBU/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:VXAXESR2QTLZEGXGCVMAGKDJBU","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":"9eb65b8b45c59614695d8f4c728b58e3b649f2508ff692dd3ed6a47ed4e7013d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-22T15:14:43Z","title_canon_sha256":"5e2284263e8c63a0402af40fb1c0699cd63173b43182fd444c259db80f51e40f"},"schema_version":"1.0","source":{"id":"1701.06173","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.06173","created_at":"2026-05-18T00:51:11Z"},{"alias_kind":"arxiv_version","alias_value":"1701.06173v1","created_at":"2026-05-18T00:51:11Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.06173","created_at":"2026-05-18T00:51:11Z"},{"alias_kind":"pith_short_12","alias_value":"VXAXESR2QTLZ","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_16","alias_value":"VXAXESR2QTLZEGXG","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_8","alias_value":"VXAXESR2","created_at":"2026-05-18T12:31:49Z"}],"graph_snapshots":[{"event_id":"sha256:419328b13e21380c0f0b059d8df688fe3b55d0a23f8672159e0c67bcc6246f98","target":"graph","created_at":"2026-05-18T00:51:11Z","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 radio galaxy IC310 located in the Perseus Cluster is one of the brightest objects in the radio and X-ray bands, and one of the closest active galactic nuclei observed in very-high energies. In GeV - TeV $\\gamma$-rays, IC310 was detected in low and high flux states by the MAGIC telescopes from October 2009 to February 2010. Taking into account that the spectral energy distribution (SED) up to a few GeV seems to exhibit a double-peak feature and that a single-zone synchrotron self-Compton (SSC) model can explain all of the multiwavelength emission except for the non-simultaneous MAGIC emissi","authors_text":"A. Galvan-Gamez, A. Marinelli, E. Aguilar-Ruiz, N. Fraija","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-22T15:14:43Z","title":"Modeling the Spectral Energy Distribution of the radio galaxy IC310"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.06173","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":"sha256:8553cd92a494f567d9f18825263b207ceb02a7a317b5ad571fe0f3efe1d30693","target":"record","created_at":"2026-05-18T00:51:11Z","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":"9eb65b8b45c59614695d8f4c728b58e3b649f2508ff692dd3ed6a47ed4e7013d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-01-22T15:14:43Z","title_canon_sha256":"5e2284263e8c63a0402af40fb1c0699cd63173b43182fd444c259db80f51e40f"},"schema_version":"1.0","source":{"id":"1701.06173","kind":"arxiv","version":1}},"canonical_sha256":"adc1724a3a84d7921ae615580328690d3af23611b309a253308a9f3a6a98b63a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"adc1724a3a84d7921ae615580328690d3af23611b309a253308a9f3a6a98b63a","first_computed_at":"2026-05-18T00:51:11.709565Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:51:11.709565Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"AjDmZX/jVdri/hf9E6C1gSetOvKH+1AxV4NfSIAuAoRF7gG8X3xKMPWgvhDBSUBzwsD0AC9c24trwlRl2etDBw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:51:11.710151Z","signed_message":"canonical_sha256_bytes"},"source_id":"1701.06173","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8553cd92a494f567d9f18825263b207ceb02a7a317b5ad571fe0f3efe1d30693","sha256:419328b13e21380c0f0b059d8df688fe3b55d0a23f8672159e0c67bcc6246f98"],"state_sha256":"834d464af9b4e991bea2f82100a3dbc314bd81ca12ea20d4bdc0d7342b8a5104"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8fWfG9YJ7Kq4lJmn4dpQyGSNLOalfah+eV4ipuGo3d2+wHug96qtNzOWjjNHkKTJgmLLgDFtZQmvqAqPcV+mAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-20T19:23:38.519539Z","bundle_sha256":"24fe0e82ba4bc9d5a0164f8e2fccedb2a1369fd52d5b0814bced53bc7cb62362"}}