{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:KYR5QVPKV4HYB54LYIQM5N34WV","short_pith_number":"pith:KYR5QVPK","canonical_record":{"source":{"id":"1501.01010","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-01-05T21:17:27Z","cross_cats_sorted":[],"title_canon_sha256":"9515bb7989a4aa200a6af7767d8522ee2374abd59a85b554ab584f7280ec4e38","abstract_canon_sha256":"b16c9d491ddead69e7ba059fc1973e77e0398fcff0db2b850c3774735e345716"},"schema_version":"1.0"},"canonical_sha256":"5623d855eaaf0f80f78bc220ceb77cb549fac2c715aa43fd04b6819436d993fa","source":{"kind":"arxiv","id":"1501.01010","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1501.01010","created_at":"2026-05-18T01:41:14Z"},{"alias_kind":"arxiv_version","alias_value":"1501.01010v1","created_at":"2026-05-18T01:41:14Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.01010","created_at":"2026-05-18T01:41:14Z"},{"alias_kind":"pith_short_12","alias_value":"KYR5QVPKV4HY","created_at":"2026-05-18T12:29:29Z"},{"alias_kind":"pith_short_16","alias_value":"KYR5QVPKV4HYB54L","created_at":"2026-05-18T12:29:29Z"},{"alias_kind":"pith_short_8","alias_value":"KYR5QVPK","created_at":"2026-05-18T12:29:29Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:KYR5QVPKV4HYB54LYIQM5N34WV","target":"record","payload":{"canonical_record":{"source":{"id":"1501.01010","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-01-05T21:17:27Z","cross_cats_sorted":[],"title_canon_sha256":"9515bb7989a4aa200a6af7767d8522ee2374abd59a85b554ab584f7280ec4e38","abstract_canon_sha256":"b16c9d491ddead69e7ba059fc1973e77e0398fcff0db2b850c3774735e345716"},"schema_version":"1.0"},"canonical_sha256":"5623d855eaaf0f80f78bc220ceb77cb549fac2c715aa43fd04b6819436d993fa","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:14.445345Z","signature_b64":"YOq3MoEevgZ3cLJSaUEaV/Sgaf1Pc8596MrrxVs8rvM47n6o8F+jXz7wMzWcfR+B9csy3hjowgyI2+NuUhPsAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5623d855eaaf0f80f78bc220ceb77cb549fac2c715aa43fd04b6819436d993fa","last_reissued_at":"2026-05-18T01:41:14.444910Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:14.444910Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1501.01010","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":"2026-05-18T01:41:14Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IahbY2aa40p8yqgzSyEH1im3WRRNGjAnQMcRc133QiJzhvLQlFYMZRNg9/D09DyFBEgCmtwpKDaG9zRWG8SZBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-29T16:51:14.626894Z"},"content_sha256":"3b167527d5222c2e4c528bd293a495fda7b4fbbb8ceb5a87abae0c4f4edd30e0","schema_version":"1.0","event_id":"sha256:3b167527d5222c2e4c528bd293a495fda7b4fbbb8ceb5a87abae0c4f4edd30e0"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:KYR5QVPKV4HYB54LYIQM5N34WV","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Jet-ISM Interaction in the Radio Galaxy 3C293: Jet-driven Shocks Heat ISM to Power X-ray and Molecular H2 emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Bjorn Emonts, Daniel Evans, Lauranne Lanz, Patrick M. Ogle, Philip N. Appleton, Pierre Guillard","submitted_at":"2015-01-05T21:17:27Z","abstract_excerpt":"We present a 70ks Chandra observation of the radio galaxy 3C293. This galaxy belongs to the class of molecular hydrogen emission galaxies (MOHEGs) that have very luminous emission from warm molecular hydrogen. In radio galaxies, the molecular gas appears to be heated by jet-driven shocks, but exactly how this mechanism works is still poorly understood. With Chandra, we observe X-ray emission from the jets within the host galaxy and along the 100 kpc radio jets. We model the X-ray spectra of the nucleus, the inner jets, and the X-ray features along the extended radio jets. Both the nucleus and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.01010","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":"2026-05-18T01:41:14Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EpUwG+n2SOCWMIRMj/UXM61tdg+FwJrYL/UsMWjk6dUiVzaH6zgzTnXigZslTkEY/EV3DJWCBJ20wmPzGbJ2CA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-29T16:51:14.627233Z"},"content_sha256":"083d870b8085ede808a58bc813d3c0f056091a8849fadbf87dd7eee291156db7","schema_version":"1.0","event_id":"sha256:083d870b8085ede808a58bc813d3c0f056091a8849fadbf87dd7eee291156db7"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/KYR5QVPKV4HYB54LYIQM5N34WV/bundle.json","state_url":"https://pith.science/pith/KYR5QVPKV4HYB54LYIQM5N34WV/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/KYR5QVPKV4HYB54LYIQM5N34WV/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":"2026-06-29T16:51:14Z","links":{"resolver":"https://pith.science/pith/KYR5QVPKV4HYB54LYIQM5N34WV","bundle":"https://pith.science/pith/KYR5QVPKV4HYB54LYIQM5N34WV/bundle.json","state":"https://pith.science/pith/KYR5QVPKV4HYB54LYIQM5N34WV/state.json","well_known_bundle":"https://pith.science/.well-known/pith/KYR5QVPKV4HYB54LYIQM5N34WV/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:KYR5QVPKV4HYB54LYIQM5N34WV","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":"b16c9d491ddead69e7ba059fc1973e77e0398fcff0db2b850c3774735e345716","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-01-05T21:17:27Z","title_canon_sha256":"9515bb7989a4aa200a6af7767d8522ee2374abd59a85b554ab584f7280ec4e38"},"schema_version":"1.0","source":{"id":"1501.01010","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1501.01010","created_at":"2026-05-18T01:41:14Z"},{"alias_kind":"arxiv_version","alias_value":"1501.01010v1","created_at":"2026-05-18T01:41:14Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.01010","created_at":"2026-05-18T01:41:14Z"},{"alias_kind":"pith_short_12","alias_value":"KYR5QVPKV4HY","created_at":"2026-05-18T12:29:29Z"},{"alias_kind":"pith_short_16","alias_value":"KYR5QVPKV4HYB54L","created_at":"2026-05-18T12:29:29Z"},{"alias_kind":"pith_short_8","alias_value":"KYR5QVPK","created_at":"2026-05-18T12:29:29Z"}],"graph_snapshots":[{"event_id":"sha256:083d870b8085ede808a58bc813d3c0f056091a8849fadbf87dd7eee291156db7","target":"graph","created_at":"2026-05-18T01:41:14Z","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":"We present a 70ks Chandra observation of the radio galaxy 3C293. This galaxy belongs to the class of molecular hydrogen emission galaxies (MOHEGs) that have very luminous emission from warm molecular hydrogen. In radio galaxies, the molecular gas appears to be heated by jet-driven shocks, but exactly how this mechanism works is still poorly understood. With Chandra, we observe X-ray emission from the jets within the host galaxy and along the 100 kpc radio jets. We model the X-ray spectra of the nucleus, the inner jets, and the X-ray features along the extended radio jets. Both the nucleus and ","authors_text":"Bjorn Emonts, Daniel Evans, Lauranne Lanz, Patrick M. Ogle, Philip N. Appleton, Pierre Guillard","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-01-05T21:17:27Z","title":"Jet-ISM Interaction in the Radio Galaxy 3C293: Jet-driven Shocks Heat ISM to Power X-ray and Molecular H2 emission"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.01010","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":"sha256:3b167527d5222c2e4c528bd293a495fda7b4fbbb8ceb5a87abae0c4f4edd30e0","target":"record","created_at":"2026-05-18T01:41:14Z","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":"b16c9d491ddead69e7ba059fc1973e77e0398fcff0db2b850c3774735e345716","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-01-05T21:17:27Z","title_canon_sha256":"9515bb7989a4aa200a6af7767d8522ee2374abd59a85b554ab584f7280ec4e38"},"schema_version":"1.0","source":{"id":"1501.01010","kind":"arxiv","version":1}},"canonical_sha256":"5623d855eaaf0f80f78bc220ceb77cb549fac2c715aa43fd04b6819436d993fa","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"5623d855eaaf0f80f78bc220ceb77cb549fac2c715aa43fd04b6819436d993fa","first_computed_at":"2026-05-18T01:41:14.444910Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:41:14.444910Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"YOq3MoEevgZ3cLJSaUEaV/Sgaf1Pc8596MrrxVs8rvM47n6o8F+jXz7wMzWcfR+B9csy3hjowgyI2+NuUhPsAg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:41:14.445345Z","signed_message":"canonical_sha256_bytes"},"source_id":"1501.01010","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3b167527d5222c2e4c528bd293a495fda7b4fbbb8ceb5a87abae0c4f4edd30e0","sha256:083d870b8085ede808a58bc813d3c0f056091a8849fadbf87dd7eee291156db7"],"state_sha256":"3a56b7aa8f7673f5ea4501b5dacc54535f7ee946d50045f0ed152e8a2a34c1d1"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"hHwBkywEZyNqbq7QTHpYd/EgOJSb3TMSk+vvBcYLqKr2+oqtfo6rA00rzgjZbqdKTgUAk3ODWcA4qeLxsJnRBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-29T16:51:14.629061Z","bundle_sha256":"5512b5a09122bdb9869232f30701223ca0c3050c526b3da10c8e397feaababe3"}}