{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:TUYLYWJBCDZDKDKVKUOGODRA4D","short_pith_number":"pith:TUYLYWJB","canonical_record":{"source":{"id":"1003.0379","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-03-01T18:05:03Z","cross_cats_sorted":[],"title_canon_sha256":"612f15ba26b466650de8e564f8e9911665f43230816c783b18110a8a729286a2","abstract_canon_sha256":"e8b8871e0faf567433562089083cb91f4eaa5a7566daec91e34739a4d58f695a"},"schema_version":"1.0"},"canonical_sha256":"9d30bc592110f2350d55551c670e20e0f3fa54ba56c30b4888fd00d6715f2128","source":{"kind":"arxiv","id":"1003.0379","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1003.0379","created_at":"2026-05-18T02:08:47Z"},{"alias_kind":"arxiv_version","alias_value":"1003.0379v2","created_at":"2026-05-18T02:08:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1003.0379","created_at":"2026-05-18T02:08:47Z"},{"alias_kind":"pith_short_12","alias_value":"TUYLYWJBCDZD","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"TUYLYWJBCDZDKDKV","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"TUYLYWJB","created_at":"2026-05-18T12:26:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:TUYLYWJBCDZDKDKVKUOGODRA4D","target":"record","payload":{"canonical_record":{"source":{"id":"1003.0379","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-03-01T18:05:03Z","cross_cats_sorted":[],"title_canon_sha256":"612f15ba26b466650de8e564f8e9911665f43230816c783b18110a8a729286a2","abstract_canon_sha256":"e8b8871e0faf567433562089083cb91f4eaa5a7566daec91e34739a4d58f695a"},"schema_version":"1.0"},"canonical_sha256":"9d30bc592110f2350d55551c670e20e0f3fa54ba56c30b4888fd00d6715f2128","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:47.992305Z","signature_b64":"RLR0QO8mP0JQavL8Epyx9wBWlP8AAk+E6LTz3mPq9JkxRYr6qekCD0eQU8+YXwzzZDU3EWeEPlJ2guYjgMrqAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d30bc592110f2350d55551c670e20e0f3fa54ba56c30b4888fd00d6715f2128","last_reissued_at":"2026-05-18T02:08:47.991639Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:47.991639Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1003.0379","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":"2026-05-18T02:08:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ik2yISa2gyc5/ZUQLzCoIakvmn4CZuUTMRpwojnpaeyTBGDD3HeBV5NtNvla+bByX3e5Y0wnqzWjA3bAObW7DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T00:15:29.152927Z"},"content_sha256":"7f282941831a93b7b00234230e5f8b201e7d98e8fc0b6a0b1f3cd2027a42eece","schema_version":"1.0","event_id":"sha256:7f282941831a93b7b00234230e5f8b201e7d98e8fc0b6a0b1f3cd2027a42eece"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:TUYLYWJBCDZDKDKVKUOGODRA4D","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Modeling the gamma-ray emission produced by runaway cosmic rays in the environment of RX J1713.7-3946","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Kawamura, D.I. Jones, F.A.Aharonian, G. Rowell, H. Sano, H. Yamamoto, K. Torii, S.Casanova, S. Gabici, T. Onishi, Y.Fukui","submitted_at":"2010-03-01T18:05:03Z","abstract_excerpt":"Diffusive shock acceleration in supernova remnants is the most widely invoked paradigm to explain the Galactic cosmic ray spectrum. Cosmic rays escaping supernova remnants diffuse in the interstellar medium and collide with the ambient atomic and molecular gas. From such collisions gamma-rays are created, which can possibly provide the first evidence of a parent population of runaway cosmic rays. We present model predictions for the GeV to TeV gamma-ray emission produced by the collisions of runaway cosmic rays with the gas in the environment surrounding the shell-type supernova remnant RX J17"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.0379","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":"2026-05-18T02:08:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"e3kljDq4sNG3vtCwBqTx94a6vqEph4Ya0snZPh7ffL9lG+bKcdO7euAoJzY1+qNYKymYww6o+bO2+Ov9ZvNWCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T00:15:29.153646Z"},"content_sha256":"ed9dc5385e2c94b1b8d515d10242bc8fdeb8ffe300141039c8e89d33d2e9acb8","schema_version":"1.0","event_id":"sha256:ed9dc5385e2c94b1b8d515d10242bc8fdeb8ffe300141039c8e89d33d2e9acb8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/TUYLYWJBCDZDKDKVKUOGODRA4D/bundle.json","state_url":"https://pith.science/pith/TUYLYWJBCDZDKDKVKUOGODRA4D/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/TUYLYWJBCDZDKDKVKUOGODRA4D/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":"2026-05-31T00:15:29Z","links":{"resolver":"https://pith.science/pith/TUYLYWJBCDZDKDKVKUOGODRA4D","bundle":"https://pith.science/pith/TUYLYWJBCDZDKDKVKUOGODRA4D/bundle.json","state":"https://pith.science/pith/TUYLYWJBCDZDKDKVKUOGODRA4D/state.json","well_known_bundle":"https://pith.science/.well-known/pith/TUYLYWJBCDZDKDKVKUOGODRA4D/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:TUYLYWJBCDZDKDKVKUOGODRA4D","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":"e8b8871e0faf567433562089083cb91f4eaa5a7566daec91e34739a4d58f695a","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-03-01T18:05:03Z","title_canon_sha256":"612f15ba26b466650de8e564f8e9911665f43230816c783b18110a8a729286a2"},"schema_version":"1.0","source":{"id":"1003.0379","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1003.0379","created_at":"2026-05-18T02:08:47Z"},{"alias_kind":"arxiv_version","alias_value":"1003.0379v2","created_at":"2026-05-18T02:08:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1003.0379","created_at":"2026-05-18T02:08:47Z"},{"alias_kind":"pith_short_12","alias_value":"TUYLYWJBCDZD","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"TUYLYWJBCDZDKDKV","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"TUYLYWJB","created_at":"2026-05-18T12:26:15Z"}],"graph_snapshots":[{"event_id":"sha256:ed9dc5385e2c94b1b8d515d10242bc8fdeb8ffe300141039c8e89d33d2e9acb8","target":"graph","created_at":"2026-05-18T02:08:47Z","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":"Diffusive shock acceleration in supernova remnants is the most widely invoked paradigm to explain the Galactic cosmic ray spectrum. Cosmic rays escaping supernova remnants diffuse in the interstellar medium and collide with the ambient atomic and molecular gas. From such collisions gamma-rays are created, which can possibly provide the first evidence of a parent population of runaway cosmic rays. We present model predictions for the GeV to TeV gamma-ray emission produced by the collisions of runaway cosmic rays with the gas in the environment surrounding the shell-type supernova remnant RX J17","authors_text":"A. Kawamura, D.I. Jones, F.A.Aharonian, G. Rowell, H. Sano, H. Yamamoto, K. Torii, S.Casanova, S. Gabici, T. Onishi, Y.Fukui","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-03-01T18:05:03Z","title":"Modeling the gamma-ray emission produced by runaway cosmic rays in the environment of RX J1713.7-3946"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.0379","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":"sha256:7f282941831a93b7b00234230e5f8b201e7d98e8fc0b6a0b1f3cd2027a42eece","target":"record","created_at":"2026-05-18T02:08:47Z","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":"e8b8871e0faf567433562089083cb91f4eaa5a7566daec91e34739a4d58f695a","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-03-01T18:05:03Z","title_canon_sha256":"612f15ba26b466650de8e564f8e9911665f43230816c783b18110a8a729286a2"},"schema_version":"1.0","source":{"id":"1003.0379","kind":"arxiv","version":2}},"canonical_sha256":"9d30bc592110f2350d55551c670e20e0f3fa54ba56c30b4888fd00d6715f2128","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"9d30bc592110f2350d55551c670e20e0f3fa54ba56c30b4888fd00d6715f2128","first_computed_at":"2026-05-18T02:08:47.991639Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:08:47.991639Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"RLR0QO8mP0JQavL8Epyx9wBWlP8AAk+E6LTz3mPq9JkxRYr6qekCD0eQU8+YXwzzZDU3EWeEPlJ2guYjgMrqAg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:08:47.992305Z","signed_message":"canonical_sha256_bytes"},"source_id":"1003.0379","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:7f282941831a93b7b00234230e5f8b201e7d98e8fc0b6a0b1f3cd2027a42eece","sha256:ed9dc5385e2c94b1b8d515d10242bc8fdeb8ffe300141039c8e89d33d2e9acb8"],"state_sha256":"97057e6e341dab2f9c4d587b82ed49106b677e0a51cfe3bef5a1367d39f60b4b"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mSDud8wWRH7zbzyoNUVTDT5YhLxxR1UD45hPmOiHfznpccvNlRmfLw9kQszMp/ODBH2/2bsNc0DKojlWzp8bBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T00:15:29.162110Z","bundle_sha256":"4cca6f7ca3a5c5ab16ee3da459fc4702c0699b3f3392f6164da7e480b7db5b9c"}}