{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:5OXRYKTHB4FPTRR6VA6PECKTK2","short_pith_number":"pith:5OXRYKTH","canonical_record":{"source":{"id":"1011.1847","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-11-08T16:42:44Z","cross_cats_sorted":[],"title_canon_sha256":"84f96cced6b54c0780c656852fae9080c062b4f02b56acb80ce8f77475981127","abstract_canon_sha256":"d29d555246bf0cae2b3cc5917e9de53b3778ceb9b5b000c994cb5b6477ef8c08"},"schema_version":"1.0"},"canonical_sha256":"ebaf1c2a670f0af9c63ea83cf2095356b16ddddd8d1be603d42ee8dcf2dd1df5","source":{"kind":"arxiv","id":"1011.1847","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1011.1847","created_at":"2026-05-18T02:04:50Z"},{"alias_kind":"arxiv_version","alias_value":"1011.1847v1","created_at":"2026-05-18T02:04:50Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.1847","created_at":"2026-05-18T02:04:50Z"},{"alias_kind":"pith_short_12","alias_value":"5OXRYKTHB4FP","created_at":"2026-05-18T12:26:04Z"},{"alias_kind":"pith_short_16","alias_value":"5OXRYKTHB4FPTRR6","created_at":"2026-05-18T12:26:04Z"},{"alias_kind":"pith_short_8","alias_value":"5OXRYKTH","created_at":"2026-05-18T12:26:04Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:5OXRYKTHB4FPTRR6VA6PECKTK2","target":"record","payload":{"canonical_record":{"source":{"id":"1011.1847","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-11-08T16:42:44Z","cross_cats_sorted":[],"title_canon_sha256":"84f96cced6b54c0780c656852fae9080c062b4f02b56acb80ce8f77475981127","abstract_canon_sha256":"d29d555246bf0cae2b3cc5917e9de53b3778ceb9b5b000c994cb5b6477ef8c08"},"schema_version":"1.0"},"canonical_sha256":"ebaf1c2a670f0af9c63ea83cf2095356b16ddddd8d1be603d42ee8dcf2dd1df5","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:50.382298Z","signature_b64":"/NHWeSjTABM5WKIc0vgfbDVu040/zl7WXE7LMSeUNJ9PzD8agYaAsMDuB52iUrWsvQp+rXb7n/PVRDSioro5Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ebaf1c2a670f0af9c63ea83cf2095356b16ddddd8d1be603d42ee8dcf2dd1df5","last_reissued_at":"2026-05-18T02:04:50.381656Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:50.381656Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1011.1847","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":"2026-05-18T02:04:50Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YyrJql2T8dQbwPdGEUGZOCF4jqbcO0b3hVxFs2Q3GyHee4BBMShnq766pKAIyKGPs/5PCvTs4W2W6CX9jaTUAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T18:50:59.148548Z"},"content_sha256":"413aaa61c9842d1707e3fb63a93f2b593d1a3f3bf2099465cb750c9dd1d4efdc","schema_version":"1.0","event_id":"sha256:413aaa61c9842d1707e3fb63a93f2b593d1a3f3bf2099465cb750c9dd1d4efdc"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:5OXRYKTHB4FPTRR6VA6PECKTK2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"F. Bocchino, M. Miceli, O. Petruk, S. Orlando","submitted_at":"2010-11-08T16:42:44Z","abstract_excerpt":"Observations of SNRs in X-ray and gamma-ray bands promise to contribute with important information in our understanding on the nature of galactic cosmic rays. The analysis of SNRs images collected in different energy bands requires the support of theoretical modeling of synchrotron and inverse Compton (IC) emission. We develop a numerical code (REMLIGHT) to synthesize, from MHD simulations, the synchrotron radio, X-ray and IC gamma-ray emission from SNRs expanding in non-uniform interstellar medium (ISM) and/or non-uniform interstellar magnetic field (ISMF). As a first application, the code is"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.1847","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":"2026-05-18T02:04:50Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6HIf1QRjVEbo3kqNottMiO0H34OvO9mAEOusSRmO2No0RUAlgVznjK99Jb583GwE/jcD6X/gBaJWcCxVWtOFCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T18:50:59.149239Z"},"content_sha256":"ee25578e918abdc11289b6c9c9a841f082d9c9a8a6567d92c2d789c2e3b0fcda","schema_version":"1.0","event_id":"sha256:ee25578e918abdc11289b6c9c9a841f082d9c9a8a6567d92c2d789c2e3b0fcda"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/5OXRYKTHB4FPTRR6VA6PECKTK2/bundle.json","state_url":"https://pith.science/pith/5OXRYKTHB4FPTRR6VA6PECKTK2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/5OXRYKTHB4FPTRR6VA6PECKTK2/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":"2026-05-18T18:50:59Z","links":{"resolver":"https://pith.science/pith/5OXRYKTHB4FPTRR6VA6PECKTK2","bundle":"https://pith.science/pith/5OXRYKTHB4FPTRR6VA6PECKTK2/bundle.json","state":"https://pith.science/pith/5OXRYKTHB4FPTRR6VA6PECKTK2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/5OXRYKTHB4FPTRR6VA6PECKTK2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:5OXRYKTHB4FPTRR6VA6PECKTK2","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":"d29d555246bf0cae2b3cc5917e9de53b3778ceb9b5b000c994cb5b6477ef8c08","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-11-08T16:42:44Z","title_canon_sha256":"84f96cced6b54c0780c656852fae9080c062b4f02b56acb80ce8f77475981127"},"schema_version":"1.0","source":{"id":"1011.1847","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1011.1847","created_at":"2026-05-18T02:04:50Z"},{"alias_kind":"arxiv_version","alias_value":"1011.1847v1","created_at":"2026-05-18T02:04:50Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.1847","created_at":"2026-05-18T02:04:50Z"},{"alias_kind":"pith_short_12","alias_value":"5OXRYKTHB4FP","created_at":"2026-05-18T12:26:04Z"},{"alias_kind":"pith_short_16","alias_value":"5OXRYKTHB4FPTRR6","created_at":"2026-05-18T12:26:04Z"},{"alias_kind":"pith_short_8","alias_value":"5OXRYKTH","created_at":"2026-05-18T12:26:04Z"}],"graph_snapshots":[{"event_id":"sha256:ee25578e918abdc11289b6c9c9a841f082d9c9a8a6567d92c2d789c2e3b0fcda","target":"graph","created_at":"2026-05-18T02:04:50Z","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":"Observations of SNRs in X-ray and gamma-ray bands promise to contribute with important information in our understanding on the nature of galactic cosmic rays. The analysis of SNRs images collected in different energy bands requires the support of theoretical modeling of synchrotron and inverse Compton (IC) emission. We develop a numerical code (REMLIGHT) to synthesize, from MHD simulations, the synchrotron radio, X-ray and IC gamma-ray emission from SNRs expanding in non-uniform interstellar medium (ISM) and/or non-uniform interstellar magnetic field (ISMF). As a first application, the code is","authors_text":"F. Bocchino, M. Miceli, O. Petruk, S. Orlando","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-11-08T16:42:44Z","title":"Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton gamma-ray morphology of SNRs"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.1847","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":"sha256:413aaa61c9842d1707e3fb63a93f2b593d1a3f3bf2099465cb750c9dd1d4efdc","target":"record","created_at":"2026-05-18T02:04:50Z","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":"d29d555246bf0cae2b3cc5917e9de53b3778ceb9b5b000c994cb5b6477ef8c08","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-11-08T16:42:44Z","title_canon_sha256":"84f96cced6b54c0780c656852fae9080c062b4f02b56acb80ce8f77475981127"},"schema_version":"1.0","source":{"id":"1011.1847","kind":"arxiv","version":1}},"canonical_sha256":"ebaf1c2a670f0af9c63ea83cf2095356b16ddddd8d1be603d42ee8dcf2dd1df5","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"ebaf1c2a670f0af9c63ea83cf2095356b16ddddd8d1be603d42ee8dcf2dd1df5","first_computed_at":"2026-05-18T02:04:50.381656Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:04:50.381656Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"/NHWeSjTABM5WKIc0vgfbDVu040/zl7WXE7LMSeUNJ9PzD8agYaAsMDuB52iUrWsvQp+rXb7n/PVRDSioro5Bg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:04:50.382298Z","signed_message":"canonical_sha256_bytes"},"source_id":"1011.1847","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:413aaa61c9842d1707e3fb63a93f2b593d1a3f3bf2099465cb750c9dd1d4efdc","sha256:ee25578e918abdc11289b6c9c9a841f082d9c9a8a6567d92c2d789c2e3b0fcda"],"state_sha256":"ae2ad593a884ea3dd0f5ecba3a091b645113b740576c3b4b63af882bf4831e33"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mkODglOO1/4Qs748Qi237+yoD95k0m0TH/YOAxpn+o1zug0Rn8ObWk4RbUI+XUrNb7uuYl9NMR53XS2kmcs9BA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-18T18:50:59.151423Z","bundle_sha256":"e8ef200c7149c1ce49de791c3ca080503d44ccf9688789861fb08c100928c514"}}