{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:ODRBONRO23BIO6IYXSMZA2CJFI","short_pith_number":"pith:ODRBONRO","schema_version":"1.0","canonical_sha256":"70e217362ed6c2877918bc999068492a326c5bab9fbc2498e7f4ef457741631c","source":{"kind":"arxiv","id":"0907.0976","version":1},"attestation_state":"computed","paper":{"title":"Predicted gamma-ray image of SN 1006 due to inverse Compton emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D.Iakubovskyi, F.Bocchino, G.Castelletti, G.Dubner, I.Telezhinsky, M.Miceli, O.Petruk, S.Orlando","submitted_at":"2009-07-06T12:49:49Z","abstract_excerpt":"We propose a method to synthesize the inverse Compton (IC) gamma-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC gamma-ray images of SN 1006 show morphology in nice agreement with that reported by the H.E.S.S. collaboration. The good correlation found between the observed very-high energy gamma-ray and X-ray/radio appearance can be considered as an evidence that the gamma-ray emission of SN 1006 observed by H.E.S.S. is lep"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0907.0976","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-07-06T12:49:49Z","cross_cats_sorted":[],"title_canon_sha256":"c6b8cfd4706791ae1d517ec8c6bd78216bb3c552ea4040b25b21aac3a45205b0","abstract_canon_sha256":"83a3d6bfbe04c4600a82bdbafe1270462d3a622f92b0979cd03b3138d74b900c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:05.063560Z","signature_b64":"UABomtxMEI07h19A+knTnK0c+i84mj3RwkoxZv1WZJR8kYFt3ffwWMNeIffwXa79hrgEXKVrFJoa+efPLMQ7AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"70e217362ed6c2877918bc999068492a326c5bab9fbc2498e7f4ef457741631c","last_reissued_at":"2026-05-18T02:13:05.063034Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:05.063034Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Predicted gamma-ray image of SN 1006 due to inverse Compton emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"D.Iakubovskyi, F.Bocchino, G.Castelletti, G.Dubner, I.Telezhinsky, M.Miceli, O.Petruk, S.Orlando","submitted_at":"2009-07-06T12:49:49Z","abstract_excerpt":"We propose a method to synthesize the inverse Compton (IC) gamma-ray image of a supernova remnant starting from the radio (or hard X-ray) map and using results of the spatially resolved X-ray spectral analysis. The method is successfully applied to SN 1006. We found that synthesized IC gamma-ray images of SN 1006 show morphology in nice agreement with that reported by the H.E.S.S. collaboration. The good correlation found between the observed very-high energy gamma-ray and X-ray/radio appearance can be considered as an evidence that the gamma-ray emission of SN 1006 observed by H.E.S.S. is lep"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0907.0976","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"0907.0976","created_at":"2026-05-18T02:13:05.063105+00:00"},{"alias_kind":"arxiv_version","alias_value":"0907.0976v1","created_at":"2026-05-18T02:13:05.063105+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0907.0976","created_at":"2026-05-18T02:13:05.063105+00:00"},{"alias_kind":"pith_short_12","alias_value":"ODRBONRO23BI","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"ODRBONRO23BIO6IY","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"ODRBONRO","created_at":"2026-05-18T12:26:01.383474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI","json":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI.json","graph_json":"https://pith.science/api/pith-number/ODRBONRO23BIO6IYXSMZA2CJFI/graph.json","events_json":"https://pith.science/api/pith-number/ODRBONRO23BIO6IYXSMZA2CJFI/events.json","paper":"https://pith.science/paper/ODRBONRO"},"agent_actions":{"view_html":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI","download_json":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI.json","view_paper":"https://pith.science/paper/ODRBONRO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0907.0976&json=true","fetch_graph":"https://pith.science/api/pith-number/ODRBONRO23BIO6IYXSMZA2CJFI/graph.json","fetch_events":"https://pith.science/api/pith-number/ODRBONRO23BIO6IYXSMZA2CJFI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI/action/storage_attestation","attest_author":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI/action/author_attestation","sign_citation":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI/action/citation_signature","submit_replication":"https://pith.science/pith/ODRBONRO23BIO6IYXSMZA2CJFI/action/replication_record"}},"created_at":"2026-05-18T02:13:05.063105+00:00","updated_at":"2026-05-18T02:13:05.063105+00:00"}