{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:JYPEIV7OMXZDI44ZEXKQ2PZB6I","short_pith_number":"pith:JYPEIV7O","schema_version":"1.0","canonical_sha256":"4e1e4457ee65f234739925d50d3f21f221ecc8564068de5aacf1235a4cbd68cb","source":{"kind":"arxiv","id":"0906.1073","version":1},"attestation_state":"computed","paper":{"title":"A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Decourchelle, E. Giacani, F. Acero, G. Cassam-Chenai, G. Dubner, J. Ballet, M. Lemoine-Goumard, M. Ortega","submitted_at":"2009-06-05T14:55:41Z","abstract_excerpt":"The supernova remnant (SNR) RX J1713.7-3946 (also known as G347.3-0.5) is part of the class of remnants dominated by synchrotron emission in X-rays. It is also one of the few shell-type SNRs observed at TeV energies allowing to investigate particle acceleration at SNRs shock.\n  Our goal is to compare spatial and spectral properties of the remnant in X- and gamma-rays to understand the nature of the TeV emission. This requires to study the remnant at the same spatial scale at both energies. To complement the non-thermal spectrum of the remnant, we attempt to provide a reliable estimate for the "},"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":"0906.1073","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-06-05T14:55:41Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"97f314072e4065ec1282d420e0e1a5015ad1ae0c377e7e566ec1f03a4484abfd","abstract_canon_sha256":"6b133e9a5155ccd62d21a7144112957220995a8c19e00f46dfe5728da7bd35b7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:28.822727Z","signature_b64":"KSsjIpm1nqux4x7IqDg2Nhr9i4rG4s+le5s2vESNnfG+jbkjKxgf17RnsikRXaLoI8iTPOcD7FyMAbbLDDGJAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e1e4457ee65f234739925d50d3f21f221ecc8564068de5aacf1235a4cbd68cb","last_reissued_at":"2026-05-18T02:13:28.822139Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:28.822139Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Decourchelle, E. Giacani, F. Acero, G. Cassam-Chenai, G. Dubner, J. Ballet, M. Lemoine-Goumard, M. Ortega","submitted_at":"2009-06-05T14:55:41Z","abstract_excerpt":"The supernova remnant (SNR) RX J1713.7-3946 (also known as G347.3-0.5) is part of the class of remnants dominated by synchrotron emission in X-rays. It is also one of the few shell-type SNRs observed at TeV energies allowing to investigate particle acceleration at SNRs shock.\n  Our goal is to compare spatial and spectral properties of the remnant in X- and gamma-rays to understand the nature of the TeV emission. This requires to study the remnant at the same spatial scale at both energies. To complement the non-thermal spectrum of the remnant, we attempt to provide a reliable estimate for the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0906.1073","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":"0906.1073","created_at":"2026-05-18T02:13:28.822239+00:00"},{"alias_kind":"arxiv_version","alias_value":"0906.1073v1","created_at":"2026-05-18T02:13:28.822239+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0906.1073","created_at":"2026-05-18T02:13:28.822239+00:00"},{"alias_kind":"pith_short_12","alias_value":"JYPEIV7OMXZD","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_16","alias_value":"JYPEIV7OMXZDI44Z","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_8","alias_value":"JYPEIV7O","created_at":"2026-05-18T12:26:00.592388+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/JYPEIV7OMXZDI44ZEXKQ2PZB6I","json":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I.json","graph_json":"https://pith.science/api/pith-number/JYPEIV7OMXZDI44ZEXKQ2PZB6I/graph.json","events_json":"https://pith.science/api/pith-number/JYPEIV7OMXZDI44ZEXKQ2PZB6I/events.json","paper":"https://pith.science/paper/JYPEIV7O"},"agent_actions":{"view_html":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I","download_json":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I.json","view_paper":"https://pith.science/paper/JYPEIV7O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0906.1073&json=true","fetch_graph":"https://pith.science/api/pith-number/JYPEIV7OMXZDI44ZEXKQ2PZB6I/graph.json","fetch_events":"https://pith.science/api/pith-number/JYPEIV7OMXZDI44ZEXKQ2PZB6I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I/action/storage_attestation","attest_author":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I/action/author_attestation","sign_citation":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I/action/citation_signature","submit_replication":"https://pith.science/pith/JYPEIV7OMXZDI44ZEXKQ2PZB6I/action/replication_record"}},"created_at":"2026-05-18T02:13:28.822239+00:00","updated_at":"2026-05-18T02:13:28.822239+00:00"}