{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:DOI3XJ4ROBLHY47KF5NSQBKQML","short_pith_number":"pith:DOI3XJ4R","schema_version":"1.0","canonical_sha256":"1b91bba79170567c73ea2f5b28055062de2f4d4cc7fa6276b75369c7b6a66b2b","source":{"kind":"arxiv","id":"0805.2232","version":1},"attestation_state":"computed","paper":{"title":"X-Ray Emission from Supernova Remnants Observed in the ASCA Galactic Plane Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Aya Bamba, Katsuji Koyama, Masaru Ueno, Shigeo Yamauchi","submitted_at":"2008-05-15T09:02:17Z","abstract_excerpt":"X-ray images and spectra of 5 cataloged supernova remnants (SNRs), G12.0-0.1, G346.6-0.2, G348.5+0.1, G348.7+0.3, and G355.6-0.0, observed in the ASCA galactic plane survey are presented. The sizes of X-ray emission from G12.0-0.1, G348.5+0.1, G348.7+0.3, and G355.6-0.0 are comparable to their radio structures, while that of G346.6-0.2 is smaller than the radio structure. The X-ray spectra of all of the SNRs were heavily absorbed by interstellar matter with N_H>10^{22} cm^{-2}. The spectrum of G355.6-0.0 exhibited emission lines, indicating that the X-ray emission has a thin thermal plasma ori"},"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":"0805.2232","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-05-15T09:02:17Z","cross_cats_sorted":[],"title_canon_sha256":"12fe33890d84891aeb25dbf3fc9945b12649d3dd439bda00c231ffc7de7b6253","abstract_canon_sha256":"43e1b9c65b4d801124c5df0dda3cf30cd088bd446073e29824def5b2b50421ac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:15:52.760109Z","signature_b64":"YMr/9yu4MbcwR33nADQqoBgTrsUXhvJSvT4A/mxsaTsu6p70hJ1BPsIQ8tyCrw3hJMJ+qNlbyQnjV/V7gPC0CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b91bba79170567c73ea2f5b28055062de2f4d4cc7fa6276b75369c7b6a66b2b","last_reissued_at":"2026-05-18T02:15:52.759570Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:15:52.759570Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-Ray Emission from Supernova Remnants Observed in the ASCA Galactic Plane Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Aya Bamba, Katsuji Koyama, Masaru Ueno, Shigeo Yamauchi","submitted_at":"2008-05-15T09:02:17Z","abstract_excerpt":"X-ray images and spectra of 5 cataloged supernova remnants (SNRs), G12.0-0.1, G346.6-0.2, G348.5+0.1, G348.7+0.3, and G355.6-0.0, observed in the ASCA galactic plane survey are presented. The sizes of X-ray emission from G12.0-0.1, G348.5+0.1, G348.7+0.3, and G355.6-0.0 are comparable to their radio structures, while that of G346.6-0.2 is smaller than the radio structure. The X-ray spectra of all of the SNRs were heavily absorbed by interstellar matter with N_H>10^{22} cm^{-2}. The spectrum of G355.6-0.0 exhibited emission lines, indicating that the X-ray emission has a thin thermal plasma ori"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0805.2232","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":"0805.2232","created_at":"2026-05-18T02:15:52.759656+00:00"},{"alias_kind":"arxiv_version","alias_value":"0805.2232v1","created_at":"2026-05-18T02:15:52.759656+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0805.2232","created_at":"2026-05-18T02:15:52.759656+00:00"},{"alias_kind":"pith_short_12","alias_value":"DOI3XJ4ROBLH","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"DOI3XJ4ROBLHY47K","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"DOI3XJ4R","created_at":"2026-05-18T12:25:57.157939+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/DOI3XJ4ROBLHY47KF5NSQBKQML","json":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML.json","graph_json":"https://pith.science/api/pith-number/DOI3XJ4ROBLHY47KF5NSQBKQML/graph.json","events_json":"https://pith.science/api/pith-number/DOI3XJ4ROBLHY47KF5NSQBKQML/events.json","paper":"https://pith.science/paper/DOI3XJ4R"},"agent_actions":{"view_html":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML","download_json":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML.json","view_paper":"https://pith.science/paper/DOI3XJ4R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0805.2232&json=true","fetch_graph":"https://pith.science/api/pith-number/DOI3XJ4ROBLHY47KF5NSQBKQML/graph.json","fetch_events":"https://pith.science/api/pith-number/DOI3XJ4ROBLHY47KF5NSQBKQML/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML/action/storage_attestation","attest_author":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML/action/author_attestation","sign_citation":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML/action/citation_signature","submit_replication":"https://pith.science/pith/DOI3XJ4ROBLHY47KF5NSQBKQML/action/replication_record"}},"created_at":"2026-05-18T02:15:52.759656+00:00","updated_at":"2026-05-18T02:15:52.759656+00:00"}