{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:GGKSXYYLLSQR4QEPSTYU77E5QT","short_pith_number":"pith:GGKSXYYL","schema_version":"1.0","canonical_sha256":"31952be30b5ca11e408f94f14ffc9d84e18ee34a172ee5606146f974f9f4f947","source":{"kind":"arxiv","id":"1705.03086","version":2},"attestation_state":"computed","paper":{"title":"Integral Field Spectroscopy of Balmer-Dominated Shocks in the Magellanic Cloud Supernova Remnant N103B","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Brian J. Williams, Frederic P. A. Vogt, Ivo R. Seitenzahl, Jason B. Terry, Michael A. Dopita, Parviz Ghavamian, P. Frank Winkler","submitted_at":"2017-05-08T21:00:21Z","abstract_excerpt":"We present results of integral field spectroscopy of Balmer-dominated shocks in the LMC supernova remnant (SNR) N103B, carried out using the Wide Field Integral Spectrograph (WiFeS) on the 2.3 m telescope at Siding Spring Observatory in Australia. Existing X-ray studies of N103B have indicated a Type Ia supernova origin. Radiative shock emission from clumpy material surrounding the SNR may result from interaction of the forward shock with relic stellar wind material, possibly implicating a thermonuclear explosion in a single-degenerate binary system. The recently discovered Balmer-dominated sh"},"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":"1705.03086","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-05-08T21:00:21Z","cross_cats_sorted":[],"title_canon_sha256":"61408e5574b4d9fa8ce416e3bfa2a7d0f0a4a1e2f13564ab5c34180450e74d7e","abstract_canon_sha256":"9f63648e57219a6d52871e047a695202d02fb9f67bd1a0f2229624c8cfcfcf74"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:33:18.370423Z","signature_b64":"RTlz/3cwbAlgkMMeCY8uMaBL4MzQOOaqjT8lPMInM7pyIMFpe104sW0I7lUTHrmxSg7tA+Y1bnd2yMXVc93WAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"31952be30b5ca11e408f94f14ffc9d84e18ee34a172ee5606146f974f9f4f947","last_reissued_at":"2026-05-18T00:33:18.369839Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:33:18.369839Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Integral Field Spectroscopy of Balmer-Dominated Shocks in the Magellanic Cloud Supernova Remnant N103B","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Brian J. Williams, Frederic P. A. Vogt, Ivo R. Seitenzahl, Jason B. Terry, Michael A. Dopita, Parviz Ghavamian, P. Frank Winkler","submitted_at":"2017-05-08T21:00:21Z","abstract_excerpt":"We present results of integral field spectroscopy of Balmer-dominated shocks in the LMC supernova remnant (SNR) N103B, carried out using the Wide Field Integral Spectrograph (WiFeS) on the 2.3 m telescope at Siding Spring Observatory in Australia. Existing X-ray studies of N103B have indicated a Type Ia supernova origin. Radiative shock emission from clumpy material surrounding the SNR may result from interaction of the forward shock with relic stellar wind material, possibly implicating a thermonuclear explosion in a single-degenerate binary system. The recently discovered Balmer-dominated sh"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.03086","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1705.03086","created_at":"2026-05-18T00:33:18.369919+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.03086v2","created_at":"2026-05-18T00:33:18.369919+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.03086","created_at":"2026-05-18T00:33:18.369919+00:00"},{"alias_kind":"pith_short_12","alias_value":"GGKSXYYLLSQR","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"GGKSXYYLLSQR4QEP","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"GGKSXYYL","created_at":"2026-05-18T12:31:15.632608+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/GGKSXYYLLSQR4QEPSTYU77E5QT","json":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT.json","graph_json":"https://pith.science/api/pith-number/GGKSXYYLLSQR4QEPSTYU77E5QT/graph.json","events_json":"https://pith.science/api/pith-number/GGKSXYYLLSQR4QEPSTYU77E5QT/events.json","paper":"https://pith.science/paper/GGKSXYYL"},"agent_actions":{"view_html":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT","download_json":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT.json","view_paper":"https://pith.science/paper/GGKSXYYL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.03086&json=true","fetch_graph":"https://pith.science/api/pith-number/GGKSXYYLLSQR4QEPSTYU77E5QT/graph.json","fetch_events":"https://pith.science/api/pith-number/GGKSXYYLLSQR4QEPSTYU77E5QT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT/action/storage_attestation","attest_author":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT/action/author_attestation","sign_citation":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT/action/citation_signature","submit_replication":"https://pith.science/pith/GGKSXYYLLSQR4QEPSTYU77E5QT/action/replication_record"}},"created_at":"2026-05-18T00:33:18.369919+00:00","updated_at":"2026-05-18T00:33:18.369919+00:00"}