{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:VCMORGNHPRJZLIPY4RYX2RSOMV","short_pith_number":"pith:VCMORGNH","schema_version":"1.0","canonical_sha256":"a898e899a77c5395a1f8e4717d464e6562d4f0550112dc40bb20c2dc833f4aed","source":{"kind":"arxiv","id":"astro-ph/0110346","version":1},"attestation_state":"computed","paper":{"title":"Advanced Compton Telescope Designs and SN Science","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J.D. Kurfess (NRL), L.-S. The (Clemson University), P.A. Milne (NRL/NRC), R.A. Kroeger","submitted_at":"2001-10-15T22:17:20Z","abstract_excerpt":"The Advanced Compton Telescope (ACT) has been suggested to be the optimal next-generation instrument to study nuclear gamma-ray lines. In this work, we investigate the potential of three hypothetical designs of the ACT to perform SN science. We provide estimates of 1) the SN detection rate, 2) the SN Ia discrimination rate, and 3) which gamma-ray lines would be detected from specific supernova remnants. We find that the prompt emission from a SN Ia is such that it is unlikely that one would be within the range that an INTERMEDIATE ACT would be able to distinguish between explosion scenarios, a"},"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":"astro-ph/0110346","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-10-15T22:17:20Z","cross_cats_sorted":[],"title_canon_sha256":"a906717170fe4993d93dc831c5d7123f52059bba47e67eced12335396f8ceedf","abstract_canon_sha256":"a4359bc920ef1e577ac6bba549935e0f60c79734f381ee0322200fb44bd2a90b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:43.920482Z","signature_b64":"rXPmjKruZz5jUR0UgI6db9to8ewlOU63J+iRpEWUSvMYW+RGaXr0CwU1eVTmAnxuz2MyulIFHI36a4ytGUFuBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a898e899a77c5395a1f8e4717d464e6562d4f0550112dc40bb20c2dc833f4aed","last_reissued_at":"2026-05-18T01:40:43.919840Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:43.919840Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Advanced Compton Telescope Designs and SN Science","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"J.D. Kurfess (NRL), L.-S. The (Clemson University), P.A. Milne (NRL/NRC), R.A. Kroeger","submitted_at":"2001-10-15T22:17:20Z","abstract_excerpt":"The Advanced Compton Telescope (ACT) has been suggested to be the optimal next-generation instrument to study nuclear gamma-ray lines. In this work, we investigate the potential of three hypothetical designs of the ACT to perform SN science. We provide estimates of 1) the SN detection rate, 2) the SN Ia discrimination rate, and 3) which gamma-ray lines would be detected from specific supernova remnants. We find that the prompt emission from a SN Ia is such that it is unlikely that one would be within the range that an INTERMEDIATE ACT would be able to distinguish between explosion scenarios, a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0110346","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":"astro-ph/0110346","created_at":"2026-05-18T01:40:43.919937+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0110346v1","created_at":"2026-05-18T01:40:43.919937+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0110346","created_at":"2026-05-18T01:40:43.919937+00:00"},{"alias_kind":"pith_short_12","alias_value":"VCMORGNHPRJZ","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_16","alias_value":"VCMORGNHPRJZLIPY","created_at":"2026-05-18T12:25:50.845339+00:00"},{"alias_kind":"pith_short_8","alias_value":"VCMORGNH","created_at":"2026-05-18T12:25:50.845339+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/VCMORGNHPRJZLIPY4RYX2RSOMV","json":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV.json","graph_json":"https://pith.science/api/pith-number/VCMORGNHPRJZLIPY4RYX2RSOMV/graph.json","events_json":"https://pith.science/api/pith-number/VCMORGNHPRJZLIPY4RYX2RSOMV/events.json","paper":"https://pith.science/paper/VCMORGNH"},"agent_actions":{"view_html":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV","download_json":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV.json","view_paper":"https://pith.science/paper/VCMORGNH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0110346&json=true","fetch_graph":"https://pith.science/api/pith-number/VCMORGNHPRJZLIPY4RYX2RSOMV/graph.json","fetch_events":"https://pith.science/api/pith-number/VCMORGNHPRJZLIPY4RYX2RSOMV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV/action/storage_attestation","attest_author":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV/action/author_attestation","sign_citation":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV/action/citation_signature","submit_replication":"https://pith.science/pith/VCMORGNHPRJZLIPY4RYX2RSOMV/action/replication_record"}},"created_at":"2026-05-18T01:40:43.919937+00:00","updated_at":"2026-05-18T01:40:43.919937+00:00"}