{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:S4LR4AY4IWNKDYUAWF5IOXBRXR","short_pith_number":"pith:S4LR4AY4","schema_version":"1.0","canonical_sha256":"97171e031c459aa1e280b17a875c31bc5492e31f71ce55ea68a9b6fe5c1fbf9b","source":{"kind":"arxiv","id":"astro-ph/0410402","version":2},"attestation_state":"computed","paper":{"title":"Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Awaki, A. Yoshida, D. Yonetoku, E. Miyata, H. Matsumoto, H. Tajima, H. Tsunemi, J. Kataoka, K. Hayashida, K. Koyama, K. Makishima, K. Nakazawa, K. Yamaoka, M. Kokubun, M. Momachi, M. Ozaki, M. Tashiro, N. Kawai, S. Kitamoto, T. Dotani, T. Kamae, T. Kohmura, T. Murakami, T. Takahashi, T. Tamagawa, T. Tsuru, Y. Fukazawa, Y. Terada","submitted_at":"2004-10-18T12:58:23Z","abstract_excerpt":"The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sensitive imaging observations up to 80 keV. The focal plane detector, which combines a fully depleted X-ray CCD and a pixellated CdTe detector, will provide spectra and images in the wide energy range from 0.5 keV to 80 keV. In the soft gamma-ray band up to ~1 MeV, a narrow field-of-view Compton gamma-ray telescope utilizing several tens of layers of thin Si or CdTe detector will provide precise spectra with much higher"},"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/0410402","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-18T12:58:23Z","cross_cats_sorted":[],"title_canon_sha256":"f48374c6dbf852f1c86ad733ee99fd4ad668c17c65c4fb555619c412e0021b1e","abstract_canon_sha256":"f96120ea07d852c86b96b4c760411acb508a7da785982f3e65b0d91fcff23c78"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:44:59.560308Z","signature_b64":"Iipidx09nmQ0S0+DqTyteysD9TbwqVL+/HQlwRGRfWBaqo276cxzbHKcTPuH13RWgRiGQUzZNOpdNEvOasT3Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"97171e031c459aa1e280b17a875c31bc5492e31f71ce55ea68a9b6fe5c1fbf9b","last_reissued_at":"2026-07-04T16:44:59.559890Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:44:59.559890Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Awaki, A. Yoshida, D. Yonetoku, E. Miyata, H. Matsumoto, H. Tajima, H. Tsunemi, J. Kataoka, K. Hayashida, K. Koyama, K. Makishima, K. Nakazawa, K. Yamaoka, M. Kokubun, M. Momachi, M. Ozaki, M. Tashiro, N. Kawai, S. Kitamoto, T. Dotani, T. Kamae, T. Kohmura, T. Murakami, T. Takahashi, T. Tamagawa, T. Tsuru, Y. Fukazawa, Y. Terada","submitted_at":"2004-10-18T12:58:23Z","abstract_excerpt":"The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sensitive imaging observations up to 80 keV. The focal plane detector, which combines a fully depleted X-ray CCD and a pixellated CdTe detector, will provide spectra and images in the wide energy range from 0.5 keV to 80 keV. In the soft gamma-ray band up to ~1 MeV, a narrow field-of-view Compton gamma-ray telescope utilizing several tens of layers of thin Si or CdTe detector will provide precise spectra with much higher"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410402","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0410402/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0410402","created_at":"2026-07-04T16:44:59.559953+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410402v2","created_at":"2026-07-04T16:44:59.559953+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410402","created_at":"2026-07-04T16:44:59.559953+00:00"},{"alias_kind":"pith_short_12","alias_value":"S4LR4AY4IWNK","created_at":"2026-07-04T16:44:59.559953+00:00"},{"alias_kind":"pith_short_16","alias_value":"S4LR4AY4IWNKDYUA","created_at":"2026-07-04T16:44:59.559953+00:00"},{"alias_kind":"pith_short_8","alias_value":"S4LR4AY4","created_at":"2026-07-04T16:44:59.559953+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/S4LR4AY4IWNKDYUAWF5IOXBRXR","json":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR.json","graph_json":"https://pith.science/api/pith-number/S4LR4AY4IWNKDYUAWF5IOXBRXR/graph.json","events_json":"https://pith.science/api/pith-number/S4LR4AY4IWNKDYUAWF5IOXBRXR/events.json","paper":"https://pith.science/paper/S4LR4AY4"},"agent_actions":{"view_html":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR","download_json":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR.json","view_paper":"https://pith.science/paper/S4LR4AY4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0410402&json=true","fetch_graph":"https://pith.science/api/pith-number/S4LR4AY4IWNKDYUAWF5IOXBRXR/graph.json","fetch_events":"https://pith.science/api/pith-number/S4LR4AY4IWNKDYUAWF5IOXBRXR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR/action/storage_attestation","attest_author":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR/action/author_attestation","sign_citation":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR/action/citation_signature","submit_replication":"https://pith.science/pith/S4LR4AY4IWNKDYUAWF5IOXBRXR/action/replication_record"}},"created_at":"2026-07-04T16:44:59.559953+00:00","updated_at":"2026-07-04T16:44:59.559953+00:00"}