{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:QDRRGX4A2IZG3FT4HPBUXEZ2QK","short_pith_number":"pith:QDRRGX4A","schema_version":"1.0","canonical_sha256":"80e3135f80d2326d967c3bc34b933a829bdec74d7ed678ed9723612e8eea92ef","source":{"kind":"arxiv","id":"1502.01491","version":1},"attestation_state":"computed","paper":{"title":"ORIGAMIX, a CdTe-based spectro-imager development for nuclear applications","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"physics.ins-det","authors_text":"C. Blondel, F. Carrel, H. Lemaire, O. Limousin, S. Dubos, S. Schanne, V. Schoepff","submitted_at":"2015-02-05T10:38:17Z","abstract_excerpt":"The Astrophysics Division of CEA Saclay has a long history in the development of CdTe based pixelated detection planes for X and gamma-ray astronomy, with time-resolved imaging and spectrometric capabilities. The last generation, named Caliste HD, is an all-in-one modular instrument that fulfills requirements for space applications. Its full-custom front-end electronics is designed to work over a large energy range from 2 keV to 1 MeV with excellent spectroscopic performances, in particular between 10 and 100 keV (0.56 keV FWHM and 0.67 keV FWHM at 13.9 and 59.5 keV). In the frame of the ORIGA"},"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":"1502.01491","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2015-02-05T10:38:17Z","cross_cats_sorted":["nucl-ex"],"title_canon_sha256":"47a24ebdaed47713fe0479ddd44da0ba174124a6817dff1d7edbba37ab83ac8c","abstract_canon_sha256":"ae17f1f1bf038fb0877a6f177154aa678d0c0bd9a0c4cb2f1618fd913156e7bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:27:51.940623Z","signature_b64":"mOshfh9HyxZpfEzoECsS7C+/yy3xgq7pbzyqg8XaMoPaOgdmirUm4iARKf+o4a2Mkft5+tmBckH6jZ50YzMsDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"80e3135f80d2326d967c3bc34b933a829bdec74d7ed678ed9723612e8eea92ef","last_reissued_at":"2026-05-18T02:27:51.940124Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:27:51.940124Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ORIGAMIX, a CdTe-based spectro-imager development for nuclear applications","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-ex"],"primary_cat":"physics.ins-det","authors_text":"C. Blondel, F. Carrel, H. Lemaire, O. Limousin, S. Dubos, S. Schanne, V. Schoepff","submitted_at":"2015-02-05T10:38:17Z","abstract_excerpt":"The Astrophysics Division of CEA Saclay has a long history in the development of CdTe based pixelated detection planes for X and gamma-ray astronomy, with time-resolved imaging and spectrometric capabilities. The last generation, named Caliste HD, is an all-in-one modular instrument that fulfills requirements for space applications. Its full-custom front-end electronics is designed to work over a large energy range from 2 keV to 1 MeV with excellent spectroscopic performances, in particular between 10 and 100 keV (0.56 keV FWHM and 0.67 keV FWHM at 13.9 and 59.5 keV). In the frame of the ORIGA"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1502.01491","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":"1502.01491","created_at":"2026-05-18T02:27:51.940186+00:00"},{"alias_kind":"arxiv_version","alias_value":"1502.01491v1","created_at":"2026-05-18T02:27:51.940186+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1502.01491","created_at":"2026-05-18T02:27:51.940186+00:00"},{"alias_kind":"pith_short_12","alias_value":"QDRRGX4A2IZG","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_16","alias_value":"QDRRGX4A2IZG3FT4","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_8","alias_value":"QDRRGX4A","created_at":"2026-05-18T12:29:37.295048+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/QDRRGX4A2IZG3FT4HPBUXEZ2QK","json":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK.json","graph_json":"https://pith.science/api/pith-number/QDRRGX4A2IZG3FT4HPBUXEZ2QK/graph.json","events_json":"https://pith.science/api/pith-number/QDRRGX4A2IZG3FT4HPBUXEZ2QK/events.json","paper":"https://pith.science/paper/QDRRGX4A"},"agent_actions":{"view_html":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK","download_json":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK.json","view_paper":"https://pith.science/paper/QDRRGX4A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1502.01491&json=true","fetch_graph":"https://pith.science/api/pith-number/QDRRGX4A2IZG3FT4HPBUXEZ2QK/graph.json","fetch_events":"https://pith.science/api/pith-number/QDRRGX4A2IZG3FT4HPBUXEZ2QK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK/action/storage_attestation","attest_author":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK/action/author_attestation","sign_citation":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK/action/citation_signature","submit_replication":"https://pith.science/pith/QDRRGX4A2IZG3FT4HPBUXEZ2QK/action/replication_record"}},"created_at":"2026-05-18T02:27:51.940186+00:00","updated_at":"2026-05-18T02:27:51.940186+00:00"}