{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:3T333L4AG23YL5H5FZWCMS4XVF","short_pith_number":"pith:3T333L4A","schema_version":"1.0","canonical_sha256":"dcf7bdaf8036b785f4fd2e6c264b97a96bb56c77f685bbf324d48ab9b0c788b2","source":{"kind":"arxiv","id":"2407.05947","version":1},"attestation_state":"computed","paper":{"title":"The path toward 500 $\\mu$m depletion of AstroPix, a pixelated silicon HVCMOS sensor for space and EIC","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Amanda L. Steinhebel, Anthony Affolder, Aware Deshmukh, Daniel Violette, Ivan Peric, Jennifer Ott, Jessica Metcalfe, Kirsten Affolder, Manoj Jadhav, Nicolas Striebig, Olivia Kroger, Regina Caputo, Richard Leys, Taylor (K.-W.) Shin, Vitaliy Fadeyev, Yasushi Fukazawa, Yusuke Suda","submitted_at":"2024-07-08T13:48:27Z","abstract_excerpt":"The precise reconstruction of Compton-scatter events is paramount for an imaging medium-energy gamma-ray telescope. The proposed AMEGO-X is enabled by a silicon tracker utilizing AstroPix chips - a pixelated silicon HVCMOS sensor novel for space use. To achieve science goals, each 500 x 500 $\\mu$m$^2$ pixel must be sensitive for energy deposits ranging from 25 - 700 keV with an energy resolution of 5 keV at 122 keV (< 10%). This is achieved through depletion of the 500 $\\mu$m thick sensor, although complete depletion poses an engineering and design challenge. This work will summarize the curre"},"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":"2407.05947","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2024-07-08T13:48:27Z","cross_cats_sorted":[],"title_canon_sha256":"62b93385435959312ff1206037e1d11b9d541b503fde7202b6a2cb1cf158f79e","abstract_canon_sha256":"a703db0b495f657d895d302395714e7f0add7b12b8b0f2567f43169067084e8b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:41:21.482440Z","signature_b64":"Xx6SmOipjDEsJ7q0UOVWU3snR7U+GCingPtkliw0g+MW0RVdUjgv/oWRkzUfXMS6wOa+R639qvlaUYNZNJPlBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dcf7bdaf8036b785f4fd2e6c264b97a96bb56c77f685bbf324d48ab9b0c788b2","last_reissued_at":"2026-07-05T08:41:21.482006Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:41:21.482006Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The path toward 500 $\\mu$m depletion of AstroPix, a pixelated silicon HVCMOS sensor for space and EIC","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Amanda L. Steinhebel, Anthony Affolder, Aware Deshmukh, Daniel Violette, Ivan Peric, Jennifer Ott, Jessica Metcalfe, Kirsten Affolder, Manoj Jadhav, Nicolas Striebig, Olivia Kroger, Regina Caputo, Richard Leys, Taylor (K.-W.) Shin, Vitaliy Fadeyev, Yasushi Fukazawa, Yusuke Suda","submitted_at":"2024-07-08T13:48:27Z","abstract_excerpt":"The precise reconstruction of Compton-scatter events is paramount for an imaging medium-energy gamma-ray telescope. The proposed AMEGO-X is enabled by a silicon tracker utilizing AstroPix chips - a pixelated silicon HVCMOS sensor novel for space use. To achieve science goals, each 500 x 500 $\\mu$m$^2$ pixel must be sensitive for energy deposits ranging from 25 - 700 keV with an energy resolution of 5 keV at 122 keV (< 10%). This is achieved through depletion of the 500 $\\mu$m thick sensor, although complete depletion poses an engineering and design challenge. This work will summarize the curre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.05947","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2407.05947/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":"2407.05947","created_at":"2026-07-05T08:41:21.482063+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.05947v1","created_at":"2026-07-05T08:41:21.482063+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.05947","created_at":"2026-07-05T08:41:21.482063+00:00"},{"alias_kind":"pith_short_12","alias_value":"3T333L4AG23Y","created_at":"2026-07-05T08:41:21.482063+00:00"},{"alias_kind":"pith_short_16","alias_value":"3T333L4AG23YL5H5","created_at":"2026-07-05T08:41:21.482063+00:00"},{"alias_kind":"pith_short_8","alias_value":"3T333L4A","created_at":"2026-07-05T08:41:21.482063+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.11987","citing_title":"Hard X-ray and gamma-ray detectors","ref_index":71,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF","json":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF.json","graph_json":"https://pith.science/api/pith-number/3T333L4AG23YL5H5FZWCMS4XVF/graph.json","events_json":"https://pith.science/api/pith-number/3T333L4AG23YL5H5FZWCMS4XVF/events.json","paper":"https://pith.science/paper/3T333L4A"},"agent_actions":{"view_html":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF","download_json":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF.json","view_paper":"https://pith.science/paper/3T333L4A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.05947&json=true","fetch_graph":"https://pith.science/api/pith-number/3T333L4AG23YL5H5FZWCMS4XVF/graph.json","fetch_events":"https://pith.science/api/pith-number/3T333L4AG23YL5H5FZWCMS4XVF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF/action/storage_attestation","attest_author":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF/action/author_attestation","sign_citation":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF/action/citation_signature","submit_replication":"https://pith.science/pith/3T333L4AG23YL5H5FZWCMS4XVF/action/replication_record"}},"created_at":"2026-07-05T08:41:21.482063+00:00","updated_at":"2026-07-05T08:41:21.482063+00:00"}