{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:7RRRR3FXGMICA4RW3QJNMERNDJ","short_pith_number":"pith:7RRRR3FX","schema_version":"1.0","canonical_sha256":"fc6318ecb73310207236dc12d6122d1a43ac3c4041896d2ed5d322bf8d9cf165","source":{"kind":"arxiv","id":"2608.02905","version":1},"attestation_state":"computed","paper":{"title":"Fast, low noise, megapixel detector and readout systems for future X-ray astronomy missions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"Abigail Y. Pan, Ajay Dakshinamurthy, Anna Schweingruber, Artem Poliszczuk, Beverly LaMarr, Catherine E. Grant, Christopher Leitz, Daniel Wilkins, Declan O'Neill, Eric D. Miller, Gregory Prigozhin, Haley R. Stueber, Jill Juneau, Keith Warner, Kevan Donlon, Marshall W. Bautz, Matthew Heine, Michael Cooper, Peter Orel, R. Glenn Morris, Sebastian Albrecht, Steven W. Allen, Sven Herrmann, Tanmoy Chattopadhyay, Tonya L. Peshel","submitted_at":"2026-08-03T21:44:22Z","abstract_excerpt":"Next-generation strategic X-ray astronomy missions will require the simultaneous achievement of high angular resolution, large effective collecting area, and wide-field imaging with large-format focal plane detectors. Realizing the associated science objectives--ranging from precision measurements of bright point sources to the detection and characterization of faint diffuse emission-places stringent and, in some cases, competing requirements on detector performance. In particular, high frame rates are necessary to mitigate photon pile-up in observations of bright sources and to reduce contami"},"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":"2608.02905","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2026-08-03T21:44:22Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"78688586176f5d3ed0c05604030c91bb485042a7854b238eed07cff6aaee7c65","abstract_canon_sha256":"0c08ddf016aaa731404893a272193b29238245feb00901054bfd9865b67bcb79"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-08-05T00:43:35.277138Z","signature_b64":"sBD1+T+9B5Ew04AibYbBwstYTQ5r0AqyKRm3i0ktU+/jTRFg1kzx2vZh8CYInFuXkOx/Ez1ApYDzpW+6OInLBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fc6318ecb73310207236dc12d6122d1a43ac3c4041896d2ed5d322bf8d9cf165","last_reissued_at":"2026-08-05T00:43:35.274601Z","signature_status":"signed_v1","first_computed_at":"2026-08-05T00:43:35.274601Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fast, low noise, megapixel detector and readout systems for future X-ray astronomy missions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"Abigail Y. Pan, Ajay Dakshinamurthy, Anna Schweingruber, Artem Poliszczuk, Beverly LaMarr, Catherine E. Grant, Christopher Leitz, Daniel Wilkins, Declan O'Neill, Eric D. Miller, Gregory Prigozhin, Haley R. Stueber, Jill Juneau, Keith Warner, Kevan Donlon, Marshall W. Bautz, Matthew Heine, Michael Cooper, Peter Orel, R. Glenn Morris, Sebastian Albrecht, Steven W. Allen, Sven Herrmann, Tanmoy Chattopadhyay, Tonya L. Peshel","submitted_at":"2026-08-03T21:44:22Z","abstract_excerpt":"Next-generation strategic X-ray astronomy missions will require the simultaneous achievement of high angular resolution, large effective collecting area, and wide-field imaging with large-format focal plane detectors. Realizing the associated science objectives--ranging from precision measurements of bright point sources to the detection and characterization of faint diffuse emission-places stringent and, in some cases, competing requirements on detector performance. In particular, high frame rates are necessary to mitigate photon pile-up in observations of bright sources and to reduce contami"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2608.02905","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/2608.02905/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":"2608.02905","created_at":"2026-08-05T00:43:35.275514+00:00"},{"alias_kind":"arxiv_version","alias_value":"2608.02905v1","created_at":"2026-08-05T00:43:35.275514+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2608.02905","created_at":"2026-08-05T00:43:35.275514+00:00"},{"alias_kind":"pith_short_12","alias_value":"7RRRR3FXGMIC","created_at":"2026-08-05T00:43:35.275514+00:00"},{"alias_kind":"pith_short_16","alias_value":"7RRRR3FXGMICA4RW","created_at":"2026-08-05T00:43:35.275514+00:00"},{"alias_kind":"pith_short_8","alias_value":"7RRRR3FX","created_at":"2026-08-05T00:43:35.275514+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/7RRRR3FXGMICA4RW3QJNMERNDJ","json":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ.json","graph_json":"https://pith.science/api/pith-number/7RRRR3FXGMICA4RW3QJNMERNDJ/graph.json","events_json":"https://pith.science/api/pith-number/7RRRR3FXGMICA4RW3QJNMERNDJ/events.json","paper":"https://pith.science/paper/7RRRR3FX"},"agent_actions":{"view_html":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ","download_json":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ.json","view_paper":"https://pith.science/paper/7RRRR3FX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2608.02905&json=true","fetch_graph":"https://pith.science/api/pith-number/7RRRR3FXGMICA4RW3QJNMERNDJ/graph.json","fetch_events":"https://pith.science/api/pith-number/7RRRR3FXGMICA4RW3QJNMERNDJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ/action/storage_attestation","attest_author":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ/action/author_attestation","sign_citation":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ/action/citation_signature","submit_replication":"https://pith.science/pith/7RRRR3FXGMICA4RW3QJNMERNDJ/action/replication_record"}},"created_at":"2026-08-05T00:43:35.275514+00:00","updated_at":"2026-08-05T00:43:35.275514+00:00"}