{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:D2N2XKICH45E2KZCHUB2TYHVSJ","short_pith_number":"pith:D2N2XKIC","schema_version":"1.0","canonical_sha256":"1e9baba9023f3a4d2b223d03a9e0f5925221dd768d24bdfdc0278c9548107985","source":{"kind":"arxiv","id":"astro-ph/0007138","version":2},"attestation_state":"computed","paper":{"title":"Properties of PACE-I HgCdTe Detectors in Space - the NICMOS Warm-up Monitoring Program","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"et al, T. Boeker","submitted_at":"2000-07-11T14:02:13Z","abstract_excerpt":"We summarize the results of a monitoring program which was executed following the cryogen exhaustion of the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) onboard the Hubble Space Telescope. During the subsequent warm-up, detector parameters such as detective quantum efficiency, dark current, bias offsets, and saturation levels have been measured over the temperature range 62K to about 100K. The measurements provide a unique database of the characteristics of PACE-I HgCdTe detector arrays in the space environment. A surprising result of the analysis is the fact that all three NICM"},"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/0007138","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2000-07-11T14:02:13Z","cross_cats_sorted":[],"title_canon_sha256":"24eccb88c3d143fb329e40d6ea8eb376f514507cbc91792af7ac6720911b3323","abstract_canon_sha256":"d2b52b20e9ea4f4b55d2832903ec4f783984a349b646232300e105b0f3497072"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:47.534870Z","signature_b64":"VV9ITOVvXe7yizgW1WMx3E1cEuddNIBseer1MHd53c97zvhDB7R+Qp8kZMRpTDUCVJNu+SUhD2o9XFGb+LfyDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1e9baba9023f3a4d2b223d03a9e0f5925221dd768d24bdfdc0278c9548107985","last_reissued_at":"2026-05-18T01:40:47.532885Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:47.532885Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Properties of PACE-I HgCdTe Detectors in Space - the NICMOS Warm-up Monitoring Program","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"et al, T. Boeker","submitted_at":"2000-07-11T14:02:13Z","abstract_excerpt":"We summarize the results of a monitoring program which was executed following the cryogen exhaustion of the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) onboard the Hubble Space Telescope. During the subsequent warm-up, detector parameters such as detective quantum efficiency, dark current, bias offsets, and saturation levels have been measured over the temperature range 62K to about 100K. The measurements provide a unique database of the characteristics of PACE-I HgCdTe detector arrays in the space environment. A surprising result of the analysis is the fact that all three NICM"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0007138","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":""},"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/0007138","created_at":"2026-05-18T01:40:47.532998+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0007138v2","created_at":"2026-05-18T01:40:47.532998+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0007138","created_at":"2026-05-18T01:40:47.532998+00:00"},{"alias_kind":"pith_short_12","alias_value":"D2N2XKICH45E","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_16","alias_value":"D2N2XKICH45E2KZC","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_8","alias_value":"D2N2XKIC","created_at":"2026-05-18T12:25:49.631198+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/D2N2XKICH45E2KZCHUB2TYHVSJ","json":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ.json","graph_json":"https://pith.science/api/pith-number/D2N2XKICH45E2KZCHUB2TYHVSJ/graph.json","events_json":"https://pith.science/api/pith-number/D2N2XKICH45E2KZCHUB2TYHVSJ/events.json","paper":"https://pith.science/paper/D2N2XKIC"},"agent_actions":{"view_html":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ","download_json":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ.json","view_paper":"https://pith.science/paper/D2N2XKIC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0007138&json=true","fetch_graph":"https://pith.science/api/pith-number/D2N2XKICH45E2KZCHUB2TYHVSJ/graph.json","fetch_events":"https://pith.science/api/pith-number/D2N2XKICH45E2KZCHUB2TYHVSJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ/action/storage_attestation","attest_author":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ/action/author_attestation","sign_citation":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ/action/citation_signature","submit_replication":"https://pith.science/pith/D2N2XKICH45E2KZCHUB2TYHVSJ/action/replication_record"}},"created_at":"2026-05-18T01:40:47.532998+00:00","updated_at":"2026-05-18T01:40:47.532998+00:00"}