{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:NLMPL3VN3QX2KFVF2FQNSUSHG2","short_pith_number":"pith:NLMPL3VN","schema_version":"1.0","canonical_sha256":"6ad8f5eeaddc2fa516a5d160d9524736882c9fbbb070c0110f594e782db9b1b2","source":{"kind":"arxiv","id":"2012.06549","version":1},"attestation_state":"computed","paper":{"title":"Transition-edge sensor detectors for the Origins Space Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Edward J. Wollack, John E. Sadleir, Peter C. Nagler","submitted_at":"2020-12-11T18:26:20Z","abstract_excerpt":"The Origins Space Telescope is one of four flagship missions under study for the 2020 Astrophysics Decadal Survey. With a 5.9 m cold (4.5 K) telescope deployed from space, Origins promises unprecedented sensitivity in the near-, mid-, and far-infrared, from 2.8 - 588 $\\mu$m. This mandates the use of ultra-sensitive and stable detectors in all of the Origins instruments. At the present, no known detectors can meet Origins' stability requirements in the near- to mid-infrared, or its sensitivity requirements in the far-infrared. In this work, we discuss the applicability of transition-edge sensor"},"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":"2012.06549","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2020-12-11T18:26:20Z","cross_cats_sorted":[],"title_canon_sha256":"994a55f0f576c9f1b943fafcb8347ad290c3deb3f9b2f22edec019c5bdb68c66","abstract_canon_sha256":"00ad438f2799def29cedd7c9e4186fe565d724315b0a60a3394da5de0d4b6e01"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:58:52.847035Z","signature_b64":"kbwuf7Vxohv5CuxDKHR4XJTMfEqRBhhbCyxmWe10lHqgCO//idhh9rlP2VG1SmINXTvQqqg9DDHk9ZHzL0F+Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ad8f5eeaddc2fa516a5d160d9524736882c9fbbb070c0110f594e782db9b1b2","last_reissued_at":"2026-07-05T01:58:52.846664Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:58:52.846664Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Transition-edge sensor detectors for the Origins Space Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Edward J. Wollack, John E. Sadleir, Peter C. Nagler","submitted_at":"2020-12-11T18:26:20Z","abstract_excerpt":"The Origins Space Telescope is one of four flagship missions under study for the 2020 Astrophysics Decadal Survey. With a 5.9 m cold (4.5 K) telescope deployed from space, Origins promises unprecedented sensitivity in the near-, mid-, and far-infrared, from 2.8 - 588 $\\mu$m. This mandates the use of ultra-sensitive and stable detectors in all of the Origins instruments. At the present, no known detectors can meet Origins' stability requirements in the near- to mid-infrared, or its sensitivity requirements in the far-infrared. In this work, we discuss the applicability of transition-edge sensor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.06549","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/2012.06549/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":"2012.06549","created_at":"2026-07-05T01:58:52.846720+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.06549v1","created_at":"2026-07-05T01:58:52.846720+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.06549","created_at":"2026-07-05T01:58:52.846720+00:00"},{"alias_kind":"pith_short_12","alias_value":"NLMPL3VN3QX2","created_at":"2026-07-05T01:58:52.846720+00:00"},{"alias_kind":"pith_short_16","alias_value":"NLMPL3VN3QX2KFVF","created_at":"2026-07-05T01:58:52.846720+00:00"},{"alias_kind":"pith_short_8","alias_value":"NLMPL3VN","created_at":"2026-07-05T01:58:52.846720+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/NLMPL3VN3QX2KFVF2FQNSUSHG2","json":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2.json","graph_json":"https://pith.science/api/pith-number/NLMPL3VN3QX2KFVF2FQNSUSHG2/graph.json","events_json":"https://pith.science/api/pith-number/NLMPL3VN3QX2KFVF2FQNSUSHG2/events.json","paper":"https://pith.science/paper/NLMPL3VN"},"agent_actions":{"view_html":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2","download_json":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2.json","view_paper":"https://pith.science/paper/NLMPL3VN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.06549&json=true","fetch_graph":"https://pith.science/api/pith-number/NLMPL3VN3QX2KFVF2FQNSUSHG2/graph.json","fetch_events":"https://pith.science/api/pith-number/NLMPL3VN3QX2KFVF2FQNSUSHG2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2/action/storage_attestation","attest_author":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2/action/author_attestation","sign_citation":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2/action/citation_signature","submit_replication":"https://pith.science/pith/NLMPL3VN3QX2KFVF2FQNSUSHG2/action/replication_record"}},"created_at":"2026-07-05T01:58:52.846720+00:00","updated_at":"2026-07-05T01:58:52.846720+00:00"}