{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:AMLU6BU627FJ56RUG6KSGCTAHO","short_pith_number":"pith:AMLU6BU6","schema_version":"1.0","canonical_sha256":"03174f069ed7ca9efa343795230a603b97aeed4cc2803f6a271ded795dd80eb1","source":{"kind":"arxiv","id":"2209.09864","version":1},"attestation_state":"computed","paper":{"title":"Development of the Low Frequency Telescope Focal Plane Detector Modules for LiteBIRD","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.IM","authors_text":"Adrian T. Lee, Amber Hornsby, Andrew Bogdan, Aritoki Suzuki, Benjamin Westbrook, Christopher Raum, Greg Jaehnig, James A. Beall, Jason E. Austermann, Johannes Hubmayr, Kaja Rotermund, Kam Arnold, Keith L. Thompson, Masashi Hazumi, Maximiliano Silva-Feaver (for the LiteBIRD collaboration), Megan Russell, Michael J. Link, Michael R. Vissers, Nicole Farias, Nils Halverson, Samantha Stever, Shannon M. Duff, Shawn Beckman, Tomasso Ghigna, Tucker Elleflot, Yuto Minami","submitted_at":"2022-09-20T17:16:57Z","abstract_excerpt":"LiteBIRD is a JAXA-led strategic large-class satellite mission designed to measure the polarization of the cosmic microwave background and Galactic foregrounds from 34 to 448 GHz across the entire sky from L2 in the late 2020s. The scientific payload includes three telescopes which are called the low-, mid-, and high-frequency telescopes each with their own receiver that covers a portion of the mission's frequency range. The low frequency telescope will map synchrotron radiation from the Galactic foreground and the cosmic microwave background. We discuss the design, fabrication, and characteri"},"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":"2209.09864","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2022-09-20T17:16:57Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"945841de98471bd23897ae1ccdc00d9173eb063d93db2a068da5a615e2e2ad1a","abstract_canon_sha256":"5f09236d333b50bef204f7752f567e6d90283d003612f284cfcc16c528e254ba"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:59:35.434629Z","signature_b64":"i3m23Oovrq+FLmyX5D/8YXHWoIQAcNA7BU20zJwkij7t0d9yABZBMI6odCqjzhsFqt5o1LFRbAZoCYnrE9xaDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"03174f069ed7ca9efa343795230a603b97aeed4cc2803f6a271ded795dd80eb1","last_reissued_at":"2026-07-05T04:59:35.434106Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:59:35.434106Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Development of the Low Frequency Telescope Focal Plane Detector Modules for LiteBIRD","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.IM","authors_text":"Adrian T. Lee, Amber Hornsby, Andrew Bogdan, Aritoki Suzuki, Benjamin Westbrook, Christopher Raum, Greg Jaehnig, James A. Beall, Jason E. Austermann, Johannes Hubmayr, Kaja Rotermund, Kam Arnold, Keith L. Thompson, Masashi Hazumi, Maximiliano Silva-Feaver (for the LiteBIRD collaboration), Megan Russell, Michael J. Link, Michael R. Vissers, Nicole Farias, Nils Halverson, Samantha Stever, Shannon M. Duff, Shawn Beckman, Tomasso Ghigna, Tucker Elleflot, Yuto Minami","submitted_at":"2022-09-20T17:16:57Z","abstract_excerpt":"LiteBIRD is a JAXA-led strategic large-class satellite mission designed to measure the polarization of the cosmic microwave background and Galactic foregrounds from 34 to 448 GHz across the entire sky from L2 in the late 2020s. The scientific payload includes three telescopes which are called the low-, mid-, and high-frequency telescopes each with their own receiver that covers a portion of the mission's frequency range. The low frequency telescope will map synchrotron radiation from the Galactic foreground and the cosmic microwave background. We discuss the design, fabrication, and characteri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.09864","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/2209.09864/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":"2209.09864","created_at":"2026-07-05T04:59:35.434182+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.09864v1","created_at":"2026-07-05T04:59:35.434182+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.09864","created_at":"2026-07-05T04:59:35.434182+00:00"},{"alias_kind":"pith_short_12","alias_value":"AMLU6BU627FJ","created_at":"2026-07-05T04:59:35.434182+00:00"},{"alias_kind":"pith_short_16","alias_value":"AMLU6BU627FJ56RU","created_at":"2026-07-05T04:59:35.434182+00:00"},{"alias_kind":"pith_short_8","alias_value":"AMLU6BU6","created_at":"2026-07-05T04:59:35.434182+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/AMLU6BU627FJ56RUG6KSGCTAHO","json":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO.json","graph_json":"https://pith.science/api/pith-number/AMLU6BU627FJ56RUG6KSGCTAHO/graph.json","events_json":"https://pith.science/api/pith-number/AMLU6BU627FJ56RUG6KSGCTAHO/events.json","paper":"https://pith.science/paper/AMLU6BU6"},"agent_actions":{"view_html":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO","download_json":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO.json","view_paper":"https://pith.science/paper/AMLU6BU6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.09864&json=true","fetch_graph":"https://pith.science/api/pith-number/AMLU6BU627FJ56RUG6KSGCTAHO/graph.json","fetch_events":"https://pith.science/api/pith-number/AMLU6BU627FJ56RUG6KSGCTAHO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO/action/storage_attestation","attest_author":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO/action/author_attestation","sign_citation":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO/action/citation_signature","submit_replication":"https://pith.science/pith/AMLU6BU627FJ56RUG6KSGCTAHO/action/replication_record"}},"created_at":"2026-07-05T04:59:35.434182+00:00","updated_at":"2026-07-05T04:59:35.434182+00:00"}