{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:YTJNKK2BLNMSJRJTY4SPHHSCNU","short_pith_number":"pith:YTJNKK2B","schema_version":"1.0","canonical_sha256":"c4d2d52b415b5924c533c724f39e426d3689198fe07578ac0c24136625f27ac3","source":{"kind":"arxiv","id":"2111.11495","version":2},"attestation_state":"computed","paper":{"title":"The Simons Observatory: Magnetic Shielding Measurements for the Universal Multiplexing Module","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"Benjamin Keller, Bradley R. Johnson, Cody J. Duell, Erin Healy, Eve M. Vavagiakis, Heather McCarrick, Jake Connors, Johannes Hubmayr, Kaiwen Zheng, Michael D. Niemack, Nicholas F. Cothard, Nicholas Galitzki, Steve K. Choi, Yaqiong Li, Yuhan Wang, Zachary B. Huber, Zhilei Xu","submitted_at":"2021-11-22T19:42:23Z","abstract_excerpt":"The Simons Observatory (SO) includes four telescopes that will measure the temperature and polarization of the cosmic microwave background using over 60,000 highly sensitive transition-edge bolometers (TES). These multichroic TES bolometers are read out by a microwave RF SQUID multiplexing system with a multiplexing factor of 910. Given that both TESes and SQUIDs are susceptible to magnetic field pickup and that it is hard to predict how they will respond to such fields, it is important to characterize the magnetic response of these systems empirically. This information can then be used to lim"},"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":"2111.11495","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2021-11-22T19:42:23Z","cross_cats_sorted":["astro-ph.CO","physics.ins-det"],"title_canon_sha256":"be39c686af9af630a99006069c257b9ff0edd51d9f1fba799ae4673b0d6844cd","abstract_canon_sha256":"1011ffcd4c1a592728e97eea3c6ed9cbfcee57b7f6671888c28c46d2c8322c83"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:47:14.577119Z","signature_b64":"0oKhXKYrMBGvJ6M+3ufXTwaJfGKCJ6BcHsyLe8/Y+sZqC9+IjlEEOLKDy0Pon+L2pB45cLudnNjVJgXKcrjCCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c4d2d52b415b5924c533c724f39e426d3689198fe07578ac0c24136625f27ac3","last_reissued_at":"2026-07-05T05:47:14.576617Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:47:14.576617Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Simons Observatory: Magnetic Shielding Measurements for the Universal Multiplexing Module","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"Benjamin Keller, Bradley R. Johnson, Cody J. Duell, Erin Healy, Eve M. Vavagiakis, Heather McCarrick, Jake Connors, Johannes Hubmayr, Kaiwen Zheng, Michael D. Niemack, Nicholas F. Cothard, Nicholas Galitzki, Steve K. Choi, Yaqiong Li, Yuhan Wang, Zachary B. Huber, Zhilei Xu","submitted_at":"2021-11-22T19:42:23Z","abstract_excerpt":"The Simons Observatory (SO) includes four telescopes that will measure the temperature and polarization of the cosmic microwave background using over 60,000 highly sensitive transition-edge bolometers (TES). These multichroic TES bolometers are read out by a microwave RF SQUID multiplexing system with a multiplexing factor of 910. Given that both TESes and SQUIDs are susceptible to magnetic field pickup and that it is hard to predict how they will respond to such fields, it is important to characterize the magnetic response of these systems empirically. This information can then be used to lim"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.11495","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2111.11495/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":"2111.11495","created_at":"2026-07-05T05:47:14.576677+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.11495v2","created_at":"2026-07-05T05:47:14.576677+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.11495","created_at":"2026-07-05T05:47:14.576677+00:00"},{"alias_kind":"pith_short_12","alias_value":"YTJNKK2BLNMS","created_at":"2026-07-05T05:47:14.576677+00:00"},{"alias_kind":"pith_short_16","alias_value":"YTJNKK2BLNMSJRJT","created_at":"2026-07-05T05:47:14.576677+00:00"},{"alias_kind":"pith_short_8","alias_value":"YTJNKK2B","created_at":"2026-07-05T05:47:14.576677+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/YTJNKK2BLNMSJRJTY4SPHHSCNU","json":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU.json","graph_json":"https://pith.science/api/pith-number/YTJNKK2BLNMSJRJTY4SPHHSCNU/graph.json","events_json":"https://pith.science/api/pith-number/YTJNKK2BLNMSJRJTY4SPHHSCNU/events.json","paper":"https://pith.science/paper/YTJNKK2B"},"agent_actions":{"view_html":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU","download_json":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU.json","view_paper":"https://pith.science/paper/YTJNKK2B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.11495&json=true","fetch_graph":"https://pith.science/api/pith-number/YTJNKK2BLNMSJRJTY4SPHHSCNU/graph.json","fetch_events":"https://pith.science/api/pith-number/YTJNKK2BLNMSJRJTY4SPHHSCNU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU/action/storage_attestation","attest_author":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU/action/author_attestation","sign_citation":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU/action/citation_signature","submit_replication":"https://pith.science/pith/YTJNKK2BLNMSJRJTY4SPHHSCNU/action/replication_record"}},"created_at":"2026-07-05T05:47:14.576677+00:00","updated_at":"2026-07-05T05:47:14.576677+00:00"}