{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:J2RGO2K6Z7QUCT4NP3QILEC7A3","short_pith_number":"pith:J2RGO2K6","schema_version":"1.0","canonical_sha256":"4ea267695ecfe1414f8d7ee085905f06f68f57bfde4da5bd6d72dd3affbbb9db","source":{"kind":"arxiv","id":"1403.6592","version":2},"attestation_state":"computed","paper":{"title":"Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Benoit, A. Catalano, A. Coulais, A. Miniussi, A. Monfardini, A. Pelissier, A. Sauv\\'e, B.P. Crill, C. Renault, C. Rosset, D. Santos, E. Br\\'eele, F. Pajot, F.-X. D\\'esert, G. Patanchon, J.J. Bock, J.-L. Puget, J. Mac\\'ias-P\\'erez, J.-M. Lamarre, L.D. Spencer, L. Fauvet, M. Chabot, M. Charra, M. Martinez, M. Piat, N. Coron, O. Guillaudin, P. Ade, P. Camus, R. Sudiwala, W. C. Jones, W. Holmes, Y. Atik, Y. Giraud-H\\'eraud","submitted_at":"2014-03-26T09:01:40Z","abstract_excerpt":"The Planck High Frequency Instrument (HFI) surveyed the sky continuously from August 2009 to January 2012. Its noise and sensitivity performance were excellent, but the rate of cosmic ray impacts on the HFI detectors was unexpectedly high. Furthermore, collisions of cosmic rays with the focal plane produced transient signals in the data (glitches) with a wide range of characteristics. A study of cosmic ray impacts on the HFI detector modules has been undertaken to categorize and characterize the glitches, to correct the HFI time-ordered data, and understand the residual effects on Planck maps "},"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":"1403.6592","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2014-03-26T09:01:40Z","cross_cats_sorted":[],"title_canon_sha256":"d3fe47d4545516b17163a06460877bd3f94d91ac25c0c27942d5cb421a5cf457","abstract_canon_sha256":"ccf1ca7951404838b40124f1f2739e1f48d537013728a4c6b63da7852087ddd9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:41:24.771225Z","signature_b64":"OmS4LwAEv2LIOJUkkyR+q5nt8BmAVIEjUXkd2722wB31tDg9KJ49TD35DkNj+qKYyc1hEc/B4oB1p5Q+CGaODw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4ea267695ecfe1414f8d7ee085905f06f68f57bfde4da5bd6d72dd3affbbb9db","last_reissued_at":"2026-05-18T02:41:24.770810Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:41:24.770810Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of particles on the Planck HFI detectors: Ground-based measurements and physical interpretation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A. Benoit, A. Catalano, A. Coulais, A. Miniussi, A. Monfardini, A. Pelissier, A. Sauv\\'e, B.P. Crill, C. Renault, C. Rosset, D. Santos, E. Br\\'eele, F. Pajot, F.-X. D\\'esert, G. Patanchon, J.J. Bock, J.-L. Puget, J. Mac\\'ias-P\\'erez, J.-M. Lamarre, L.D. Spencer, L. Fauvet, M. Chabot, M. Charra, M. Martinez, M. Piat, N. Coron, O. Guillaudin, P. Ade, P. Camus, R. Sudiwala, W. C. Jones, W. Holmes, Y. Atik, Y. Giraud-H\\'eraud","submitted_at":"2014-03-26T09:01:40Z","abstract_excerpt":"The Planck High Frequency Instrument (HFI) surveyed the sky continuously from August 2009 to January 2012. Its noise and sensitivity performance were excellent, but the rate of cosmic ray impacts on the HFI detectors was unexpectedly high. Furthermore, collisions of cosmic rays with the focal plane produced transient signals in the data (glitches) with a wide range of characteristics. A study of cosmic ray impacts on the HFI detector modules has been undertaken to categorize and characterize the glitches, to correct the HFI time-ordered data, and understand the residual effects on Planck maps "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.6592","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":"1403.6592","created_at":"2026-05-18T02:41:24.770872+00:00"},{"alias_kind":"arxiv_version","alias_value":"1403.6592v2","created_at":"2026-05-18T02:41:24.770872+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1403.6592","created_at":"2026-05-18T02:41:24.770872+00:00"},{"alias_kind":"pith_short_12","alias_value":"J2RGO2K6Z7QU","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_16","alias_value":"J2RGO2K6Z7QUCT4N","created_at":"2026-05-18T12:28:33.132498+00:00"},{"alias_kind":"pith_short_8","alias_value":"J2RGO2K6","created_at":"2026-05-18T12:28:33.132498+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/J2RGO2K6Z7QUCT4NP3QILEC7A3","json":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3.json","graph_json":"https://pith.science/api/pith-number/J2RGO2K6Z7QUCT4NP3QILEC7A3/graph.json","events_json":"https://pith.science/api/pith-number/J2RGO2K6Z7QUCT4NP3QILEC7A3/events.json","paper":"https://pith.science/paper/J2RGO2K6"},"agent_actions":{"view_html":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3","download_json":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3.json","view_paper":"https://pith.science/paper/J2RGO2K6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1403.6592&json=true","fetch_graph":"https://pith.science/api/pith-number/J2RGO2K6Z7QUCT4NP3QILEC7A3/graph.json","fetch_events":"https://pith.science/api/pith-number/J2RGO2K6Z7QUCT4NP3QILEC7A3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3/action/storage_attestation","attest_author":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3/action/author_attestation","sign_citation":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3/action/citation_signature","submit_replication":"https://pith.science/pith/J2RGO2K6Z7QUCT4NP3QILEC7A3/action/replication_record"}},"created_at":"2026-05-18T02:41:24.770872+00:00","updated_at":"2026-05-18T02:41:24.770872+00:00"}