{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2015:XVNJ3JVTVIUK4OPIH4O6XGSI2K","short_pith_number":"pith:XVNJ3JVT","canonical_record":{"source":{"id":"1505.01647","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-05-07T10:07:24Z","cross_cats_sorted":["physics.ins-det"],"title_canon_sha256":"8e5a89eaba4e70d222c48dfb825ed87accff0971a3ef82f4fa2c24f0d93a880d","abstract_canon_sha256":"47fa4d9e0cd0727015270b93759a8e89dcb874cd5bea9406150515427a30a230"},"schema_version":"1.0"},"canonical_sha256":"bd5a9da6b3aa28ae39e83f1deb9a48d2b9c72a5e0a203a68ae0c53c99433bb33","source":{"kind":"arxiv","id":"1505.01647","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1505.01647","created_at":"2026-05-18T02:16:40Z"},{"alias_kind":"arxiv_version","alias_value":"1505.01647v1","created_at":"2026-05-18T02:16:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.01647","created_at":"2026-05-18T02:16:40Z"},{"alias_kind":"pith_short_12","alias_value":"XVNJ3JVTVIUK","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_16","alias_value":"XVNJ3JVTVIUK4OPI","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_8","alias_value":"XVNJ3JVT","created_at":"2026-05-18T12:29:50Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2015:XVNJ3JVTVIUK4OPIH4O6XGSI2K","target":"record","payload":{"canonical_record":{"source":{"id":"1505.01647","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-05-07T10:07:24Z","cross_cats_sorted":["physics.ins-det"],"title_canon_sha256":"8e5a89eaba4e70d222c48dfb825ed87accff0971a3ef82f4fa2c24f0d93a880d","abstract_canon_sha256":"47fa4d9e0cd0727015270b93759a8e89dcb874cd5bea9406150515427a30a230"},"schema_version":"1.0"},"canonical_sha256":"bd5a9da6b3aa28ae39e83f1deb9a48d2b9c72a5e0a203a68ae0c53c99433bb33","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:16:40.387501Z","signature_b64":"3UVdYmrSCt8V8xGBUrrvi3arWSZZ3tQRGW6pNbfZnKT7+v3bw0NxLTFBQPgse9hJK4do/+2ywRfvTvcjsLqQAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bd5a9da6b3aa28ae39e83f1deb9a48d2b9c72a5e0a203a68ae0c53c99433bb33","last_reissued_at":"2026-05-18T02:16:40.387013Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:16:40.387013Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1505.01647","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:16:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6bE+spUH/cdeOERsXeyiZjlPhxZ0UtNu6bst53NDk06+fNCaIlGjxRBlC8V4CKdwH/ok/lnVahSZyU5/B+h4AQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T20:39:20.660470Z"},"content_sha256":"a005df672351915d91a56ebced2e94eaec3af3e87489622c2d5caf2aec544cdc","schema_version":"1.0","event_id":"sha256:a005df672351915d91a56ebced2e94eaec3af3e87489622c2d5caf2aec544cdc"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2015:XVNJ3JVTVIUK4OPIH4O6XGSI2K","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"High-energy interactions in Kinetic Inductance Detectors arrays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A. Benoit, A. Catalano, A. D'Addabbo, A. Monfardini, J. F. Macias-Perez, J. Goupy, M. Calvo, O. Bourrion","submitted_at":"2015-05-07T10:07:24Z","abstract_excerpt":"The impacts of Cosmic Rays on the detectors are a key problem for space-based missions. We are studying the effects of such interactions on arrays of Kinetic Inductance Detectors (KID), in order to adapt this technology for use on board of satellites. Before proposing a new technology such as the Kinetic Inductance Detectors for a space-based mission, the problem of the Cosmic Rays that hit the detectors during in-flight operation has to be studied in detail. We present here several tests carried out with KID exposed to radioactive sources, which we use to reproduce the physical interactions i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.01647","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":""},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:16:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mkSqnabNkcTrwU2b8RnB6czpN3htMa2/OcpqhYI9ZdmA9pAoNZcIa8VqFqUTiqVaWlckfhkDlXq8f+nb1DhuAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-05T20:39:20.661165Z"},"content_sha256":"012ac5d91197c96832b5140c4df7d3d583dcb3f3edb9252c14997be3597aaaf7","schema_version":"1.0","event_id":"sha256:012ac5d91197c96832b5140c4df7d3d583dcb3f3edb9252c14997be3597aaaf7"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K/bundle.json","state_url":"https://pith.science/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-05T20:39:20Z","links":{"resolver":"https://pith.science/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K","bundle":"https://pith.science/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K/bundle.json","state":"https://pith.science/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K/state.json","well_known_bundle":"https://pith.science/.well-known/pith/XVNJ3JVTVIUK4OPIH4O6XGSI2K/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2015:XVNJ3JVTVIUK4OPIH4O6XGSI2K","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"47fa4d9e0cd0727015270b93759a8e89dcb874cd5bea9406150515427a30a230","cross_cats_sorted":["physics.ins-det"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-05-07T10:07:24Z","title_canon_sha256":"8e5a89eaba4e70d222c48dfb825ed87accff0971a3ef82f4fa2c24f0d93a880d"},"schema_version":"1.0","source":{"id":"1505.01647","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1505.01647","created_at":"2026-05-18T02:16:40Z"},{"alias_kind":"arxiv_version","alias_value":"1505.01647v1","created_at":"2026-05-18T02:16:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1505.01647","created_at":"2026-05-18T02:16:40Z"},{"alias_kind":"pith_short_12","alias_value":"XVNJ3JVTVIUK","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_16","alias_value":"XVNJ3JVTVIUK4OPI","created_at":"2026-05-18T12:29:50Z"},{"alias_kind":"pith_short_8","alias_value":"XVNJ3JVT","created_at":"2026-05-18T12:29:50Z"}],"graph_snapshots":[{"event_id":"sha256:012ac5d91197c96832b5140c4df7d3d583dcb3f3edb9252c14997be3597aaaf7","target":"graph","created_at":"2026-05-18T02:16:40Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"The impacts of Cosmic Rays on the detectors are a key problem for space-based missions. We are studying the effects of such interactions on arrays of Kinetic Inductance Detectors (KID), in order to adapt this technology for use on board of satellites. Before proposing a new technology such as the Kinetic Inductance Detectors for a space-based mission, the problem of the Cosmic Rays that hit the detectors during in-flight operation has to be studied in detail. We present here several tests carried out with KID exposed to radioactive sources, which we use to reproduce the physical interactions i","authors_text":"A. Benoit, A. Catalano, A. D'Addabbo, A. Monfardini, J. F. Macias-Perez, J. Goupy, M. Calvo, O. Bourrion","cross_cats":["physics.ins-det"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-05-07T10:07:24Z","title":"High-energy interactions in Kinetic Inductance Detectors arrays"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1505.01647","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:a005df672351915d91a56ebced2e94eaec3af3e87489622c2d5caf2aec544cdc","target":"record","created_at":"2026-05-18T02:16:40Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"47fa4d9e0cd0727015270b93759a8e89dcb874cd5bea9406150515427a30a230","cross_cats_sorted":["physics.ins-det"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2015-05-07T10:07:24Z","title_canon_sha256":"8e5a89eaba4e70d222c48dfb825ed87accff0971a3ef82f4fa2c24f0d93a880d"},"schema_version":"1.0","source":{"id":"1505.01647","kind":"arxiv","version":1}},"canonical_sha256":"bd5a9da6b3aa28ae39e83f1deb9a48d2b9c72a5e0a203a68ae0c53c99433bb33","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"bd5a9da6b3aa28ae39e83f1deb9a48d2b9c72a5e0a203a68ae0c53c99433bb33","first_computed_at":"2026-05-18T02:16:40.387013Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:16:40.387013Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"3UVdYmrSCt8V8xGBUrrvi3arWSZZ3tQRGW6pNbfZnKT7+v3bw0NxLTFBQPgse9hJK4do/+2ywRfvTvcjsLqQAw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:16:40.387501Z","signed_message":"canonical_sha256_bytes"},"source_id":"1505.01647","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:a005df672351915d91a56ebced2e94eaec3af3e87489622c2d5caf2aec544cdc","sha256:012ac5d91197c96832b5140c4df7d3d583dcb3f3edb9252c14997be3597aaaf7"],"state_sha256":"4cba2c9af71311c14ea37073b21f96e06fc756a1761fe456363af6db5848ab1e"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Vki8lZ6Ts1tAP00740LAFDtfAzFA+FHG89HyLJvhasysp0JPX9oTc/mpWdbku/L0JKWEYqVOeVytpJAPpCCPBQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-05T20:39:20.664684Z","bundle_sha256":"4e5c98d6b396f587638b2a84868f75bf8e59367e022cc6a687ad34ba298fc530"}}