{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:Q5ICDVEPLXUGIIJOSXEVEYMSYK","short_pith_number":"pith:Q5ICDVEP","canonical_record":{"source":{"id":"1807.11446","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2018-07-30T17:03:26Z","cross_cats_sorted":[],"title_canon_sha256":"b0d12831c5ef1a12dd128b05fe38d0ce1a8b8b240e0340f07f8d1dd449c6d624","abstract_canon_sha256":"cd18da4bc92f2306478b5044dd181ac37af1536a383c05d8e68635eb3d82bf9f"},"schema_version":"1.0"},"canonical_sha256":"875021d48f5de864212e95c9526192c2b3c00c8a4bba16c27450233d9bca8a90","source":{"kind":"arxiv","id":"1807.11446","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1807.11446","created_at":"2026-05-17T23:58:59Z"},{"alias_kind":"arxiv_version","alias_value":"1807.11446v3","created_at":"2026-05-17T23:58:59Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.11446","created_at":"2026-05-17T23:58:59Z"},{"alias_kind":"pith_short_12","alias_value":"Q5ICDVEPLXUG","created_at":"2026-05-18T12:32:46Z"},{"alias_kind":"pith_short_16","alias_value":"Q5ICDVEPLXUGIIJO","created_at":"2026-05-18T12:32:46Z"},{"alias_kind":"pith_short_8","alias_value":"Q5ICDVEP","created_at":"2026-05-18T12:32:46Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:Q5ICDVEPLXUGIIJOSXEVEYMSYK","target":"record","payload":{"canonical_record":{"source":{"id":"1807.11446","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2018-07-30T17:03:26Z","cross_cats_sorted":[],"title_canon_sha256":"b0d12831c5ef1a12dd128b05fe38d0ce1a8b8b240e0340f07f8d1dd449c6d624","abstract_canon_sha256":"cd18da4bc92f2306478b5044dd181ac37af1536a383c05d8e68635eb3d82bf9f"},"schema_version":"1.0"},"canonical_sha256":"875021d48f5de864212e95c9526192c2b3c00c8a4bba16c27450233d9bca8a90","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:59.114583Z","signature_b64":"VHfQiGwfjnaH5MCOcGXtViJIx3UG9GqAF/8UUo2QpXLixfu5QZmp3lXBCga5NqXefz1yPwglvveDffnb8AE4Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"875021d48f5de864212e95c9526192c2b3c00c8a4bba16c27450233d9bca8a90","last_reissued_at":"2026-05-17T23:58:59.113926Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:59.113926Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1807.11446","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-17T23:58:59Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ww9x+nX0mDoLr0AQydE1RShf829qte6Nb9u6SOZ3/VYQzQ4P9/5OirqWKn70AfyLk7JRHnmRXXxN9cMMpbe2Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T16:51:21.900700Z"},"content_sha256":"a6c14057449d2e3aed2e5751347e6398491c751b2a1c9bdd718738da14208481","schema_version":"1.0","event_id":"sha256:a6c14057449d2e3aed2e5751347e6398491c751b2a1c9bdd718738da14208481"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:Q5ICDVEPLXUGIIJOSXEVEYMSYK","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A data acquisition and control system for large mass bolometer arrays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.ins-det","authors_text":"A. Branca, A. Caminata, A. Giachero, E. Guardincerri, L. Canonica, L. Marini, M. Pallavicini, M. Vignati, S. Copello, S. Di Domizio","submitted_at":"2018-07-30T17:03:26Z","abstract_excerpt":"During the last couple of decades, the use of arrays of bolometers has represented one of the leading techniques for the search for rare events. CUORE, an array of 988 TeO$_2$ bolometers that is taking data since April 2017 at the Laboratori Nazionali del Gran Sasso (Italy), exploits the large mass, low background, good energy resolution and low energy threshold of these detectors successfully. Thanks to these characteristics, they could be also sensitive to other low energy rare processes, such as galactic dark matter interactions. In this paper we describe the data acquisition system that wa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.11446","kind":"arxiv","version":3},"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":"2026-05-17T23:58:59Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"f5SYLGl3MWDEzAPAZUXTVXxmz/hOHPfQ5IJ0kiQ1pH6smhbMUjolVNUvQ0xBDGnUZT+pxOXNqhAir8eap8eyCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T16:51:21.901440Z"},"content_sha256":"bfcc9628dc1298c2548c1e5ff5cf3f2b02c84dfd63ba3f029d207da85b7187ee","schema_version":"1.0","event_id":"sha256:bfcc9628dc1298c2548c1e5ff5cf3f2b02c84dfd63ba3f029d207da85b7187ee"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK/bundle.json","state_url":"https://pith.science/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK/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":"2026-05-25T16:51:21Z","links":{"resolver":"https://pith.science/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK","bundle":"https://pith.science/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK/bundle.json","state":"https://pith.science/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK/state.json","well_known_bundle":"https://pith.science/.well-known/pith/Q5ICDVEPLXUGIIJOSXEVEYMSYK/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:Q5ICDVEPLXUGIIJOSXEVEYMSYK","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":"cd18da4bc92f2306478b5044dd181ac37af1536a383c05d8e68635eb3d82bf9f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2018-07-30T17:03:26Z","title_canon_sha256":"b0d12831c5ef1a12dd128b05fe38d0ce1a8b8b240e0340f07f8d1dd449c6d624"},"schema_version":"1.0","source":{"id":"1807.11446","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1807.11446","created_at":"2026-05-17T23:58:59Z"},{"alias_kind":"arxiv_version","alias_value":"1807.11446v3","created_at":"2026-05-17T23:58:59Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.11446","created_at":"2026-05-17T23:58:59Z"},{"alias_kind":"pith_short_12","alias_value":"Q5ICDVEPLXUG","created_at":"2026-05-18T12:32:46Z"},{"alias_kind":"pith_short_16","alias_value":"Q5ICDVEPLXUGIIJO","created_at":"2026-05-18T12:32:46Z"},{"alias_kind":"pith_short_8","alias_value":"Q5ICDVEP","created_at":"2026-05-18T12:32:46Z"}],"graph_snapshots":[{"event_id":"sha256:bfcc9628dc1298c2548c1e5ff5cf3f2b02c84dfd63ba3f029d207da85b7187ee","target":"graph","created_at":"2026-05-17T23:58:59Z","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":"During the last couple of decades, the use of arrays of bolometers has represented one of the leading techniques for the search for rare events. CUORE, an array of 988 TeO$_2$ bolometers that is taking data since April 2017 at the Laboratori Nazionali del Gran Sasso (Italy), exploits the large mass, low background, good energy resolution and low energy threshold of these detectors successfully. Thanks to these characteristics, they could be also sensitive to other low energy rare processes, such as galactic dark matter interactions. In this paper we describe the data acquisition system that wa","authors_text":"A. Branca, A. Caminata, A. Giachero, E. Guardincerri, L. Canonica, L. Marini, M. Pallavicini, M. Vignati, S. Copello, S. Di Domizio","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2018-07-30T17:03:26Z","title":"A data acquisition and control system for large mass bolometer arrays"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.11446","kind":"arxiv","version":3},"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:a6c14057449d2e3aed2e5751347e6398491c751b2a1c9bdd718738da14208481","target":"record","created_at":"2026-05-17T23:58:59Z","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":"cd18da4bc92f2306478b5044dd181ac37af1536a383c05d8e68635eb3d82bf9f","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2018-07-30T17:03:26Z","title_canon_sha256":"b0d12831c5ef1a12dd128b05fe38d0ce1a8b8b240e0340f07f8d1dd449c6d624"},"schema_version":"1.0","source":{"id":"1807.11446","kind":"arxiv","version":3}},"canonical_sha256":"875021d48f5de864212e95c9526192c2b3c00c8a4bba16c27450233d9bca8a90","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"875021d48f5de864212e95c9526192c2b3c00c8a4bba16c27450233d9bca8a90","first_computed_at":"2026-05-17T23:58:59.113926Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-17T23:58:59.113926Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"VHfQiGwfjnaH5MCOcGXtViJIx3UG9GqAF/8UUo2QpXLixfu5QZmp3lXBCga5NqXefz1yPwglvveDffnb8AE4Cg==","signature_status":"signed_v1","signed_at":"2026-05-17T23:58:59.114583Z","signed_message":"canonical_sha256_bytes"},"source_id":"1807.11446","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:a6c14057449d2e3aed2e5751347e6398491c751b2a1c9bdd718738da14208481","sha256:bfcc9628dc1298c2548c1e5ff5cf3f2b02c84dfd63ba3f029d207da85b7187ee"],"state_sha256":"b341ac71be8ff148a901567683a1c2a4d14f2197ae7049f223789619360ee368"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"w+jm3eKXi2lyKDw8v5bMTeopkuE1JI2Pslqrw2Lvd18mQfqqTCl9059vXdWgOv9laJNBCOYpVRfqSilIb4NADA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T16:51:21.905974Z","bundle_sha256":"e6d7f95fb27878a3c5d222bef4cc4b9c7c50b8b7d10b04d4b6950104ede53b01"}}