{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:42NWD73A4VZ3OHHBFSIRL2CWNK","short_pith_number":"pith:42NWD73A","schema_version":"1.0","canonical_sha256":"e69b61ff60e573b71ce12c9115e8566a9508562d9864bf12d2a846f9c6b386cc","source":{"kind":"arxiv","id":"1204.2920","version":1},"attestation_state":"computed","paper":{"title":"The 10 Tesla muSR instrument: detector solutions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.ins-det","authors_text":"A.Amato, A.Stoykov, J.Rodriguez, K.Sedlak, R.Scheuermann, U.Greuter","submitted_at":"2012-04-13T08:51:29Z","abstract_excerpt":"Solutions to the detector system of the High-Field muSR instrument at the Paul Scherrer Institut (PSI) in Switzerland are presented. The strict technical requirements are fulfilled through the application of Geiger-mode Avalanche Photodiodes."},"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":"1204.2920","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2012-04-13T08:51:29Z","cross_cats_sorted":[],"title_canon_sha256":"00fdc4c9da32e1aa457217b0811154810f5898d1cd48a0e351444321324be12c","abstract_canon_sha256":"eed4b4dde2a62fa8593eaf39527acfea7c0f9696f92115013cd028337265af1f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:54:14.804597Z","signature_b64":"kgHZ5l/gtZ/8q+3EnbZXs7qbMC/xK9Mw1px9jlsrKBpkE3XtI8v88MC6SFHWyb/qszTH8e05TZiiZSJ+T50YBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e69b61ff60e573b71ce12c9115e8566a9508562d9864bf12d2a846f9c6b386cc","last_reissued_at":"2026-05-18T03:54:14.804067Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:54:14.804067Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The 10 Tesla muSR instrument: detector solutions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.ins-det","authors_text":"A.Amato, A.Stoykov, J.Rodriguez, K.Sedlak, R.Scheuermann, U.Greuter","submitted_at":"2012-04-13T08:51:29Z","abstract_excerpt":"Solutions to the detector system of the High-Field muSR instrument at the Paul Scherrer Institut (PSI) in Switzerland are presented. The strict technical requirements are fulfilled through the application of Geiger-mode Avalanche Photodiodes."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.2920","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1204.2920","created_at":"2026-05-18T03:54:14.804136+00:00"},{"alias_kind":"arxiv_version","alias_value":"1204.2920v1","created_at":"2026-05-18T03:54:14.804136+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.2920","created_at":"2026-05-18T03:54:14.804136+00:00"},{"alias_kind":"pith_short_12","alias_value":"42NWD73A4VZ3","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_16","alias_value":"42NWD73A4VZ3OHHB","created_at":"2026-05-18T12:26:53.410803+00:00"},{"alias_kind":"pith_short_8","alias_value":"42NWD73A","created_at":"2026-05-18T12:26:53.410803+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/42NWD73A4VZ3OHHBFSIRL2CWNK","json":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK.json","graph_json":"https://pith.science/api/pith-number/42NWD73A4VZ3OHHBFSIRL2CWNK/graph.json","events_json":"https://pith.science/api/pith-number/42NWD73A4VZ3OHHBFSIRL2CWNK/events.json","paper":"https://pith.science/paper/42NWD73A"},"agent_actions":{"view_html":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK","download_json":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK.json","view_paper":"https://pith.science/paper/42NWD73A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1204.2920&json=true","fetch_graph":"https://pith.science/api/pith-number/42NWD73A4VZ3OHHBFSIRL2CWNK/graph.json","fetch_events":"https://pith.science/api/pith-number/42NWD73A4VZ3OHHBFSIRL2CWNK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK/action/storage_attestation","attest_author":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK/action/author_attestation","sign_citation":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK/action/citation_signature","submit_replication":"https://pith.science/pith/42NWD73A4VZ3OHHBFSIRL2CWNK/action/replication_record"}},"created_at":"2026-05-18T03:54:14.804136+00:00","updated_at":"2026-05-18T03:54:14.804136+00:00"}