{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:WM4PWKPLJRR2Z4LYW7DZ4QTMZF","short_pith_number":"pith:WM4PWKPL","schema_version":"1.0","canonical_sha256":"b338fb29eb4c63acf178b7c79e426cc960204f5888142cb7af9e0bb7a40503a7","source":{"kind":"arxiv","id":"2208.10337","version":2},"attestation_state":"computed","paper":{"title":"CorrSim: A Multiwavelength Timing Observation Simulator","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"John A. Paice, Poshak Gandhi, Ranjeev Misra","submitted_at":"2022-08-19T10:11:34Z","abstract_excerpt":"Studying the rapid variability of many astronomical objects is key to understanding the underlying processes at play. However, a combination of limited telescope availability, viewing constraints, and the unpredictable nature of many sources mean that obtaining data well-suited to this task can be tricky, especially when it comes to simultaneous multiwavelength observations. Researchers can often find themselves tuning observational parameters in real-time, or may realise later that their observation did not achieve their goals. Here, we present CorrSim, a program to aid planning of multiwavel"},"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":"2208.10337","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-sa/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2022-08-19T10:11:34Z","cross_cats_sorted":[],"title_canon_sha256":"50793fc506da728e22c0b6fbdd3d97ba7471015cceae9216b23aadc42e6cc034","abstract_canon_sha256":"2af04503fd658765919d44023264d49a292bd0e51709767a450d018e6bde4a70"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:55:56.268991Z","signature_b64":"siUu6h7u9LcW274bKchO3j8vB+Kw1gq9jIblKGz1aRavBrefJnrZ5KmjBX+VlFU1GYDjc/QOlcLxucrQg8O7Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b338fb29eb4c63acf178b7c79e426cc960204f5888142cb7af9e0bb7a40503a7","last_reissued_at":"2026-07-05T07:55:56.268568Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:55:56.268568Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CorrSim: A Multiwavelength Timing Observation Simulator","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"John A. Paice, Poshak Gandhi, Ranjeev Misra","submitted_at":"2022-08-19T10:11:34Z","abstract_excerpt":"Studying the rapid variability of many astronomical objects is key to understanding the underlying processes at play. However, a combination of limited telescope availability, viewing constraints, and the unpredictable nature of many sources mean that obtaining data well-suited to this task can be tricky, especially when it comes to simultaneous multiwavelength observations. Researchers can often find themselves tuning observational parameters in real-time, or may realise later that their observation did not achieve their goals. Here, we present CorrSim, a program to aid planning of multiwavel"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.10337","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/2208.10337/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":"2208.10337","created_at":"2026-07-05T07:55:56.268627+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.10337v2","created_at":"2026-07-05T07:55:56.268627+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.10337","created_at":"2026-07-05T07:55:56.268627+00:00"},{"alias_kind":"pith_short_12","alias_value":"WM4PWKPLJRR2","created_at":"2026-07-05T07:55:56.268627+00:00"},{"alias_kind":"pith_short_16","alias_value":"WM4PWKPLJRR2Z4LY","created_at":"2026-07-05T07:55:56.268627+00:00"},{"alias_kind":"pith_short_8","alias_value":"WM4PWKPL","created_at":"2026-07-05T07:55:56.268627+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/WM4PWKPLJRR2Z4LYW7DZ4QTMZF","json":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF.json","graph_json":"https://pith.science/api/pith-number/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/graph.json","events_json":"https://pith.science/api/pith-number/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/events.json","paper":"https://pith.science/paper/WM4PWKPL"},"agent_actions":{"view_html":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF","download_json":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF.json","view_paper":"https://pith.science/paper/WM4PWKPL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.10337&json=true","fetch_graph":"https://pith.science/api/pith-number/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/graph.json","fetch_events":"https://pith.science/api/pith-number/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/action/storage_attestation","attest_author":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/action/author_attestation","sign_citation":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/action/citation_signature","submit_replication":"https://pith.science/pith/WM4PWKPLJRR2Z4LYW7DZ4QTMZF/action/replication_record"}},"created_at":"2026-07-05T07:55:56.268627+00:00","updated_at":"2026-07-05T07:55:56.268627+00:00"}