{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:QPHNP2267RXWQM4ZDMVJFNMI2B","short_pith_number":"pith:QPHNP226","schema_version":"1.0","canonical_sha256":"83ced7eb5efc6f6833991b2a92b588d054e5899830d62ba0514dc8050fba322f","source":{"kind":"arxiv","id":"1412.6825","version":1},"attestation_state":"computed","paper":{"title":"The process of data formation for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Anna Maria Massone, Michele Piana, Nicola Pinamonti, Sara Giordano","submitted_at":"2014-12-21T19:43:17Z","abstract_excerpt":"The Spectrometer/Telescope for Imaging X-rays (STIX) is a hard X-ray imaging spectroscopy device to be mounted in the Solar Orbiter cluster with the aim of providing images and spectra of solar flaring regions at different photon energies in the range from a few keV to around 150 keV. The imaging modality of this telescope is based on the Moire pattern concept and utilizes 30 sub-collimators, each one containing a pair of co-axial grids. This paper applies Fourier analysis to provide the first rigorous description of the data formation process in STIX. Specifically, we show that, under first h"},"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":"1412.6825","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-12-21T19:43:17Z","cross_cats_sorted":[],"title_canon_sha256":"7b723215c5de248f1a4fcd9fcd2444e78f38d573422c0f2dab9d843f249e1f9a","abstract_canon_sha256":"b07956f25b0ea3682a8200f2b12832809b2807c166a30604d63a73d507dc25e9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:30:46.129932Z","signature_b64":"J8y+ffQSrVo712B/KLg0WcdXGIicxn68Mzj9ZH7PSJ/h9eqFX02uyJwMd31cmAZ30aQCT7ssBV71Y4gGy30IAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"83ced7eb5efc6f6833991b2a92b588d054e5899830d62ba0514dc8050fba322f","last_reissued_at":"2026-05-18T02:30:46.129516Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:30:46.129516Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The process of data formation for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Anna Maria Massone, Michele Piana, Nicola Pinamonti, Sara Giordano","submitted_at":"2014-12-21T19:43:17Z","abstract_excerpt":"The Spectrometer/Telescope for Imaging X-rays (STIX) is a hard X-ray imaging spectroscopy device to be mounted in the Solar Orbiter cluster with the aim of providing images and spectra of solar flaring regions at different photon energies in the range from a few keV to around 150 keV. The imaging modality of this telescope is based on the Moire pattern concept and utilizes 30 sub-collimators, each one containing a pair of co-axial grids. This paper applies Fourier analysis to provide the first rigorous description of the data formation process in STIX. Specifically, we show that, under first h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.6825","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":"1412.6825","created_at":"2026-05-18T02:30:46.129573+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.6825v1","created_at":"2026-05-18T02:30:46.129573+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.6825","created_at":"2026-05-18T02:30:46.129573+00:00"},{"alias_kind":"pith_short_12","alias_value":"QPHNP2267RXW","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"QPHNP2267RXWQM4Z","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"QPHNP226","created_at":"2026-05-18T12:28:46.137349+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/QPHNP2267RXWQM4ZDMVJFNMI2B","json":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B.json","graph_json":"https://pith.science/api/pith-number/QPHNP2267RXWQM4ZDMVJFNMI2B/graph.json","events_json":"https://pith.science/api/pith-number/QPHNP2267RXWQM4ZDMVJFNMI2B/events.json","paper":"https://pith.science/paper/QPHNP226"},"agent_actions":{"view_html":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B","download_json":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B.json","view_paper":"https://pith.science/paper/QPHNP226","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.6825&json=true","fetch_graph":"https://pith.science/api/pith-number/QPHNP2267RXWQM4ZDMVJFNMI2B/graph.json","fetch_events":"https://pith.science/api/pith-number/QPHNP2267RXWQM4ZDMVJFNMI2B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B/action/storage_attestation","attest_author":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B/action/author_attestation","sign_citation":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B/action/citation_signature","submit_replication":"https://pith.science/pith/QPHNP2267RXWQM4ZDMVJFNMI2B/action/replication_record"}},"created_at":"2026-05-18T02:30:46.129573+00:00","updated_at":"2026-05-18T02:30:46.129573+00:00"}