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Radio occultation is a technique used to study planetary atmospheres by means of the refraction and absorption of a spacecraft carrier signal through the atmosphere of the celestial body of interest, as detected from a ground station on Earth. This technique is usually employed by the deep space tracking and communication facilities (e.g., NASA's Deep Space Network (DSN), ESA's Estrack). Aims. We want to characterize the capabilities of the Planetary Radio Interferometry and Doppler Experiment (PRIDE) technique for radio occultation experiments, using radio telescopes equipped with Ve"},"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":"1903.01582","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2019-03-04T23:20:07Z","cross_cats_sorted":[],"title_canon_sha256":"ff538a2db95ce134ed8f64a4cffb1bea61fed74d84590bac87d719ad6599420c","abstract_canon_sha256":"520aeecaf605e63d110d3d2dab65acc3675cd17f4a3f2b16096e893ec8bacc4f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:49:01.698336Z","signature_b64":"pZkex1nApqfgQrPywE+ekvVtg6ooIM4VCyCyzyKAMYczIco6ihq5zHOGnOQzYsnJRuuVI5xdB72ZNn+EiUpBDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"590386366e85fd9f69ac329bc5cd2a4427b777dbc01880f12a22145bc8be646b","last_reissued_at":"2026-05-17T23:49:01.697912Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:49:01.697912Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Venus Express radio occultation observed by PRIDE","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A.G. 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