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Selection of 147 stars, which show membership probabilities $P\\geq0.5$ were classified as likely members. The mean trigonometric parallaxes and proper-motion components of the cluster were found to be $\\varpi = 1.674 \\pm0.045$ mas and ($\\mu_{\\alpha}\\cos \\delta$,~$\\mu_{\\delta}$) =($3.814\\pm0.031$,~$3.547\\pm0.034$) mas yr$^{-1}$. Fundamental astrophysical parameters of NGC 6793 are derived simultaneously as $t$ = $650 \\pm 50$ Myr, $\\mu$ = $9.508\\pm0.07"},"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":"2503.19015","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-03-24T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"6460fef9cbb15e8ca5365b98bc4c258f187c826f54d3fb00d108ca7d5df410e4","abstract_canon_sha256":"7108ad29735c5888eaced7fe7dbbff2e9e873cfcb133ca37cf62d1e36fd5c548"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:38:48.304009Z","signature_b64":"zOQ+9LfcWl2UHuNgON2s8dETEmjSzSXjPsd4VlPIOCcizzlN8REcTR8Q0x/UEa5pp3sfqPUuo+hUYe/yXvAmDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dbc887f650f2c080bd523dc961d7d816576fb9c36fc91671fb645e2877f5b537","last_reissued_at":"2026-07-05T10:38:48.303471Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:38:48.303471Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comprehensive Analysis of Middle-Aged Open Cluster NGC 6793 in Vulpecula via Gaia DR3 Data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aly Haroon, Deniz Cennet \\c{C}{\\i}nar, Remziye Canbay, Serkan Ta\\c{s}tan, Seval Ta\\c{s}demir, Waleed Elsanhoury","submitted_at":"2025-03-24T18:00:00Z","abstract_excerpt":"We conducted an in-depth analysis of NGC 6793 open cluster via Gaia DR3 data, including astrometric, spectroscopic, and photometric measurements. 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