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A combined analysis of three different photometric data set ($Tycho$ B$_T$ and V$_T$ photometry, H$_p$-band data of $Hipparcos$ and $V-$band data of ASAS3 photometry) and radial velocities indicates that the system has an orbital period of 4.90494 $\\pm$ 0.00005 days and an inclination of 69$\\pm$1 degrees. This solution yields masses and radii of $M_{\\rm 1}$ = 7.57$\\pm$0.08 $M_{\\odot}$ and $R_{\\rm 1}$ = 5.82$\\pm$0.03 $R_{\\odot}$ for the primary and $M_{\\rm 2}$ = 5"},"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":"1106.5355","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-06-27T10:47:14Z","cross_cats_sorted":[],"title_canon_sha256":"5b0b2b4d16a8582b5cf21b127dd633f8afc8658e7290b565436dfff1f52ea3cb","abstract_canon_sha256":"bef8acf272353208f19f79a9708d0d299b06a975d1fec45c9b15187e38120966"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:30.451533Z","signature_b64":"pPQM5zQO7osHwKrpW87ZUWiLYCvq93PhWEVmO2sXx2EbSfUVeAqs1NmKSwF4/29m05FsC5/4LRsTf5T5fHT3Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e20ec1698e4b93246a04844f6c7ee108f1eae22d8a0195a331537ca0f543c0f9","last_reissued_at":"2026-05-18T02:01:30.451144Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:30.451144Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Absolute properties of the neglected eclipsing B-type binary HD 194495","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Cafer \\.Ibano\\u{g}lu, Esin S\\.ipah\\.i, \\\"Om\\\"ur \\c{C}akirli","submitted_at":"2011-06-27T10:47:14Z","abstract_excerpt":"We present the results of the high-resolution spectroscopic observations of the neglected binary system HD\\,194495 (B3\\,IV-V+B4\\,V). A combined analysis of three different photometric data set ($Tycho$ B$_T$ and V$_T$ photometry, H$_p$-band data of $Hipparcos$ and $V-$band data of ASAS3 photometry) and radial velocities indicates that the system has an orbital period of 4.90494 $\\pm$ 0.00005 days and an inclination of 69$\\pm$1 degrees. 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