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The mean column density of O {\\small VI} in the MW is found to be log N(O {\\small VI})=14.257$_{-0.084}^{+0.096}$. The results confirm the patchiness of O {\\small VI} absorption in the MW and the column densities are higher or comparable to the LMC."},"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":"1307.6928","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-07-26T05:50:40Z","cross_cats_sorted":[],"title_canon_sha256":"1636d1b74e2cd225a16542c6b4017af90865b99fc2d59002743921aee4b24549","abstract_canon_sha256":"2193561c2d389b31abd59005788e26d0d4400f95166f541cb99e3eef31e7c604"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:48:34.335508Z","signature_b64":"T5ThEABbhhxeckeJwTwdwOjIgR6M4MVWXCti3v6DxPhhL0846aTYQ76UQL6og34c8ogyXW//PrEnnVfmvZlECg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7da5dfc1551550f398f89ce90a9a72dfca9ea56aa83c73dde8201eb8dc652c60","last_reissued_at":"2026-05-18T01:48:34.334932Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:48:34.334932Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"O~{\\small VI} absorption in the Milky Way along the Large Magellanic Cloud lines of sight","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Amit Pathak, Ananta C. 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