{"paper":{"title":"Faint Extended OH Emission from the Local Interstellar Medium in the Direction l \\approx 108\\circ, b \\approx 5\\circ","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"John H. Black, M\\'onica Ivette Rodr\\'iguez, Ronald J. Allen, Roy S. Booth","submitted_at":"2012-02-20T19:49:37Z","abstract_excerpt":"We have mapped faint 1667 OH line emission (TA \\approx 20 - 40 mK in our \\approx 30' beam) along many lines of sight in the Galaxy covering an area of \\approx 4\\circ \\times 4\\circ in the general direction of l \\approx 108\\circ, b \\approx 5\\circ. The OH emission is widespread, similar in extent to the local HI (r </= 2 kpc) both in space and in velocity. The OH profile amplitudes show a good general correlation with those of HI in spectral channels of \\approx 1 km/s; this relation is described by TA(OH) \\approx 1.50 \\times 10^{-4} TB(HI) for values of TB(HI) </\\approx 60 - 70 K. Beyond this the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.4434","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"}