{"paper":{"title":"A New Galactic Extinction Map in High Ecliptic Latitudes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Hiroshi Shibai, Misato Fukagawa, Takahiro Sumi, Tsunehito Kohyama, Yasunori Hibi","submitted_at":"2012-11-11T07:46:10Z","abstract_excerpt":"In this study, we derived a galactic extinction map in high ecliptic latitudes for |\\beta| > 30 degrees. The dust temperature distribution was derived from the intensities at 100 and 140 \\mu m with a spatial resolution of 5'. The intensity at 140 \\mu m was derived from the intensities at 60 and 100 \\mu m of the IRAS data assuming two tight correlations between the intensities at 60, 100, and 140 \\mu m of the COBE/DIRBE data. We found that these correlations can be separated into two correlations by the antenna temperature of the radio continuum at 41 GHz.\n  Because the present study can trace "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.2382","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"}