Replication data for: Ursa Major, de Vries (DHT20)

Owing to the high latitude of this survey, the longitude spacing of the observations is 0.1429 °, slightly larger than our normal \"beamwidth\" spacing of 0.125°. For incorporation into the whole-Galaxy cubes presented elsewhere in this archive, these spectra were interpolated onto a standard beamwidth spaced grid. There are additional clouds in Ursa Major.

鉴于本巡天项目的观测纬度较高，观测的经度间隔为0.1429°，略大于常规的‘波束宽度（beamwidth）’间隔0.125°。为将这些光谱数据整合至本档案库其他章节所刊载的全银河数据立方体（whole-Galaxy cubes）中，我们将其插值至标准波束宽度间隔的网格上。大熊座（Ursa Major）区域还存在额外的星际云团。