Replication data for: Polaris Flare (DHT16)

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 the archive, the Polaris spectra were interpolated onto a standard beamwidth spaced grid.由于本次巡天观测处于高银纬区域，其观测的经度间隔为0.1429°，略大于我们常规的0.125°波束宽度（beamwidth）间隔。为将北极星光谱整合至科学档案库其他篇章发布的全银河系数据立方体中，我们将其插值至标准波束宽度间隔的网格上。