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

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https://doi.org/10.7910/DVN/5LGNQ3
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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.
创建时间:
2012-10-11
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