Abstract
We have used the Westerbork array to carry out an unbiased wide-field survey for H I emission features, achieving an RMS sensitivity of about 18 mJy/Beam at a velocity resolution of 17 km s-1 over 1800 deg2 and between -1000 < VHel
Cite
CITATION STYLE
APA
Braun, R., & Thilker, D. A. (2004). The WSRT wide-field H I survey. Astronomy & Astrophysics, 417(2), 421–435. https://doi.org/10.1051/0004-6361:20034423
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