HI4PI: a full-sky H i survey based on EBHIS and GASS

作者：Nadya Ben Bekhti, L. Flöer, Reinhard Keller, J. Kerp, Daniel R. Lenz, B. Winkel, Jeremy Bailin, Mark R. Calabretta, Leonidas Dedes, H. Alyson Ford, Brad K. Gibson, U. Haud, Steven Janowiecki, P. M. W. Kalberla, F. J. Lockman, N. M. McClure‐Griffiths, Tara Murphy, H. Nakanishi, Daniel Joseph Pisano, Lister Staveley‐Smith · 发表于：Astronomy and Astrophysics · 年份：2016 · DOI：10.1051/0004-6361/201629178 · 被引用次数：1657 · 研究领域：Astrophysics and Star Formation Studies、Stellar, planetary, and galactic studies、Astrophysical Phenomena and Observations

Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, NH i, and brightness temperatures, TB, is of high scientific value for a broad range of astrophysical disciplines. In the past two decades, one of the most-used legacy H i datasets has been the Leiden/Argentine/Bonn Survey (LAB).