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

Authors: N. Ben Bekhti, L. Flöer, Reinhard Keller, J. Kerp, Daniel Lenz, B. Winkel, Jeremy Bailin, M. R. Calabretta, L. Dedes, H. Alyson Ford, B. K. Gibson, U. Haud, Steven Janowiecki, P. M. W. Kalberla, F. J. Lockman, N. M. McClure‐Griffiths, Tara Murphy, H. Nakanishi, D. J. Pisano, L. Staveley‐Smith - Astronomy and Astrophysics 2016 cited by 1,594

Context. Measurement of the Galactic neutral atomic hydrogen (H i) column density, N H i , and brightness temperatures, T B , 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).