N. Ben Bekhti
HI4PI: A full-sky Hi survey based on EBHIS and GASS
Ben Bekhti, N.; Flöer, L.; Keller, R.; Kerp, J.; Lenz, D.; Winkel, B.; Bailin, J.; Calabretta, M. R.; Dedes, L.; Ford, H. A.; Gibson, B. K.; Haud, U.; Janowiecki, S.; Kalberla, P. M. W.; Lockman, F. J.; McClure-Griffiths, N. M.; Murphy, T.; Nakanishi, H.; Pisano, D. J.; Staveley-Smith, L.; HI4PI Collaboration:
Authors
L. Flöer
R. Keller
J. Kerp
D. Lenz
B. Winkel
J. Bailin
M. R. Calabretta
L. Dedes
H. A. Ford
B. K. Gibson
U. Haud
S. Janowiecki
P. M. W. Kalberla
F. J. Lockman
N. M. McClure-Griffiths
T. Murphy
H. Nakanishi
D. J. Pisano
L. Staveley-Smith
HI4PI Collaboration:
Abstract
© 2016 ESO. 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). Aims. We release the H i 4π survey (HI4PI), an all-sky database of Galactic H i, which supersedes the LAB survey. Methods. The HI4PI survey is based on data from the recently completed first coverage of the Effelsberg-Bonn H i Survey (EBHIS) and from the third revision of the Galactic All-Sky Survey (GASS). EBHIS and GASS share similar angular resolution and match well in sensitivity. Combined, they are ideally suited to be a successor to LAB. Results. The new HI4PI survey outperforms the LAB in angular resolution (νFWHM= 16′.2) and sensitivity (σrms= 43 mK). Moreover, it has full spatial sampling and thus overcomes a major drawback of LAB, which severely undersamples the sky. We publish all-sky column density maps of the neutral atomic hydrogen in the Milky Way, along with full spectroscopic data, in several map projections including HEALPix.
Citation
Ben Bekhti, N., Flöer, L., Keller, R., Kerp, J., Lenz, D., Winkel, B., Bailin, J., Calabretta, M. R., Dedes, L., Ford, H. A., Gibson, B. K., Haud, U., Janowiecki, S., Kalberla, P. M. W., Lockman, F. J., McClure-Griffiths, N. M., Murphy, T., Nakanishi, H., Pisano, D. J., Staveley-Smith, L., & HI4PI Collaboration:. (2016). HI4PI: A full-sky Hi survey based on EBHIS and GASS. Astronomy and Astrophysics, 594, A116. https://doi.org/10.1051/0004-6361/201629178
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 7, 2016 |
Online Publication Date | Oct 20, 2016 |
Publication Date | Oct 1, 2016 |
Deposit Date | Jun 28, 2018 |
Publicly Available Date | Jul 12, 2018 |
Journal | Astronomy and Astrophysics |
Print ISSN | 0004-6361 |
Publisher | EDP Sciences |
Peer Reviewed | Peer Reviewed |
Volume | 594 |
Article Number | A116 |
Pages | A116 |
DOI | https://doi.org/10.1051/0004-6361/201629178 |
Keywords | Surveys; ISM : atoms; Techniques : spectroscopic |
Public URL | https://hull-repository.worktribe.com/output/889168 |
Publisher URL | http://www.aanda.org/articles/aa/abs/2016/10/aa29178-16/aa29178-16.html |
Contract Date | Oct 31, 2016 |
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Copyright Statement
© ESO, 2016
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