HI4PI: a full-sky H i survey based on EBHIS and GASS
University of Bonn · Max Planck Institute for Radio Astronomy · +17 more institutions
Indexed inarxivcrossrefdoaj
Abstract
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).
Citation impact
1,570
total citations
- FWCI
- 23.84
- Percentile
- 100%
- References
- 124
Citations per year
Authors
20Topics & keywords
Topics
Keywords
- Sky
- Milky Way
- Physics
- Astronomy
- Astrophysics
- Angular resolution (graph drawing)
- Stars
No related works found for this paper.
Funding
- NSNational Science FoundationAwards: AST-1149491, CAREER, 1149491
- NANational Aeronautics and Space Administration
- CICalifornia Institute of Technology
- NRNational Radio Astronomy Observatory
- IMInternational Max Planck Research School for Environmental, Cellular and Molecular Microbiology
- CSCommonwealth Scientific and Industrial Research Organisation
- DFDeutsche ForschungsgemeinschaftAward: KE757/7-1
- ETEesti TeadusagentuurAwards: TK133, IUT26-2
- IMInternational Max Planck Research School for Advanced Methods in Process and Systems Engineering
- JPJet Propulsion Laboratory
- EREuropean Regional Development FundAwards: IUT26-2, TK133