The BINGO project. V. Further steps in component separation and bispectrum analysis
Context. Observing the neutral hydrogen distribution across the Universe via redshifted 21 cm line intensity mapping constitutes a powerful probe for cosmology. However, the redshifted 21 cm signal is obscured by the foreground emission from our Galaxy and other extragalactic foregrounds. This paper addresses the capabilities of the BINGO survey to
Fornazier, Karin S. F. et al.
Fecha de publicación:
8
2022