Clustering redshifts with the 21cm-galaxy cross-bispectrum
The cross-correlation between 21-cm intensity mapping (IM) experiments and photometric surveys of galaxies (or any other cosmological tracer with a broad radial kernel) is severely degraded by the loss of long-wavelength radial modes due to Galactic foreground contamination. Higher-order correlators...
Auteurs principaux: | Guandalin, C, Carucci, IP, Alonso, D, Moodley, K |
---|---|
Format: | Journal article |
Langue: | English |
Publié: |
Oxford University Press
2022
|
Documents similaires
-
The anomalous 21-cm absorption at high redshifts
par: Fulvio Melia
Publié: (2021-03-01) -
A comparative study of intervening and associated H I 21-cm absorption profiles in redshifted galaxies
par: Curran, S, et autres
Publié: (2016) -
Probing the epoch of reionization with redshifted 21 cm HI emission
par: Bowman, Judd D. (Judd David)
Publié: (2009) -
The 2dF galaxy redshift survey: Hierarchical galaxy clustering
par: Baugh, C, et autres
Publié: (2004) -
The 2dF Galaxy Redshift Survey: hierarchical galaxy clustering
par: Baugh, C, et autres
Publié: (2004)