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2018

HI Intensity Mapping for Clustering-Based Redshift Estimation

Cunnington, Steven, Harrison, Ian, Pourtsidou, Alkistis et al.

Understand

Precision cosmology requires accurate galaxy redshifts, but next generation optical surveys will observe unprecedented numbers of resolved galaxies, placing strain on the amount of spectroscopic follow-up required.

We show how useful information can be gained on the redshift distributions of optical galaxy samples from spatial cross-correlations with intensity maps of unresolved HI (21cm) spectral line emission.
We construct a redshift distribution estimator, which we test using simulations.
We utilise the S3-SAX catalogue which includes HI emission information for each galaxy, which we use to construct HI intensity maps.