The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective

We model the power spectrum of galaxies in the IllustrisTNG simulation when they are weighted by their star formation rate.

Such a weighting is relevant in the context of line-intensity mapping (LIM).

On intermediate to large scales, the model accounts for non-linear bias of star-forming galaxies and halo exclusion (a 2-halo term).

On small scales, it incorporates the weighted distribution of satellite galaxies within haloes (a 1-halo term).

The random sampling of satellite galaxies adds a shot noise term to the power spectrum on small scales, and their confinement to haloes introduces a halo shot noise term on large scales.

The full model reproduces the measured power spectrum to within a few per cent on all scales, and the fitting parameters have a clear physical meaning.

Omitting satellite galaxies from the analysis leads to an underestimation of both the large-scale bias and the mean LIM intensity by approximately 30 per cent each at redshift 1.5.

Assigning the LIM intensity of satellites to the centre of their respective haloes affects the power spectrum on scales $k > 0.3$ h Mpc$^{-1}$.

We discuss how the LIM power spectrum can be used to constrain cosmology on large scales, and galaxy formation on smaller scales, with our fitting function providing an accurate and well-motivated parametrisation.

;Comment: 31 pages, 25 figures.

Submitted to MNRAS.

We welcome comments