Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations

TL;DR

This study investigates the intrinsic alignments of star-forming gas in galaxies within the EAGLE simulations, revealing weaker alignments than stars and implications for radio weak lensing surveys.

Contribution

It provides the first detailed analysis of star-forming gas alignments in simulations, highlighting differences from stellar alignments and their impact on cosmic shear measurements.

Findings

Star-forming gas shows radial alignment decreasing with separation.

Alignment remains significant beyond 1 Mpc at z=0.

Weaker alignment of gas compared to stars implies less systematic uncertainty in radio surveys.

Abstract

We present measurements of the intrinsic alignments (IAs) of the star-forming gas of galaxies in the EAGLE simulations. Radio continuum imaging of this gas enables cosmic shear measurements complementary to optical surveys. We measure the orientation of star-forming gas with respect to the direction to, and orientation of, neighbouring galaxies. Star-forming gas exhibits a preferentially radial orientation-direction alignment that is a decreasing function of galaxy pair separation, but remains significant to $\gtrsim 1$ Mpc at $z=0$. The alignment is qualitatively similar to that exhibited by the stars, but is weaker at fixed separation. Pairs of galaxies hosted by more massive subhaloes exhibit stronger alignment at fixed separation, but the strong alignment of close pairs is dominated by ${\sim}L^\star$ galaxies and their satellites. At fixed comoving separation, the radial alignment is stronger at higher redshift. The orientation-orientation alignment is consistent with random at all separations, despite subhaloes exhibiting preferential parallel minor axis alignment. The weaker IA of star-forming gas than for stars stems from the former's tendency to be less well aligned with the dark matter structure of galaxies than the latter, and implies that the systematic uncertainty due to IA may be less severe in radio continuum weak lensing surveys than in optical counterparts. Alignment models equating the orientation of star-forming gas discs to that of stellar discs or the DM structure of host subhaloes will therefore overestimate the impact of IAs on radio continuum cosmic shear measurements.