MIGHTEE-HI: HI galaxy properties in the large scale structure environment at z 0.37 from a stacking experiment
arxiv(2024)
摘要
We present the first measurement of HI mass of star-forming galaxies in
different large scale structure environments from a blind survey at z∼
0.37. In particular, we carry out a spectral line stacking analysis
considering 2875 spectra of colour-selected star-forming galaxies undetected
in HI at 0.23 < z < 0.49 in the COSMOS field, extracted from the MIGHTEE-HI
Early Science datacubes, acquired with the MeerKAT radio telescope. We stack
galaxies belonging to different subsamples depending on three different
definitions of large scale structure environment: local galaxy overdensity,
position inside the host dark matter halo (central, satellite, or isolated),
and cosmic web type (field, filament, or knot). We first stack the full
star-forming galaxy sample and find a robust HI detection yielding an average
galaxy HI mass of M_ HI=(8.12± 0.75)× 10^9 M_⊙ at
∼ 11.8σ. Next, we investigate the different subsamples finding a
negligible difference in M_ HI as a function of the galaxy overdensity.
We report an HI excess compared to the full sample in satellite galaxies
(M_ HI=(11.31±1.22)× 10^9, at ∼ 10.2 σ) and in
filaments (M_ HI=(11.62± 0.90)× 10^9. Conversely, we report
non-detections for the central and knot galaxies subsamples, which appear to be
HI-deficient. We find the same qualitative results also when stacking in units
of HI fraction (f_ HI). We conclude that the HI amount in star-forming
galaxies at the studied redshifts correlates with the large scale structure
environment.
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