Neutral hydrogen (H I) gas content of galaxies at z ≈ 0.32
We use observations made with the Giant Metrewave Radio Telescope (GMRT) to probe the neutral hydrogen (H I) gas content of field galaxies in the VIMOS VLT Deep Survey (VVDS) 14h field at z ≈ 0.32. Because the HI emission from individual galaxies is too faint to detect at this redshift, we use an HI spectral stacking technique using the known optical positions and redshifts of the 165 galaxies in our sample to co-add theirHI spectra and thus obtain the average HI mass of the galaxies. Stacked...[Show more]
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|Access Rights:||Open Access|
|01_Rhee_Neutral_hydrogen_%28H_I%29_gas_2018.pdf||3.77 MB||Adobe PDF|
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