The H <scp>i</scp> content of red geyser galaxies

ABSTRACT Red geysers are a specific type of quiescent galaxy, denoted by twin jets emerging from their galactic centres. These bisymmetric possibly inject energy and heat into the surrounding material, effectively suppressing star formation stabilizing cool gas. In order to confirm presence evolutionary consequences these jets, this paper discusses scaling, stacking, conversion 21-cm H i flux data sourced i-MaNGA survey gas-to-stellar mass (G/S) spectra. Our samples were dominated non-detections, or galaxies with weak signals, consequently upper limits. The stacking technique discussed successfully resolved emission features in both red geyser G/S spectrum control sample spectrum. From stacked spectra, we find that on average, have 0.086 ± 0.011 (random) + 0.029 (systematic), while non-red similar stellar ratio 0.039 0.018 0.013 (systematic). Therefore, no statistically significant evidence content is different general population.