Measuring the gas reservoirs in 10^{8}< M_\star<10^{11} M_\odot galaxies at 1\leq z\leq3

Understanding the gas content in galaxies, its consumption and replenishment, remains pivotal in our comprehension of the evolution of the Universe. Numerous studies have addressed this, utilizing various observational tools and analytical methods. These include examining low-transition ^{12}CO millimeter rotational lines and exploring the far-infrared and the (sub-)millimeter emission of... Show more