Lah, PhilipChengalur, Jayaram NBriggs, FranklinColless, MatthewDe Propris, RobertoPracy, Michaelde Blok, WillemFujita, ShinobuAjiki, MasaruShioya, YasuhiroNagao, TohruMurayama, TakashiTaniguchi, YoshiakiYagi, MasafumiOkamura, Sadanori2015-12-070035-8711http://hdl.handle.net/1885/18345We use observations from the Giant Metrewave Radio Telescope (GMRT) to measure the atomic hydrogen gas content of star-forming galaxies at z = 0.24 (i.e. a look-back time of ∼3 Gyr). The sample of galaxies studied were selected from Hα-emitting fieldgaKeywords: Galaxies: evolution; Galaxies: ISM; Radio continuum: galaxies; Radio lines: galaxies200610.1111/j.1365-2966.2007.11540.x2015-12-07