The Lyman-alpha forest refers to a series of absorption lines in the spectra of distant quasars caused by intervening hydrogen gas in the intergalactic medium. These absorption lines occur at the wavelength of the Lyman-alpha transition, which is a specific electromagnetic radiation emitted by hydrogen atoms. The presence of the Lyman-alpha forest allows astronomers to study the distribution and evolution of hydrogen in the universe, revealing important information about the structure of the cosmos and the processes involved in galaxy formation and evolution.