Compute and plot some HI Lyman-alpha line transmission profiles with plots as a funtion of HI column density and doppler width: beta.
Requirements:
Some useful HI absorption plots relevant to IGM at high redshift
Compute and plot some HI Lyman-alpha line transmission profiles with plots as a funtion of HI column density and doppler width: beta.
Requirements:
Some useful HI absorption plots relevant to IGM at high redshift