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Previous version returned an error where calling f1['rho'] did not work since 'f1' still contained an index for the star particles.
Since all we care about are the gas particles, and the star particles are at the end of the iorder (as per convention), we can set the 'iorder' and 'particle_nums' arrays to be the size of 'f.g' instead of 'f'. Then, since 'clump_nums' will be the size of 'f', we can slice the star particles at the end of the array out and mask 'f.g', 'iorder', and 'particle_nums' where 'clump_nums' > 0. This ensures that 'f1' contains only gas particles, and that all the arrays are the same size.