Files deposited are python script and Mathematica notebook for the ApJ paper, entitled “Anisotropic Magnetized Asteroseismic Waves.” The file "mathematica_notebook_calc.nb" is the Mathematica notebook where analytical manipulations of lengthy terms are carried out. The script "polytrope_run10.py" numerically evaluates—using the spectral solver Dedalus (https://dedalus-project.org/) and MPI-parallelization—eigenmodes for a wide range of $(k_x, k_y)$ for the linear waves in a polytropic atmosphere. An inhomogeneous magnetic field, directed orthogonal to a constant vertical gravity, varies as $\mathbf{B_0}(z) \sim z^{(n+1)/2} \hat{\mathbf{e}}_{x}$. Gas pressure and magnetic pressure both vary as $\sim z^{n+1}$, and density varies as $\sim z^n$ where n is the polytropic index. Authors: B. TripathiDepartment of Physics, University of Wisconsin–Madison, Madison, Wisconsin 53706, USAORCID: 0000-0002-4723-2170Email: btripathi@wisc.edu Dhrubaditya MitraNordita, KTH Royal Institute of Technology and Stockholm University, Hannes Alfvéns väg 12, 114 19 Stockholm, SwedenORCID: 0000-0003-4861-8152Email: dhruba.mitra@gmail.com