Movie (16 comoving Mpc volume):  lowres_16Mpc.mov  lowres_16Mpc_high.mov  lowres_16Mpc_short_fast.mov  lowres_16Mpc.avi  lowres_16Mpc_high.avi   - z>3, ~120 pc resolution, LSS background   - visualization courtesy of Ralf Kaehler |
  Movie (40 physical kpc volume):  highres_40kpc.mov  highres_40kpc.avi   - z<3, 350 Myrs, 15.2 pc resolution   - movie sequence generated with YT |
  See sections 2.4-2.5 (MC),   and sections 2.6-2.8 (MBH)   in my paper, for details |
  (1) |   The initial condition of the simulation at z=3   showing the target halo of 9.2e11 Msun |
  (2) |   The face-on views of the gas disks   sliced through the MBHs (white dots)   comparing the temperature at z=2.75   (left: no MBH Fbck / right: with MBH Fbck) |
  (3) |   Joint probability distribution functions   for the central 200 kpc sphere at z=2.75   (left: no MBH Fbck / right: with MBH Fbck) |
  (4) |   Stellar density profiles in the 20 kpc sphere   centered on the MBH at z=2.75   (red: no MBH Fbck / green: with MBH Fbck) |
  (5) |   The distribution of newly-formed stars, i.e.   molecular cloud particles of age < 10 Myr,   colored with particle mass at z=2.75 |
  (6) |   Black hole mass accretion history   (red: no MBH Fbck / green: with MBH Fbck)   (top: mass / bottom: mass accretion rate) |