Extended Data Table 1 Properties of halo candidates hosting supermassive star formation

From: Formation of massive black holes in rapidly growing pre-galactic gas clouds

  1. The growth rate is averaged over the last 20 Myr of the simulation. The values of JLW and of the gas temperature Tc are given at the densest point. Dgal is the distance to the nearest galaxy with at least 106Mʘ of stars. The gas infall rate is the mass-averaged value within 100 pc. All data are given at z = 15 from the original Renaissance simulation of the rare-peak region.
  2. MMH.
  3. LWH.