The authors found that the merger rate per unit redshift is nearly universal and independent of redshift, scaling simply with halo mass and mass ratio.
The identifier refers to the last part of a Digital Object Identifier (DOI) for a specific academic paper. The paper associated with this identifier is: 🌌 The Paper
Monthly Notices of the Royal Astronomical Society (MNRAS), Vol. 386, Issue 2, pp. 577–592 (May 2008) Full DOI: 10.1111/j.1365-2966.2008.13075.x 📝 Summary of Content
It utilizes the massive public database of the Millennium Simulation to track merger trees over a wide dynamic range in time and mass.
The authors found that the merger rate per unit redshift is nearly universal and independent of redshift, scaling simply with halo mass and mass ratio.
The identifier refers to the last part of a Digital Object Identifier (DOI) for a specific academic paper. The paper associated with this identifier is: 🌌 The Paper
Monthly Notices of the Royal Astronomical Society (MNRAS), Vol. 386, Issue 2, pp. 577–592 (May 2008) Full DOI: 10.1111/j.1365-2966.2008.13075.x 📝 Summary of Content
It utilizes the massive public database of the Millennium Simulation to track merger trees over a wide dynamic range in time and mass.