You will find the joint probability distribution of the host galaxies of the different merging compact objects split into three different folders:
DBH: merging black hole binaries; DNS: double neutron star; BHNS: black hole neutron star binaries
Each table contains a range for stellar masses (Ms) and star formation rate (SFR) of the simulated galaxies.
You will find the following information:
- logMsmin: first column. Minimum stellar mass in log. Units: Msun
- logMsmax: second column. Maximum stellar mass in log. Units: Msun
- logSFRmin: third column. Minimum SFR in log. Units: Msum/yr
- logSFRmax: forth column. Maximum SFR in log. Units: Msun/yr
- Prob: fifth column. Joint probability distribution in the range of logMsmin-logMsmax and logSFRmin-logSFRmax
| SNAPSHOTS | REDSHIFT |
|---|---|
| 27-28 | <~ 0.1 |
| 19 | 1.0 |
| 15 | 2.0 |
| 6 | 6.0 |
I will provide a larger sample at different redshifts in the near future.
The tables were created combining the galaxy catalogs from EAGLE simulation of 25Mpc of side, RecalL0025N0752 (see Schaye et al. 2015 for further details) togheter with the results from the population synthesis model MOBSE CC15α5 from Giacobbo & Mapelli (2018)