Underlying data for initial conditions for MOCCA star cluster models simulated in Bhat et al. 2024

We provide the initial conditions for the MOCCA star cluster models simulated for the publication Bhat et al. 2024 (https://ui.adsabs.harvard.edu/abs/2024ApJ...968....2B/abstract). The CSV file contains the following information for the 108 models that were simulated as part of this study. 

Model Name: The unique identifier for each simulation model. It is constructed based on the initial conditions of the model using the following format:Example: N500_K0_RG2_TF0.1_W05 corresponds to a simulation with 500K stars, k=0, Rg=2 kpc. TF=0.1 and W0=5.

N (K): The total number of objects in the simulation, in units of thousands (K). For instance, 500 means 500,000 objects. All simulate models had 10% initial binary fraction.

W0: The dimensionless central potential of the King model used to define the initial density profile of the star cluster. Values include 5, 7, etc.

k: The parameter representing the Black Hole (BH) kick velocity prescription:

0: Maxwellian distribution of kick velocities with σ=265  km/s (Hobbs et al., 2005).

1: Reduced kick velocities based on the mass fallback prescription (Belczynski et al., 2002).

Rg (kpc): The initial galactocentric distance of the cluster in kiloparsecs (kpc). Possible values are 2, 4, and 6 kpc.

TF (rh/rt): The tidal filling factor, defined as the ratio of the half-mass radius to the tidal radius (rh/rt). Possible values are 0.025, 0.05, and 0.1.