Welcome to CRIMSONS tool!

Crimsons (Chemical evolution with the random sampling of the Initial Mass function: Studying the Origin of Nucleosynthesis Stellar products)
is a tool to study the chemical enrichment evolution from a single burst of star formation accounting the random sampling of the Initial Mass Function.

- How to run your simulations -

Global Selection

You are selecting the global parameters of the simulation

Run your simulation

N_runs:	Please specify the number of runs
M_★
Z_★	Z must be a number between -15 and 1
Δt _{SN Ia}
ƒ_{SN Ia}
seed	random fixed

Pop III Selection

You are selecting a metallicity in the Pop III range (Z_★ ≤ -4.5)

Initial Mass Function (IMF) Selection

IMF type:

m_ch

Yields Selection

AGB yields
SNe yields:
PISN yields:
SNe Ia yields

Pop II Selection

You are selecting a metallicity in the POP II range (Z_★ > -4.5)

Initial Mass Function (IMF) Selection

IMF type

m_ch = 0.35M_⊙