NuGrid Data Releases

Overview of available models

Set1 (Pignatari et al. 2016). AGB and massive stars for metallicities Z = 0.02, 0.01.
Set1ext (Ritter et al. 2018). Extension of Set1. New Z = 0.006, 0.001, 0.0001. New masses at all metallicities. All models computed with MESA.
Set1upd (Battino et al. 2019, Battino et al. 2021). Update for low-mass AGB models (M = 2 and 3 Msun) for existing metallicities (Z = 0.02, 0.01, 0.001) and new metallicities (Z = 0.03, 0.002).
super-AGB (Jones et al. 2016), super-AGB evolution with H ingestion into the He-burning convection zones.
Radioactive isotopes ccSN (Lawson et al 2022), Analysis of yields from 62 core-collapse supernovae models
iRAWD (Stephens et al 2021), i-process in rapidly accreting white dwarfs (RAWD)
Type Ia SN (Keegans et al), common envelope

NuGrid data are publically available (see below), and can be analyzed online via the Cyberhubs instance WENDI.

Nomenclature In each metallicity directory, data are organized as follows.

Sub-directory	Data
see_wind	Stellar evolution output (pre-SN)
see_exp	Massive star explosion data (delayed and rapid)
ppd_wind	Post-processing data of see_wind
ppd_exp	Post-processing data of see_exp

Sub-directories ending with yemcut include data where the remnant mass (mass-cut) of massive star models were defined using the Ye value.