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).
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.
||Stellar evolution output (pre-SN)
||Massive star explosion data (delayed and rapid)
||Post-processing data of see_wind
||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.