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).

Data access

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

Set1
Z = 0.02	Globus	Webpage
Z = 0.01	Globus	Webpage
Yield tables	Globus	Webpage
Root directory	Globus	Webpage

Set1ext
Z = 0.02	Globus	Webpage	Canfar
Z = 0.01	Globus	Webpage	Canfar
Z = 0.006	Globus	Webpage	Canfar
Z = 0.001	Globus	Webpage	Canfar
Z = 0.0001	Globus	Webpage	Canfar
Yield tables	Globus	Webpage	Canfar
Root directory	Globus	Webpage	Canfar

Set1upd
Z = 0.03	Globus	Webpage
Z = 0.02	Globus	Webpage
Z = 0.01	Globus	Webpage
Z = 0.002	Globus	Webpage
Z = 0.001	Globus	Webpage
Yield tables	Globus	Webpage
Root directory	Globus	Webpage

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.