Installation
About
A pipeline for estimating the stellar age, mass, and radius given observational effective temperature, [Fe/H], and astroseismic parameters. The results are obtained adopting a maximum likelihood technique over a grid of pre-computed stellar models, as described in Valle et al. (2014) doi:10.1051/0004-6361/201322210.
Key Metrics
Downloads
| Last 24 hours | 0 -100% |
| Last 7 days | 48 +45% |
| Last 30 days | 189 +10% |
| Last 90 days | 507 -4% |
| Last 365 days | 2.318 -40% |