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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>.
| Version: | 0.2-4 |
| Depends: | R (≥ 3.1.0), MASS, parallel |
| Suggests: | lattice |
| Published: | 2021-03-29 |
| DOI: | 10.32614/CRAN.package.SCEPtER |
| Author: | Matteo Dell'Omodarme [aut, cre], Giada Valle [aut] |
| Maintainer: | Matteo Dell'Omodarme <mattdell at fastmail.fm> |
| License: | GPL-2 | GPL-3 [expanded from: GPL (≥ 2)] |
| NeedsCompilation: | yes |
| In views: | ChemPhys |
| CRAN checks: | SCEPtER results |
| Reference manual: | SCEPtER.pdf |
| Package source: | SCEPtER_0.2-4.tar.gz |
| Windows binaries: | r-devel: SCEPtER_0.2-4.zip, r-release: SCEPtER_0.2-4.zip, r-oldrel: SCEPtER_0.2-4.zip |
| macOS binaries: | r-release (arm64): SCEPtER_0.2-4.tgz, r-oldrel (arm64): SCEPtER_0.2-4.tgz, r-release (x86_64): SCEPtER_0.2-4.tgz, r-oldrel (x86_64): SCEPtER_0.2-4.tgz |
| Old sources: | SCEPtER archive |
| Reverse depends: | SCEPtERbinary |
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These binaries (installable software) and packages are in development.
They may not be fully stable and should be used with caution. We make no claims about them.