tonalli: an asexual genetic code to characterise APOGEE-2 stellar spectra. I. Validation with synthetic and solar spectra
arXiv:2411.15342 · doi:10.1093/rasti/rzae052
Abstract
We present tonalli, a spectroscopic analysis python code that efficiently predicts effective temperature, stellar surface gravity, metallicity, -element abundance, and rotational and radial velocities for stars with effective temperatures between 3200 and 6250 K, observed with the Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2). tonalli implements an asexual genetic algorithm to optimise the finding of the best comparison between a target spectrum and the continuum-normalised synthetic spectra library from the Model Atmospheres with a Radiative and Convective Scheme (MARCS), which is interpolated in each generation. Using simulated observed spectra and the APOGEE-2 solar spectrum of Vesta, we study the performance, limitations, accuracy and precision of our tool. Finally, a Monte Carlo realisation was implemented to estimate the uncertainties of each derived stellar parameter. The ad hoc continuum-normalised library is publicly available on Zenodo (DOI 10.5281/zenodo.12736546).
35 pages, 22 figures. Accepted to RASTI. Supplemental continuum-normalised library available at: 10.5281/zenodo.12736546
References in corpus (25)
- Array Programming with NumPy
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- The GALAH Survey: Scientific Motivation
- New Grids of ATLAS9 Model Atmospheres
- APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South
- Target Selection for the SDSS-IV APOGEE-2 Survey
- Dos and don'ts of reduced chi-squared
- The Stagger-grid: A grid of 3D stellar atmosphere models - IV. Limb darkening coefficients
- Close companions around young stars
- Final Targeting Strategy for the SDSS-IV APOGEE-2N Survey
- An empirical calibration to estimate cool dwarf fundamental parameters from H-band spectra
- IN-SYNC I: Homogeneous Stellar Parameters from High Resolution APOGEE Spectra for Thousands of Pre-main Sequence Star
- Open clusters in APOGEE and GALAH: Combining Gaia and ground-based spectroscopic surveys
- Model Atmospheres From Very Low Mass Stars to Brown Dwarfs
- The Gaia-ESO Survey: a new approach to chemically characterising young open clusters
- MONOS: Multiplicity Of Northern O-type Spectroscopic systems. I. Project description and spectral classifications and visual multiplicity of previously known objects
- Gaia Data Release 3: Chemical cartography of the Milky Way
- The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region
- APOGEE Net: An expanded spectral model of both low mass and high mass stars
- A simple algorithm for optimization and model fitting: AGA (asexual genetic algorithm)
- OCCASO V. Chemical-abundance trends with Galactocentric distance and age
- The stellar parameters and elemental abundances from low-resolution spectra I: 1.2 million giants from LAMOST DR8
- The Rotation of M Dwarfs Observed by the Apache Point Galactic Evolution Experiment
- Stellar Properties for a Comprehensive Collection of Star Forming Regions in the SDSS APOGEE-2 Survey
- A Combined Chandra and LAMOST Study of Stellar Activity