Uncertainties in the solar photospheric oxygen abundance

@article{Armas2017UncertaintiesIT,
  title={Uncertainties in the solar photospheric oxygen abundance},
  author={M. C. Armas and A. Ramos and H. Socas-Navarro},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2017}
}
The purpose of this work is to better understand the confidence limits of the photospheric solar oxygen abundance derived from three-dimensional models using the forbidden [OI] line at 6300 \AA , including correlations with other parameters involved. We worked with a three-dimensional empirical model and two solar intensity atlases. We employed Bayesian inference as a tool to determine the most probable value for the solar oxygen abundance given the model chosen. We considered a number of error… Expand

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DETERMINING THE ELEMENTAL AND ISOTOPIC COMPOSITION OF THE PRESOLAR NEBULA FROM GENESIS DATA ANALYSIS: THE CASE OF OXYGEN.
Spatially resolved measurements of the solar photospheric oxygen abundance

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