A general method for the estimation of the confidence interval of molecular absorption coefficients is presented. It combines statistical numerical experiments with analytical calculations. The method uses line parameter predictions (position and intensity) with known estimated uncertainties. The propagation of errors from line parameters to absorption coefficients or cross-sections are analyzed in detail as a function of the resolution. This work is especially intended to provide expert information for applications requiring theoretical predictions for which the present state of the art of line by line high-resolution modeling is not accurate enough to meet the experimental precision. As an illustration, it is applied to predict the absorp...
Infrared absorption spectra of hot methane up to 1000 K were recorded with a high-resolution Fourier...
Aims. We describe an ab initio-based numerical method of obtaining infrared spectroscopic data (line...
Author Institution: Department of Physics, College of William and Mary, Williamsburg, VA 23187-8795;...
A general method for the estimation of the confidence interval of molecular absorption coefficients ...
A general method for the estimation of the confidence interval of molecular absorption coefficients ...
La version V2 inclut les modifications proposées par les reviewers.International audienceA general m...
International audienceAstrophysical investigations generally need both complete and accurate spectro...
Astrophysical investigations generally need both complete and accurate spectroscopic databases. Desp...
International audienceRemote sensing of the atmosphere of astrophysical objects relies essentially o...
Spectra of hot methane were recorded using a tube furnace and a high-resolution Fourier transform sp...
Hot methane is found in many cool sub-stellar astronomical sources including brown dwarfs and exop...
In this work, we report first-principle theoretical predictions of methane spectral line intensities...
Author Institution:A $0.02 cm^{-1}$ resolution study of the absorption line strengths of methane in...
Author Institution: Department of Chemistry, University of Missouri-St. LouisMethane spectral featur...
The spectroscopic knowledge of methane is important to study the greenhouse effect and some planetar...
Infrared absorption spectra of hot methane up to 1000 K were recorded with a high-resolution Fourier...
Aims. We describe an ab initio-based numerical method of obtaining infrared spectroscopic data (line...
Author Institution: Department of Physics, College of William and Mary, Williamsburg, VA 23187-8795;...
A general method for the estimation of the confidence interval of molecular absorption coefficients ...
A general method for the estimation of the confidence interval of molecular absorption coefficients ...
La version V2 inclut les modifications proposées par les reviewers.International audienceA general m...
International audienceAstrophysical investigations generally need both complete and accurate spectro...
Astrophysical investigations generally need both complete and accurate spectroscopic databases. Desp...
International audienceRemote sensing of the atmosphere of astrophysical objects relies essentially o...
Spectra of hot methane were recorded using a tube furnace and a high-resolution Fourier transform sp...
Hot methane is found in many cool sub-stellar astronomical sources including brown dwarfs and exop...
In this work, we report first-principle theoretical predictions of methane spectral line intensities...
Author Institution:A $0.02 cm^{-1}$ resolution study of the absorption line strengths of methane in...
Author Institution: Department of Chemistry, University of Missouri-St. LouisMethane spectral featur...
The spectroscopic knowledge of methane is important to study the greenhouse effect and some planetar...
Infrared absorption spectra of hot methane up to 1000 K were recorded with a high-resolution Fourier...
Aims. We describe an ab initio-based numerical method of obtaining infrared spectroscopic data (line...
Author Institution: Department of Physics, College of William and Mary, Williamsburg, VA 23187-8795;...