In this work, we report first-principle theoretical predictions of methane spectral line intensities that are competitive with (and complementary to) the best laboratory measurements. A detailed comparison with the most accurate data shows that discrepancies in integrated polyad intensities are in the range of 0.4%–2.3%. This corresponds to estimations of the best available accuracy in laboratory Fourier Transform spectra measurements for this quantity. For relatively isolated strong lines the individual intensity deviations are in the same range. A comparison with the most precise laser measurements of the multiplet intensities in the 2ν3 band gives an agreement within the experimental error margins (about 1%). This is achieved for the fir...
We have recorded laboratory high resolution Fourier transform spectra of methane (CH4) emission at 8...
Astrophysical investigations generally need both complete and accurate spectroscopic databases. Desp...
Author Institution: Laboratoire de Spectronomie Mol\'eculaire, Universit\'e de DIJON; Laboratoire de...
In this work, we report first-principle theoretical predictions of methane spectral line intensities...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
<p>Our aim is to address the question: how to generate line lists for molecular spectra containing l...
Our aim is to address the question: how to generate line lists for molecular spectra containing line...
The paper describes the construction of complete sets of hot methane lines based on accurate ab init...
The paper describes the construction of complete sets of hot methane lines based on accurate ab init...
Author Institution: Department of Physics, The Florida State University; Jet Propulsion Laboratory, ...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
Author Institution: Laboratoire de Physique (Unit\'{e} associ\'{e}e au C.N.R.S.), Universit\'{e} de ...
We have recorded laboratory high resolution Fourier transform spectra of methane (CH4) emission at 8...
Astrophysical investigations generally need both complete and accurate spectroscopic databases. Desp...
Author Institution: Laboratoire de Spectronomie Mol\'eculaire, Universit\'e de DIJON; Laboratoire de...
In this work, we report first-principle theoretical predictions of methane spectral line intensities...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
<p>Our aim is to address the question: how to generate line lists for molecular spectra containing l...
Our aim is to address the question: how to generate line lists for molecular spectra containing line...
The paper describes the construction of complete sets of hot methane lines based on accurate ab init...
The paper describes the construction of complete sets of hot methane lines based on accurate ab init...
Author Institution: Department of Physics, The Florida State University; Jet Propulsion Laboratory, ...
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency...
Author Institution: Laboratoire de Physique (Unit\'{e} associ\'{e}e au C.N.R.S.), Universit\'{e} de ...
We have recorded laboratory high resolution Fourier transform spectra of methane (CH4) emission at 8...
Astrophysical investigations generally need both complete and accurate spectroscopic databases. Desp...
Author Institution: Laboratoire de Spectronomie Mol\'eculaire, Universit\'e de DIJON; Laboratoire de...