Potassium hydroxide (KOH) and sodium hydroxide (NaOH) are expected to occur in the atmospheres of hot rocky super-Earth exoplanets but a lack of spectroscopic data is hampering their potential detection. Using robust first-principles methodologies, comprehensive molecular line lists for KOH and NaOH that are applicable for temperatures up to T = 3500 K are presented. The KOH OYT4 line list covers the 0–6000 cm−1 (wavelengths λ > 1.67 µm) range and comprises 38 billion transitions between 7.3 million energy levels with rotational excitation up to J = 255. The NaOH OYT5 line list covers the 0–9000 cm−1 (wavelengths λ > 1.11 µm) range and contains almost 50 billion lines involving 7.9 million molecular states with rotational excitation up to J...
A new line list for H216O is presented. This line list, which is called POKAZATEL, includes transiti...
The discovery of extrasolar planets is one of the major scientific advances of the last two decades...
Here we present a publicly available database of opacities for molecules of astrophysical interest n...
Accurate rotation-vibration line lists for two molecules, NaCl and KCl, in their ground electronic s...
The atmospheres of hot rocky super-Earths will have very different spectroscopic signatures compared...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...
The desire to characterize and model the atmospheres of the many extrasolar planets that have been d...
This research is a composite of projects which have individually contributed new results to their re...
Any future detection of the calcium monohydroxide radical (CaOH) in stellar and exoplanetary atmosph...
The paper describes the construction of complete sets of hot methane lines based on accurate ab init...
Molecular line lists are of utmost importance in understanding and characterising the molecular comp...
For ten years, the ExoMol database of molecular line lists has provided vital spectroscopic data for...
The ExoMol database (www.exomol.com) provides molecular data for spectroscopic studies of hot atmosp...
Author Institution: Department of Chemistry, University of York, Heslington, York, YO10 5DD, UK; Har...
New molecular line lists for lithium hydroxide (6Li16O1H and 7Li16O1H isotopologues) covering wavele...
A new line list for H216O is presented. This line list, which is called POKAZATEL, includes transiti...
The discovery of extrasolar planets is one of the major scientific advances of the last two decades...
Here we present a publicly available database of opacities for molecules of astrophysical interest n...
Accurate rotation-vibration line lists for two molecules, NaCl and KCl, in their ground electronic s...
The atmospheres of hot rocky super-Earths will have very different spectroscopic signatures compared...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...
The desire to characterize and model the atmospheres of the many extrasolar planets that have been d...
This research is a composite of projects which have individually contributed new results to their re...
Any future detection of the calcium monohydroxide radical (CaOH) in stellar and exoplanetary atmosph...
The paper describes the construction of complete sets of hot methane lines based on accurate ab init...
Molecular line lists are of utmost importance in understanding and characterising the molecular comp...
For ten years, the ExoMol database of molecular line lists has provided vital spectroscopic data for...
The ExoMol database (www.exomol.com) provides molecular data for spectroscopic studies of hot atmosp...
Author Institution: Department of Chemistry, University of York, Heslington, York, YO10 5DD, UK; Har...
New molecular line lists for lithium hydroxide (6Li16O1H and 7Li16O1H isotopologues) covering wavele...
A new line list for H216O is presented. This line list, which is called POKAZATEL, includes transiti...
The discovery of extrasolar planets is one of the major scientific advances of the last two decades...
Here we present a publicly available database of opacities for molecules of astrophysical interest n...