Here we present a publicly available database of opacities for molecules of astrophysical
interest named ExoMolOP that has been compiled for over 80 species, and is based on the …

Y dwarfs are the coolest spectral class of brown dwarf. They have effective temperatures
less than 500 K, with the coolest detection as low as∼ 250 K. They make up the low-mass …

The discovery of super-Earth and mini-Neptune exoplanets means that atmospheric signals
from low-mass, temperate exoplanets are being increasingly studied. The signal acquired as …

Studies of water vapor in the atmospheres of Venus, Mars and Earth by spectroscopic
techniques are being made routinely with different instruments on board of interplanetary …

CO 2-rich planetary atmospheres such as those of Mars and Venus require accurate
knowledge of CO 2 broadened HDO half-width coefficients and their temperature …

A new method for estimation of broadening coefficients of vibrational-rotational lines of
asymmetric tops is presented. The method allows finding line widths on the basis of a few …

Air-broadening coefficients of the water isotopologue HD 16 O up to J= 50 for P, Q and R
branches calculated using different methods are presented. For partially labeled lines …

A simulation of the atmospheric solar spectra with different databanks of water vapor line
parameters is carried out. A comparison of the modeled spectra and the atmospheric …

Molecular line parameters of line strengths, self-and foreign-broadening by nitrogen, carbon
dioxide and helium gas have been experimentally determined for infrared ro-vibrational …

The air- and self-broadening coefficients of HD O (H OD) calculated using semiempirical
method Page 1 The air- and self-broadening coefficients of HD 16 O (H 16 OD) calculated …