Photochemically produced SO2 in the atmosphere of WASP-39b
Photochemistry is a fundamental process of planetary atmospheres that regulates the
atmospheric composition and stability. However, no unambiguous photochemical products …
atmospheric composition and stability. However, no unambiguous photochemical products …
[HTML][HTML] The 2024 release of the ExoMol database: Molecular line lists for exoplanet and other hot atmospheres
The ExoMol database (www. exomol. com) provides molecular data for spectroscopic
studies of hot atmospheres. These data are widely used to model atmospheres of …
studies of hot atmospheres. These data are widely used to model atmospheres of …
The ExoMolOP database: Cross sections and k-tables for molecules of interest in high-temperature exoplanet atmospheres
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 …
interest named ExoMolOP that has been compiled for over 80 species, and is based on the …
What it takes to compute highly accurate rovibrational line lists for use in astrochemistry
Conspectus We review the Best Theory+ Reliable High-Resolution Experiment (BTRHE)
strategy for obtaining highly accurate molecular rovibrational line lists with InfraRed (IR) …
strategy for obtaining highly accurate molecular rovibrational line lists with InfraRed (IR) …
The impending opacity challenge in exoplanet atmospheric characterization
With a new generation of observatories coming online this decade, the process of
characterizing exoplanet atmospheres will need to be reinvented. Currently mostly on the …
characterizing exoplanet atmospheres will need to be reinvented. Currently mostly on the …
Atmospheric regimes and trends on exoplanets and brown dwarfs
X Zhang - Research in Astronomy and Astrophysics, 2020 - iopscience.iop.org
A planetary atmosphere is the outer gas layer of a planet. Besides its scientific significance
among the first and most accessible planetary layers observed from space, it is closely …
among the first and most accessible planetary layers observed from space, it is closely …
[HTML][HTML] Collisional broadening of molecular rovibronic lines
J Buldyreva, RP Brady, SN Yurchenko… - Journal of Quantitative …, 2024 - Elsevier
To meet burning needs of high-resolution pressure-induced line-shape parameters in the
UV/visible regions for hot-temperature industrial and atmospheric applications as well as …
UV/visible regions for hot-temperature industrial and atmospheric applications as well as …
Water-vapor absorption database using dual comb spectroscopy from 300 to 1300 K part I: Pure H2O, 6600 to 7650 cm-1
We present broadband dual frequency comb laser measurements of pure H 2 O absorption
(natural isotopic abundance of 99.7% H 2 16 O) from 6600 to 7650 cm− 1 (1307–1515 nm) …
(natural isotopic abundance of 99.7% H 2 16 O) from 6600 to 7650 cm− 1 (1307–1515 nm) …
Detectability of biosignatures on LHS 1140 b
F Wunderlich, M Scheucher, JL Grenfell… - Astronomy & …, 2021 - aanda.org
Context. Terrestrial extrasolar planets around low-mass stars are prime targets when
searching for atmospheric biosignatures with current and near-future telescopes. The …
searching for atmospheric biosignatures with current and near-future telescopes. The …
[HTML][HTML] Accurate calculations of beyond-Voigt line-shape parameters from first principles for the He-perturbed HD rovibrational lines: A comprehensive dataset in the …
We report a comprehensive dataset of beyond-Voigt line-shape parameters (pressure
broadening and shift coefficients, their speed-dependences, and the complex Dicke …
broadening and shift coefficients, their speed-dependences, and the complex Dicke …