The atmospheric chemistry suite (ACS) of three spectrometers for the ExoMars 2016 trace gas orbiter

O Korablev, F Montmessin, A Trokhimovskiy… - Space Science …, 2018 - Springer
Abstract The Atmospheric Chemistry Suite (ACS) package is an element of the Russian
contribution to the ESA-Roscosmos ExoMars 2016 Trace Gas Orbiter (TGO) mission. ACS …

Recent advances in collisional effects on spectra of molecular gases and their practical consequences

JM Hartmann, H Tran, R Armante, C Boulet… - Journal of Quantitative …, 2018 - Elsevier
We review progress, since publication of the book``Collisional effects on molecular spectra:
Laboratory experiments and models, consequences for applications"(Elsevier, Amsterdam …

The ExoMol database: molecular line lists for exoplanet and other hot atmospheres

J Tennyson, SN Yurchenko, AF Al-Refaie… - Journal of Molecular …, 2016 - Elsevier
The ExoMol database (www. exomol. com) provides extensive line lists of molecular
transitions which are valid over extended temperature ranges. The status of the current …

The 2015 edition of the GEISA spectroscopic database

N Jacquinet-Husson, R Armante, NA Scott… - Journal of Molecular …, 2016 - Elsevier
The GEISA database (Gestion et Etude des Informations Spectroscopiques Atmosphériques:
Management and Study of Atmospheric Spectroscopic Information) has been developed …

[HTML][HTML] W2020: A database of validated rovibrational experimental transitions and empirical energy levels of H216O

T Furtenbacher, R Tóbiás, J Tennyson… - Journal of Physical …, 2020 - pubs.aip.org
A detailed understanding of the complex rotation–vibration spectrum of the water molecule
is vital for many areas of scientific and human activity, and thus, it is well studied in a number …

[HTML][HTML] Laboratory spectra of hot molecules: Data needs for hot super-Earth exoplanets

J Tennyson, SN Yurchenko - Molecular Astrophysics, 2017 - Elsevier
The majority of stars are now thought to support exoplanets. Many of those exoplanets
discovered thus far are categorized as rocky objects with an atmosphere. Most of these …

[HTML][HTML] Room temperature line lists for deuterated water

AA Kyuberis, NF Zobov, OV Naumenko… - Journal of Quantitative …, 2017 - Elsevier
Line lists are presented for six deuterated isotopologues of water vapor namely HD 16 O,
HD 17 O, HD 18 O, D 2 16 O, D 2 17 O and D 2 18 O. These line lists are prepared using …

A spectral line list for water isotopologues in the 1100–4100 cm− 1 region for application to CO2-rich planetary atmospheres

RR Gamache, M Farese, CL Renaud - Journal of Molecular Spectroscopy, 2016 - Elsevier
A line list of transitions for seven isotopologues of water vapor in the 1100–4100
wavenumber range has been constructed for application to atmospheres rich in CO 2. The …

The CO2 continuum absorption in the 1.10-and 1.18-μm windows on Venus from Maxwell Montes transits by SPICAV IR onboard Venus express

A Fedorova, B Bézard, JL Bertaux, O Korablev… - Planetary and Space …, 2015 - Elsevier
One of the difficulties in modeling Venus' nightside atmospheric windows is the need to
apply CO 2 continuum opacity due to collision-induced CO 2 bands and/or extreme far …

The need for laboratory work to aid in the understanding of exoplanetary atmospheres

JJ Fortney, TD Robinson, S Domagal-Goldman… - arXiv preprint arXiv …, 2016 - arxiv.org
Advancements in our understanding of exoplanetary atmospheres, from massive gas giants
down to rocky worlds, depend on the constructive challenges between observations and …