Infrared laser-absorption spectroscopy (IR-LAS) sensors play an important role in
diagnosing and characterizing a wide range of combustion systems. Of all the laser …

The nature of the early martian climate is one of the major unanswered questions of
planetary science. Key challenges remain, but a new wave of orbital and in situ observations …

Identifying terrestrial planets in the habitable zones (HZs) of other stars is one of the primary
goals of ongoing radial velocity (RV) and transit exoplanet surveys and proposed future …

The TRAPPIST-1 system, consisting of an ultracool host star having seven known Earth-
sized planets, will be a prime target for atmospheric characterization with the James Webb …

On the basis of geological evidence, it is often stated that the early martian climate was
warm enough for liquid water to flow on the surface thanks to the greenhouse effect of a thick …

The presence of valleys on ancient terrains of Mars suggests that liquid water flowed on the
martian surface 3.8 Gyr ago or before. The above-freezing temperatures required to explain …

TRAPPIST-1 planets are invaluable for the study of comparative planetary science outside
our solar system and possibly habitability. Both transit timing variations (TTV) of the planets …

We used ground‐based near‐infrared (NIR) observations of thermal emission from the
Venus nightside to determine the temperature structure and water vapor distribution …

Statistical narrow-band (SNB) model parameters for H2O, CO2, CH4 and CO, and correlated-
k (CK) parameters for H2O and CO2 are generated from line by line calculations and …

The upcoming deployment of the James Webb Space Telescope will dramatically advance
our ability to characterize exoplanet atmospheres, both in terms of precision and sensitivity …