Exoplanetary atmospheres: key insights, challenges, and prospects
N Madhusudhan - Annual Review of Astronomy and …, 2019 - annualreviews.org
Exoplanetary science is on the verge of an unprecedented revolution. The thousands of
exoplanets discovered over the past decade have most recently been supplemented by …
exoplanets discovered over the past decade have most recently been supplemented by …
Exoplanetary atmospheres—chemistry, formation conditions, and habitability
Characterizing the atmospheres of extrasolar planets is the new frontier in exoplanetary
science. The last two decades of exoplanet discoveries have revealed that exoplanets are …
science. The last two decades of exoplanet discoveries have revealed that exoplanets are …
ExoMol molecular line lists XXX: a complete high-accuracy line list for water
ABSTRACT A new line list for HO is presented. This line list, which is called POKAZATEL,
includes transitions between rotational–vibrational energy levels up to 41 000 cm− 1 and is …
includes transitions between rotational–vibrational energy levels up to 41 000 cm− 1 and is …
A chemical survey of exoplanets with ARIEL
Thousands of exoplanets have now been discovered with a huge range of masses, sizes
and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host …
and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host …
batman: basic transit model calculation in Python
L Kreidberg - Publications of the Astronomical Society of the …, 2015 - iopscience.iop.org
I introduce batman, a Python package for modeling exoplanet transit and eclipse light
curves. The batman package supports calculation of light curves for any radially symmetric …
curves. The batman package supports calculation of light curves for any radially symmetric …
Water vapour in the atmosphere of the habitable-zone eight-Earth-mass planet K2-18 b
In the past decade, observations from space and the ground have found water to be the
most abundant molecular species, after hydrogen, in the atmospheres of hot, gaseous …
most abundant molecular species, after hydrogen, in the atmospheres of hot, gaseous …
The transit light source effect: false spectral features and incorrect densities for M-dwarf transiting planets
Transmission spectra are differential measurements that utilize stellar illumination to probe
transiting exoplanet atmospheres. Any spectral difference between the illuminating light …
transiting exoplanet atmospheres. Any spectral difference between the illuminating light …
Characterizing transiting exoplanet atmospheres with JWST
We explore how well spectra from the James Webb Space Telescope (JWST) will likely
constrain bulk atmospheric properties of transiting exoplanets. We start by modeling the …
constrain bulk atmospheric properties of transiting exoplanets. We start by modeling the …
Spectrally resolved helium absorption from the extended atmosphere of a warm Neptune-mass exoplanet
Stellar heating causes atmospheres of close-in exoplanets to expand and escape. These
extended atmospheres are difficult to observe because their main spectral signature …
extended atmospheres are difficult to observe because their main spectral signature …
A population study of gaseous exoplanets
We present here the analysis of 30 gaseous extrasolar planets, with temperatures between
600 and 2400 K and radii between 0.35 and 1.9 R Jup. The quality of the HST/WFC3 …
600 and 2400 K and radii between 0.35 and 1.9 R Jup. The quality of the HST/WFC3 …