We introduce a new time-series analysis strategy for combined-light exoplanet spectroscopic phase curves called the Variable Planetary Infrared Excess (VPIE) method. VPIE can be used to extract information about the […]
JWST
JWST Spectral Retrieval Of Cold Directly Imaged Planet WD0806 b And The First
WD0806 b is a rare exoplanet companion orbiting a white dwarf, currently with a projected orbital distance of 2500 au. The Spitzer mid-IR photometry suggests that the temperature is as […]
James Webb Space Telescope Reveals An Exceptional Richness Of Organic Molecules In One Of The Most Infrared Luminous Galaxies In The Local Universe
The study focuses on IRAS 07251–0248, an ultra-luminous infrared galaxy whose nucleus is hidden behind vast amounts of gas and dust. This material absorbs most of the radiation emitted by […]
A Chemistry-First Centered Icy Chemical Inventory of Protostellar Sources with JWST
The chemical evolution in star forming regions is driven by the interplay between gas and ice mantles. Identifying the ice compositions at the early stage of star formation thus provides […]
Broadband Infrared Spectroscopy Of Methanol Isotopologues In pure, H2O-rich, And CO-rich Ice Analogues
Deuterium fractionation is highly efficient during the early stages of star formation, particularly in starless and prestellar cores where temperatures are low (<10 K) and molecular freeze-out onto dust grains […]
Abundant Hydrocarbons In A Buried Galactic Nucleus With Signs Of Carbonaceous Grain And Polycyclic Aromatic Hydrocarbon Processing
Hydrocarbons play a key role in shaping the chemistry of the interstellar medium (ISM), but their enrichment and relationship with carbonaceous grains and polycyclic aromatic hydrocarbons (PAHs) still lack clear […]
The Effect of Tidal Heating and Volatile Budgets on the Outgassed Atmosphere of 55 Cancri e
55 Cancri e is a ∼8 Gyr rocky world (1.95 R⊕, 8.8 M⊕) orbiting a K-type star. JWST observations suggest a carbon-dominated atmosphere (CO2/CO) over a global magma ocean (>3000 […]
The Role of Intrinsic Temperature and Vertical Mixing in Characterizing Sub-Neptune Atmospheres
Sub-Neptune planets are often modeled with a dense rocky or metal-rich interior beneath a thick hydrogen/helium (H/He) atmosphere; though their bulk densities could also be explained by a water-rich interior […]
Climates Of Terrestrial Exoplanets And Biosignatures
Understanding the climates of terrestrial exoplanets and the detectability of biosignatures is an inherently interdisciplinary challenge, requiring the integration of insights from Solar System exploration, exoplanet observations and climate science. […]
H182O In The Terrestrial Planet-forming Regions Of Protoplanetary Disks
Isotopologues play an important role in solar system cosmochemistry studies, revealing details of early planet formation physics and chemistry.
