Column density ratios of complex organic molecules are generally constant across protostellar systems with some low-level scatter.
Spectroscopy
Cold Coulomb Crystals, Cosmic Clues: Unraveling The Mysteries Of Space Chemistry
While it may not look like it, the interstellar space between stars is far from empty. Atoms, ions, molecules, and more reside in this ethereal environment known as the Interstellar […]
In The Search For Alien Life, Purple May Be The New Green
In the search for life across the cosmos, the familiar green hue we most associate with life on Earth may not be the best indicator. An Earth-like planet orbiting another […]
Constraints On Atmospheric Water Abundance and Cloud Deck Pressure in the Warm Neptune GJ 3470 b via CARMENES Transmission Spectroscopy
Observations of cooler atmospheres of super-Earths and Neptune sized objects often show flat transmission spectra.
Radial and Vertical Constraints On The Icy Origin Of H2CO In The HD 163296 Protoplanetary Disk
H2CO is a small organic molecule widely detected in protoplanetary disks. As a precursor to grain-surface formation of CH3OH, H2CO is considered an important precursor of O-bearing organic molecules that […]
Doppler Tomography As A Tool For Characterising Exoplanet Atmospheres II: An Analysis of HD 179949 b
High-resolution Doppler spectroscopy provides an avenue to study the atmosphere of both transiting and non-transiting planets. This powerful method has also yielded some of the most robust atmospheric detections to […]
The Impact of Extended H2O Cross-Sections on Temperate Anoxic Planet Atmospheres: Implications for Spectral Characterization of Habitable Worlds
JWST has created a new era of terrestrial exoplanet atmospheric characterization, and with it the possibility to detect potential biosignature gases like CH4.
NLTE Modelling Of Water-rich Exoplanet Atmospheres. Cooling And Heating Rates
The hydrogen and water molecules respond very differently to the collisional-radiative processes taking place in planetary atmospheres. Naturally, the question arises whether H2O-rich atmospheres are more (or less) resilient to […]
Data Availability And Requirements Relevant For The Ariel Space Mission And Other Exoplanet Atmosphere Applications
The goal of this white paper is to provide a snapshot of the data availability and data needs primarily for the Ariel space mission, but also for related atmospheric studies […]
Retrieved Atmospheres and Inferred Surface Properties for Exoplanets Using Transmission and Reflected Light Spectroscopy
Future astrophysics missions will seek extraterrestrial life via transmission and direct imaging observations.
