The detection of exoplanets using astrometry has long been an area of interest, but is fraught with challenges. The Gaia mission is fundamentally reshaping this field thanks to its unprecedentedly […]
Spectrograph
The Ocean Worlds Science Case For The Pollux Spectropolarimeter
Pollux is a candidate European instrument contribution to the Habitable Worlds Observatory (HWO), designed to advance our understanding of the formation and evolution of cosmic structures in the universe, and […]
Atmospheric Constraints On GJ 1214 b From CRIRES+ And Prospects For Characterisation With ANDES
In this study, we aim to constrain the atmospheric composition of GJ 1214 b using all available transits observed with the upgraded CRIRES+ spectrograph at the VLT by searching for […]
Probing The Geological Setting Of Exoplanets Through Atmospheric Analysis: Using Mars As A Test Case
One of the frontier research fields of exoplanetary science is the study of the composition and variability of exoplanetary atmospheres.
The CARMENES Search For Exoplanets Around M Dwarfs. Revisiting The GJ 317, GJ 463, and GJ 3512 Systems And Two Newly Discovered Planets Orbiting GJ 9773 And GJ 508.2
Surveys for exoplanets indicate that the occurrence rate of gas giant planets orbiting late-type stars in orbits with periods shorter than 1000 days is lower than in the case of […]
TOI-1846b: A super-Earth In The Radius Valley Orbiting A Nearby M dwarf
We present the discovery and validation of a super-Earth planet orbiting the M dwarf star TOI-1846 (TIC 198385543).
Short-Term Balmer Line Emission Variability in M Dwarfs
M Dwarfs make up the majority of stars, offering an avenue for discovering exoplanets due to their smaller sizes. However, their magnetic activity poses challenges for exoplanet detection, characterization, and […]
High-precision NEID Spectrograph Helps Confirm First Gaia Astrometric Planet Discovery
NEID (rhymes with fluid) is a high-precision radial-velocity spectrograph that is designed to measure the extremely minute wobble of nearby stars using the radial velocity effect. This effect results from […]
The NCORES Program: Precise Planetary Masses, Null Results, and Insight Into The Planet Mass Distribution Near The Radius Gap
NCORES was a large observing program on the ESO HARPS spectrograph, dedicated to measuring the masses of Neptune-like and smaller transiting planets discovered by the TESS satellite using the radial […]
A Disintegrating Rocky World Shrouded in Dust and Gas: Mid-IR Observations of K2-22b using JWST
The disintegrating ultra-short period rocky exoplanet K2-22b periodically emits dusty clouds in a dynamically chaotic process resulting in a variable transit depth from 0-1.3%.
