In this communication, we report on the results of the second phase of the Exoplanet Imaging Data Challenge started in 2019.
astro-ph.IM
Generative AI for Overall Mission Effectiveness at the Habitable Worlds Observatory
Here we present several use cases for using Generative AI (Gen AI) to improve systems engineering and cognitive knowledge management related to the future of astronomy from a culmination of […]
Cthulhu: An Open Source Molecular and Atomic Cross Section Computation Code for Substellar Atmospheres
Atmospheric studies of exoplanets and brown dwarfs are a cutting-edge and rapidly evolving area of astrophysics research. Calculating models of exoplanet or brown dwarf spectra requires knowledge of the wavelength-dependent […]
SETI In 2022
In this third installment of SETI in 20xx, we very briefly and subjectively review developments in SETI in 2022.
Starshade Exoplanet Data Challenge: What We Learned
Starshade is one of the technologies that will enable the observation and characterization of small planets around nearby stars through direct imaging.
MODEL&CO: Exoplanet Detection In Angular Differential Imaging By Learning Across Multiple Observations
Direct imaging of exoplanets is particularly challenging due to the high contrast between the planet and the star luminosities, and their small angular separation. In addition to tailored instrumental facilities […]
Impact of Exoplanet Science on Society: Professional Contributions, Citizen Science Engagement and Public Perception
The impact of exoplanet science on both the scientific community and on the general public is presented through various indicators and examples. It is estimated that about 3-4% of all […]
An Alternating Minimization Algorithm with Trajectory for Direct Exoplanet Detection — The AMAT Algorithm
Effective image post-processing algorithms are vital for the successful direct imaging of exoplanets. Standard PSF subtraction methods use techniques based on a low-rank approximation to separate the rotating planet signal […]
Estimating Atmospheric Wind Speeds From Gemini Planet Imager Adaptive Optic Telemetry
The Earth’s atmosphere is comprised of turbulent layers that result in speckled and blurry images from ground-based visible and infrared observations. Adaptive Optics (AO) systems are employed to measure the […]
Optical Design Options For Pollux: UV Spectropolarimeter Project For The Habitable Worlds Observatory
Pollux is a project of UV spectropolarimeter proposed as a European contribution for the planned NASA-led Habitable Worlds Observatory.
