works on

From the 1 of 7 linked papers with an AI index.

collaborators

7 papers

astro-ph.IM2026

Detecting habitable exoplanet atmospheres with LIFE, the Large Interferometer for Exoplanets

Sarah Rugheimer, Aiden Weatherbee, James Fecanin +21

A key goal of astronomers with the next generation telescopes is to detect signs of life in exoplanet atmospheres. NASA's next flagship is the Habitable Worlds Observatory (HWO). I…

astro-ph.EP2026

Atmospheric evolution through outgassing and escape on young molten rocky exoplanets

Emma Postolec, Tim Lichtenberg, Harrison Nicholls +2

The paper models how outgassing from a cooling magma ocean and atmospheric escape together shape the early atmospheres of rocky exoplanets, exploring how factors like stellar type,…

astro-ph.GA2026

Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8

Fengwei Xu, Ke Wang, Nicola Schneider +12

A dynamic view of mass assembly is essential for understanding the formation of massive stars and clusters. Interpreting evolutionary diagnostics from Galactic-wide surveys, howeve…

astro-ph.GA2025

Super-resolving Herschel - a deep learning based deconvolution and denoising technique

Dennis Koopmans, Lingyu Wang, Berta Margalef-Bentabol +9

Dusty star-forming galaxies (DSFGs) dominate the far-infrared and sub-millimetre number counts, but single-dish surveys suffer from poor angular resolution, complicating mult-wavel…

astro-ph.GA2025

Likelihood and appearance of life beyond the Earth: An astronomical perspective

Floris van der Tak

As of 2025, over 6000 planets are known to orbit stars other than our Sun. We can measure their sizes and orbital periods, infer their masses and temperatures, and constrain their…

astro-ph.GA2025

Unmasking the physical information inherent to interstellar spectral line profiles with Machine Learning. I. Application of LTE to HCN and HNC transitions

Edgar Mendoza, Pietro Dall'Olio, Luciene S. Coelho +4

Physical and chemical conditions (kinetic temperature, volume density, molecular composition) of interstellar clouds are inherent in their mm-submm line spectra, making spectral li…