papers

Publications (9)

astro-ph.SR2019

Stars at High Spatial Resolution

Kenneth G. Carpenter, Gerard van Belle, Alexander Brown +19

We summarize some of the compelling new scientific opportunities for understanding stars and stellar systems that can be enabled by sub-milliarcsec (sub-mas) angular resolution, UV…

astro-ph.SR2010

Stellar Imager (SI): developing and testing a predictive dynamo model for the Sun by imaging other stars

Kenneth G. Carpenter, Carolus J. Schrijver, Margarita Karovska +39

The Stellar Imager mission concept is a space-based UV/Optical interferometer designed to resolve surface magnetic activity and subsurface structure and flows of a population of Su…

astro-ph.SR2009

Mass Transport Processes and their Roles in the Formation, Structure, and Evolution of Stars and Stellar Systems

Kenneth G. Carpenter, Margarita Karovska, Carolus J. Schrijver +15

We summarize some of the compelling new scientific opportunities for understanding stars and stellar systems that can be enabled by sub-mas angular resolution, UV/Optical spectral…

astro-ph.IM2010

Simulations of coronagraphy with a dynamic hologram for the direct detection of exo-planets

Davide Ricci, Hervé Le Coroller, Antoine Labeyrie +1

In a previous paper, we discussed an original solution to improve the performances of coronagraphs by adding, in the optical scheme, an adaptive hologram removing most of the resid…

astro-ph.IM2024

Astronomy from the Moon: From Exoplanets to Cosmology in Visible Light and Beyond

Jean Schneider, Pierre Kervella, Antoine Labeyrie

We look at what astronomy from the Moon might be like in the visible over the next few decades. The Moon offers the possibility of installing large telescopes or interferometers wi…

astro-ph.IM2014

Towards Laser-Guide-Stars for Multi-Aperture Interferometry: an application to the Hypertelescope

Paul D. Nuñez, Antoine Labeyrie, Pierre Riaud

Optical interferometry has been successful at achieving milliarcsecond resolution on bright stars. Imaging performance can improve greatly by increasing the number of baselines, wh…