Results 191 to 200 of about 140,874 (259)

MEC: the MKID exoplanet camera for high contrast astronomy at Subaru (Conference Presentation)

open access: closedGround-based and Airborne Instrumentation for Astronomy VII, 2018
Direct Imaging of exoplanets is one of the most technically difficult techniques used to study exoplanets, but holds immense promise for not just detecting but characterizing planets around the nearest stars. Ambitious instruments at the world’s largest telescopes have been built to carry out this science: the Gemini Planet Imager (GPI), SPHERE at VLT,
Alexander B. Walter   +13 more
semanticscholar   +4 more sources

THEIA: Telescope for Habitable Exoplanets and Interstellar/Intergalactic Astronomy

open access: closedAIP Conference Proceedings, 2009
In this paper, we provide an overview of the scientific potential of the THEIA mission concept. THEIA consists of a 4‐meter telescope diffraction limited to 300 nm, and a 40‐meter external occulter to provide high‐contrast imaging. Operating from 250 to 1000 nm, it will provide a rich family of science projects, including exoplanet characterization ...
David N. Spergel   +49 more
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The search for exoplanets using ultra-long wavelength radio astronomy

open access: closed2017 IEEE Aerospace Conference, 2017
Recent studies on extra solar planets (exoplanets) provide us with a new glimpse into the Milky Way's composition. Exoplanets appear to be very typical around Sunlike stars. Most of these exoplanets are observed via indirect measurements. If a direct radio observation of the exoplanet's signal was possible, new scientific information will help us in ...
Mark Bentum
openalex   +2 more sources

Training on Machine Learning Applied to Space Astronomy Data and Exoplanet Research

open access: closedIAF Space Exploration Symposium
E. S. Cheng   +7 more
openalex   +2 more sources
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A secondary atmosphere on the rocky exoplanet 55 Cancri e

Nature
Characterizing rocky exoplanets is a central aim of astronomy, and yet the search for atmospheres on rocky exoplanets has so far resulted in either tight upper limits on the atmospheric mass1–3 or inconclusive results4–6.
R. Hu   +16 more
semanticscholar   +1 more source

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