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Exoplanet detection techniques – from astronomy to astrobiology
Wolfgang Brandner
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Exoplanet detection from starshade images using convolutional neural networks
Optical Engineering + Applications, 2023High-contrast, direct imaging of exoplanets is a key objective for the future of astronomy. Underpinning both the development and successful deployment of future direct imaging missions is the ability to analyze the resulting data. Therefore, in order to
Zahra Ahmed+3 more
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Exoplanet Detection Using Feature Engineering with Ensemble Learning
2023 3rd International Conference on Pervasive Computing and Social Networking (ICPCSN), 2023In this work, a novel technique for detecting extra-terrestrial bodies using the transit method, with the aim of improving traditional algorithmic strategies in astronomy through machine learning algorithms.
G. Venkata+6 more
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Ozone-like layer in an exoplanet atmosphere [PDF]
The nature of exoplanetary atmospheres is hotly debated. The thermal spectrum of an exoplanet called a hot Jupiter reveals the presence of an analogue of Earth's ozone layer, although its composition is unknown. See Letter p.58 Earth's atmosphere consists of layers that are partially defined by ...
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The impending opacity challenge in exoplanet atmospheric characterization
Nature Astronomy, 2022With a new generation of observatories coming online this decade, the process of characterizing exoplanet atmospheres will need to be reinvented. Currently mostly on the instrumental side, characterization bottlenecks will soon appear at the models used ...
P. Niraula+5 more
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Training on Machine Learning Applied to Space Astronomy Data and Exoplanet Research
E. S. Cheng+7 more
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A secondary atmosphere on the rocky Exoplanet 55 Cancri e.
NatureCharacterizing rocky exoplanets is a central endeavor of astronomy, and yet the search for atmospheres on rocky exoplanets has hitherto resulted in either tight upper limits on the atmospheric mass1-3 or inconclusive results4-6.
R. Hu+16 more
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Nature, 2014
Spectroscopic observations of a young exoplanet have allowed its spin velocity to be directly measured. Its fast spin is in accord with the extrapolation of the known trend in spin velocity as a function of planet mass. See Letter p.63 Near-infrared spectroscopic observations of the young extrasolar
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Spectroscopic observations of a young exoplanet have allowed its spin velocity to be directly measured. Its fast spin is in accord with the extrapolation of the known trend in spin velocity as a function of planet mass. See Letter p.63 Near-infrared spectroscopic observations of the young extrasolar
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A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
Nature AstronomyObserving exoplanets through transmission spectroscopy supplies detailed information about their atmospheric composition, physics and chemistry. Before the James Webb Space Telescope (JWST), these observations were limited to a narrow wavelength range ...
A. Carter+79 more
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