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Trojan Exoplanets
Co-orbital exoplanets are a by-product of the models of formation of planetary systems. However, none have been detected in nature thus far. Although...
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Exoplanets and SETI
The discovery of exoplanets has both focused and expanded the search for extraterrestrial intelligence. The consideration of Earth as an exoplanet,...
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Finding exoplanets using object detection
Since the initial finding of exoplanets, planet detection has gained prominence as a field of research in astronomy. Using a variety of techniques,...
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Ephemeris Updates for Seven Selected Hatnet Survey Transiting Exoplanets
We refined the ephemeris of seven transiting exoplanets HAT-P-6b, HAT-P-12b, HAT-P-18b, HAT-P-22b, HAT-P-32b, HAT-P-33b, and HAT-P-52b. We observed...
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Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds
Spectroscopy of transiting exoplanets has revealed a wealth of information about their atmospheric compositions and thermal structures. In...
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Inferring chemical disequilibrium biosignatures for Proterozoic Earth-like exoplanets
Chemical disequilibrium quantified using the available free energy has previously been proposed as a potential biosignature. However, researchers...
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Stellar Wind and the Efficiency of Plasma Radio Emission from Exoplanets
AbstractWe present the results of our study of the influence of stellar activity on the efficiency of the plasma radio emission generation mechanism...
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Atmospheric carbon depletion as a tracer of water oceans and biomass on temperate terrestrial exoplanets
The conventional observables to identify a habitable or inhabited environment in exoplanets, such as an ocean glint or abundant atmospheric O 2 , will...
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Investigations of Optical Properties of the Atmospheres of Hot Exoplanets by Numerical Simulation of Transit Absorptions in the HeI 10 830-Å Line
Abstract —Transit observations of exoplanets make it possible to measure temperature and relative abundance of various elements in their atmospheres....
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Aeronomic Model of Hydrogen–Helium Upper Atmospheres of Hot Giant Exoplanets
AbstractThe paper presents a one-dimensional aeronomic model of hydrogen–helium upper atmospheres of hot giant exoplanets based on the approximation...
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Creation and Evolution of Life in Black Hole Exoplanets
AbstractContrary to science-fiction movies such as Interstellar , planets orbiting around black holes cannot be stable. Because due to the extreme...
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Planetary Systems. Exoplanets
This chapter is centered on the methods of chaos diagnosis based on the Fast Fourier Transform (FFT) and the dynamical maps on dense grids and their...
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Using Convolutional Neural Networks to Detect and Confirm Exoplanets
In this research, I developed a Python software program with a convolutional neural network (CNN), a deep learning (DL) approach, mainly from...
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OWL-Moon: Very high resolution spectropolarimetric interferometry and imaging from the Moon: exoplanets to cosmology
We outline a concept for OWL-Moon, a 50-100 m aperture telescope located on the surface of the Moon, to address three major areas in astronomy,...
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Io as an Analog for Tidally Heated Exoplanets
Jupiter’s moon Io is unique in our Solar System. A rocky body orbiting close to its parent planet, in resonant orbits with its sibling satellites, Io...
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