Detecting Exoplanets with Radial Velocity and Transit Methods: A Comparative Analysis
This paper presents a comprehensive comparative analysis of two prominent methods for detecting exoplanets: the Radial Velocity (RV) method and the Transit Photometry method. These methods have significantly contributed to the discovery and characterization of exoplanets, expanding our understanding of planetary systems beyond our own.
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Quantum-inspired exoplanet detection in the presence of experimental imperfections
Ideal spatial demultiplexing (SPADE) is proven to be a quantum-optimal tool for exoplanet detection, i.e., asymmetric source discrimination. However, recent investigations into the related problems of separation estimation and symmetric source ...
Schlichtholz, Konrad +2 more
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A Stellar magnesium to silicon ratio in the atmosphere of an exoplanet. [PDF]
Sanchez JA +19 more
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Dirt or type? Clarifying fungal nomenclature in the DNA age. [PDF]
Fachada V, Druzhinina IS.
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Reassessment of Kepler's habitable zone Earth-like exoplanets with data-driven null signal templates. [PDF]
Robnik J, Seljak U.
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Prospects for detecting signs of life on exoplanets in the JWST era. [PDF]
Seager S +4 more
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Exo-Geoscience Perspectives Beyond Habitability. [PDF]
Spohn T +7 more
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Training a convolutional neural network for exoplanet classification with transit photometry data. [PDF]
Wang J.
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A precise metallicity and carbon-to-oxygen ratio for a warm giant exoplanet from its panchromatic JWST emission spectrum. [PDF]
Wiser LS +13 more
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