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Methods for Detecting Cyclotron Maser Radio Emissions from Stars and Exoplanets
The Cyclotron Maser Instability (CMI) is a well-known mechanism responsible for auroral radio emissions from the Earth, Jupiter, Saturn, Uranus, and Neptune. These emissions occur at frequencies near or equal to the local electron cyclotron frequency, which is directly related to the local magnetic field strength.Corentin Louis +6 more
openaire +1 more source
Study and Analysis of Detection Methods and Physical Characteristics of Exoplanets
2022Mr Edoardo Altamura +6 more
openaire +1 more source
Size does matter: Exoplanet detection with a sparse convolutional neural network
Astronomy and Computing, 2022exaly
Improving the RSM map exoplanet detection algorithm
Astronomy and Astrophysics, 2021Olivier Absil, Carl-Henrik Dahlqvist
exaly
Understanding the Radial Velocity Method for Exoplanet Detection: A Simple and Detailed Guide
The Radial Velocity (RV) method is one of the most widely used techniques for discovering ex- oplanets. This paper presents a student-friendly, yet deep, explanation of the physical principles, mathematical foundations, observational techniques, and practical limitations of the method.openaire +2 more sources
Book Review: “Methods of Detecting Exoplanets”
Journal of Astronomical Instrumentation, 2017openaire +1 more source
Semi-Supervised Standardized Detection of Periodic Signals with Application to Exoplanet Detection
2022Sophia Sulis, L Bigot
exaly
Some Aspects of Exoplanets Detection with the Transit Method
Earth, Moon, and Planets, 1998openaire +1 more source