Results 11 to 20 of about 631 (181)

Statistical Methods for Exoplanet Detection with Radial Velocities

open access: yesAnnual Review of Statistics and Its Application, 2023
Exoplanets can be detected with various observational techniques. Among them, radial velocity (RV) has the key advantages of revealing the architecture of planetary systems and measuring planetary mass and orbital eccentricities. RV observations are poised to play a key role in the detection and characterization of Earth twins.
Hara, Nathan C., Ford, Eric B.
openaire   +2 more sources

Exoplanet Detection Methods [PDF]

open access: yes, 2013
60 pp, 12 figures. To appear as Chapter 59 of "Planets, Stars, and Stellar Systems" Editor-in-chief Terry Oswalt, volume editor Paul Kalas.
Wright, Jason T., Gaudi, B. Scott
openaire   +2 more sources

The Comparison of Five Methods of Detecting Exoplanets

open access: yesHighlights in Science, Engineering and Technology, 2023
Detecting exoplanets has become a hot topic, where various detection scenarios have been proposed. Five of these methods have all found more than 50 exoplanets, which are the transit method, the radial velocity method, the microlensing method, the imaging method, and the timing method.
openaire   +1 more source

Variability of Known Exoplanet Host Stars Observed by TESS

open access: yesThe Astronomical Journal, 2023
Both direct and indirect methods of exoplanet detection rely upon detailed knowledge of the potential host stars. Such stellar characterization allows for accurate extraction of planetary properties, as well as contributing to our overall understanding ...
Emilie R. Simpson   +5 more
doaj   +1 more source

A bootstrap method for sinusoid detection in colored noise and uneven sampling. Application to exoplanet detection [PDF]

open access: yes2017 25th European Signal Processing Conference (EUSIPCO), 2017
Accepted in the European Signal Processing Conference (EUSIPCO 2017).
Sophia Sulis, David Mary, Lionel Bigot
openaire   +3 more sources

Revised Properties and Dynamical History for the HD 17156 System

open access: yesThe Astronomical Journal, 2023
From the thousands of known exoplanets, those that transit bright host stars provide the greatest accessibility toward detailed system characterization.
Stephen R. Kane   +9 more
doaj   +1 more source

Optimal method for exoplanet detection by spectral and angular differential imaging [PDF]

open access: yesSPIE Proceedings, 2010
ABSTRACT In the context of the SPHERE planet “nder project, we further develop and characterize a recently proposedmethod for the ecient direct detection of exoplanets f rom the ground using spectral and angular dierentialimaging. The method, called ANDROMEDA, combines images appropriately into pseudo-dataŽ, then uses allof them in a Maximum ...
Cornia, A.   +11 more
openaire   +3 more sources

Detection of Exoplanets based on the Transit Method

open access: yesHighlights in Science, Engineering and Technology, 2023
Exoplanets are planets orbiting a star other than the Sun. These exoplanets may exist in many different forms, such as a hot Jupiter and super earth. Detecting is the first step to further studying the properties of these exoplanets. In this paper, based on data of star Qatar-1 gathered from July 22nd 2022, a light flux curve is developed during the ...
openaire   +1 more source

A new method for finding nearby white dwarfs exoplanets and detecting biosignatures

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT We demonstrate that the James Webb Space Telescope (JWST) can detect infrared (IR) excess from the blended light spectral energy distribution of spatially unresolved terrestrial exoplanets orbiting nearby white dwarfs. We find that JWST is capable of detecting warm (habitable-zone; Teq = 287 K) Earths or super-Earths and hot ...
Mary Anne Limbach   +7 more
openaire   +2 more sources

Assessing telluric correction methods for Na detections with high-resolution exoplanet transmission spectroscopy [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT Using high-resolution ground-based transmission spectroscopy to probe exoplanetary atmospheres is difficult due to the inherent telluric contamination from absorption in Earth’s atmosphere. A variety of methods have previously been used to remove telluric features in the optical regime and calculate the planetary transmission ...
Adam B Langeveld   +3 more
openaire   +2 more sources

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