Results 1 to 10 of about 12,652 (214)
New Completeness Methods for Estimating Exoplanet Discoveries by Direct Detection [PDF]
We report new methods for evaluating realistic observing programs that search stars for planets by direct imaging, where observations are selected from an optimized star list, and where stars can be observed multiple times.
Brown +9 more
core +4 more sources
Exoplanet imaging data challenge: benchmarking the various image processing methods for exoplanet detection [PDF]
36 pages, 27 figures.
F Cantalloube +2 more
exaly +5 more sources
Five Methods of Exoplanet Detection
Abstract The study of exoplanetary systems can help us understand the formation and evolution of the solar system itself and search for terrestrial planets in the habitable and extrasolar lives in exoplanetary systems. Exoplanets have become an important area of astrophysics in the last two decades.
Ziqi Dai +3 more
exaly +2 more sources
Bayesian Methods for Joint Exoplanet Transit Detection and Systematic Noise Characterization [PDF]
Abstract The treatment of systematic noise is a significant aspect of transit exoplanet data processing due to the signal strength of systematic noise relative to a transit signal. Typically, the standard approach to transit detection is to estimate and remove systematic noise independently of and prior to a transit detection test.
Jamila S Taaki, Athol Kemball
exaly +3 more sources
VaTEST. II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars
NASA’s Transiting Exoplanet Survey Satellite (TESS) is an all-sky survey mission designed to find transiting exoplanets orbiting nearby bright stars. It has identified more than 329 transiting exoplanets, and almost 6000 candidates remain unvalidated. In
Priyashkumar Mistry +50 more
doaj +1 more source
Large-scale exoplanet surveys like the Transiting Exoplanet Survey Satellite (TESS) mission are powerful tools for discovering large numbers of exoplanet candidates.
Christopher R. Mann +50 more
doaj +1 more source
Statistical Methods for Exoplanet Detection with Radial Velocities
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
We perform an in-depth analysis of the recently validated TOI-3884 system, an M4-dwarf star with a transiting super-Neptune. Using high-precision light curves obtained with the 3.5 m Apache Point Observatory and radial velocity observations with the ...
Jessica E. Libby-Roberts +27 more
doaj +1 more source
OGLE-2019-BLG-1180Lb: Discovery of a Wide-orbit Jupiter-mass Planet around a Late-type Star
We report on the discovery and analysis of the planetary microlensing event OGLE-2019-BLG-1180 with a planet-to-star mass ratio q ∼ 0.003. The event OGLE-2019-BLG-1180 has unambiguous cusp-passing and caustic-crossing anomalies, which were caused by a ...
Sun-Ju Chung +35 more
doaj +1 more source
Exoplanet Detection Methods [PDF]
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

