Results 91 to 100 of about 1,437 (218)
Direct Optical Detection of Microorganisms in Exoplanet Atmospheres: Methods
The purpose of this project is to develop an optical method for detecting the presence of life, specifically microorganisms, in the atmosphere of an exoplanet.
Eads, Ryker +4 more
core
Extrasolar planets : detection methods and observational campaigns [PDF]
The universe is vast and it contains hundreds of billions of galaxies, which still remains unexplored. Each of these galaxies have unexplored planetary systems with interesting planets that awaits to be discovered.
Halsio, Eetu
core
Machine learning for exoplanet detection in high-contrast spectroscopy [PDF]
Context. The new generation of observatories and instruments (VLT/ERIS, JWST, ELT) motivate the development of robust methods to detect and characterise faint and close-in exoplanets. Molecular mapping and cross-correlation for spectroscopy use molecular
Dominique Petit dit de la Roche +26 more
core +3 more sources
It has been suggested that giant planet occurrence peaks for stars with M _* ≈ 3 M _⊙ at a value a factor of 4 higher than observed for solar-mass stars.
Sihao Cheng +2 more
doaj +1 more source
Predicting flux data for exoplanet detection.
This paper will focus on utilizing five different methods of machine learning models to properly classify celestial bodies orbiting a star as an exoplanet or a false positive. We will be utilizing a recurrent neural network (RNN), a logistical regression
Kroening, Ronald
core
Cílem této práce je navrhnout a implementovat způsob analýzy dat z tranzitní metody pro detekci exoplanet. Použitá data pochází z vesmírného teleskopu TESS a jsou v podobě světelných křivek, které zachycují pozorované změny jasu hvězdy v čase. Tato práce
Škvařilová, Nikol
core +1 more source
We report the discovery of a new massive giant planet, HD 164604 c ( ${a}_{c}=5.55{6}_{-0.10}^{+0.093}$ au, ${e}_{c}=0.19{6}_{-0.078}^{+0.078}$ , and ${m}_{c}=9.{5}_{-1.25}^{+1.2}$ , or $7.{6}_{-1.0}^{+1.0}\,{M}_{{\rm{Jup}}}$ ), orbiting a K3.5 dwarf ...
Guang-Yao Xiao +6 more
doaj +1 more source
The Interpolation Constraint in the RV Analysis of M Dwarfs Using Empirical Templates
Precise radial velocity (pRV) measurements of M dwarfs in the near-infrared rely on empirical templates due to the lack of accurate stellar spectral models in this regime.
Dhvani Doshi +6 more
doaj +1 more source
We present new VLTI/GRAVITY astrometry and updated orbit fits for the directly imaged companions YSES 1 b and HR 2562 B, substellar objects straddling the planet–brown-dwarf boundary.
Jonathan Roberts +22 more
doaj +1 more source
A Pair of Dynamically Interacting Sub-Neptunes around TOI-6054
We confirm the planetary nature of a pair of transiting sub-Neptune exoplanets orbiting the bright F-type subgiant star TOI-6054 ( V = 8.02, K = 6.673) as a part of the OrCAS radial velocity survey using WIYN/NEID observations. We find that TOI-6054b and
Maxwell A. Kroft +33 more
doaj +1 more source

