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pro vyhledávání: '"Fatheddin, Hossein"'
Autor:
Sajadian, Sedighe, Fatheddin, Hossein
In an edge-on and detached binary system, including a white dwarf (WD) and a main-sequence star (WDMS), when the source star is passing behind the compact companion its light is bent and magnified. Meanwhile, some part of its images' area is obscured
Externí odkaz:
http://arxiv.org/abs/2410.04550
We study the statistics and properties of microlensing events that can be detected by the Transiting Exoplanet Survey Satellite(TESS) based on Monte Carlo simulations. We simulate potential microlensing events from a sample of the TESS Candidate Targ
Externí odkaz:
http://arxiv.org/abs/2408.14231
Autor:
Fatheddin, Hossein, Sajadian, Sedighe
Transit photometry is currently the most efficient and sensitive method for detecting extrasolar planets (exoplanets) and a large majority of confirmed exoplanets have been detected with this method. The substantial success of space-based missions su
Externí odkaz:
http://arxiv.org/abs/2404.05323
Autor:
Sajadian, Sedighe, Fatheddin, Hossein
Wavelets are waveform functions that describe transient and unstable variations, such as noises. In this work, we study the advantages of discrete and continuous wavelet transforms (DWT and CWT) of microlensing data to denoise them and extract their
Externí odkaz:
http://arxiv.org/abs/2310.03338
Autor:
Fatheddin, Hossein, Sajadian, Sedighe
It is plausible that most of the Stars in the Milky Way (MW) Galaxy, like the Sun, consist of planetary systems, instead of a single planet. Out of the estimately discovered 3,950 planet-hosting stars, about 860 of them are known to be multiplanetary
Externí odkaz:
http://arxiv.org/abs/2305.19099
Autor:
Fatheddin, Hossein, Sajadian, Sedighe
The stellar kinematics of the Galactic disk are main factors for constraining disk formation and evolution processes in the Milky Way (MW) Galaxy. In this paper we investigate a statistical relation between stellar Mass, Age and Velocity Dispersion f
Externí odkaz:
http://arxiv.org/abs/2212.13349
Autor:
Fatheddin, Hossein, Sajadian, Sedighe
In gravitational microlensing formalism and for modeling binary light curves, the key step is solving the binary lens equation. Currently, a combination of the Newton's and Laguerre's methods which was first introduced by Skowron \& Gould (SG) is use
Externí odkaz:
http://arxiv.org/abs/2206.00482
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Akademický článek
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