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相关论文: Determination of orbital parameters of interacting…

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The main problems in modeling interacting galaxies are the extended parameter space and the fairly high CPU costs of self-consistent N-body simulations. Therefore, traditional modeling techniques suffer from either extreme CPU demands or…

天体物理学 · 物理学 2007-05-23 Ch. Theis , Ch. Gerds , Ch. Spinneker

Here we show how to determine the orbital parameters of a system composed of a star and N companions (that can be planets, brown-dwarfs or other stars), using a simple Fourier analysis of the radial velocity data of the star. This method…

地球与行星天体物理 · 物理学 2022-08-01 Alexandre C. M. Correia

We describe an analytical method for computing the orbital parameters of a planet from the periodogram of a radial velocity signal. The method is very efficient and provides a good approximation of the orbital parameters. The accuracy is…

地球与行星天体物理 · 物理学 2016-06-01 J. -B. Delisle , D. Ségransan , N. Buchschacher , F. Alesina

Genetic algorithms are a powerful tool in optimization for single and multi-modal functions. This paper provides an overview of their fundamentals with some analytical examples. In addition, we explore how they can be used as a parameter…

We have used a Galactic sample of OB stars and associations to test the performance of an automatic grouping algorithm designed to identify extragalactic OB associations. The algorithm identifies the known Galactic OB associations correctly…

天体物理学 · 物理学 2009-10-28 Christine D. Wilson , Karen J. Bakker

A flood of reliable seismic data will soon arrive. The migration to larger telescopes on the ground may free up 4-m class instruments for multi-site campaigns, and several forthcoming satellite missions promise to yield nearly uninterrupted…

天体物理学 · 物理学 2007-05-23 Travis S. Metcalfe

By combining test-particle and self-consistent techniques, we have developed a method to rapidly explore the parameter space of galactic encounters. Our method, implemented in an interactive graphics program, can be used to find the…

天体物理学 · 物理学 2009-11-13 Joshua E. Barnes , John E. Hibbard

The parameter space of dynamical systems arising in applications is often found to be high-dimensional and difficult to explore. We construct a fast algorithm to numerically analyze "quantitative features" of dynamical systems depending on…

数值分析 · 数学 2008-07-15 Christian Kuehn

This paper presents a machine learning approach for tuning the parameters of a family of stabilizing controllers for orbital tracking. An augmented random search algorithm is deployed, which aims at minimizing a cost function combining…

系统与控制 · 电气工程与系统科学 2023-08-08 Gianni Bianchini , Andrea Garulli , Antonio Giannitrapani , Mirko Leomanni , Renato Quartullo

The science behind galaxy interaction and mergers has a fundamental role and gives us an insight into galaxy formation and its evolution. Fluctuating angular momentum is responsible for extraordinary events like polar rings, tidal tails,…

星系天体物理 · 物理学 2021-12-24 Adarsh Mahor , Janvita Reddy , Amitesh Singh , Shashwat Singh

To determine the parameters (masses, orbital period) of a binary, one requires among others the inclination, which is best determined from a visual orbit. The next generation of interferometers can provide visual orbits for a large number…

天体物理学 · 物理学 2007-05-23 Frank Verbunt

It is believed that some numerical technique must be employed for the determination of the system parameters of a visual binary or a star with a planet because the relevant equations are not only highly nonlinear but also transcendental…

天体物理学 · 物理学 2015-06-24 Hideki Asada , Toshio Akasaka , Masumi Kasai

In this work we focus on the determination of the relative distributions of young, intermediate-age and old populations of stars in galaxies. Starting from a grid of theoretical population synthesis models we constructed a set of model…

天体物理学 · 物理学 2007-05-23 Thamar Solorio , Olac Fuentes , Roberto Terlevich , Elena Terlevich , Sandro Bressan

It is difficult to discover pulsars via their gamma-ray emission because current instruments typically detect fewer than one photon per million rotations. This creates a significant computing challenge for isolated pulsars, where the…

高能天体物理现象 · 物理学 2020-10-23 L. Nieder , B. Allen , C. J. Clark , H. J. Pletsch

We present a novel orbit parameterization in spherical coordinates. This parameterization enables the mixing of varying and invariant orbital parameters, and clarifies the physics of the orbit. It also simplifies the process of placing…

地球与行星天体物理 · 物理学 2024-10-07 Kevin J Napier , Matthew J Holman

High-volume feature-rich data sets are becoming the bread-and-butter of 21st century astronomy but present significant challenges to scientific discovery. In particular, identifying scientifically significant relationships between sets of…

天体物理仪器与方法 · 物理学 2015-06-15 Matthew J. Graham , S. G. Djorgovski , Ashish A. Mahabal , Ciro Donalek , Andrew J. Drake

An effective procedure to determine the optimal parameters appearing in artificial flockings is proposed in terms of optimization problems. We numerically examine genetic algorithms (GAs) to determine the optimal set of parameters such as…

生物物理 · 物理学 2015-03-13 Motohiro Makiguchi , Jun-ichi Inoue

The numerical optimized shooting method for finding periodic orbits in nonlinear dynamical systems was employed to determine the existence of periodic orbits in the well-known R\"ossler system. By optimizing the period $T$ and the three…

混沌动力学 · 物理学 2014-08-15 A. E. Botha , W. Dednam

This study presents the approach to analyzing the evolution of an arbitrary complex system whose behavior is characterized by a set of different time-dependent factors. The key requirement for these factors is only that they must contain an…

数据分析、统计与概率 · 物理学 2020-12-01 Anatolii V. Mokshin , Vladimir V. Mokshin , Diana A. Mirziyarova

A simple procedure is developed to determine orbital elements of an object orbiting in a central force field which contribute more than three independent celestial positions. By manipulation of formal three point Gauss method of orbit…

地球与行星天体物理 · 物理学 2015-06-17 Taghi Mirtorabi
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