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Hierarchical multispectral galaxy decomposition using a MCMC algorithm with multiple temperature simulated annealing

机译:使用多温度模拟退火的MCMC算法进行分层多光谱星系分解

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摘要

We present a new method for the parametric decomposition of barred spiral galaxies in multispectral observations. The observation is modelled with a realistic image formation model and the galaxy is composed of physically significant parametric structures. The model also includes a parametric filtering to remove non-desirable aspects of the observation. Both the model and the filter parameters are estimated by a robust Monte Carlo Markov chain (MCMC) algorithm. The algorithm is based on a Gibbs sampler combined with a novel strategy of simulated annealing in which several temperatures allow to manage efficiently the simulation effort. Besides, the overall decomposition is performed following an original framework: a hierarchy of models from a coarse model to the finest one is defined. At each step of the hierarchy the estimate of a coarse model is used to initialize the estimation of the finer model. This leads to an unsupervised decomposition scheme with a reduced computation time. We have validated the method on simulated and real 5-band images: the results showed the accuracy and the robustness of the proposed approach.
机译:我们提出了一种在多光谱观测中禁止螺旋星系参数分解的新方法。该观测以逼真的图像形成模型建模,并且星系由物理上重要的参数结构组成。该模型还包括参数过滤,以去除观察结果中不希望的方面。通过鲁棒的蒙特卡洛马尔可夫链(MCMC)算法估算模型和滤波器参数。该算法基于Gibbs采样器,并结合了一种新颖的模拟退火策略,该策略中几个温度都可以有效地管理模拟工作。此外,整体分解是按照原始框架执行的:定义了从粗略模型到最佳模型的模型层次。在层次结构的每个步骤中,都会使用粗略模型的估算值来初始化精细模型的估算值。这导致具有减少的计算时间的无监督分解方案。我们已经在模拟和真实的5波段图像上验证了该方法:结果表明了该方法的准确性和鲁棒性。

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