Chao Jerry, Ram Sripad, Ward E Sally, Ober Raimund J
Dept. of Electrical Engineering, University of Texas at Dallas, Richardson, TX, USA ; Dept. of Immunology, University of Texas Southwestern Medical Center, Dallas, TX, USA.
Dept. of Immunology, University of Texas Southwestern Medical Center, Dallas, TX, USA.
Proc SPIE Int Soc Opt Eng. 2013 Feb 22;8589:858905. doi: 10.1117/12.2004621.
The extraction of information from images acquired under low light conditions represents a common task in diverse disciplines. In single molecule microscopy, for example, techniques for superresolution image reconstruction depend on the accurate estimation of the locations of individual particles from generally low light images. In order to estimate a quantity of interest with high accuracy, however, an appropriate model for the image data is needed. To this end, we previously introduced a data model for an image that is acquired using the electron-multiplying charge-coupled device (EMCCD) detector, a technology of choice for low light imaging due to its ability to amplify weak signals significantly above its readout noise floor. Specifically, we proposed the use of a geometrically multiplied branching process to model the EMCCD detector's stochastic signal amplification. Geometric multiplication, however, can be computationally expensive and challenging to work with analytically. We therefore describe here two approximations for geometric multiplication that can be used instead. The high gain approximation is appropriate when a high level of signal amplification is used, a scenario which corresponds to the typical usage of an EMCCD detector. It is an accurate approximation that is computationally more efficient, and can be used to perform maximum likelihood estimation on EMCCD image data. In contrast, the Gaussian approximation is applicable at all levels of signal amplification, but is only accurate when the initial signal to be amplified is relatively large. As we demonstrate, it can importantly facilitate the analysis of an information-theoretic quantity called the noise coefficient.
从低光照条件下获取的图像中提取信息是不同学科中的一项常见任务。例如,在单分子显微镜中,超分辨率图像重建技术依赖于从一般的低光照图像中准确估计单个粒子的位置。然而,为了高精度地估计感兴趣的量,需要一个合适的图像数据模型。为此,我们之前引入了一种用于使用电子倍增电荷耦合器件(EMCCD)探测器获取的图像的数据模型,由于其能够将微弱信号放大到显著高于其读出噪声底限的能力,EMCCD探测器是低光照成像的首选技术。具体而言,我们提出使用几何倍增分支过程来模拟EMCCD探测器的随机信号放大。然而,几何倍增在计算上可能很昂贵,并且在分析处理时具有挑战性。因此,我们在此描述两种可替代使用的几何倍增近似方法。高增益近似在使用高水平信号放大时适用,这种情况对应于EMCCD探测器的典型使用场景。它是一种准确的近似方法,计算效率更高,可用于对EMCCD图像数据进行最大似然估计。相比之下,高斯近似适用于所有信号放大水平,但仅在待放大的初始信号相对较大时才准确。正如我们所展示的,它可以重要地促进对一种称为噪声系数的信息论量的分析。