Compressive Sensing Based Space Flight Instrument Constellation for Measuring Gravitational Microlensing Parallax

Signals Pub Date : 2022-08-15 DOI:10.3390/signals3030034
Asmita Korde-Patel, R. Barry, T. Mohsenin
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引用次数: 1

Abstract

In this work, we provide a compressive sensing architecture for implementing on a space based observatory for detecting transient photometric parallax caused by gravitational microlensing events. Compressive sensing (CS) is a simultaneous data acquisition and compression technique, which can greatly reduce on-board resources required for space flight data storage and ground transmission. We simulate microlensing parallax observations using a space observatory constellation, based on CS detectors. Our results show that average CS error is less than 0.5% using 25% Nyquist rate samples. The error at peak magnification time is significantly lower than the error for distinguishing any two microlensing parallax curves at their peak magnification. Thus, CS is an enabling technology for detecting microlensing parallax, without causing any loss in detection accuracy.
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基于压缩感知的空间飞行仪器星座引力微透镜视差测量
在这项工作中,我们提供了一种压缩感知架构,用于在天基天文台上实现对引力微透镜事件引起的瞬态光度视差的检测。压缩感知(CS)是一种同时进行数据采集和压缩的技术,可以大大减少空间飞行数据存储和地面传输所需的机载资源。我们模拟微透镜视差观测利用空间天文台星座,基于CS探测器。我们的结果表明,使用25%奈奎斯特率的样本,平均CS误差小于0.5%。在峰值放大时的误差明显小于任意两个微透镜视差曲线在其峰值放大时的误差。因此,CS是一种检测微透镜视差的使能技术,不会造成任何检测精度的损失。
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来源期刊
CiteScore
3.20
自引率
0.00%
发文量
0
审稿时长
11 weeks
期刊最新文献
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