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Pointing effects and their consequences for Spitzer IRAC exoplanet observations

机译:指向效应及其对Spitzer IRAC系外行星观测的影响

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Spitzer observations of exoplanets routinely yield accuracies of better than one part in 10,000. However, there remain anumber of issues that limit the attainable precision, particularly for long duration observations. These include initialpointing inaccuracies, pointing wobble, initial target drift, long-term pointing drifts, and low and high frequency jitter.Coupled with small scale, intrapixel sensitivity variations, all of these pointing issues have the potential to producesignificant, correlated photometric noise. We examine each of these issues in turn, discussing their suspected causes andconsequences, and describing possible and planned mitigation techniques.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:Spitzer对系外行星的观测结果通常得出的精确度要超过万分之一。但是,仍然存在许多限制可达到的精度的问题,特别是对于长时间观测而言。这些问题包括初始指向不准确,指向摆动,初始目标漂移,长期指向漂移以及低频和高频抖动,再加上小范围的像素内灵敏度变化,所有这些指向问题都有可能产生大量相关的光度噪声。我们依次研究这些问题,讨论它们的可疑原因和后果,并描述可能的和计划的缓解技术。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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