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Simplified Color Photometry Using APASS Data

机译:使用APASS数据简化彩色光度法

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摘要

APASS, the AAVSO Photometric All-Sky Survey, now contains 47 million stars and covers 97% of the Northern and Southern hemisphere sky. Its extraordinary coverage means that there are multiple APASS-calibrated stars available for color photometry in the field of view of virtually every amateur image. This paper presents a simplified spreadsheet-based procedure that combines raw photometric data with APASS data to calibrate target objects in the same field of view. The complete photometric equations are reviewed and a simplified form is obtained for use within a limited field of view. Raw photometric data and APASS data for that image from AAVSO are combined on a spreadsheet to produce calibrated photometric measurements of target objects within the field of view. The consistency of the fit to the data is shown graphically. Error terms are tracked through the equations to provide the standard deviation of each measurement.
机译:APASS是AAVSO光度全天候测量,目前包含4,700万颗恒星,覆盖了北半球和南半球的97%。其出色的覆盖范围意味着几乎每一个业余图像的视野中都可以使用多个APASS校准的恒星进行彩色光度测量。本文介绍了一种简化的基于电子表格的过程,该过程将原始光度数据与APASS数据结合在一起,以在同一视野中校准目标对象。审查了完整的光度方程,并获得了简化的形式以在有限的视野内使用。来自AAVSO的该图像的原始光度数据和APASS数据在电子表格上进行合并,以生成视野内目标物体的校准光度测量结果。数据拟合的一致性以图形方式显示。通过方程式跟踪误差项,以提供每次测量的标准偏差。

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