论文标题
宽场光度测验的光度校准方法
Photometric calibration methods for wide-field photometric surveys
论文作者
论文摘要
均匀，准确的光度校准在电流和下一代宽视野成像调查中起重要作用。在此，我们回顾了现代的光度校准方法，包括经典的标准星方法，“硬件/观察驱动”方法（例如UberCalibration，UberCalibration，AfferCalibration和Forward Global Global Calibration方法）以及“软件/物理驱动的”方法（例如，Stellar locus Recressions，Stellar Recressions，Stellar locus locus and stellar locuss and stellar colorsess and sertellar colorseds seltellar colorsess and seltellar colorsesssssss）。此外，我们讨论了它们对毫米级精确校准的优势，局限性和未来的发展。
Uniform and accurate photometric calibration plays an important role in the current and next-generation wide-field imaging surveys. Herein, we review the modern photometric calibration methods, including the classic standard star method, "hardware/observation-driven" methods (such as the Ubercalibration, Hypercalibration, and Forward Global Calibration Methods), and "software/physics-driven" methods (e.g., the Stellar Locus Regression, Stellar Locus, and Stellar Color Regression Methods). Further, we discuss their advantages, limitations, and future developments toward millimagnitude precision calibration.
