http://arxiv.org/abs/2206.01007
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.
B. Huang, K. Xiao and H. Yuan
Fri, 3 Jun 22
19/57
Comments: Scientia Sinica Physica, Mechanica & Astronomica accepted, in Chinese language