Standard Photometric Systems
Standard star photometry dominated the latter half of the twentieth century reaching its zenith in the 1980s. It was introduced to take advantage of the high sensitivity and large dynamic range of photomultiplier tubes compared to photographic plates. As
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|Source:||Annual Review of Astronomy and Astrophysics|
|01_Bessell_Standard_Photometric_Sy_2005.pdf||651.73 kB||Adobe PDF||Request a copy|
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