Stars-894

to find "hidden" satellite galaxies by tracking their white dwarf populations. IOPscience

By taking a spectrum of STARS-894 simultaneously with a target galaxy, data processing pipelines can compare the observed spectrum of the calibration star against its theoretical model. The differences between the two reveal the precise absorption signature of Earth's atmosphere at that exact moment, altitude, and weather condition. This profile is then used to clean the target data. Data Release Context: The SDSS Framework STARS-894

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