Image Details
Caption: Figure 4.
The spectra of an M31 globular cluster between 4800 Å and 5100 Å, showing our raw data, along with the data after sky subtraction, Doppler shifting, and template subtraction. Note that after template subtraction, the [O iii] λ5007 emission line is easily seen. This is a well-detected and well-measured emission-line source containing ~1000 counts in [O iii] λ5007.
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