Traditionally the H-beta index has been used as a reddening free index to measure the surface temperature of stars. Prof. Joner in the department has developed a new H-alpha index that has great promise. We are working together to spectrophotometrically compare the two systems.
The skills of Phscs 529 would be a great deal of help. However, you could learn the spectral reductions as you went along.
If you have questions or are interested in pursuing this research project, contact Eric Hintz for more information.
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