Constraining Galaxy Evolution With Hubble’s Next Generation Spectral Library
We present Hubble’s Next Generation Spectral Library, a library of UV-optical spectra (0.2-1.0 μ) of 378 stars. We show that the mid-UV spectrum can be used to constrain the ages and metallicities of high-redshift galaxies presently being observed with large, ground-based telescopes.
KeywordsSpectral Index Stellar Population Chromospheric Emission Blue Straggler Simple Stellar Population
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