SEGUE stellar parameter pipeline. V.
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/926ad1d9-994a-590e-849a-c509226e2b17
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We present a method for the determination of [{alpha}/Fe] ratios from low-resolution (R=2000) SDSS/SEGUE stellar spectra. By means of a star-by-star comparison with degraded...
