research.md

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page	Research

Actinide Abundances Using New U Lines.

In this project, I am using high-quality optical spectra to detect uranium at 4050 angstrom and 4090 angstrom.

An Abundance Pattern From Z=3 to Z=92 of a Metal-Poor Star Using UV + Optical Spectra.

Hubble Constant in the Era of LIGO

Maunder Minimum Candidate in a Sun-Like Star