A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu II and Zn II Lines
Copper abundance from Cu I and Cu II lines in metal-poor star spectra: NLTE versus LTE
The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars HD 19445, HD 84937, HD 94028, HD 140283, and HD 160617
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
2017-02-10T02:20:17Z/2017-08-23T09:57:29Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Peterson comma Ruth C., 2017, 'Tracing the Earliest Nucleosynthesis from Elements Just Past the Iron Peak in Extremely Metal-Poor Dwarfs', 1.0, European Space Agency, https://doi.org/10.5270/esa-wy81b50