A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu II and Zn II Lines
CoolCAT
Copper abundance from Cu I and Cu II lines in metal-poor star spectra: NLTE versus LTE
Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
Detection of Neutral Phosphorus in the Near-ultraviolet Spectra of Late-type Stars
Detection of the Second r-process Peak Element Tellurium in Metal-poor Stars
Germanium, Arsenic, and Selenium Abundances in Metal-poor Stars
New Fe I Level Energies and Line Identifications from Stellar Spectra
New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra
Precise boron abundance in a sample of metal-poor stars from far-ultraviolet lines
Scientific problems addressed by the Spektr-UV space project (world space Observatory--Ultraviolet)
The boron absorption line at 2089.6 A in HD 140283?
The Chemical Evolution of Phosphorus
The Extreme Overabundance of Molybdenum in Two Metal-poor Stars
The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
The R-process Alliance: A Nearly Complete R-process Abundance Template Derived from Ultraviolet Spectroscopy of the R-process-enhanced Metal-poor Star HD 222925
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
1999-02-15T02:16:11Z/1999-04-09T03:52:19Z
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.
