Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
Detection of the Second r-process Peak Element Tellurium in Metal-poor Stars
Hubble Space Telescope Observations of Chromospheres in Metal-Deficient Field Giants
Hubble Space Telescope Observations of Heavy Elements in Metal-Poor Galactic Halo Stars
Improved Laboratory Transition Probabilities for Pt I and Application to the Platinum Abundances of BD +17deg3248 and the Sun
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
New Abundance Determinations of Cadmium, Lutetium, and Osmium in the r-process Enriched Star BD +17 3248
StarCAT: A Catalog of Space Telescope Imaging Spectrograph Ultraviolet Echelle Spectra of Stars
The Chemical Composition and Age of the Metal-poor Halo Star BD +17deg3248
The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
1999-06-03T23:27:44Z/2001-01-31T11:08:26Z
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, Cowan comma John, 2006, 'ABUNDANCES IN HALO STARS AND GALACTIC ELEMENT FORMATION', 1.0, European Space Agency, https://doi.org/10.5270/esa-6eusq4a
