Atomic Transition Probabilities for Ultraviolet and Optical Lines of Tm II
Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations
Detection of Pb II in the Ultraviolet Spectra of Three Metal-poor Stars
Improved Atomic Transition Probabilities for UV and Optical Lines of Hf II and Determination of the Hf Abundance in Two Metal-poor Stars
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
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
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
2019-10-03T18:27:37Z/2020-03-20T08:07:47Z
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, Roederer et al., 2020, 'HD 222925: A unique opportunity to study the full range of nuclei produced by a single r-process event', 1.0, European Space Agency, https://doi.org/10.5270/esa-1k0ijbm
