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 Phosphorus, Sulphur, and Zinc in the Carbon-enhanced Metal-poor Star BD+44 493
Hubble Space Telescope Near-Ultraviolet Spectroscopy of Bright CEMP-s Stars
Hubble Space Telescope Near-ultraviolet Spectroscopy of the Bright CEMP-no Star BD+44deg493
Hubble Space Telescope Ultraviolet Spectroscopy of the Most Iron-poor Star Known
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
Revisiting the Iron Abundance in the Hyper Iron-poor Star HE 1327-2326 with UV COS/HST Data
The Chemical Evolution of Phosphorus
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
2012-02-28T02:06:12Z/2012-09-23T01:23:19Z
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.
European Space Agency, Beers comma Timothy C., 2013, 'The Origins of Carbon-Enhanced Metal-Poor Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-l1lc3sp