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
Hubble Space Telescope Near-ultraviolet Spectroscopy of the Bright CEMP-no Star BD+44deg493
In the Trenches of the Solar-Stellar Connection. VII. Wilson-Bappu 2022
New Detections of Arsenic, Selenium, and Other Heavy Elements in Two Metal-poor Stars
New Hubble Space Telescope Observations of Heavy Elements in Four Metal-Poor Stars
Non-LTE aluminium abundances in late-type stars
Scientific problems addressed by the Spektr-UV space project (world space Observatory--Ultraviolet)
The Chemical Evolution of Phosphorus
Instrument
STIS, STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
2011-06-11T13:07:02Z/2011-09-06T03:58:21Z
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 comma Ian U., 2012, 'Production of the Heavy Elements in the Universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-e2nudv2
