A New Test of Copper and Zinc Abundances in Late-type Stars Using Ultraviolet Cu II and Zn II Lines, Roederer, Ian U.,Barklem, Paul S., The Astrophysical Journal, 857, 2018-04-01 00:00:00, 2018ApJ...857....2R||CoolCAT, Ayres, T. R., 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, 560, 2005-03-01 00:00:00, 2005ESASP.560..419A||Copper abundance from Cu I and Cu II lines in metal-poor star spectra: NLTE versus LTE, Korotin, S. A.,Andrievsky, S. M.,Zhukova, A. V., Monthly Notices of the Royal Astronomical Society, 480, 2018-10-01 00:00:00, 2018MNRAS.480..965K||Detection of Al II in the Ultraviolet Spectra of Metal-poor Stars: An Empirical LTE Test of NLTE Aluminum Abundance Calculations, Roederer, I. U.,Lawler, James E., The Astrophysical Journal, 912, 2021-05-01 00:00:00, 2021ApJ...912..119R||Detection of Neutral Phosphorus in the Near-ultraviolet Spectra of Late-type Stars, Roederer, Ian U.,Jacobson, Heather R.,Thanathibodee, Thanawuth, The Astrophysical Journal, 797, 2014-12-01 00:00:00, 2014ApJ...797...69R||Detection of the Second r-process Peak Element Tellurium in Metal-poor Stars, Roederer, Ian U.,Lawler, James E.,Cowan, John J., The Astrophysical Journal, 747, 2012-03-01 00:00:00, 2012ApJ...747L...8R||Germanium, Arsenic, and Selenium Abundances in Metal-poor Stars, Roederer, Ian U., The Astrophysical Journal, 756, 2012-09-01 00:00:00, 2012ApJ...756...36R||New Fe I Level Energies and Line Identifications from Stellar Spectra. III. Initial Results from UV, Optical, and Infrared Spectra, Peterson, Ruth C.,Kurucz, Robert L., The Astrophysical Journal Supplement Series, 260, 2022-06-01 00:00:00, 2022ApJS..260...28P||New Fe I Level Energies and Line Identifications from Stellar Spectra, Peterson, Ruth C.,Kurucz, Robert L., The Astrophysical Journal Supplement Series, 216, 2015-01-01 00:00:00, 2015ApJS..216....1P||Scientific problems addressed by the Spektr-UV space project (world space Observatory—U...ltraviolet), Boyarchuk, A. A.,Shustov, B. M.,Savanov, I. S., Astronomy Reports, 60, 2016-01-01 00:00:00, 2016ARep...60....1B||The boron absorption line at 2089.6 Å in HD 140283?, Thorén, P.,Edvardsson, B., Astronomy and Astrophysics, 363, 2000-11-01 00:00:00, 2000A&A...363L..33T||The Chemical Evolution of Phosphorus, Jacobson, Heather R.,Thanathibodee, Thanawuth,Frebel, Anna, The Astrophysical Journal, 796, 2014-12-01 00:00:00, 2014ApJ...796L..24J||The Extreme Overabundance of Molybdenum in Two Metal-poor Stars, Peterson, Ruth C., The Astrophysical Journal, 742, 2011-11-01 00:00:00, 2011ApJ...742...21P||The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks, Roederer, I. U.,Cowan, John J.,Pignatari, Marco, The Astrophysical Journal, 936, 2022-09-01 00:00:00, 2022ApJ...936...84R||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, Roederer, I. U.,Lawler, James E.,Den Hartog, Elizabeth A., The Astrophysical Journal Supplement Series, 260, 2022-06-01 00:00:00, 2022ApJS..260...27R||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, Peterson, R. C.,Barbuy, B.,Spite, M., Astronomy and Astrophysics, 638, 2020-06-01 00:00:00, 2020A&A...638A..64P
Instrument
STIS/CCD, STIS/NUV-MAMA
Temporal Coverage
1999-02-15T02:00:16Z/1999-04-09T05:58:33Z
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.
