VizieR Online Data Catalog: Abundances in 6 metal-poor stars (Roederer+, 2018)

We download UV spectra from the Mikulski Archive for Space Telescopes (MAST). These spectra were collected using the Space Telescope Imaging Spectrograph (STIS) on board the Hubble Space Telescope (HST). We consider a star for inclusion in the sample if extant R~30000 or R~114000 spectra cover at least 2037<=λ<=2127Å, where the CuII and ZnII lines are found. We supplement the UV spectra with high-resolution optical spectra downloaded from online archives, including the European Southern Observatory (ESO) Science Archive Facility and the Keck Observatory Archives. These data were collected with the Ultraviolet and Visual Echelle Spectrograph (UVES) on the Very Large Telescope, the High Accuracy Radial velocity Planet Searcher (HARPS) on the ESO 3.6m Telescope at La Silla, and the High Resolution Echelle Spectrometer (HIRES) on the Keck I Telescope. An optical spectrum of one star was collected previously using the Robert G. Tull Coude Spectrograph at the Harlan J. Smith Telescope at McDonald Observatory (see the details in Roederer+ 2014, J/AJ/147/136).

(3 data files).