The goal of this research is to use the Sloan Digital Sky Survey (SDSS) to data mine the spectra of quasars and identify redshifted absorption troughs as outflows. Of the thousands of objects found in the SDSS, the ones deemed most interesting are analyzed using custom computer software (
Spectral Trough ID) that identifies doublets in the spectra, such as CIV, SiII, and NV. The tables below show our list of future targets for the William Herschel Telescope (WHT), the Very Large Telescope (VLT) at the European Southern Observatory in Chile, and the Hubble Space Telescope (HST).
Maintained by the Virginia Tech Quasar Outflow Group. Please cite responsibly.