Abstract
Ultraviolet (UV) and vacuum ultraviolet (VUV;i.e., below 200nm) astronomy with the GHRS (Goddard High Resolution Spectrograph) and now the STIS (Space Telescope Imaging Spectrograph) on the Hubble Space Telescope requires accurate and complete atomic wavelengths, energy levels, and oscillator strengths.
© 1999 Optical Society of America
PDF ArticleMore Like This
Juliet C. Pickering, Darren G. Smillie, Anne P. Thorne, Gillian Nave, Richard Blackwell-Whitehead, and Peter L. Smith
FWB2 Fourier Transform Spectroscopy (FTS) 2009
Juliet C. Pickering, Richard Blackwell-Whitehead, Darren G. Smillie, Anne P. Thorne, Peter L. Smith, and Gillian Nave
JWA2 Fourier Transform Spectroscopy (FTS) 2007
M. Ruffoni, Juliet C. Pickering, Anne P. Thorne, C. E. Holmes, and Richard Blackwell-Whitehead
FThA3 Fourier Transform Spectroscopy (FTS) 2011