The Performance and Scientific Rationale for an Ir Imaging Fourier Transform Spectrograph on a Large Space Telescope

نویسندگان

  • James R. Graham
  • Mark Abrams
چکیده

We describe a concept for an imaging spectrograph for a large orbiting observatory such as NASA’s proposed Next Generation Space Telescope (NGST) based on an imaging Fourier transform spectrograph (IFTS). An IFTS has several important advantages which make it an ideal instrument to pursue the scientific objectives of NGST. We review the operation of an IFTS and make a quantitative evaluation of the signal-to-noise performance of such an instrument in the context of NGST.

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تاریخ انتشار 1998