Wavelength: Å Source flux at above wavelength (observed) : Total flux: ergs cm-2 s-1 Å-1 Area flux per arcsec squared: ergs cm-2 s-1 Å-1 arcsec-2 Instrument: Short Wavelength VUVES Short Wavelength VUVES (GaN + LiF) Long Wavelength UVES (CsTe + MgF2) Long Wavelength UVES (GaN + MgF2) Long Wavelength UVES (GaN + Quartz) Long Slit Spectrometer (UV) Long Slit Spectrometer (UV / GaN + MgF2) Long Slit Spectrometer (VUV) Long Slit Spectrometer (VUV / GaN + LiF) Redundant Detector: Science requirements: Calculate the integration time necessary to reach a signal-to-noise ratio of Calculate signal-to-noise ratio (per spectral bin) obtained in an integration of seconds Spectral Bin Size: Pixels
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