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Session 55 - Space Instrumentation.
Display session, Wednesday, June 12
Tripp Commons,

[55.11] Spectrophotometric Standards from the Far-UV to the Near-IR on the White Dwarf Flux Scale

R. C. Bohlin (STScI)

The second generation instruments to be installed in 1997 on the Hubble Space Telescope (HST)\/ require spectrophotometric standard stars for flux calibrations to 1.1 \mum for the imaging spectrograph (STIS) and to 2.5 \mum for the infrared camera (NICMOS). Calculated model atmosphere flux distributions from 0.1 to 3 \mum for four pure hydrogen white dwarfs provide the fundamental basis for a new set of spectrophotometric standard stars. Precise visual photometry sets the absolute level of the model fluxes, while FOS spectrophotometry validates the relative V magnitudes to \sim1% and the relative fluxes at other wavelengths to \sim2%. Extensive FOS observations of four more stars from 1140--8500Å\ expand the set of primary standards to eight stars.

These eight flux distributions are compared with IUE fluxes in the UV and with Oke spectrophotometry in the visual to define corrections as a function of wavelength. These corrections plus a wavelength independent correction to the Oke fluxes are accurate to \sim3% and provide 18 additional standards on the WD scale from 1150--9200ÅOne more standard \alpha Lyr consists of IUE data plus the ground based spectrum of Hayes. This library of standard star fluxes can be accessed via the world wide web with the URL

Program listing for Wednesday