UVIS G280 Wavelength Calibration

Details UVIS G280 Wavelength Calibration UVIS G280 Wavelength Calibration

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11935b&link_type=abstract

HST Proposal ID #11935. Cycle 17

Computer Science

Scientific paper

Wavelength calibration of the UVIS G280 grism will be established using observations of the Wolf Rayet star WR14. Accompanying direct exposures will provide wavelength zeropoints for dispersed exposures. The calibrations will be obtained at the central position of each CCD chip and at the center of the UVIS field. No additional field-dependent variations will be obtained.;

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