NUV High S/N Verification

Details NUV High S/N Verification NUV High S/N Verification

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11481s&link_type=abstract

HST Proposal ID #11481. Cycle 17

Physics

Scientific paper

Collect data at several central wavelengths for each NUV grating in TIME-TAG mode, using multiple FP-POS positions, in order to verify that high signal-to-noise spectra can be obtained. All spectra will have enough counts to permit standard reduction techniques to be used to obtain spectra with a signal-to-noise ratio of at least 30. Very high signal-to-noise spectra will also be obtained in some medium resolution modes in order to demonstrate that a signal-to-noise ratio of at least 100 is possible. This is SMOV Activity COS-21;

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