Characterization of the WFC3 IR Grisms

Details Characterization of the WFC3 IR Grisms Characterization of the WFC3 IR Grisms

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11552b&link_type=abstract

HST Proposal ID #11552. Cycle 17

Physics

Scientific paper

Image displacement, spectral trace and dispersion, and throughput of the IR G102 and G141 grisms will be verified. The HST flux standard GD 153 will be observed in a 5-point pattern in the IR field of view, which will provide image displacement, spectral trace, and throughput measurements as a function of location within the FOV. Similarly, the planetary nebula PN HB12 will be observed in a 9-point pattern in the IR field of view, which will provide dispersion measurements as a function of FOV position.;

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