Grism/Prism Calibration

Details Grism/Prism Calibration Grism/Prism Calibration

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hst..prop.9568p&link_type=abstract

HST Proposal ID #9568

Computer Science

Hst Proposal Id #9568

Scientific paper

A Planetary Nebula in the LMC and a Galactic White Dwarf are observed through the prism of the High Resolution Channel to measure: 1} the dispersion of the prism and its field dependence; 2} the prism throughput and its field dependence. Therefore, these measurements will be carried out at several positions on the chip including the centre and the corners of the HRC chip. The same White Dwarf is observed together with a Galactic Wolf-Rayet star through the grism of the Wide Field Channel in a number of positions complementing those already observed in SMOV. The purpose here is to better characterise the field dependence of the grism dispersion in the WFC.

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