NICMOS Count Rate DependentNon-Linearity in G096 and G141

Details NICMOS Count Rate DependentNon-Linearity in G096 and G141 NICMOS Count Rate DependentNon-Linearity in G096 and G141

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006nicm.rept....2b&link_type=abstract

Instrument Science Report NICMOS 2006-002, 21 pages

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Hubble Space Telescope, Hst, Space Telescope Science Institute, Nicmos

Scientific paper

Since the discovery of the NICMOS count rate dependent non-linearitydocumented in NICMOS ISR 2005-002, additional tests have been conducted tofurther understand and quantify the effect. Long integrations of up to 25 minutesexhibited the same level of non-linearity as the original 1-3 minute integrations.Observations of the star P041C on high background from an internal flat fieldlamp provides another measure of the wavelength dependence of the nonlinearityto compliment the measures based on pure hydrogen WD models.

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